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			<title>EGU Blogs - Recent Division Posts</title>
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					<title><![CDATA[The beauty of Soil!]]></title>
					<link>https://blogs.egu.eu/divisions/bg/2026/05/29/the-beauty-of-soil/</link>
					<comments>https://blogs.egu.eu/divisions/bg/2026/05/29/the-beauty-of-soil/#comments</comments>
					<pubDate>Fri, 29 May 2026 10:07:38 +0000</pubDate>
					<dc:creator><![CDATA[Saule Akhmetkaliyeva]]></dc:creator>
							<category><![CDATA[Biogeosciences]]></category>
		<category><![CDATA[Fun]]></category>
		<category><![CDATA[Science]]></category>
		<category><![CDATA[biogeosciences]]></category>
		<category><![CDATA[EU Soil Monitoring Law]]></category>
		<category><![CDATA[soil health]]></category>
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											<description><![CDATA[The Life Beneath Our Feet Where would we be without healthy soil? A lot of our research live would be in turmoil I’m here today to spread some soil appreciation, Which may require some thought transformation. Soil Is the base of our beautiful landscapes, Often where we go for some restorative escapes, Some key reasons to save soils from destruction They support 95% of global food production, And act as a filter for water purification, Don’t forget it’s major role in carbon sequestration  So how do we generate the respect and love it deserves? By learning about the life-sources it serves! Think not of the chicken, the sheep or the cattle, When that’s really only half of the battle, Think of the livestock that lives under the surface, As they hold a much more meaningful purpose. Earthworms are by far the most popular soil dwellers, Aerating the soil for the smallest of fellas Some organisms you would need a microscope to spot, But their presence can really tell us a lot, Enchytraieds and eathworms share a connection, But often they don’t get as much attention, Enchytraeids prefer acidic soils, high in peat, Fungi and bacteria is what they eat Look for collembola as soil health indication, Due to their habitat specification Leaf litter and moss is their preferred habitation, Driving the engine of organic matter rotation, Both springtails and mites can help to distribute Many different microbes as they are so minute, Attached to their backs and through digestion, The many soil benefits not even in question Last on our list are these nematode creatures, Which possess a whole litany of soil beneficial features. From nutrient cycling to plant protection, Parasitic species can kill pests through infection! We simply need to get people excited, to get them involved, their passions ignited! Show them why soil biodiversity really matters, Providing the food they see on their platters, The monitoring law will help us by tracking, A suite of soil data that is currently lacking, Which soils need protection and perhaps some improvement Lets get people on board this healthy soil movement! Not just Dirt: Why we need to care about Soil health Soil is often overlooked. It is something we walk over without a second thought. We admire the life it sustains, wandering through forests, woodlands, and grasslands, marvelling at the beauty of the above ground systems. The reality is that without healthy soil, these landscapes would cease to exist. Our food, our water, and even the air we breathe are fundamentally dependent on what lies beneath our feet. Recognising this, the European Union is rolling out the EU Soil Monitoring Law. Member states now have three years to develop their own national monitoring plans. However, current guidelines remain quite loose. In terms of biology, the only compulsory parameter is DNA barcoding, largely because scientific consensus on the most effective indicators for soil health remains elusive. While soil chemistry and physics have been extensively studied, our understanding of the biological realm lags somewhat behind. I believe that to gain a truly realistic snapshot of soil health, we must move toward an integrated approach where biology, chemistry, and physics work in cohesion. This is a challenge I grappled with during my first postdoc, where I investigated the intricate links between soil biology and geochemistry. I sampled 200 sites across Ireland, collecting mites, collembola, nematodes, and enchytraeids from soils with known geochemical profiles. My findings confirmed that geochemistry is just as vital as land use in explaining the distribution of these biological organisms. The poem above is my reflection of this research. Written by Aisling Moffat, edited by Saule Akhmetkaliyeva]]></description>
													<content:encoded><![CDATA[<p style="text-align: center"><b style="background-color: transparent;font-size: 24px;color: #2b2b2b">The Life Beneath Our Feet</b></p>
<p style="text-align: center"><span style="font-weight: 400">Where would we be without healthy soil?
</span><span style="font-weight: 400">A lot of our research live would be in turmoil
</span><span style="font-weight: 400">I’m here today to spread some soil appreciation,
</span><span style="font-weight: 400">Which may require some thought transformation.</span></p>
<p style="text-align: center"><span style="font-weight: 400">Soil Is the base of our beautiful landscapes,
</span><span style="font-weight: 400">Often where we go for some restorative escapes,
</span><span style="font-weight: 400">Some key reasons to save soils from destruction
</span><span style="font-weight: 400">They support 95% of global food production,
</span><span style="font-weight: 400">And act as a filter for water purification,
</span><span style="font-weight: 400">Don’t forget it’s major role in carbon sequestration</span><span style="font-weight: 400"> </span></p>
<p style="text-align: center"><span style="font-weight: 400">So how do we generate the respect and love it deserves?
</span><span style="font-weight: 400">By learning about the life-sources it serves!
</span><span style="font-weight: 400">Think not of the chicken, the sheep or the cattle,
</span><span style="font-weight: 400">When that’s really only half of the battle,
</span><span style="font-weight: 400">Think of the livestock that lives under the surface,
</span><span style="font-weight: 400">As they hold a much more meaningful purpose.</span></p>
<p style="text-align: center"><span style="font-weight: 400">Earthworms are by far the most popular soil dwellers,
</span><span style="font-weight: 400">Aerating the soil for the smallest of fellas
</span><span style="font-weight: 400">Some organisms you would need a microscope to spot,
</span><span style="font-weight: 400">But their presence can really tell us a lot,
</span><span style="font-weight: 400">Enchytraieds and eathworms share a connection,
</span><span style="font-weight: 400">But often they don’t get as much attention,
</span><span style="font-weight: 400">Enchytraeids prefer acidic soils, high in peat,
</span><span style="font-weight: 400">Fungi and bacteria is what they eat</span></p>
<p style="text-align: center"><span style="font-weight: 400">Look for collembola as soil health indication,
</span><span style="font-weight: 400">Due to their habitat specification
</span><span style="font-weight: 400">Leaf litter and moss is their preferred habitation,
</span><span style="font-weight: 400">Driving the engine of organic matter rotation,
</span><span style="font-weight: 400">Both springtails and mites can help to distribute
</span><span style="font-weight: 400">Many different microbes as they are so minute,
</span><span style="font-weight: 400">Attached to their backs and through digestion,
</span><span style="font-weight: 400">The many soil benefits not even in question</span></p>
<p style="text-align: center"><span style="font-weight: 400">Last on our list are these nematode creatures,
</span><span style="font-weight: 400">Which possess a whole litany of soil beneficial features.
</span><span style="font-weight: 400">From nutrient cycling to plant protection,
</span><span style="font-weight: 400">Parasitic species can kill pests through infection!</span></p>
<p style="text-align: center"><span style="font-weight: 400">We simply need to get people excited,
</span><span style="font-weight: 400">to get them involved, their passions ignited!
</span><span style="font-weight: 400">Show them why soil biodiversity really matters,
</span><span style="font-weight: 400">Providing the food they see on their platters,
</span><span style="font-weight: 400">The monitoring law will help us by tracking,
</span><span style="font-weight: 400">A suite of soil data that is currently lacking,
</span><span style="font-weight: 400">Which soils need protection and perhaps some improvement
</span><span style="font-weight: 400">Lets get people on board this healthy soil movement!</span></p>


[caption id="attachment_4081" align="alignleft" width="1600"]<a href="https://blogs.egu.eu/divisions/bg/files/2026/05/soil1.png"><img class="wp-image-4081 size-full" src="https://blogs.egu.eu/divisions/bg/files/2026/05/soil1.png" alt="" width="1600" height="533" /></a> Images taken from fieldwork across Ireland, depicting the vast differences in soil management practices and the associated biology (photo credit Aisling Moffat).[/caption]

<b style="font-size: 24px;color: #2b2b2b">Not just Dirt: Why we need to care about Soil health</b>

<span style="font-weight: 400">Soil is often overlooked. It is something we walk over without a second thought. We admire the life it sustains, wandering through forests, woodlands, and grasslands, marvelling at the beauty of the above ground systems. The reality is that without healthy soil, these landscapes would cease to exist. Our food, our water, and even the air we breathe are fundamentally dependent on what lies beneath our feet.</span>

<span style="font-weight: 400">Recognising this, the European Union is rolling out the EU Soil Monitoring Law. Member states now have three years to develop their own national monitoring plans. However, current guidelines remain quite loose. In terms of biology, the only compulsory parameter is DNA barcoding, largely because scientific consensus on the most effective indicators for soil health remains elusive.</span>

<span style="font-weight: 400">While soil chemistry and physics have been extensively studied, our understanding of the biological realm lags somewhat behind. I believe that to gain a truly realistic snapshot of soil health, we must move toward an integrated approach where biology, chemistry, and physics work in cohesion.</span>

<span style="font-weight: 400">This is a challenge I grappled with during my first postdoc, where I investigated the intricate links between soil biology and geochemistry. I sampled 200 sites across Ireland, collecting mites, collembola, nematodes, and enchytraeids from soils with known geochemical profiles. My findings confirmed that geochemistry is just as vital as land use in explaining the distribution of these biological organisms. </span><span style="font-weight: 400">The poem above is my reflection of this research.</span>

[caption id="attachment_4078" align="alignleft" width="1280"]<a href="https://blogs.egu.eu/divisions/bg/files/2026/05/Mites_Nematodes_EGU.png"><img class="wp-image-4078 size-full" src="https://blogs.egu.eu/divisions/bg/files/2026/05/Mites_Nematodes_EGU.png" alt="" width="1280" height="720" /></a> Mites surrounding a springtail (left), and two adult nematodes from the same soil sample showing striking size differences (right) ((photo credit Aisling Moffat).[/caption]

<em><span style="font-weight: 400">Written by Aisling Moffat, edited by <span class="_pe_N2 PersonaPaneLauncher" role="presentation"><span class="_pe_l"><span class="bidi allowTextSelection" aria-label="Von Saule Akhmetkaliyeva &lt;saule.akhmetkaliyeva@ucd.ie&gt;. Drücken Sie die EINGABETASTE, um die Visitenkarte zu öffnen."><span id="0.4782608037071714" class="highlight">Saule</span> Akhmetkaliyeva</span></span></span></span></em>]]></content:encoded>
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					<title><![CDATA[Listening to reflections: What GNSS signals can tell us about a changing environment]]></title>
					<link>https://blogs.egu.eu/divisions/g/2026/05/29/bits-and-bites-gnss-ir/</link>
					<comments>https://blogs.egu.eu/divisions/g/2026/05/29/bits-and-bites-gnss-ir/#comments</comments>
					<pubDate>Fri, 29 May 2026 09:15:23 +0000</pubDate>
					<dc:creator><![CDATA[Leire Retegui-Schiettekatte]]></dc:creator>
							<category><![CDATA[Bits & Bites]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Global Navigation Satellite Systems (GNSS) are best known for positioning, navigation, and monitoring Earth surface motions with high precision (see two of our previous posts on GNSS here and here). But did you know that the same satellite signals can also provide information about snow, soil moisture, or sea level, without installing any additional instruments? This idea lies at the heart of GNSS Interferometric Reflectometry (GNSS-IR). What may initially sound like a specialised remote sensing technique is, in fact, a clever reinterpretation of signals that GNSS was never designed to observe. When “bad signals” become useful As explained in previous posts, GNSS positioning relies on electromagnetic signals sent from satellites to ground receivers. However, due to objects and surfaces in the environment of the receiver instrument (e.g., buildings, vegetation, ground or water bodies), the instrument might also receive reflections (or “echoes”) of this signal in addition to the direct signal emitted by the satellite (Fig. 1). When signals reach a receiver both directly and after reflecting off nearby surfaces, they interfere and introduce errors. This is referred to as the “multipath effect”. Considerable effort has been devoted over many years to mitigating this multipath effect in positioning applications. GNSS-IR takes the opposite view. Instead of suppressing multipath, it uses it as a source of information. The key observable is the signal-to-noise ratio (SNR), a variable that defines the intensity of noise in relation to the intensity of the signal. As satellites rise or set, the changing path difference between direct and reflected signals produces oscillations in the SNR time series. The frequency of these oscillations is linked to the distance between the antenna and the reflecting surface, commonly referred to as the reflector height. Analysing these patterns allows changes in the surrounding environment to be inferred (Fig. 1). &nbsp; Measuring changes from land surfaces to the coast How can these oscillations be used to infer information on the environment of the GNSS receiver? The principle is simple. Over the coast, changes in sea level modify the reflector height and therefore the SNR oscillation pattern. Analyzing these SNR oscillations can therefore provide information on sea level changes. Over land, snow accumulation, soil moisture variations, or vegetation can leave similar signatures in the reflected signal and can hence also be tracked through GNSS-IR. GNSS-IR relies entirely on existing GNSS infrastructure that is already operating worldwide. This makes it particularly attractive for environmental monitoring, as no dedicated sensors or transmitters are required. In fact, since its first demonstrations nearly two decades ago, it has been successfully applied to measure changes in all of the natural elements described above, complementing established techniques such as tide gauges and satellite radar altimetry. In coastal settings, GNSS-IR is especially useful. Tide gauges provide high temporal sampling but are affected by vertical land motion and uneven global distribution. Satellite altimetry offers global coverage but performs less reliably close to the coast (read more about satellite altimetry in one of our previous posts here). GNSS-IR fills part of this gap by providing local sea level estimates with comparatively high temporal and spatial resolution at many existing coastal GNSS stations (Fig. 2). In some cases, long archives of GNSS data can even be reprocessed to study past sea level variations. GNSS-IR in practice Despite its conceptual simplicity, GNSS-IR is not a push-button technique. Several factors can challenge or facilitate these measurements: Reflection geometry: Useful reflections are limited to specific satellite viewing angles and directions that depend on local topography. Some stations remain challenging regardless of how much data is available. For example, a station surrounded by buildings or steep terrain may block the low-angle signals that GNSS-IR relies on most. Surface characteristics: GNSS-IR performs best near wide, relatively flat, and stable reflecting surfaces. Over land, open and homogeneous areas are favourable, while coastal applications require an unobstructed view of the sea. Signal diversity: Not all satellite signals perform equally well for reflectometry. Different signal types show varying sensitivity to reflections, and increasing the number of satellites or frequencies generally improves robustness, but does not compensate for poor site geometry. Receiver and antenna setup: The hardware used at a station can strongly influence the quality of reflected signals. Recording data at higher rates can improve results, especially at sites with larger antenna heights. It is also essential that signal strength information is retained in the observation files, as this is the primary input for GNSS-IR analysis. Site documentation: Photographing the station environment is a simple but valuable step. It helps assess whether a site is suitable for GNSS-IR and guides the selection of appropriate analysis parameters. Strengths, limitations, and why GNSS-IR matters GNSS-IR does not replace tide gauges or satellite altimetry. Instead, it complements them. Its strengths include low cost, flexible deployment, and the ability to reuse existing GNSS data streams. Importantly, GNSS-IR does not require high-end geodetic equipment. Low-cost GNSS receivers and even smartphones, which are usually more affected by multipath and therefore less suitable for precise positioning, can be advantageous for reflectometry. Stronger multipath signatures often make reflected signals easier to detect and analyse. Open-source software further enhances accessibility. Community-driven tools such as the MATLAB based GIRAS package and the Python toolbox gnssrefl support a wide range of GNSS-IR analyses, lowering the entry barrier and improving transparency and reproducibility. More broadly, GNSS-IR illustrates a recurring theme in geodesy. Signals often contain more information than initially expected. By rethinking what was once treated as an error, GNSS-IR turns unwanted reflections into a valuable source of environmental information. So next time a GNSS receiver struggles with multipath, it may be worth listening more closely. Those reflections could be telling a story about the world beneath our feet. Further reading For those interested in learning more about GNSS-IR, the following resources provide a good starting point: Larson, K.M., 2016. GPS interferometric reflectometry: applications to surface soil moisture, snow depth, and vegetation water content in the western United States. WIREs Water 3, 775–787. https://doi.org/10.1002/wat2.1167 Larson, K.M., Williams, S.D.P., 2023. Water level measurements using reflected GNSS signals. IHR 29, 66–76. https://doi.org/10.58440/ihr-29-2-a30 For an interactive introduction to the technique, visit gnss-reflections.org. &#8211; Edited by: Leire Retegui-Schiettekatte]]></description>
													<content:encoded><![CDATA[Global Navigation Satellite Systems (GNSS) are best known for positioning, navigation, and monitoring Earth surface motions with high precision (see two of our previous posts on GNSS <a href="https://blogs.egu.eu/divisions/g/2025/07/25/bits-and-bites-of-geodesy-trilateration-on-vacation-how-gnss-locates-you/" target="_blank" rel="noopener"><u>here </u></a>and <a href="https://blogs.egu.eu/divisions/g/2025/11/28/beyond_navigationhow-gnssrevealsearthshiddensecrets/" target="_blank" rel="noopener"><u>here</u></a>). But did you know that the same satellite signals can also provide information about snow, soil moisture, or sea level, without installing any additional instruments?

This idea lies at the heart of GNSS Interferometric Reflectometry (GNSS-IR). What may initially sound like a specialised remote sensing technique is, in fact, a clever reinterpretation of signals that GNSS was never designed to observe.

<strong>When “bad signals” become useful</strong>

As explained in previous posts, GNSS positioning relies on electromagnetic signals sent from satellites to ground receivers. However, due to objects and surfaces in the environment of the receiver instrument (e.g., buildings, vegetation, ground or water bodies), the instrument might also receive reflections (or “echoes”) of this signal in addition to the direct signal emitted by the satellite (Fig. 1).

When signals reach a receiver both directly and after reflecting off nearby surfaces, they interfere and introduce errors. This is referred to as the “multipath effect”. Considerable effort has been devoted over many years to mitigating this multipath effect in positioning applications.

GNSS-IR takes the opposite view. Instead of suppressing multipath, it uses it as a source of information. The key observable is the signal-to-noise ratio (SNR), a variable that defines the intensity of noise in relation to the intensity of the signal. As satellites rise or set, the changing path difference between direct and reflected signals produces oscillations in the SNR time series. The frequency of these oscillations is linked to the distance between the antenna and the reflecting surface, commonly referred to as the reflector height. Analysing these patterns allows changes in the surrounding environment to be inferred (Fig. 1).

[caption id="attachment_5763" align="aligncenter" width="483"]<a href="https://blogs.egu.eu/divisions/g/files/2026/05/GNSS_IR_K_Larson_HR.png"><img class="wp-image-5763 " src="https://blogs.egu.eu/divisions/g/files/2026/05/GNSS_IR_K_Larson_HR-300x225.png" alt="Illustration of the GNSS-IR principle using signal interference to determine reflector height." width="483" height="362" /></a> <strong>Fig. 1: Illustration of the GNSS-IR principle using signal interference to determine reflector height</strong>. Source: K. Larson, <span style="text-decoration: underline"><a href="https://gnss-reflections.org/static/images/overview.png">https://gnss-reflections.org/static/images/overview.png</a></span>.[/caption]

&nbsp;

<strong>Measuring changes </strong><strong>f</strong><strong>rom land surfaces to the coast</strong>

How can these oscillations be used to infer information on the environment of the GNSS receiver? The principle is simple. Over the coast, changes in sea level modify the reflector height and therefore the SNR oscillation pattern. Analyzing these SNR oscillations can therefore provide information on sea level changes. Over land, snow accumulation, soil moisture variations, or vegetation can leave similar signatures in the reflected signal and can hence also be tracked through GNSS-IR.

GNSS-IR relies entirely on existing GNSS infrastructure that is already operating worldwide. This makes it particularly attractive for environmental monitoring, as no dedicated sensors or transmitters are required. In fact, since its first demonstrations nearly two decades ago, it has been successfully applied to measure changes in all of the natural elements described above, complementing established techniques such as tide gauges and satellite radar altimetry.

In coastal settings, GNSS-IR is especially useful. Tide gauges provide high temporal sampling but are affected by vertical land motion and uneven global distribution. Satellite altimetry offers global coverage but performs less reliably close to the coast (read more about satellite altimetry in one of our previous posts <a href="https://blogs.egu.eu/divisions/g/2024/03/01/bits-and-bites-of-geodesy-satellite-radar-altimetry-how-do-we-know-that-sea-level-is-rising/" target="_blank" rel="noopener"><u>here</u></a>). GNSS-IR fills part of this gap by providing local sea level estimates with comparatively high temporal and spatial resolution at many existing coastal GNSS stations (Fig. 2). In some cases, long archives of GNSS data can even be reprocessed to study past sea level variations.

[caption id="attachment_5780" align="aligncenter" width="600"]<a href="https://blogs.egu.eu/divisions/g/files/2026/05/GNSS_IR_time_series_Cemali_Altuntas_HR.png"><img class="wp-image-5780" src="https://blogs.egu.eu/divisions/g/files/2026/05/GNSS_IR_time_series_Cemali_Altuntas_HR-300x160.png" alt="Fig. 2: An example of GNSS-IR sea level estimation comparing solutions versus tide gauge data at station Ijmuiden, Netherlands (IJMU00NLD) (2025-02-01 to 2025-02-07). GNSS-IR solutions (black dots) were obtained using the WinLSP method within an elevation range of 2°–12° and an azimuth range of 0°–110°, showing strong agreement with the reference tide gauge (orange line). The data was processed using a 1-hour sliding window shifted every 10 minutes. Outliers were removed based on standard deviation thresholds for height (&lt;0.2 m) and height rate (&lt;0.5 m/h)." width="600" height="320" /></a> <strong>Fig. 2: An example of GNSS-IR sea level estimation comparing solutions versus tide gauge data at station Ijmuiden, Netherlands (IJMU00NLD) (2025-02-01 to 2025-02-07).</strong> GNSS-IR solutions (black dots) were obtained using the WinLSP method within an elevation range of 2°–12° and an azimuth range of 0°–110°, showing strong agreement with the reference tide gauge (orange line). The data was processed using a 1-hour sliding window shifted every 10 minutes. Outliers were removed based on standard deviation thresholds for height (&lt;0.2 m) and height rate (&lt;0.5 m/h).[/caption]

<strong>GNSS-IR in practice</strong>

Despite its conceptual simplicity, GNSS-IR is not a push-button technique. Several factors can challenge or facilitate these measurements:
<ul>
 	<li><strong>Reflection geometry:</strong> Useful reflections are limited to specific satellite viewing angles and directions that depend on local topography. Some stations remain challenging regardless of how much data is available. For example, a station surrounded by buildings or steep terrain may block the low-angle signals that GNSS-IR relies on most.</li>
 	<li><strong>Surface characteristics:</strong> GNSS-IR performs best near wide, relatively flat, and stable reflecting surfaces. Over land, open and homogeneous areas are favourable, while coastal applications require an unobstructed view of the sea.</li>
 	<li><strong>Signal diversity:</strong> Not all satellite signals perform equally well for reflectometry. Different signal types show varying sensitivity to reflections, and increasing the number of satellites or frequencies generally improves robustness, but does not compensate for poor site geometry.</li>
 	<li><strong>Receiver and antenna setup:</strong> The hardware used at a station can strongly influence the quality of reflected signals. Recording data at higher rates can improve results, especially at sites with larger antenna heights. It is also essential that signal strength information is retained in the observation files, as this is the primary input for GNSS-IR analysis.</li>
 	<li><strong>Site documentation:</strong> Photographing the station environment is a simple but valuable step. It helps assess whether a site is suitable for GNSS-IR and guides the selection of appropriate analysis parameters.</li>
</ul>
<strong>Strengths, limitations, and why GNSS-IR matters</strong>

GNSS-IR does not replace tide gauges or satellite altimetry. Instead, it complements them.

Its strengths include low cost, flexible deployment, and the ability to reuse existing GNSS data streams. Importantly, GNSS-IR does not require high-end geodetic equipment. Low-cost GNSS receivers and even smartphones, which are usually more affected by multipath and therefore less suitable for precise positioning, can be advantageous for reflectometry. Stronger multipath signatures often make reflected signals easier to detect and analyse.

Open-source software further enhances accessibility. Community-driven tools such as the MATLAB based<a href="https://link.springer.com/article/10.1007/s10291-021-01201-3"> </a><a href="https://link.springer.com/article/10.1007/s10291-021-01201-3" target="_blank" rel="noopener"><u>GIRAS</u></a> package and the Python toolbox<a href="https://link.springer.com/article/10.1007/s10291-024-01694-8"> </a><a href="https://link.springer.com/article/10.1007/s10291-024-01694-8" target="_blank" rel="noopener"><u>gnssrefl</u></a> support a wide range of GNSS-IR analyses, lowering the entry barrier and improving transparency and reproducibility.

More broadly, GNSS-IR illustrates a recurring theme in geodesy. Signals often contain more information than initially expected. By rethinking what was once treated as an error, GNSS-IR turns unwanted reflections into a valuable source of environmental information.

So next time a GNSS receiver struggles with multipath, it may be worth listening more closely. Those reflections could be telling a story about the world beneath our feet.
<pre><strong>Further reading</strong>
For those interested in learning more about GNSS-IR, the following resources provide a good starting point:
 
Larson, K.M., 2016. GPS interferometric reflectometry: applications to surface soil moisture, snow depth, and vegetation water content in the western United States. WIREs Water 3, 775–787. <span style="text-decoration: underline"><a href="https://doi.org/10.1002/wat2.1167" target="_blank" rel="noopener">https://doi.org/10.1002/wat2.1167</a></span>
 
Larson, K.M., Williams, S.D.P., 2023. Water level measurements using reflected GNSS signals. IHR 29, 66–76. <span style="text-decoration: underline"><a href="https://doi.org/10.58440/ihr-29-2-a30" target="_blank" rel="noopener">https://doi.org/10.58440/ihr-29-2-a30</a></span>
 
For an interactive introduction to the technique, visit <span style="text-decoration: underline"><a href="https://gnss-reflections.org/" target="_blank" rel="noopener">gnss-reflections.org</a></span>.</pre>
<p style="text-align: right"><em>- Edited by: Leire Retegui-Schiettekatte</em></p>]]></content:encoded>
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							<item>
					<title><![CDATA[Are we valuing poster sessions enough?]]></title>
					<link>https://blogs.egu.eu/divisions/as/2026/05/28/are-we-valuing-poster-sessions-enough/</link>
					<comments>https://blogs.egu.eu/divisions/as/2026/05/28/are-we-valuing-poster-sessions-enough/#comments</comments>
					<pubDate>Thu, 28 May 2026 13:26:18 +0000</pubDate>
					<dc:creator><![CDATA[Roxana S. Cremer]]></dc:creator>
							<category><![CDATA[Academic career]]></category>
		<category><![CDATA[EGU]]></category>
		<category><![CDATA[guest author]]></category>
		<category><![CDATA[academia]]></category>
		<category><![CDATA[conference]]></category>
		<category><![CDATA[EGU26]]></category>
		<category><![CDATA[session]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Do not get me wrong, EGUs General Assembly is a great conference and it’s a real pleasure to explore all the science on display, reconnect with colleagues from other institutes, cities and disciplines. But, wandering the venue and seeing all the empty poster walls left a sad feeling. It’s not only singular gaps in an otherwise packed hall, it’s whole empty corridors and not only Monday morning or Friday afternoon. One might ask themselves, if that’s a symptom of how we value posters as a community? Maybe authors do not bother to show up at all, if they got ‘just’ a poster instead of an oral talk? Standing in front of an empty wall, I bothered to check the online abstract: no indication of withdrawal. Is it not a thing to withdraw posters? (According to the official numbers, the retraction rates are similar for talks and posters, but maybe it’s not tracked (or marked) as rigorously for the latter ones.) Are ECSs discouraged to travel to a conference, where they did not get an oral? In a different occasion multiple posters were put down even before the attendance time slot ended. Maybe that was a personal conflict of schedule, but why not keep the poster on display for others to read during the non-attendance time? In fact, the guidelines emphasize the display time exceeding the attendance time. I am a fan of posters! As audience, I can flexibly decide on where to stroll by, where to read the key messages and where to stop, engage and discuss. I can easily identify posters I want to visit beforehand, even session hopping works like a breeze. Posters also benefit the presenters, they allow for detailed questions, in-depth discussion, feedback and development of ideas. There is just so much more time compared to the short talk time in oral sessions. Lastly, the poster spot serves as a contact point. At least during the attendance time people know where to find me out of the 20.000 other on-site participants (numbers from egu26.eu). &nbsp; More of them, please There is another problem, which poster are helping to address. Too many oral sessions with almost identical topics are happening in parallel. As an individuum I have to decide on which of the equally interesting and relevant sessions I gift my attendance, as a community we are diluting audience for arduously prepared contributions. At the same time poster walls remain empty. A look into the statistics after the conference actually supports that impression. Up to 2019, usually the number of posters was double that of talks. Since 2024 it’s almost equal shares. Shifting the balance (back) from orals to posters will help to ease the scheduling conflicts. And if it’s about broadcasting your message: Why not having condensed poster pitches at each oral session? – Oh wait, maybe there is already an (equally undervalued) format for that: the PICOs. For sure there are more ideas to advance the format of the general assembly, especially the poster sessions. To resume some of the threads from coffee break conversations: maybe the posters could be printed and displayed, even if the author cannot attend; or to improve the virtual poster presentations by having an open videocall next to the poster. Let’s have that discussion, but most importantly: care about your posters, embrace the poster sessions, make time for them. They are worth it!]]></description>
													<content:encoded><![CDATA[Do not get me wrong, EGUs General Assembly is a great conference and it’s a real pleasure to explore all the science on display, reconnect with colleagues from other institutes, cities and disciplines.

But, wandering the venue and seeing all the empty poster walls left a sad feeling. It’s not only singular gaps in an otherwise packed hall, it’s whole empty corridors and not only Monday morning or Friday afternoon. One might ask themselves, if that’s a symptom of how we value posters as a community?

Maybe authors do not bother to show up at all, if they got ‘just’ a poster instead of an oral talk? Standing in front of an empty wall, I bothered to check the online abstract: no indication of withdrawal. Is it not a thing to withdraw posters? (According to the official numbers, the retraction rates are similar for talks and posters, but maybe it’s not tracked (or marked) as rigorously for the latter ones.) Are ECSs discouraged to travel to a conference, where they did not get an oral? In a different occasion multiple posters were put down even before the attendance time slot ended. Maybe that was a personal conflict of schedule, but why not keep the poster on display for others to read during the non-attendance time? In fact, the guidelines emphasize the display time exceeding the attendance time.

<strong>I am a fan of posters!</strong>

As audience, I can flexibly decide on where to stroll by, where to read the key messages and where to stop, engage and discuss. I can easily identify posters I want to visit beforehand, even session hopping works like a breeze. Posters also benefit the presenters, they allow for detailed questions, in-depth discussion, feedback and development of ideas. There is just so much more time compared to the short talk time in oral sessions. Lastly, the poster spot serves as a contact point. At least during the attendance time people know where to find me out of the 20.000 other on-site participants (numbers from egu26.eu).

[caption id="attachment_2092" align="aligncenter" width="600"]<a href="https://blogs.egu.eu/divisions/as/files/2026/05/EGU_no_presentations_v4_comment.png"><img class="wp-image-2092" src="https://blogs.egu.eu/divisions/as/files/2026/05/EGU_no_presentations_v4_comment-300x185.png" alt="" width="600" height="369" /></a> Development of presentation numbers per type. Data from 2013 to 2019 and 2022 to 2023 was retrieved from the respective website (eguYYYY.eu, eguYY.eu). Data since 2024 was provided by the EGU/Copernicus.[/caption]

&nbsp;

<strong>More of them, please</strong>

There is another problem, which poster are helping to address. Too many oral sessions with almost identical topics are happening in parallel.
<blockquote>As an individuum I have to decide on which of the equally interesting and relevant sessions I gift my attendance, as a community we are diluting audience for arduously prepared contributions.</blockquote>
At the same time poster walls remain empty. A look into the statistics after the conference actually supports that impression. Up to 2019, usually the number of posters was double that of talks. Since 2024 it’s almost equal shares. Shifting the balance (back) from orals to posters will help to ease the scheduling conflicts. And if it’s about broadcasting your message: Why not having condensed poster pitches at each oral session? – Oh wait, maybe there is already an (equally undervalued) format for that: the PICOs.

For sure there are more ideas to advance the format of the general assembly, especially the poster sessions. To resume some of the threads from coffee break conversations: maybe the posters could be printed and displayed, even if the author cannot attend; or to improve the virtual poster presentations by having an open videocall next to the poster. Let’s have that discussion, but most importantly: care about your posters, embrace the poster sessions, make time for them. They are worth it!

[caption id="attachment_2099" align="aligncenter" width="600"]<a href="https://blogs.egu.eu/divisions/as/files/2026/05/IMG_9578_roxana.jpg"><img class="wp-image-2099" src="https://blogs.egu.eu/divisions/as/files/2026/05/IMG_9578_roxana-300x225.jpg" alt="" width="600" height="450" /></a> Photo taken by Roxana Cremer during EGU26 in Hall X5.[/caption]]]></content:encoded>
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					<slash:comments>0</slash:comments>
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					<title><![CDATA[EGU Campfire Geodesy – Share Your Research – 19th Edition]]></title>
					<link>https://blogs.egu.eu/divisions/g/2026/05/28/egu-campfire-geodesy-share-your-research-19th-edition/</link>
					<comments>https://blogs.egu.eu/divisions/g/2026/05/28/egu-campfire-geodesy-share-your-research-19th-edition/#comments</comments>
					<pubDate>Thu, 28 May 2026 09:30:57 +0000</pubDate>
					<dc:creator><![CDATA[Fikri Bamahry]]></dc:creator>
							<category><![CDATA[EGU Campfire]]></category>
		<category><![CDATA[early career scientists]]></category>
		<category><![CDATA[ECS]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[We are excited to announce the 19th edition of Geodesy Campfire – Share Your Research in April. The Geodesy EGU Campfire Events “Share Your Research” give (early career) researchers the chance to talk about their work. We have two exciting talks by our guest speakers, Yuting Cheng and Hamed Izadgoshasb. Below, you can find the details of the topics awaiting us. We will have time to network after the presentations. Please join us on Zoom on 18th June 2026 from 14:00 to 16:00 (CEST). Register for this webinar here. Yuting Cheng @Royal Observatory of Belgium: VLBI single station experiment with ASO304 data in preparation for the Genesis mission. Yuting Cheng is currently a postdoc researcher at the Royal Observatory of Belgium, working on the Genesis project of ESA. Genesis is a geodetic satellite hosting all four geodetic techniques for the first time, among which a VLBI transmitter is being developed in Belgium. The current research focus of Yuting is exploring and quantifying challenging aspects of the PRN signal processing of the VLBI transmitter, helping to build the baseline of expected performance of VLBI satellite observations, and assessing the transmitter&#8217;s potential to contribute to the ITRF as a space-tie. &nbsp; Hamed Izadgoshasb @GFZ Helmholtz Centre for Geosciences / Sapienza University of Rome: Explainable AI and GNSS Reflectometry for global soil moisture retrieval. Hamed is an AI and Earth Observation researcher with a PhD from Sapienza University of Rome, where his doctoral work focused on spaceborne GNSS Reflectometry for soil moisture retrieval, from physics-based modelling to hybrid deep learning. He is currently working at GFZ Helmholtz Centre for Geosciences in Potsdam, Germany, developing machine learning and deep learning workflows for large-scale satellite and environmental datasets. His research focuses on GNSS Reflectometry, global soil moisture estimation, satellite data processing pipelines, and explainable AI for Earth observation. He has contributed to ESA’s HydroGNSS mission processor and CYGNSS-based soil moisture studies, with a broader interest in robust, reproducible AI systems for environmental monitoring. &nbsp; &nbsp; Time to connect! After the presentations, we invite everyone in the audience to turn on their camera and microphones, if possible. Participation via the chat is of course also possible. We will start with a short introduction round to get an idea of who is in the room. So if you like to, you can already think about how to summarise your research in a few words so that mortals can also understand it! We’re also open to hear about your favourite dinosaur, your latest burnout, or the 4th element on your tasks list today. Just be there and be talking, we guarantee for the awkwardness. We are always looking for speakers for upcoming Geodesy EGU Campfire Events “Share Your Research”. Are you interested in giving a talk? Then, please express your interest by filling out this form. If you have any questions about the Geodesy EGU Campfire Event, please contact the Geodesy ECS Team via ecs-g@egu.eu. We look forward to seeing you at the Campfire! &nbsp;]]></description>
													<content:encoded><![CDATA[We are excited to announce the 19th edition of Geodesy Campfire – Share Your Research in April. The Geodesy EGU Campfire Events “Share Your Research” give (early career) researchers the chance to talk about their work. We have two exciting talks by our guest speakers, Yuting Cheng and Hamed Izadgoshasb. Below, you can find the details of the topics awaiting us. We will have time to network after the presentations.

Please join us on Zoom on <strong>18th June 2026 </strong>from <strong>14:00 </strong>to<strong> 16:00 (CEST)</strong>. Register for this webinar<strong><a href="https://www.egu.eu/webinars/814/geodesy-campfire-share-your-research/" target="_blank" rel="noopener"> here</a>.</strong>

<strong><a href="https://blogs.egu.eu/divisions/g/files/2026/05/WhatsApp-Image-2025-06-19-at-09.31.17_e4de9868.jpg"><img class="wp-image-5692 alignleft" src="https://blogs.egu.eu/divisions/g/files/2026/05/WhatsApp-Image-2025-06-19-at-09.31.17_e4de9868-230x300.jpg" alt="" width="190" height="248" /></a>Yuting Cheng</strong> @Royal Observatory of Belgium:
<p style="text-align: left"><strong>VLBI single station experiment with ASO304 data in preparation for the Genesis mission.</strong></p>
Yuting Cheng is currently a postdoc researcher at the Royal Observatory of Belgium, working on the Genesis project of ESA. Genesis is a geodetic satellite hosting all four geodetic techniques for the first time, among which a VLBI transmitter is being developed in Belgium. The current research focus of Yuting is exploring and quantifying challenging aspects of the PRN signal processing of the VLBI transmitter, helping to build the baseline of expected performance of VLBI satellite observations, and assessing the transmitter's potential to contribute to the ITRF as a space-tie.

&nbsp;

<a href="https://blogs.egu.eu/divisions/g/files/2026/05/Hamed.jpg"><img class="wp-image-5695 alignright" src="https://blogs.egu.eu/divisions/g/files/2026/05/Hamed-235x300.jpg" alt="" width="190" height="243" /></a><strong>Hamed Izadgoshasb </strong>@GFZ Helmholtz Centre for Geosciences / Sapienza University of Rome:
<p style="text-align: left"><strong>Explainable AI and GNSS Reflectometry for global soil moisture retrieval.</strong></p>
Hamed is an AI and Earth Observation researcher with a PhD from Sapienza University of Rome, where his doctoral work focused on spaceborne GNSS Reflectometry for soil moisture retrieval, from physics-based modelling to hybrid deep learning. He is currently working at GFZ Helmholtz Centre for Geosciences in Potsdam, Germany, developing machine learning and deep learning workflows for large-scale satellite and environmental datasets. His research focuses on GNSS Reflectometry, global soil moisture estimation, satellite data processing pipelines, and explainable AI for Earth observation. He has contributed to ESA’s HydroGNSS mission processor and CYGNSS-based soil moisture studies, with a broader interest in robust, reproducible AI systems for environmental monitoring.

&nbsp;

&nbsp;

[caption id="attachment_4753" align="alignleft" width="293"]<a href="https://blogs.egu.eu/divisions/g/files/2025/09/penguins.jpg"><img class="wp-image-4753" src="https://blogs.egu.eu/divisions/g/files/2025/09/penguins-300x200.jpg" alt="A group of penguins huddling together on the rocky and icy sea side." width="293" height="195" /></a> Image credit Baptiste Gombert (distributed via imaggeo.egu.eu)[/caption]

<strong>Time to connect!</strong>

After the presentations, we invite everyone in the audience to turn on their camera and microphones, if possible. Participation via the chat is of course also possible. We will start with a short introduction round to get an idea of who is in the room. So if you like to, you can already think about how to summarise your research in a few words so that mortals can also understand it! We’re also open to hear about your favourite dinosaur, your latest burnout, or the 4th element on your tasks list today. Just be there and be talking, we guarantee for the awkwardness.

We are always looking for speakers for upcoming Geodesy EGU Campfire Events “Share Your Research”. Are you interested in giving a talk? Then, please express your interest by filling out <strong><a href="https://cloud.egu.eu/apps/forms/s/QdXHNNX9nTFx5AifrGjZFWjA" target="_blank" rel="noopener">this form</a></strong>.

If you have any questions about the Geodesy EGU Campfire Event, please contact the Geodesy ECS Team via <a href="mailto:ecs-g@egu.eu">ecs-g@egu.eu</a>.

<em>We look forward to seeing you at the Campfire!</em>

&nbsp;]]></content:encoded>
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					<slash:comments>0</slash:comments>
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					<title><![CDATA[The AI Revolution in Mining: Overhyped, Understood and Absolutely Unavoidable]]></title>
					<link>https://blogs.egu.eu/divisions/gd/2026/05/27/the-ai-revolution-in-mining-overhyped-understood-and-absolutely-unavoidable/</link>
					<comments>https://blogs.egu.eu/divisions/gd/2026/05/27/the-ai-revolution-in-mining-overhyped-understood-and-absolutely-unavoidable/#comments</comments>
					<pubDate>Wed, 27 May 2026 08:00:04 +0000</pubDate>
					<dc:creator><![CDATA[Editorial team 1]]></dc:creator>
							<category><![CDATA[News & Views]]></category>
		<category><![CDATA[AI Exploration]]></category>
		<category><![CDATA[Artificial Intelligence]]></category>
		<category><![CDATA[CriticalRawMaterials]]></category>
		<category><![CDATA[exploration]]></category>
		<category><![CDATA[geosciences]]></category>
		<category><![CDATA[Mining]]></category>
		<category><![CDATA[Technology]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Artificial Intelligence has dominated the world across various sectors. However, it is yet to be decided whether the use of AI in Mineral Exploration (and more broadly in Geosciences) will diminish the expertise and know-how of Geologists or instead provide a valuable tool for the years ahead. In this week’s blog, Dr. Nicholas Vafeas shares his perspective on AI technology in the mining industry and how it could reshape the narrative for the betterment of society. Artificial Intelligence (AI) has become the buzzword of our age, cutting across finance, digital tech, and more recently, mining and mineral exploration. An industry once defined by grit, gut instinct and months-on-end in remote locations now finds itself increasingly shaped by algorithms and predictive models (much to the dismay of some of the older fundamentalists). But like any shiny new tool, the reality is far more nuanced than the hype swirling around it. To appreciate how things have shifted, it’s worth remembering where you were just three or four years ago, reading fantastical claims about AI exploration, claims most investors (and many geologists) quietly dismissed. AI was seen as a mysterious black box, “unreliable”, “not ready”, or, in some circles, little more than tech-flavoured snake oil. Then, in a perfect pendulum swing, the narrative jumped to the opposite extreme: AI everywhere. Suddenly, it was going to revolutionise exploration, replace human interpretation, and (apparently) solve every geological problem from here to the Archean. Now, having moved past that inflationary bubble, some are quietly stepping back, concluding (somewhat unfairly) that AI “doesn’t work”. But expecting AI to magically answer every geological question is a bit like trying mathematics once and declaring the whole thing useless because it couldn’t instantly solve your taxes. The truth is that AI is exceptionally powerful at what it is designed to do, and that is to recognise patterns, process extensive datasets, and flag anomalies the human eye would almost certainly miss. These models can ingest geochemistry, geophysics, mapping, drill logs, and even satellite data in combinations and volumes that far exceed human cognitive limits. And, in doing so, they can reduce unnecessary drilling, optimise planning and steadily push up the probability of exploration success. Not through miracles, but through hundreds of small, compounding gains. The kind nobody writes press releases about, but which reshape margins over time. In that sense, AI is less a magic wand and more akin to the invention of the spreadsheet. When VisiCalc appeared in 1979, it didn’t “replace” anyone. Instead, it allowed people to work smarter, faster, and with far more insight, and the entire computing industry accelerated as a result. AI in exploration plays the same role. It’s an amplifier of human capability, not a substitute for it, even branching into the world of creativity. Would you believe the lepidolite in Figure 1 was AI generated? Those who have seen lepidolite samples will know that it’s usually a purplish-grey, flaky mineral. &nbsp; For those of you who went back to check Figure 1, how sure are you now? Impressive as it may be, the power of AI comes with an important caveat, it is only as effective as the data it is given. Geological uncertainty, incomplete datasets, inconsistent sampling, and the chaotic reality of fieldwork, often expose the limits of algorithmic neatness. “Garbage-in, garbage-out”, as they say. Historical drill logs are a classic example. They are notoriously unique to each logging geologist and shaped not only by personal interpretation, but also by academic training and local jargon. This is where AI fundamentally struggles, it lacks the human ability to interpret ambiguity and the “feel” of geology. This is particularly challenging in greenfields exploration, where data is sparse by definition. You are often working with limited signals, wide uncertainty, and patterns that may or may not even exist. This environment is brutal for algorithms and it explains why some early AI tools appeared to “underperform”, such as Kobold’s “zero copper” hole (Steinberg and Patterson, 2024). But rather than discarding the technology, Kobold treated the result as feedback, refining its models and improving prospecting strategies. In that sense, abandoning AI after one “misfire” is like throwing away your cake before you’ve finished baking. Yes, companies like GeologicAI and VERAI now offer real-time, high-resolution core scanning, hyperspectral imaging, and automated structural logging (all genuinely impressive), essentially replacing the need for an on-site geology team. But even these systems can miss the subtle features such as foliation changes, micro-vein sets and metamorphic nuances, the kinds of things a trained geologist spots almost subconsciously. Now what if I told you that I lied, and that the lepidolite in Figure 1 is not AI, and in fact a real gem? That’s the difference between understanding the deposit and knowing the rock. So while we’ll likely reach a point within the next 2–3 years where most AI project code is written by AI itself, and while the future may involve fewer geologists physically on site, the value of geological experience will almost certainly rise, not fall. At the end of the day, AI remains a tool. A powerful one, yes, but still a tool. Geology is still (and will always be) about the rocks, the landscapes, the questions we ask, and the societal choices those answers inform. If we strike the right balance, hammer in one hand, algorithm in the other, a balance that demands not only technological integration but also the willingness to cross social and disciplinary boundaries, the future of exploration will be shaped not by machines or humans alone, but by the partnership between them. References Steinberg, J., and Patterson, S., 2024. The Silicon Valley Startup Using AI to Scour the Earth for Copper and Lithium. The Wall Street Journal, 28 July. Available at: https://www.wsj.com/tech/ai/kobold-metals-ai-copper-lithium-caad58da?msockid=05c8c5d6a23e6e380f4ad03aa3456fc0]]></description>
													<content:encoded><![CDATA[<strong>Artificial Intelligence has dominated the world across various sectors. However, it is yet to be decided whether the use of AI in Mineral Exploration (and more broadly in Geosciences) will diminish the expertise and know-how of Geologists or instead provide a valuable tool for the years ahead. In this week’s blog, Dr. Nicholas Vafeas shares his perspective on AI technology in the mining industry and how it could reshape the narrative for the betterment of society.</strong>

[caption id="attachment_42526" align="alignright" width="241"]<a href="https://blogs.egu.eu/divisions/gd/?attachment_id=42526" rel="attachment wp-att-42526"><img class="wp-image-42526" src="https://blogs.egu.eu/divisions/gd/files/2026/05/Picture1-283x300.jpg" alt="" width="241" height="255" /></a> Dr. Nicholas Vafeas is an economic geologist specialising in critical raw materials, mineral supply chains, and energy policy. More of his work can be found on his official website: https://www.nicholasvafeas.com/.[/caption]

<strong>Artificial Intelligence (AI) has become the buzzword of our age, cutting across finance, digital tech, and more recently, mining and mineral exploration.</strong> An industry once defined by grit, gut instinct and months-on-end in remote locations now finds itself increasingly shaped by algorithms and predictive models (much to the dismay of some of the older fundamentalists). But like any shiny new tool, the reality is far more nuanced than the hype swirling around it.

To appreciate how things have shifted, it’s worth remembering where you were just three or four years ago, reading fantastical claims about AI exploration, claims most investors (and many geologists) quietly dismissed. AI was seen as a mysterious black box, “unreliable”, “not ready”, or, in some circles, little more than tech-flavoured snake oil. <strong>Then, in a perfect pendulum swing, the narrative jumped to the opposite extreme: AI everywhere.</strong> Suddenly, it was going to revolutionise exploration, replace human interpretation, and (apparently) solve every geological problem from here to the Archean.

Now, having moved past that inflationary bubble, some are quietly stepping back, concluding (somewhat unfairly) that AI “doesn’t work”. But expecting AI to magically answer every geological question is a bit like trying mathematics once and declaring the whole thing useless because it couldn’t instantly solve your taxes.

The truth is that AI is exceptionally powerful at what it <em>is</em> designed to do, and that is to recognise patterns, process extensive datasets, and flag anomalies the human eye would almost certainly miss. These models can ingest geochemistry, geophysics, mapping, drill logs, and even satellite data in combinations and volumes that far exceed human cognitive limits. And, in doing so, they can reduce unnecessary drilling, optimise planning and steadily push up the probability of exploration success. Not through miracles, but through hundreds of small, compounding gains. The kind nobody writes press releases about, but which reshape margins over time.

In that sense, AI is less a magic wand and more akin to the invention of the spreadsheet. When VisiCalc appeared in 1979, it didn’t “replace” anyone. Instead, it allowed people to work smarter, faster, and with far more insight, and the entire computing industry accelerated as a result. <em>AI in exploration plays the same role.</em> It’s an amplifier of human capability, not a substitute for it, even branching into the world of creativity. <strong>Would you believe the lepidolite in Figure 1 was AI generated? Those who have seen lepidolite samples will know that it’s usually a purplish-grey, flaky mineral.</strong>

[caption id="attachment_42540" align="aligncenter" width="744"]<a href="https://blogs.egu.eu/divisions/gd/?attachment_id=42540" rel="attachment wp-att-42540"><img class="wp-image-42540 size-full" src="https://blogs.egu.eu/divisions/gd/files/2026/05/Picture2.jpg" alt="" width="744" height="992" /></a> Figure 1. Pink, gem-quality lepidolite from an exploration project in northern Mozambique (Source: Private photograph Nicholas Vafeas).[/caption]

&nbsp;

<strong>For those of you who went back to check Figure 1, how sure are you now? Impressive as it may be, the power of AI comes with an important caveat, it is only as effective as the data it is given. Geological uncertainty, incomplete datasets, inconsistent sampling, and the chaotic reality of fieldwork, often expose the limits of algorithmic neatness. “<em>Garbage-in, garbage-out”</em>, as they say.</strong>

Historical drill logs are a classic example. They are notoriously unique to each logging geologist and shaped not only by personal interpretation, but also by academic training and local jargon. This is where AI fundamentally struggles, it lacks the human ability to interpret ambiguity and the “feel” of geology. This is particularly challenging in greenfields exploration, where data is sparse by definition. You are often working with limited signals, wide uncertainty, and patterns that may or may not even exist. This environment is brutal for algorithms and it explains why some early AI tools appeared to “underperform”, such as <a href="https://www.wsj.com/tech/ai/kobold-metals-ai-copper-lithium-caad58da?msockid=05c8c5d6a23e6e380f4ad03aa3456fc0">Kobold’s “zero copper” hole</a> (Steinberg and Patterson, 2024). But rather than discarding the technology, Kobold treated the result as feedback, refining its models and improving prospecting strategies. In that sense, abandoning AI after one “misfire” is like throwing away your cake before you’ve finished baking.

Yes, companies like <a href="https://www.geologicai.com/">GeologicAI</a> and <a href="https://ver-ai.com/">VERAI</a> now offer real-time, high-resolution core scanning, hyperspectral imaging, and automated structural logging (all genuinely impressive), essentially replacing the need for an on-site geology team. <strong>But even these systems can miss the subtle features such as foliation changes, micro-vein sets and metamorphic nuances, the kinds of things a trained geologist spots almost subconsciously.</strong> <em>Now what if I told you that I lied, and that the lepidolite in Figure 1 is not AI, and in fact a real gem? That’s the difference between understanding the deposit and knowing the rock. </em>

So while we’ll likely reach a point within the next 2–3 years where most AI project code is written by AI itself, and while the future may involve fewer geologists physically on site, the value of geological experience will almost certainly rise, not fall.

<strong>At the end of the day, AI remains a tool. A powerful one, yes, but still a tool. Geology is still (and will always be) about the rocks, the landscapes, the questions we ask, and the societal choices those answers inform. </strong>

<strong>If we strike the right balance, hammer in one hand, algorithm in the other, a balance that demands not only technological integration but also the willingness to cross social and disciplinary boundaries, the future of exploration will be shaped not by machines or humans alone, but by the partnership between them.</strong>
<pre> References

 Steinberg, J., and Patterson, S., 2024. The Silicon Valley Startup Using AI to Scour the Earth for Copper and Lithium. The Wall Street Journal, 28 July. Available at: https://www.wsj.com/tech/ai/kobold-metals-ai-copper-lithium-caad58da?msockid=05c8c5d6a23e6e380f4ad03aa3456fc0</pre>]]></content:encoded>
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					<title><![CDATA[Weaker but more frequent: how sea breezes are changing in a warming climate]]></title>
					<link>https://blogs.egu.eu/divisions/cl/2026/05/26/mediterranean_sea_breezes/</link>
					<comments>https://blogs.egu.eu/divisions/cl/2026/05/26/mediterranean_sea_breezes/#comments</comments>
					<pubDate>Tue, 26 May 2026 11:04:33 +0000</pubDate>
					<dc:creator><![CDATA[Shalenys Bedoya]]></dc:creator>
							<category><![CDATA[Climate of the Present]]></category>
		<category><![CDATA[heatwaves]]></category>
		<category><![CDATA[mediterranean]]></category>
		<category><![CDATA[occurrence]]></category>
		<category><![CDATA[sea breeze]]></category>
		<category><![CDATA[speeds]]></category>
		<category><![CDATA[weather stations]]></category>
		<category><![CDATA[winds]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[For the 500 million people living along the Mediterranean coast, the sea breeze is an essential component of the regional climate. They are more than a pleasant coastal wind, as they are critical for easing summer heat stress, dispersing pollutants, and triggering convection (the rapid upward movement of warm, moist air), sometimes leading to severe storms, among many others. But the Mediterranean basin is warming 20% to 40% faster than the globe, with the land warming faster than the ocean, driving significant shifts in its atmospheric and oceanic dynamics. As a result, the land-sea temperature difference is intensifying, being this thermal contrast the primary thermodynamic driver (the physical force powered by heat differences) triggering sea breezes everywhere. As the Mediterranean is a well-known climate change hotspot experiencing more frequent, long-lasting, and intense extreme temperatures (e.g., both atmospheric and marine heatwaves, i.e., prolonged periods of abnormally high temperatures in the air or ocean), we wonder how the anthropogenic warming (human-caused global temperature rise) and its extreme temperatures are altering sea breezes in the region. In our recent study1, we provide regional observational evidence that, in a warming climate, sea breezes are becoming weaker, yet more frequent in the Western Mediterranean basin, based on an unprecedented 41-year observational database covering 39 weather stations (1981–2021). Sea breezes in change Until now, the scarcity of multidecadal, high-resolution observations made it difficult to quantify regional sea breeze trends. By homogenizing data from multiple stations across France, Italy, Spain, and North Africa, a clear pattern emerged (Figure 1): &nbsp; &nbsp; A weakening in intensity: since the 1980s, sea breeze speeds (intensity) have decreased by up to 10% per decade, particularly during the spring and summer months. &nbsp; A likely change in their seasonality: Conversely, the occurrence of sea breezes has increased, most notably in the winter, rising by roughly 10% per decade. &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; As we already mentioned: As land warms faster than the ocean, the land-sea thermal contrast intensifies. One would expect that a stronger thermal contrast should drive stronger sea breezes. So, why are they weakening? Possible answers lie not at the surface, but high above the basin: it might be the result of a complex interplay between regional warming and broader atmospheric circulation (Figure 2). Summer weakening Intensity loses are probably linked to the unprecedented warming that the Mediterranean region has been experiencing over the last century. Yet, the increased frequency and intensification of atmospheric heatwaves (prolonged periods of excessively hot weather) play also a key role: Regional warming and shifts in the jet stream2 (fast-flowing, high-altitude winds that steer weather systems) have led to more frequent high-pressure systems staying stationary over the Mediterranean. These systems draw warm tropical continental air masses over the region, positioning them above the planetary boundary layer. This layer of warm air creates a stable atmospheric barrier that suppresses vertical air mixing. Consequently, the sea breeze circulation cell is vertically compressed, reducing wind speeds on the ground (Figure 2b). During atmospheric heatwaves, our observational data shows sea breeze speeds drop by an average of 8% to 10%. Figure 3. Summer sea breeze speeds and the heatwave weakening effect in their intensity. Seasonal change The increased winter frequency may be a cascading response to atmospheric dynamics, specifically the expansion of the Azores High3 (a large, persistent high-pressure system over the Atlantic Ocean) and a tendency toward positive North Atlantic Oscillation (NAO+) phases3 (an atmospheric pressure pattern that favours dry, stable weather in the Mediterranean). This has led to a higher frequency of winter anticyclones over the Western Mediterranean. The resulting clear skies and weak background winds create the adequate conditions to trigger sea breezes during the colder months. Our results also point to more sea breezes in winter, yet some locations evidence less days in summer. Consequently, a potential shift in their seasonality from the peak of summer and towards the winter may be inferred. Why this matters? Changes in sea breezes carry significant risks for coastal and inland environments, as well as for the societies living there: Heat Extremes: As summer breezes weaken, their natural cooling effect diminishes exactly when it is needed most: during severe heatwaves. This threatens to exacerbate urban heat stress4 and increase public health risks. Not only are these winds becoming too weak to reach and cool inland areas, but they might be also becoming less frequent in summer, precisely when maximum temperatures are regularly exceeding 40ºC. Air Quality: While stronger winds disperse atmospheric pollutants, weaker and more frequent sea breezes can trap and recirculate pollutants along coastal and inland areas for days, worsening exposure for densely populated cities. Hydrological Cycles: Changes in these winds may impact moisture transport, potentially influencing deep summer convection (which causes severe storms). Furthermore, other studies5 suggest that anthropogenic (human-driven) land-use changes have left sea breezes with less available water to transport inland. Consequently, weaker breezes carrying less water vapour from evapotranspiration (water released into the atmosphere by soil and plants) may fail to trigger the summer storms necessary to sustain the hydrological cycle in already dry and arid regions. Looking Ahead Our findings position sea breezes as a critical, yet historically underexplored, element of regional climate change. As the Mediterranean continues to warm, relying solely on large-scale global models, which often struggle to capture highly localized coastal winds, is not enough. By analysing long-term regional observations, we can gather a more accurate picture of how local winds are shifting. This empirical understanding is necessary to properly assess climate-related risks and provide a realistic foundation for mitigation and adaptation strategies along the Mediterranean coast. “Sea breezes may be local winds, but their response to climate change tells a much larger story: one of complex interactions between warming, atmospheric dynamics, and the lived experience of climate along our coasts.” Read the full open-access study in Scientific Reports here. This post has been edited by the editorial board References: 1. Bedoya-Valestt, S., Azorin-Molina, C., Plaza-Martin, N.P. et al. Weaker and more frequent Mediterranean sea breezes in a warming climate. Sci Rep (2026). https://doi.org/10.1038/s41598-026-47025-4 2. Moon, W., Kim, B.-M., Yang, G.-H. &amp; Wettlaufer, J. S. Proc. Natl Acad. Sci. USA 119, e2200890119 (2022). https://doi.org/10.1073/pnas.2200890119 3. Cresswell-Clay, N. et al. Twentieth-century Azores High expansion unprecedented in the past 1,200 years. Nat. Geosci. 15, 548–553 (2022). https://doi.org/10.1038/s41561- 022-00971-w 4. Di Napoli, C., Lavers, D.A., Bechtold, P. et al. Relief or Aggravation? A 31-Year study of sea-Land Breezes and Their Impacts on Coastal Heat Stress. Earth Syst Environ (2025). https://doi.org/10.1007/s41748-025-00917-3 5. Pausas, J. G. &amp; Millán, M. M. Greening and browning in a climate change hotspot: The Mediterranean Basin. BioScience 69, 143–151 (2019). https://doi.org/10.1093/biosci/biy157 &nbsp;]]></description>
													<content:encoded><![CDATA[For the 500 million people living along the Mediterranean coast, the sea breeze is an essential component of the regional climate. They are more than a pleasant coastal wind, as they are critical for easing summer heat stress, dispersing pollutants, and triggering convection (the rapid upward movement of warm, moist air), sometimes leading to severe storms, among many others.

But the Mediterranean basin is warming 20% to 40% faster than the globe, with the land warming faster than the ocean, driving significant shifts in its atmospheric and oceanic dynamics. As a result, the land-sea temperature difference is intensifying, being this thermal contrast the primary thermodynamic driver (the physical force powered by heat differences) triggering sea breezes everywhere.

As the Mediterranean is a well-known climate change hotspot experiencing more frequent, long-lasting, and intense extreme temperatures (e.g., both atmospheric and marine heatwaves, i.e., prolonged periods of abnormally high temperatures in the air or ocean), we wonder how the anthropogenic warming (human-caused global temperature rise) and its extreme temperatures are altering sea breezes in the region.

In our <a href="https://doi.org/10.1038/s41598-026-47025-4">recent study</a><sup>1</sup>, we provide regional observational evidence that, in a warming climate, sea breezes are becoming weaker, yet more frequent in the Western Mediterranean basin, based on an unprecedented 41-year observational database covering 39 weather stations (1981–2021).
<h5><strong>Sea breezes in change</strong></h5>
Until now, the scarcity of multidecadal, high-resolution observations made it difficult to quantify regional sea breeze trends. By homogenizing data from multiple stations across France, Italy, Spain, and North Africa, a clear pattern emerged (<strong>Figure 1</strong>):

[caption id="attachment_5632" align="alignleft" width="400"]<a href="https://blogs.egu.eu/divisions/cl/files/2026/05/Fig-1_brief.jpg"><img class="wp-image-5632" src="https://blogs.egu.eu/divisions/cl/files/2026/05/Fig-1_brief-300x291.jpg" alt="" width="400" height="388" /></a> <strong>Figure 1.</strong> 41-years of sea breeze changes in their intensity and occurrence across the Mediterranean basin. Red triangles indicate upward trends while blue triangles indicate downward trends.[/caption]

&nbsp;

&nbsp;
<ul>
 	<li><strong>A weakening in intensity:</strong> since the 1980s, sea breeze speeds (intensity) have decreased by up to 10% per decade, particularly during the spring and summer months.</li>
</ul>
&nbsp;
<ul>
 	<li><strong>A likely change in their seasonality:</strong> Conversely, the occurrence of sea breezes has increased, most notably in the winter, rising by roughly 10% per decade.</li>
</ul>
&nbsp;

&nbsp;

&nbsp;

&nbsp;

&nbsp;

As we already mentioned: As land warms faster than the ocean, the land-sea thermal contrast intensifies. One would expect that a stronger thermal contrast should drive <em>stronger</em> sea breezes. So, why are they weakening? Possible answers lie not at the surface, but high above the basin: it might be the result of a complex interplay between regional warming and broader atmospheric circulation (<strong>Figure 2</strong>).

[caption id="attachment_5641" align="aligncenter" width="1600"]<a href="https://blogs.egu.eu/divisions/cl/files/2026/05/Figure-8_600ppi.png"><img class="wp-image-5641 size-full" src="https://blogs.egu.eu/divisions/cl/files/2026/05/Figure-8_600ppi.png" alt="" width="1600" height="569" /></a> <strong>Figure 2.</strong> Schematic summary of the mechanisms driving changes in sea breezes of the Mediterranean. In summer, the subsidence (sinking) of warm air masses over the planetary boundary layer (the lowest part of the atmosphere near the ground) acts as a stable barrier that flattens and weakens the sea breeze circulation. In winter, a higher frequency of anticyclones (high-pressure systems) increases sea breeze occurrences during the colder months.[/caption]
<h5><strong>Summer weakening</strong></h5>
Intensity loses are probably linked to the unprecedented warming that the Mediterranean region has been experiencing over the last century. Yet, the increased frequency and intensification of atmospheric heatwaves (prolonged periods of excessively hot weather) play also a key role: Regional warming and <a href="https://www.pnas.org/doi/full/10.1073/pnas.2200890119">shifts in the jet stream</a><sup>2</sup> (fast-flowing, high-altitude winds that steer weather systems) have led to more frequent high-pressure systems staying stationary over the Mediterranean. These systems draw warm tropical continental air masses over the region, positioning them above the planetary boundary layer. This layer of warm air creates a stable atmospheric barrier that suppresses vertical air mixing. Consequently, the sea breeze circulation cell is vertically compressed, reducing wind speeds on the ground (<strong>Figure 2b</strong>).

During atmospheric heatwaves, our observational data shows sea breeze speeds drop by an average of 8% to 10%.

<a style="font-weight: bold;background-color: transparent;font-size: 16px" href="https://blogs.egu.eu/divisions/cl/files/2026/05/Figure-5_600ppi-e1779270308531.jpg"><img class="alignnone wp-image-5643" src="https://blogs.egu.eu/divisions/cl/files/2026/05/Figure-5_600ppi-e1779270308531-1024x453.jpg" alt="" width="724" height="320" /></a>

<strong>Figure 3.</strong> Summer sea breeze speeds and the heatwave weakening effect in their intensity.
<h5><strong>Seasonal change</strong></h5>
The increased winter frequency may be a cascading response to atmospheric dynamics, specifically the <a href="https://www.pnas.org/doi/full/10.1073/pnas.2200890119">expansion of the Azores High</a><sup>3</sup> (a large, persistent high-pressure system over the Atlantic Ocean) and a tendency toward positive North Atlantic Oscillation (NAO+) phases<sup>3</sup> (an atmospheric pressure pattern that favours dry, stable weather in the Mediterranean). This has led to a higher frequency of winter anticyclones over the Western Mediterranean. The resulting clear skies and weak background winds create the adequate conditions to trigger sea breezes during the colder months. Our results also point to more sea breezes in winter, yet some locations evidence less days in summer. Consequently, a potential shift in their seasonality from the peak of summer and towards the winter may be inferred.
<h5><strong>Why this matters?</strong></h5>
Changes in sea breezes carry significant risks for coastal and inland environments, as well as for the societies living there:
<ol>
 	<li><strong>Heat Extremes:</strong> As summer breezes weaken, their natural cooling effect diminishes exactly when it is needed most: during severe heatwaves. This threatens <a href="https://link.springer.com/article/10.1007/s41748-025-00917-3">to exacerbate urban heat stress</a><sup>4</sup> and increase public health risks. Not only are these winds becoming too weak to reach and cool inland areas, but they might be also becoming less frequent in summer, precisely when maximum temperatures are regularly exceeding 40ºC.</li>
</ol>
<ol>
 	<li><strong>Air Quality:</strong> While stronger winds disperse atmospheric pollutants, weaker and more frequent sea breezes can trap and recirculate pollutants along coastal and inland areas for days, worsening exposure for densely populated cities.</li>
 	<li><strong>Hydrological Cycles:</strong> Changes in these winds may impact moisture transport, potentially influencing deep summer convection (which causes severe storms). Furthermore, <a href="https://doi.org/10.1093/biosci/biy157">other studies</a><sup>5</sup> suggest that anthropogenic (human-driven) land-use changes have left sea breezes with less available water to transport inland. Consequently, weaker breezes carrying less water vapour from evapotranspiration (water released into the atmosphere by soil and plants) may fail to trigger the summer storms necessary to sustain the hydrological cycle in already dry and arid regions.</li>
</ol>
<h5>Looking Ahead</h5>
Our findings position sea breezes as a critical, yet historically underexplored, element of regional climate change. As the Mediterranean continues to warm, relying solely on large-scale global models, which often struggle to capture highly localized coastal winds, is not enough.

By analysing long-term regional observations, we can gather a more accurate picture of how local winds are shifting. This empirical understanding is necessary to properly assess climate-related risks and provide a realistic foundation for mitigation and adaptation strategies along the Mediterranean coast.
<blockquote>
<p style="text-align: center">“Sea breezes may be local winds, but their response to climate change tells a much larger story: one of complex interactions between warming, atmospheric dynamics, and the lived experience of climate along our coasts.”</p>
</blockquote>
Read the full open-access study in <em>Scientific Reports</em> <a href="https://doi.org/10.1038/s41598-026-47025-4">here</a>.
<p style="text-align: right"><strong>This post has been edited by the editorial board</strong></p>

<pre style="font-weight: 400">References:
1. Bedoya-Valestt, S., Azorin-Molina, C., Plaza-Martin, N.P. et al. Weaker and more frequent Mediterranean sea breezes in a warming climate. Sci Rep (2026). https://doi.org/10.1038/s41598-026-47025-4

2. Moon, W., Kim, B.-M., Yang, G.-H. &amp; Wettlaufer, J. S. Proc. Natl Acad. Sci. USA 119, e2200890119 (2022). https://doi.org/10.1073/pnas.2200890119

3. Cresswell-Clay, N. et al. Twentieth-century Azores High expansion unprecedented in the past 1,200 years. Nat. Geosci. 15, 548–553 (2022). https://doi.org/10.1038/s41561- 022-00971-w

4. Di Napoli, C., Lavers, D.A., Bechtold, P. et al. Relief or Aggravation? A 31-Year study of sea-Land Breezes and Their Impacts on Coastal Heat Stress. Earth Syst Environ (2025). https://doi.org/10.1007/s41748-025-00917-3

5. Pausas, J. G. &amp; Millán, M. M. Greening and browning in a climate change hotspot: The Mediterranean Basin. BioScience 69, 143–151 (2019). https://doi.org/10.1093/biosci/biy157

</pre>
&nbsp;]]></content:encoded>
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					<title><![CDATA[What Lies Beneath an Ice Shelf]]></title>
					<link>https://blogs.egu.eu/divisions/cr/2026/05/22/what-lies-beneath-an-ice-shelf/</link>
					<comments>https://blogs.egu.eu/divisions/cr/2026/05/22/what-lies-beneath-an-ice-shelf/#comments</comments>
					<pubDate>Fri, 22 May 2026 14:56:32 +0000</pubDate>
					<dc:creator><![CDATA[Sophie Berger]]></dc:creator>
							<category><![CDATA[Cryo Adventures]]></category>
		<category><![CDATA[Antarctic]]></category>
		<category><![CDATA[Antarctic ice sheet]]></category>
		<category><![CDATA[drilling]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Beneath Antarctica’s largest ice shelf lies a hidden ocean—dark, cold, and almost impossible to reach. Scientists drilled through hundreds of metres of ice to access it, revealing a world that plays a crucial role in how ice shelves melt. Years later, we had the chance to explore this unseen environment—not in the field, but through the data that the expedition left behind. Antarctica’s ice shelf cavities – the hidden underside Antarctica is fringed by ice shelves, formed where ice from the continent flows outward and begins to float on top of the ocean. Some extend only a few tens of kilometers, while others rival the size of major countries. Together, they act as a buffer, slowing the flow of the grounded ice sheet behind them—which holds enough ice to raise global sea levels by many meters. Beneath these shelves lies a hidden ocean cavity, where relatively warm seawater can circulate and interact with the ice above. This interaction plays a key role in controlling how quickly ice shelves melt, and how effectively they can continue to hold back the ice sheet. Despite their importance, these environments remain among the least observed parts of the Earth system. Direct measurements from beneath ice shelves are rare, leaving much of this hidden ocean largely unexplored. Drilling into the unknown  Accessing the ocean beneath an ice shelf is not a small task. At a site on the central Ross Ice Shelf, a team of scientists and engineers used hot-water drilling to melt a narrow borehole—only about 30 cm in diameter—through hundreds of metres of ice. Through this small opening, they deployed instruments into the ocean below, creating a rare window into one of the most inaccessible environments on Earth. Despite its modest size, this borehole enabled years of continuous measurements beneath the ice. This site, known as HWD2 (Hot Water Drill site number 2), collected ocean data between 2018 and 2022, capturing how temperature, salinity, and currents change in this hidden environment. Because the site moves with the ice shelf at roughly 550 metres per year, the instruments also drifted with the ice over the course of the measurements. Figure 1: Instrument deployment through a hot-water–drilled borehole at the HWD2 site on the central Ross Ice Shelf, Antarctica, enabling access to the ocean beneath the ice. [Credit: Craig Stevens/ESNZ] A glimpse beneath the ice What does the underside of an ice shelf actually look like? Through the HWD2 borehole, a camera was lowered into the ocean below, capturing a rare glimpse of this hidden environment. Rather than a smooth, static boundary, the ice–ocean interface appears alive—constantly changing over time. The footage reveals delicate, plate-like ice crystals forming directly from seawater and accumulating beneath the ice shelf. This process, known as frazil ice formation, shows that the ocean is not only capable of melting the ice from below, but in some places, actively building it. Imagery from this footage has been used in scientific studies to document thin layers of ice crystals at the ice base, providing insight into conditions at the ice–ocean interface. But while the camera captures these processes in action, it only provides a snapshot. To understand how and why this environment changes over time, we need to look beyond the video. Figure 2: Camera footage from the HWD2 borehole beneath the central Ross Ice Shelf, Antarctica, showing ice crystals forming at the base of the ice shelf. [Credit: Craig Stevens/ESNZ] From snapshots to timeseries This is where the long-term measurements from HWD2 come in. Instruments moored to the ice shelf recorded ocean conditions continuously between 2018 and 2022, including temperature, salinity, and ocean currents. These measurements captured variability across seasons and years, revealing that the ocean beneath the ice shelf is structured and connected, with variability shaped by processes both within the cavity and far beyond it. One striking result is that conditions beneath the central Ross Ice Shelf are connected to the open ocean hundreds of kilometers away. Our analysis shows that variability within the cavity aligns with changes in the Ross Ice Shelf Polynya—a wind-driven, ice-free region where dense, salty water forms, as shown in our recent study. This connection highlights how distant processes can influence the ocean beneath the ice shelf. The data also reveal a layered structure within the seawater that fills the cavity, which persists over time but shifts with the seasons, with temperatures often dropping below the local freezing point. First observed decades ago, this structure remains a defining feature today, pointing to a consistent driving mechanism that redistributes heat and freshwater beneath the ice shelf. Interpreting the mooring data is, in many ways, an expedition of a different kind—one that happens behind a computer screen. By reconstructing variability across seasons and years, we can uncover the hidden dynamics of an environment that remains almost entirely out of reach. From beneath the ice to the wider ocean The ocean beneath ice shelves is not isolated—it is connected to the wider ocean system. Our results show that processes far from the ice shelf, such as sea ice formation in the Ross Ice Shelf Polynya, can influence how rapidly the base of the ice shelf melts. This connection provides a pathway through which changes in the open ocean can reach the ice. As sea ice patterns and ocean conditions shift, so too may the balance of heat beneath ice shelves. These changes extend beyond Antarctica. Over time, shifts in ice shelves and the Southern Ocean can influence global ocean circulation, marine ecosystems, and sea level. Ice shelves may seem remote, but they are part of a connected Earth system. By uncovering how the ocean beneath them behaves, studies like ours help understand not only what is happening under the ice—but what it could mean far beyond it. Further Reading Beneath Antarctica’s largest ice shelf, a hidden ocean is revealing its secrets A Long-Term Look Beneath an Antarctic Ice Shelf Edited by Mirjam Paasch and Mack Baysinger &nbsp;]]></description>
													<content:encoded><![CDATA[<em>Beneath Antarctica’s largest ice shelf lies a hidden ocean—dark, cold, and almost impossible to reach. Scientists drilled through hundreds of metres of ice to access it, revealing a world that plays a crucial role in how ice shelves melt. Years later, we had the chance to explore this unseen environment—not in the field, but through the data that the expedition left behind.</em>

<hr />

<h3><strong>Antarctica’s ice shelf cavities – the hidden underside</strong></h3>
Antarctica is fringed by <a href="https://nsidc.org/learn/parts-cryosphere/ice-shelves">ice shelves</a>, formed where ice from the continent flows outward and begins to float on top of the ocean. Some extend only a few tens of kilometers, while others rival the size of major countries. Together, they act as a buffer, slowing the flow of the grounded ice sheet behind them—which holds enough ice to raise global sea levels by many meters.

Beneath these shelves lies a hidden ocean cavity, where relatively warm seawater can circulate and interact with the ice above. This interaction plays a key role in controlling how quickly ice shelves melt, and how effectively they can continue to hold back the ice sheet.

Despite their importance, these environments remain among the least observed parts of the Earth system. Direct measurements from beneath ice shelves are rare, leaving much of this hidden ocean largely unexplored.
<h3><strong>Drilling into the unknown  </strong></h3>
Accessing the ocean beneath an ice shelf is not a small task. At a site on the central Ross Ice Shelf, a team of scientists and engineers used <a href="https://eos.org/articles/drilling-into-the-past-to-predict-the-future">hot-water drilling</a> to melt a narrow borehole—only about 30 cm in diameter—through hundreds of metres of ice.

Through this small opening, they deployed instruments into the ocean below, creating a rare window into one of the most inaccessible environments on Earth. Despite its modest size, this borehole enabled years of continuous measurements beneath the ice.

This site, known as <a href="https://theconversation.com/climate-scientists-explore-hidden-ocean-beneath-antarcticas-largest-ice-shelf-90006">HWD2</a> (Hot Water Drill site number 2), collected ocean data between 2018 and 2022, capturing how temperature, salinity, and currents change in this hidden environment. Because the site moves with the ice shelf at roughly <a href="https://doi.org/10.1029/2025JC023511">550 metres per year</a>, the instruments also drifted with the ice over the course of the measurements.

[video width="1280" height="720" mp4="https://blogs.egu.eu/divisions/cr/files/2026/05/hwd2_deployment.mp4" loop="true" autoplay="true"][/video]

<em>Figure 1: Instrument deployment through a hot-water–drilled borehole at the HWD2 site on the central Ross Ice Shelf, Antarctica, enabling access to the ocean beneath the ice. [Credit: Craig Stevens/ESNZ]</em>
<h3><strong>A glimpse beneath the ice</strong></h3>
What does the underside of an ice shelf actually look like?

Through the HWD2 borehole, a camera was lowered into the ocean below, capturing a rare glimpse of this hidden environment. Rather than a smooth, static boundary, the <a href="https://www.antarctica.gov.au/news/2025/little-things-make-big-ice-shelves-melt/">ice–ocean interface</a> appears alive—constantly changing over time.

The footage reveals delicate, plate-like ice crystals forming directly from seawater and accumulating beneath the ice shelf. This process, known as <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/94JC03224">frazil ice formation</a>, shows that the ocean is not only capable of melting the ice from below, but in some places, actively building it. Imagery from this footage has been used in <a href="https://www.pnas.org/doi/10.1073/pnas.1910760117">scientific studies</a> to document thin layers of ice crystals at the ice base, providing insight into conditions at the ice–ocean interface.

But while the camera captures these processes in action, it only provides a snapshot. To understand how and why this environment changes over time, we need to look beyond the video.

[video width="2104" height="1190" mp4="https://blogs.egu.eu/divisions/cr/files/2026/05/yingpu_ice_view-1.mp4" loop="true" autoplay="true"][/video]

<em>Figure 2: Camera footage from the HWD2 borehole beneath the central Ross Ice Shelf, Antarctica, showing ice crystals forming at the base of the ice shelf. [Credit: Craig Stevens/ESNZ]</em>
<h3><strong>From snapshots to timeseries</strong></h3>
This is where the long-term measurements from HWD2 come in. Instruments moored to the ice shelf recorded ocean conditions continuously between 2018 and 2022, including temperature, salinity, and ocean currents. These measurements captured variability across seasons and years, revealing that the ocean beneath the ice shelf is structured and connected, with variability shaped by processes both within the cavity and far beyond it.

One striking result is that conditions beneath the central Ross Ice Shelf are connected to the open ocean hundreds of kilometers away. Our analysis shows that variability within the cavity aligns with changes in the Ross Ice Shelf <a href="https://eos.org/articles/holes-in-ross-sea-ice-grow-and-shrink-in-unexpected-cycle">Polynya</a>—a wind-driven, ice-free region where dense, salty water forms, as shown in <a href="https://doi.org/10.1029/2025JC023511">our recent study</a>. This connection highlights how distant processes can influence the ocean beneath the ice shelf.

The data also reveal a layered structure within the seawater that fills the cavity, which persists over time but shifts with the seasons, with temperatures often dropping below the local <a href="https://glossary.ametsoc.org/wiki/freezing-point/">freezing point</a>. First observed <a href="https://doi.org/10.1029/JC088iC04p02556">decades ago</a>, this structure remains a defining feature today, pointing to a consistent driving mechanism that redistributes heat and freshwater beneath the ice shelf.

Interpreting the mooring data is, in many ways, an expedition of a different kind—one that happens behind a computer screen. By reconstructing variability across seasons and years, we can uncover the hidden dynamics of an environment that remains almost entirely out of reach.

[caption id="attachment_17460" align="aligncenter" width="1600"]<a href="https://blogs.egu.eu/divisions/cr/files/2026/05/JGRO_schematic.jpg"><img class="size-full wp-image-17460" src="https://blogs.egu.eu/divisions/cr/files/2026/05/JGRO_schematic.jpg" alt="" width="1600" height="638" /></a> Figure 3: Schematic of ocean circulation beneath the central Ross Ice Shelf, highlighting the connection between the cavity and the open ocean (solid blue lines). Panels a and b illustrate seasonal differences in the layered structure within the cavity. The dark blue spiral symbols represent ocean eddies, swirling motions in the water that can help drive seasonal changes in the cavity structure. Variability in water masses such as Ice Shelf Water (ISW) and High Salinity Shelf Water (HSSW) reflects processes both within the cavity and in the distant Ross Ice Shelf Polynya. [Credit: Reproduced from Xiahou et al. (2026).][/caption]
<h3><strong>From beneath the ice to the wider ocean</strong></h3>
The ocean beneath ice shelves is not isolated—it is connected to the wider ocean system. Our results show that processes far from the ice shelf, such as <a href="https://www.antarcticscienceplatform.org.nz/updates/sea-ice-and-ocean-circulation">sea ice formation</a> in the Ross Ice Shelf Polynya, can influence how rapidly the base of the ice shelf melts. This connection provides a pathway through which changes in the open ocean can reach the ice. As sea ice patterns and ocean conditions shift, so too may the balance of heat beneath ice shelves.

These changes extend beyond Antarctica. Over time, shifts in ice shelves and the Southern Ocean can influence global ocean circulation, marine ecosystems, and sea level. Ice shelves may seem remote, but they are part of a connected Earth system. By uncovering how the ocean beneath them behaves, studies like ours help understand not only what is happening under the ice—but what it could mean far beyond it.
<h3><strong>Further Reading</strong></h3>
<ul>
 	<li><a href="https://theconversation.com/beneath-antarcticas-largest-ice-shelf-a-hidden-ocean-is-revealing-its-secrets-273219">Beneath Antarctica’s largest ice shelf, a hidden ocean is revealing its secrets</a></li>
 	<li><a href="https://eos.org/research-spotlights/a-long-term-look-beneath-an-antarctic-ice-shelf?fbclid=IwY2xjawQZylRleHRuA2FlbQIxMQBzcnRjBmFwcF9pZBAyMjIwMzkxNzg4MjAwODkyAAEeIZxwDy1aMHsE-WHAPdTEeBjXn7Rv7APTe45bL7WTzaxA0RFsnn4G2fbTV1A_aem_bi5eQG7OxPB90sMnCVK6gg">A Long-Term Look Beneath an Antarctic Ice Shelf</a></li>
</ul>
<p style="text-align: right"><strong><em>Edited by <span data-olk-copy-source="MessageBody">Mirjam Paasch</span> and Mack Baysinger</em></strong></p>


<hr />

&nbsp;]]></content:encoded>
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					<title><![CDATA[Regarding Flowing Waters - The Science and Art of Hydrology]]></title>
					<link>https://blogs.egu.eu/divisions/hs/2026/05/22/regarding-flowing-waters-the-science-and-art-of-hydrology/</link>
					<comments>https://blogs.egu.eu/divisions/hs/2026/05/22/regarding-flowing-waters-the-science-and-art-of-hydrology/#comments</comments>
					<pubDate>Fri, 22 May 2026 08:00:00 +0000</pubDate>
					<dc:creator><![CDATA[Bettina Schaefli]]></dc:creator>
							<category><![CDATA[Opinion]]></category>
		<category><![CDATA[art]]></category>
		<category><![CDATA[photography]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[About a decade ago, I formally retired from Lancaster University (albeit retaining an emeritus position and still producing the occasional paper).   In that time, I have been able to pursue my interests in the history of hydrology but also devote more time to my other passion which is landscape photography, especially images of water. As a hydrologist, I do understand that to spend my spare time photographing water is definitely on the rather sad side of social behaviour but, on the other hand, some of the results are quite nice (and it is not the only photographic project I have followed – more can be found at the www.mallerstangmagic.co.uk site including series of books of Boring Postcards, Visual Haiku, and the Mallerstang Valley). The Depiction of Water in Art Artists have, of course, long been interested in water as a subject, one of the most famous documented examples being the drawings of the nature of turbulence in the sketchbooks of Leonardo da Vinci. He was one of the first people to study the dynamics of flowing water in detail (he even prepared, but never published, a Treatise on Water), though it has been suggested that his interest was driven as much by an interest in how to make practical use of the power of water, how to improve canal design, and how to protect people against devastating floods, than in the artistic potential. One of the reasons for that artistic interest is surely that water flows are dynamic, changing constantly in response to the changing hydrology and boundary conditions, including the effect of roughness elements and wind. The water will have varying degrees of transparency depending on water quality and sediment loads. Flowing water produces complex and changing patterns of light due to reflection and refraction with skypools, landpools and caustics. The result is that the artistic representation of water is a huge challenge. Actually, however, the situation is not that much better for the scientist. We do have a really beautiful representation of the dynamics of water in the 3 dimensional Navier-Stokes equations. The problem is that we cannot solve those equations in most applications of practical interest because of the uncertainties associated with the knowledge of the relevant boundary conditions (and also, still today, the sheer computer power needed to produce numerical solutions at useful scales). Another problem for the hydrologist is that a lot of the water flows that are of interest take place under the ground surface where it is very difficult to study exactly what is going on, except in small samples. We often resort to inferring what is going on from larger scale flow and tracer observations. Some of the artistic difficulties of representing water are discussed in an interesting book by David Clarke (Water and Art, 2010). He suggests that one of the first and most influential treatments of water was by JWM Turner, in part because of his skill in using the medium of watercolour to represent effects of light and water in the outdoors, with a view to representing the sublime (as originally defined by Edmund Burke in the 1750s). Water was an essential part of the sublime – the sound and fury of mountain torrents and the dramatic presence of glaciers adding to the atmosphere as the Grand Tourists passed through the Alps[BS2] . Many of J.M.W. Turner’s most famous large-scale watercolours are of waterfalls in Switzerland he had encountered on his travels. David Clarke also suggests that it was the dissolution of the subject matter in his watercolours (which Turner also carried over into his later oil paintings), using water as a medium to represent water as the subject, that started the path towards a more abstract art, particularly in the water-related art of Monet, Mondrian, Kandinsky, Pollock, De Kooning and Frankenthaler. He suggests that these artists (and others of course) had been all influenced by living close to and interacting visually with, water on a daily basis. The Challenge of Water in Photography With the invention of photography, the representation of water has become somewhat easier. Water has been a subject for images made since the very earliest days of photography, even more so once exposure times became short enough to be able to capture waves (e.g.Gustav Le Gray’s images of the sea in the 1880s). Photography has been used extensively in experimental laboratory studies in hydraulics. There are whole books devoted to photographic studies and surveys of water images, and we have now become used to pictures of blurred waterfalls, autumn colours reflected in rivers and lakes and, since the work of Hiroshi Sugimoto and Michael Kenna, of minimalist water stilled by the use of long exposures to emphasise the nature of the light.  The challenge now, as with so many aspects of photography is trying to avoid cliché (but there are some striking examples of doing so, see, for example, the River Taw work of Susan Derges, the Atlantic and Scottish Rivers work of Thomas Joshua Cooper, the Thames Studies of Roni Horn, and the early Sea Horizon work of Garry Fabian Miller). Water moves; it (mostly) flows downhill.  In doing so it organises and shapes itself into different forms that are dynamic while also retaining recognisable forms of waves and ripples and curves.  The light and the additional dimension of the sound of flowing water would seem to make the recording of these sensations the realm of video and not the still image.  Yet video seems to result in a less than satisfactory imitation of the real thing.  It has movement, it has sound, but it is, in some sense, evidently false in being flattened to two dimensions. A still image is also evidently false but somehow those discrete moments of time of the stilled dynamics seem to work quite well. The water is in stasis and no longer flows but the possibility of taking some time to explore the nature of the stilled flow is still somehow satisfying as well as providing wonderful abstract images in their own right.  There is something about the nature of the flow being closed in its balance of forces and boundary conditions that produces the intricate self-organised forms and imperfections to provide an image both true to the flow and attractive to the viewer.  Yet the underlying ambiguities of a still image of the dynamic reality remain. Water and a Photographic Practice In making photographic images of water that I have wanted to show the life and intrinsic beauty of the flow in a realistic way, while recognising the approximate way in which we can represent the dynamics. How has this been done? The compositional possibilities are endless but by trying to capture images that “feel right” – which is clearly a more artistic concept. Uncertainty also plays a role – I find some of the most satisfying images are those that require the viewer to make some effort to understand. Regarding Flowing Waters is the third book of water images I have published under the imprint of the Mallerstang Magic Press, after The Still Dynamic in 2021 and Panta Rhei – Everything Flows in 2022 (in homage to the IAHS Panta Rhei programme).   The images include images taken in a number of bisses in the Canton of Valais in Switzerland: small, man-made channels built to bring water from reliable springs and glaciers to where it was needed for water supply and irrigation of pastures and crops.   The bisses are quite variable in size, slope and construction but all represent an enormous effort by both the men and women of the communes involved to both create and maintain them over long periods of time. Some were suspended on the sides of cliffs, others involved tunnelling through rock faces. Some, such as the Bisse de Sion, are still in active use.  They offer many opportunities for intimate landscapes of the water within them. I remain fascinated by the science that lies behind the forms that produce an attractive image of a water flow, but I hope that the images can be appreciated for themselves: simple attempts to capture the essence of different types of flow.   Regarding Flowing Waters is published in a limited edition of 100 copies and is available through the shop on the www.mallerstangmagic.co.uk site (or, to keep postage costs down for those of you in Switzerland, contact me directly at k.beven@bluewin.ch). &nbsp; Related posts: https://blogs.egu.eu/divisions/hs/tag/history-of-hydrology/ Edited by B. Schaefli]]></description>
													<content:encoded><![CDATA[About a decade ago, I formally retired from Lancaster University (albeit retaining an emeritus position and still producing the occasional paper).   In that time, I have been able to pursue my interests in the <a href="https://blogs.egu.eu/divisions/hs/2023/08/02/history-of-hydrology/">history of hydrology </a>but also devote more time to my other passion which is landscape photography, especially images of water. As a hydrologist, I do understand that to spend my spare time photographing water is definitely on the rather sad side of social behaviour but, on the other hand, some of the results are quite nice (and it is not the only photographic project I have followed – more can be found at the<a href="http://www.mallerstangmagic.co.uk"> www.mallerstangmagic.co.uk</a> site including series of books of Boring Postcards, Visual Haiku, and the Mallerstang Valley).
<h3><b>The Depiction of Water in Art</b></h3>
Artists have, of course, long been interested in water as a subject, one of the most famous documented examples being the drawings of the nature of turbulence in the sketchbooks of Leonardo da Vinci. He was one of the first people to study the dynamics of flowing water in detail (he even prepared, but never published, a Treatise on Water), though it has been suggested that his interest was driven as much by an interest in how to make practical use of the power of water, how to improve canal design, and how to protect people against devastating floods, than in the artistic potential.

One of the reasons for that artistic interest is surely that water flows are dynamic, changing constantly in response to the changing hydrology and boundary conditions, including the effect of roughness elements and wind. The water will have varying degrees of transparency depending on water quality and sediment loads. Flowing water produces complex and changing patterns of light due to reflection and refraction with skypools, landpools and caustics. The result is that the artistic representation of water is a huge challenge.

Actually, however, the situation is not that much better for the scientist. We do have a really beautiful representation of the dynamics of water in the 3 dimensional Navier-Stokes equations. The problem is that we cannot solve those equations in most applications of practical interest because of the uncertainties associated with the knowledge of the relevant boundary conditions (and also, still today, the sheer computer power needed to produce numerical solutions at useful scales). Another problem for the hydrologist is that a lot of the water flows that are of interest take place under the ground surface where it is very difficult to study exactly what is going on, except in small samples. We often resort to inferring what is going on from larger scale flow and tracer observations.

Some of the artistic difficulties of representing water are discussed in an interesting book by David Clarke (<a href="https://reaktionbooks.co.uk/work/water-and-art">Water and Art, 2010</a>). He suggests that one of the first and most influential treatments of water was by JWM Turner, in part because of his skill in using the medium of watercolour to represent effects of light and water in the outdoors, with a view to representing the <i>sublime </i>(as originally defined by <a href="https://fr.wikipedia.org/wiki/Edmund_Burke">Edmund Burke</a> in the 1750s). Water was an essential part of the sublime – the sound and fury of mountain torrents and the dramatic presence of glaciers adding to the atmosphere as the<a href="https://en.wikipedia.org/wiki/Grand_tour"> Grand Tourists</a> passed through the Alps[BS2] . Many of J.M.W. Turner’s most famous large-scale watercolours are of waterfalls in Switzerland he had encountered on his travels. David Clarke also suggests that it was the dissolution of the subject matter in his watercolours (which Turner also carried over into his later oil paintings), using water as a medium to represent water as the subject, that started the path towards a more abstract art, particularly in the water-related art of Monet, Mondrian, Kandinsky, Pollock, De Kooning and Frankenthaler. He suggests that these artists (and others of course) had been all influenced by living close to and interacting visually with, water on a daily basis.
<h3><b>The Challenge of Water in Photography</b></h3>
With the invention of photography, the representation of water has become somewhat easier. Water has been a subject for images made since the very earliest days of photography, even more so once exposure times became short enough to be able to capture waves (e.g.Gustav Le Gray’s images of the sea in the 1880s). Photography has been used extensively in experimental laboratory studies in hydraulics. There are whole books devoted to photographic studies and surveys of water images, and we have now become used to pictures of blurred waterfalls, autumn colours reflected in rivers and lakes and, since the work of Hiroshi Sugimoto and Michael Kenna, of minimalist water stilled by the use of long exposures to emphasise the nature of the light.  The challenge now, as with so many aspects of photography is trying to avoid cliché (but there are some striking examples of doing so, see, for example, the River Taw work of Susan Derges, the Atlantic and Scottish Rivers work of Thomas Joshua Cooper, the Thames Studies of Roni Horn, and the early Sea Horizon work of Garry Fabian Miller).

Water moves; it (mostly) flows downhill.  In doing so it organises and shapes itself into different forms that are dynamic while also retaining recognisable forms of waves and ripples and curves.  The light and the additional dimension of the sound of flowing water would seem to make the recording of these sensations the realm of video and not the still image.  Yet video seems to result in a less than satisfactory imitation of the real thing.  It has movement, it has sound, but it is, in some sense, evidently false in being flattened to two dimensions.

A still image is also evidently false but somehow those discrete moments of time of the stilled dynamics seem to work quite well. The water is in stasis and no longer flows but the possibility of taking some time to explore the nature of the stilled flow is still somehow satisfying as well as providing wonderful abstract images in their own right.  There is something about the nature of the flow being closed in its balance of forces and boundary conditions that produces the intricate self-organised forms and imperfections to provide an image both true to the flow and attractive to the viewer.  Yet the underlying ambiguities of a still image of the dynamic reality remain.
<h3><b>Water and a Photographic Practice</b></h3>
In making photographic images of water that I have wanted to show the life and intrinsic beauty of the flow in a realistic way, while recognising the approximate way in which we can represent the dynamics. How has this been done? The compositional possibilities are endless but by trying to capture images that “feel right” – which is clearly a more artistic concept. Uncertainty also plays a role – I find some of the most satisfying images are those that require the viewer to make some effort to understand.

<i>Regarding Flowing Waters </i>is the third book of water images I have published under the imprint of the Mallerstang Magic Press, after <i>The Still Dynamic</i> in 2021 and <i>Panta Rhei – Everything Flows </i>in 2022 (in homage to the IAHS Panta Rhei programme).   The images include images taken in a number of <i>bisses </i>in the Canton of Valais in Switzerland: small, man-made channels built to bring water from reliable springs and glaciers to where it was needed for water supply and irrigation of pastures and crops.   The bisses are quite variable in size, slope and construction but all represent an enormous effort by both the men and women of the communes involved to both create and maintain them over long periods of time. Some were suspended on the sides of cliffs, others involved tunnelling through rock faces. Some, such as the Bisse de Sion, are still in active use.  They offer many opportunities for intimate landscapes of the water within them.

I remain fascinated by the science that lies behind the forms that produce an attractive image of a water flow, but I hope that the images can be appreciated for themselves: simple attempts to capture the essence of different types of flow.   <i>Regarding Flowing Waters </i>is published in a limited edition of 100 copies and is available through the shop on the<a href="http://www.mallerstangmagic.co.uk"> www.mallerstangmagic.co.uk</a> site (or, to keep postage costs down for those of you in Switzerland, contact me directly at k.beven@bluewin.ch).

[caption id="attachment_13732" align="aligncenter" width="300"]<img class="size-medium wp-image-13732" src="https://blogs.egu.eu/divisions/hs/files/2026/05/Petit-Ruisseau-Champex-300x300.jpg" alt="" width="300" height="300" /> Bisse de Petit Ruisseau, Valais, Switzerland[/caption]

&nbsp;

Related posts:

<a href="https://blogs.egu.eu/divisions/hs/tag/history-of-hydrology/">https://blogs.egu.eu/divisions/hs/tag/history-of-hydrology/</a>
<p style="text-align: right"><em>Edited by B. Schaefli</em></p>]]></content:encoded>
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					<title><![CDATA[Observational constraints help narrowing down uncertainty on the future of the AMOC]]></title>
					<link>https://blogs.egu.eu/divisions/np/2026/05/20/observational-constraints-help-narrowing-down-uncertainty-on-the-future-of-the-amoc/</link>
					<comments>https://blogs.egu.eu/divisions/np/2026/05/20/observational-constraints-help-narrowing-down-uncertainty-on-the-future-of-the-amoc/#comments</comments>
					<pubDate>Wed, 20 May 2026 14:18:22 +0000</pubDate>
					<dc:creator><![CDATA[Valerio Lembo]]></dc:creator>
							<category><![CDATA[Climate]]></category>
		<category><![CDATA[Climate Change]]></category>
		<category><![CDATA[Climate of the Future]]></category>
		<category><![CDATA[Nonlinear]]></category>
		<category><![CDATA[Science Communication]]></category>
		<category><![CDATA[Uncategorised]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[The Atlantic Meridional Overturning Circulation — the AMOC — has become one of the most discussed elements of the climate system. It is often portrayed as a looming tipping point, a potential disruptor of European climate, and a symbol of the uncertainties that still surround climate projections. We spoke with Didier Swingedouw, a leading researcher in ocean–climate interactions from the CNRS and based at University of Bordeaux, who coauthored a recent work aiming to refine our understanding of how the AMOC may evolve in the coming decades. The paper, appeared on Science Advances, is authored by Valentin Portmann, and is available for reading at this link.  From the very beginning of our conversation, Swingedouw stressed that several factors influence AMOC changes, but different parts of the AMOC respond differently to climate forcing, and not all of them are equally relevant when discussing long‑term stability. When it comes to timing, the message is both reassuring and sobering. According to Swingedouw, no climate model currently predicts a full collapse of the AMOC before 2100. “According to CMIP6 models there won’t be any full collapse before the end of the century,” he said, summarizing the consensus across modelling centres. But the picture becomes more complex beyond 2100. Some studies, such as work by Drijfhout and colleagues, show that shortly after the turn of the century, many models reach a very low level of AMOC strength, below 5-6 Sv at 26°N, a threshold value that has been associated with irreversible AMOC changes in a recent study of Jackson et al. based on idealized NAhosMIP experiments. The difficulty is that most modelling centres still stop their simulations at 2100, a legacy of early IPCC practice that no longer matches the lifespan of today’s newborns. As Swingedouw put it, “People born today will likely know 2100.” Why does all this matter? Because the AMOC is not just an abstract oceanic conveyor belt — it is a major regulator of climate. Its influence extends from European and North American climate and seasonality, from the position of the Intertropical Convergence Zone to the strength of monsoon systems in Africa and Asia. It affects fisheries, oceanic carbon uptake, and even regional sea level, which could rise by several tens of centimetres along parts of the Atlantic coast if the AMOC weakens strongly. And yet, despite its importance, the uncertainty surrounding its future evolution remains enormous. In his study, Swingedouw found that the projected weakening by 2100 ranges from almost zero to around 70 percent. “That’s huge,” he emphasized — and it has direct consequences for climate adaptation strategies, especially in Europe. This is where their recent work comes in. The study applies a statistical framework known as observational constraint, which attempts to reduce uncertainty by linking present‑day model biases to future projections. The idea is simple in principle: if a model misrepresents key aspects of the current climate, that misrepresentation may also affect its projections. By quantifying this relationship, one can weight models according to how well they match observations. Their approach stands out for several reasons. Instead of relying on a single observational dataset — such as the RAPID array at 26°N — the study incorporates multiple variables, including sea‑surface temperature and salinity patterns that are closely tied to the density gradients driving the AMOC. It also tests several statistical methods, from traditional linear regression to ridge regression and random forests, and validates them using a leave‑one‑out approach to estimate overfitting. Therefore, machine‑learning techniques, he explained, were also tested, but they were simply too unstable given the small sample of available models. “We have so few data,” he said. “Neural networks were even more unstable.” The method with the lowest LOO is found to be muti-variate Ridge Regression, a method hardly used in climate studies. The result is striking: the method yields an estimated 51 percent weakening of the AMOC by 2100, with an uncertainty of only ±8 percent (at 90% probability). This is a much narrower range than raw model projections, and it points toward a stronger weakening than the ensemble mean would suggest. While the exact number should not be taken as definitive, the reduction in uncertainty is itself a major step forward. Of course, no method is without assumptions. Swingedouw acknowledged that the choice of regions used for the constraints is partly subjective, and that observational uncertainties may be underestimated. His team has already begun addressing these issues by incorporating more variables, using clustering techniques to define regions more objectively, and refining the statistical formulation of the method.  Our conversation eventually turned to the broader climatic implications of an AMOC that weakens by half. The strongest effects would likely be felt in winter in the Northern high latitudes, particularly in Europe, where the AMOC plays a key role in shaping temperature patterns and storm tracks. A weaker AMOC could mean colder winters than standard projections suggest, greater seasonal contrasts, and shifts in atmospheric circulation that can affect ecosystems and agriculture. Summer, by contrast, is less sensitive: heatwaves are driven primarily by atmospheric blocking, and the ocean plays a more modest role. Globally, the AMOC can influence teleconnections through Rossby waves and other mechanisms, but quantifying these effects requires targeted experiments — something the upcoming TIPMIP-OCEAN initiative aims to provide. He therefore invites as many modeling center as possible to contribute to this MIP (see protocol here). Looking ahead, Swingedouw sees several priorities for future research. Understanding the physical processes behind AMOC weakening remains essential, as does studying the possibility of recovery after a collapse or after large‑scale CO₂ removal. Another key question is how different degrees of weakening — say 30 percent versus 50 percent — translate into concrete climatic impacts. And, of course, extending projections beyond 2100 will be crucial for capturing the full trajectory of the AMOC under continued warming. In the end, the message is nuanced. The AMOC is not on the verge of collapsing within this century, but it is very likely to weaken substantially — and that weakening will matter. Thanks to studies like Swingedouw’s, we now have a clearer, more constrained picture of what to expect. But the AMOC remains a complex, dynamic system, and understanding its future will require both scientific innovation and sustained international collaborations and observations.]]></description>
													<content:encoded><![CDATA[[caption id="attachment_2713" align="alignright" width="266"]<a href="https://blogs.egu.eu/divisions/np/files/2026/05/Swingedouw-e1714126592599.jpg"><img class="wp-image-2713 size-medium" src="https://blogs.egu.eu/divisions/np/files/2026/05/Swingedouw-e1714126592599-266x300.jpg" alt="" width="266" height="300" /></a> Didier Swingedouw (Credits: <a href="https://tipesm.eu/about/people/didier-swingedouw/">https://tipesm.eu/about/people/didier-swingedouw/</a>)[/caption]

<span style="font-weight: 400">The Atlantic Meridional Overturning Circulation — the AMOC — has become one of the most discussed elements of the climate system. It is often portrayed as a looming tipping point, a potential disruptor of European climate, and a symbol of the uncertainties that still surround climate projections. We spoke with </span><b>Didier Swingedouw</b><span style="font-weight: 400">, a leading researcher in ocean–climate interactions from the CNRS and based at University of Bordeaux, who coauthored a recent work aiming to refine our understanding of how the AMOC may evolve in the coming decades. The paper, appeared on Science Advances, is authored by <strong>Valentin Portmann</strong>, and is available for reading <strong>at this </strong></span><strong><a href="https://www.science.org/doi/10.1126/sciadv.adx4298">link</a></strong><span style="font-weight: 400">. </span>

<span style="font-weight: 400">From the very beginning of our conversation, Swingedouw stressed that several factors influence AMOC changes, but different parts of the AMOC respond differently to climate forcing, and not all of them are equally relevant when discussing long‑term stability. When it comes to timing, the message is both reassuring and sobering. According to Swingedouw, no climate model currently predicts a full collapse of the AMOC before 2100. “According to CMIP6 models there won’t be any full collapse before the end of the century,” he said, summarizing the consensus across modelling centres. But the picture becomes <strong>more complex</strong> beyond 2100. Some studies, such as </span><a href="https://iopscience.iop.org/article/10.1088/1748-9326/adfa3b"><span style="font-weight: 400">work</span></a><span style="font-weight: 400"> by Drijfhout and colleagues, show that shortly after the turn of the century, many models reach a very low level of AMOC strength, below 5-6 Sv at 26°N, a threshold value that has been associated with irreversible AMOC changes in a recent study of </span><a href="https://gmd.copernicus.org/articles/16/1975/2023/"><span style="font-weight: 400">Jackson et al.</span></a><span style="font-weight: 400"> based on idealized NAhosMIP experiments. The difficulty is that most modelling centres still stop their simulations at 2100, a legacy of early IPCC practice that no longer matches the lifespan of today’s newborns. As Swingedouw put it, “People born today will likely know 2100.”</span>

<span style="font-weight: 400">Why does all this matter? Because the AMOC is not just an abstract oceanic conveyor belt — it is a major regulator of climate. Its influence extends from European and North American climate and seasonality, from the position of the Intertropical Convergence Zone to the strength of monsoon systems in Africa and Asia. It affects fisheries, oceanic carbon uptake, and even regional sea level, which could rise by several tens of centimetres along parts of the Atlantic coast if the AMOC weakens strongly. And yet, despite its importance, the uncertainty surrounding its future evolution remains enormous. In his study, Swingedouw found that the projected weakening by 2100 ranges from almost zero to around 70 percent. “That’s huge,” he emphasized — and it has direct consequences for climate adaptation strategies, especially in Europe.</span>

<span style="font-weight: 400">This is where their recent work comes in. The study applies a statistical framework known as </span><b>observational constraint</b><span style="font-weight: 400">, which attempts to reduce uncertainty by linking present‑day model biases to future projections. The idea is simple in principle: if a model misrepresents key aspects of the current climate, that misrepresentation may also affect its projections. By quantifying this relationship, one can weight models according to how well they match observations.</span>

<span style="font-weight: 400">Their approach stands out for several reasons. Instead of relying on a single observational dataset — such as the RAPID array at 26°N — the study incorporates multiple variables, including sea‑surface temperature and salinity patterns that are closely tied to the density gradients driving the AMOC. It also tests several statistical methods, from traditional linear regression to ridge regression and random forests, and validates them using a leave‑one‑out approach to estimate overfitting. Therefore, machine‑learning techniques, he explained, were also tested, but they were simply too unstable given the small sample of available models. “We have so few data,” he said. “Neural networks were even more unstable.” The method with the lowest LOO is found to be muti-variate Ridge Regression, a method hardly used in climate studies.</span>

<span style="font-weight: 400">The result is striking: the method yields an estimated </span><b>51 percent weakening of the AMOC by 2100</b><span style="font-weight: 400">, with an uncertainty of only ±8 percent (at 90% probability). This is a much narrower range than raw model projections, and it points toward a stronger weakening than the ensemble mean would suggest. While the exact number should not be taken as definitive, the reduction in uncertainty is itself a major step forward.</span>

<span style="font-weight: 400">Of course, no method is without assumptions. Swingedouw acknowledged that the choice of regions used for the constraints is partly subjective, and that observational uncertainties may be underestimated. His team has already begun addressing these issues by incorporating more variables, using clustering techniques to define regions more objectively, and refining the statistical formulation of the method. </span>

<span style="font-weight: 400">Our conversation eventually turned to the <strong>broader climatic implications</strong> of an AMOC that weakens by half. The strongest effects would likely be felt in winter in the Northern high latitudes, particularly in Europe, where the AMOC plays a key role in shaping temperature patterns and storm tracks. A weaker AMOC could mean colder winters than standard projections suggest, greater seasonal contrasts, and shifts in atmospheric circulation that can affect ecosystems and agriculture. Summer, by contrast, is less sensitive: heatwaves are driven primarily by atmospheric blocking, and the ocean plays a more modest role. Globally, the AMOC can influence teleconnections through Rossby waves and other mechanisms, but quantifying these effects requires targeted experiments — something the upcoming TIPMIP-OCEAN initiative aims to provide. He therefore invites as many modeling center as possible to contribute to this MIP (see protocol </span><a href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-1698/"><span style="font-weight: 400">here</span></a><span style="font-weight: 400">).</span>

<span style="font-weight: 400">Looking ahead, Swingedouw sees several priorities for future research. Understanding the physical processes behind AMOC weakening remains essential, as does studying the possibility of recovery after a collapse or after large‑scale CO₂ removal. Another key question is how different degrees of weakening — say 30 percent versus 50 percent — translate into concrete climatic impacts. And, of course, extending projections beyond 2100 will be crucial for capturing the full trajectory of the AMOC under continued warming.</span>

<span style="font-weight: 400">In the end, the message is nuanced. The AMOC is not on the verge of collapsing within this century, but it is very likely to <strong>weaken substantially</strong> — and that weakening will matter. Thanks to studies like Swingedouw’s, we now have a clearer, more constrained picture of what to expect. But the AMOC remains a complex, dynamic system, and understanding its future will require both scientific innovation and sustained international collaborations and observations.</span>]]></content:encoded>
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					<title><![CDATA[“You belong here”: reflections on gender inequality in Academia]]></title>
					<link>https://blogs.egu.eu/divisions/gd/2026/05/20/you-belong-here-reflections-on-gender-inequality-in-academia/</link>
					<comments>https://blogs.egu.eu/divisions/gd/2026/05/20/you-belong-here-reflections-on-gender-inequality-in-academia/#comments</comments>
					<pubDate>Wed, 20 May 2026 08:00:50 +0000</pubDate>
					<dc:creator><![CDATA[Editorial Team 4]]></dc:creator>
							<category><![CDATA[News & Views]]></category>
		<category><![CDATA[#equality]]></category>
		<category><![CDATA[Academic life]]></category>
		<category><![CDATA[EDI]]></category>
		<category><![CDATA[PhD life]]></category>
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											<description><![CDATA[Academia is often imagined as a space driven by merit, curiosity, and scientific collaboration. Still behind publications, conferences, and research achievements, many women in STEM continue to navigate environments shaped by subtle exclusion, normalized inequalities, and power imbalances that are not always openly discussed. In Earth Sciences, where collaboration and field-based research are fundamental, conversations about gender inequality are becoming increasingly visible. However, visibility does not necessarily mean resolution. Experiences such as being underestimated, interrupted, professionally devalued, or discouraged still affect many women throughout their academic careers, many often in ways that are difficult to quantify, but deeply impactful over time. To reflect on these issues, this blog post week, Katherine Villavicencio spoke with Dr. Karen Gariboldi, Senior Researcher from the Department of Earth Sciences at the University of Pisa, whose work focuses on marine micropaleontology and paleoenvironmental reconstruction. Drawing from her personal and professional experience, she shared thoughtful perspectives on impostor syndrome, academic power dynamics, mentorship networks, institutional responsibility, and the kind of cultural transformation that academia still urgently needs. Her reflections remind us that gender equality is not only about policies or representation in numbers. It is also about creating academic environments where people feel respected, heard, supported, and genuinely allowed to belong. Could you briefly introduce your research background and explain the main focus of your work?    I graduated from the University of Milan Bicocca with a degree in Geological Sciences and Technologies, following the Marine Geology curriculum. My Master’s thesis focused on diatom assemblages (microalgae with a siliceous skeleton) characterizing the rocks of the Miocene Pisco Formation in Peru. I then completed a PhD in Earth Sciences at the University of Pisa, again working on diatom assemblages from the Pisco Formation. I investigated the information they provide from a biostratigraphic, paleoclimatic, and sedimentological/diagenetic perspective. I am currently a Senior Researcher at the Department of Earth Sciences at the University of Pisa, where I continue my work as a marine micropaleontologist, also in Arctic regions, with a focus on the Holocene as well, not only the Miocene. Diatoms, however, remain my main area of expertise. From your experience in academia, what forms of gender-based inequality do you believe are still most persistent today, even if they are often normalized or overlooked?  I think there is now much greater awareness of gender-based inequalities; however, this doesn’t mean that these issues have been fully overcome. There is still a lot of work to be done, but the fact that these topics are discussed so widely is, in my opinion, a big step forward. Many studies clearly show that in academia—especially in STEM fields—the gap between women and men tends to widen as you move toward higher or more “powerful” positions. Many women in academia report being subtly dismissed, interrupted, or underestimated in professional settings. How do these behaviors affect confidence, visibility, and career progression over time?  I don’t think there is a single, clear-cut answer; it definitely depends on the individual. Based on what I have observed and on my personal experience, being constantly belittled—or simply not having one’s work properly acknowledged—undermines confidence in one’s abilities and often fuels impostor syndrome, which is already very widespread in academia. This can lead to depressive episodes, sometimes quite severe. You start feeling completely out of place, inadequate; you get the sense that you have wasted your life doing something you are actually not capable of doing. These are very tough moments, and they are hard to overcome. And if this is what you are experiencing right now, please remember that these are distorted feelings, not facts. You are where you are because you are absolutely capable of what you do—and you belong there. On the other hand, some women, in order to assert themselves and advance their careers, begin to adopt behaviors that are typical of patriarchal systems. This is not a positive outcome. Achieving gender equality should instead mean bringing a different model into leadership positions—a model of leadership that is more empathetic, able to build a workplace based on trust, genuine collaboration, and mutual respect. Some women have managed to do this (and it really is appropriate to call it an achievement), but they are still too few. We should probably ask them how they managed it—although I am convinced that the context in which one grows up plays a major role in this kind of development. If girls are trusted from a young age and encouraged to engage in constructive dialogue, they will have no difficulty, as adults, in embodying the role of a positive leader.   Harassment in academic environments is still widely underreported. In your view, what power dynamics or institutional factors make it so difficult for women to speak out?  Quite clearly, the fear of losing one’s position—or, in the case of students, of failing an exam or not completing their thesis—often plays a major role. Universities are starting to put systems in place that allow harassment episodes to be reported and investigated more easily, but until we begin to see real consequences and sanctions for those who commit such behaviors, reports will always remain few. Universities carry a great responsibility in this regard.   How important are mentorship networks and allies in creating safer and more inclusive academic spaces, and how can they be strengthened?  As I mentioned before, the system that I believe women should foster is one based on empathy, trust, and respect. From this perspective, mentorship networks and allies in creating safer and more inclusive academic spaces are clearly fundamental. Specifically, within our department, among female colleagues, we organize lunches together every 2–3 months. Starting these meetings has been very helpful, as it allowed us to discuss issues of discrimination and realize that some of the challenges we personally experienced are shared by other colleagues.Talking and sharing experiences helped us understand that we were not alone and that, together, we could find solutions. Most importantly, supporting each other makes us stronger. To strengthen these networks, it is important to engage in discussions with male colleagues as well, especially younger ones who are sensitive to the issue and can help drive change within the male sphere. It is essential, even if it seems obvious, that they point out to their peers when sexist jokes are inappropriate, and help highlight and overcome problematic or harmful behaviors. Intervening to defuse these behaviors even when no women are present is essential.   As a senior scientist, how do you think established academics can and should intervene when they witness discrimination, harassment, or abuse of power?  They should definitely stand up for the person who is experiencing abuse and help them find the appropriate channels to report it. However, this is not always easy to do. Very often, people worry about the repercussions on their own careers. Even with a tenured position at a university, there are many ways in which others can create obstacles; for example, by ensuring that one of your projects is not approved. This is another example of how, having a strong network behind you is essential, as it allows you to act with greater confidence and support.   What strategies can early-career women adopt to protect themselves from professional devaluation or hostile academic environments, without feeling that they are risking their careers?  First of all, it is important for them to be aware of their own worth, even if someone tries to undermine it. I would advise them to familiarize with the resources and key contacts within their institution in case they witness or experience any form of harassment. However, it is ultimately the responsibility of institutions to monitor these situations and provide people with the tools to protect themselves. As educators, it is our duty to educate.   Do you think formal equality and anti-harassment policies are sufficient, or is a deeper cultural change within academia still urgently needed?  Anti-harassment policies are necessary, but not sufficient. A profound cultural change is required, which will take years, if not decades, and continuous efforts to raise awareness. However, I have faith in the new generations.   What message would you like to share with young women entering Earth Sciences who may already feel discouraged, marginalized, or unsure of their place in academia?  Remember what brought you to this career. If you have become Earth scientists, it is surely because, even from a young age, you felt a deep connection with our Planet. Think about it—can anyone take that away from you? No. This love is a part of you, and no one can take it away!]]></description>
													<content:encoded><![CDATA[<!-- wp:paragraph -->
<p><strong>Academia is often imagined as a space driven by merit, curiosity, and scientific collaboration. Still behind publications, conferences, and research achievements, many women in STEM continue to navigate environments shaped by subtle exclusion, normalized inequalities, and power imbalances that are not always openly discussed. In Earth Sciences, where collaboration and field-based research are fundamental, conversations about gender inequality are becoming increasingly visible. However, visibility does not necessarily mean resolution. Experiences such as being underestimated, interrupted, professionally devalued, or discouraged still affect many women throughout their academic careers, many often in ways that are difficult to quantify, but deeply impactful over time. </strong><strong>To reflect on these issues, this blog post week, Katherine Villavicencio spoke with Dr. Karen Gariboldi, Senior Researcher from the Department of Earth Sciences at the University of Pisa, whose work focuses on marine micropaleontology and paleoenvironmental reconstruction. Drawing from her personal and professional experience, she shared thoughtful perspectives on impostor syndrome, academic power dynamics, mentorship networks, institutional responsibility, and the kind of cultural transformation that academia still urgently needs. Her reflections remind us that gender equality is not only about policies or representation in numbers. It is also about creating academic environments where people feel respected, heard, supported, and genuinely allowed to belong.</strong></p>
[caption id="attachment_42837" align="alignright" width="295"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/05/WhatsApp-Image-2026-03-30-at-13.32.00-e1778745885996.jpeg"><img class="wp-image-42837" src="https://blogs.egu.eu/divisions/gd/files/2026/05/WhatsApp-Image-2026-03-30-at-13.32.00-768x1024.jpeg" alt="" width="295" height="349" /></a> Dr. Karen Gariboldi, Senior Scientist at Department of Earth Sciences, University of Pisa (Italy).[/caption]
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><strong><strong><span style="color: #000080">Could you briefly introduce your research background and explain the main focus of your work? </span></strong></strong>
<p style="text-align: justify"> </p>
</div>
<p><span data-ogsc="rgb(12&lt;p style=">I graduated from the University of Milan Bicocca with a degree in Geological Sciences and Technologies, following the <i data-ogsc="">Marine Geology</i> curriculum. My Master’s thesis focused on diatom assemblages (microalgae with a siliceous skeleton) characterizing the rocks of the Miocene Pisco Formation in Peru. I then completed a PhD in Earth Sciences at the University of Pisa, again working on diatom assemblages from the Pisco Formation. I investigated the information they provide from a biostratigraphic, paleoclimatic, and sedimentological/diagenetic perspective. I am currently a Senior Researcher at the Department of Earth Sciences at the University of Pisa, where I continue my work as a marine micropaleontologist, also in Arctic regions, with a focus on the Holocene as well, not only the Miocene. Diatoms, however, remain my main area of expertise.</span></p>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><strong><span style="color: #000080">From your experience in academia, what forms of gender-based inequality do you believe are still most persistent today, even if they are often normalized or overlooked?</span></strong><span data-ogsc="rgb(12, 100, 192)"> </span></div>
<p><span style="text-align: justify" data-ogsc="&lt;p">I think there is now much greater awareness of gender-based inequalities; however, this doesn’t mean that these issues have been fully overcome. There is still a lot of work to be done, but the fact that these topics are discussed so widely is, in my opinion, a big step forward. Many studies clearly show that in academia—especially in STEM fields—the gap between women and men tends to widen as you move toward higher or more “powerful” positions.</span></p>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><strong><span style="color: #000080">Many women in academia report being subtly dismissed, interrupted, or underestimated in professional settings. How do these behaviors affect confidence, visibility, and career progression over time? </span></strong></div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><span style="text-align: justify" data-o="">I don’t think there is a single, clear-cut answer; it definitely depends on the individual. Based on what I have observed and on my personal experience, being constantly belittled—or simply not having one’s work properly acknowledged—undermines confidence in one’s abilities and often fuels impostor syndrome, which is already very widespread in academia. <span style="color: #3366ff"><em>This can lead to depressive episodes, sometimes quite severe.</em></span> You start feeling completely out of place, inadequate; <em><span style="color: #3366ff">you get the sense that you have wasted your life doing something you are actually not capable of doing</span></em>. These are very tough moments, and they are hard to overcome. And if this is what you are experiencing right now, please remember that these are distorted feelings, not facts. <span style="color: #800080"><strong>You are where you are because you are absolutely capable of what you do—and you belong there</strong></span>. On the other hand, some women, in order to assert themselves and advance their careers, begin to adopt behaviors that are typical of patriarchal systems. This is not a positive outcome. Achieving gender equality should instead mean bringing a different model into leadership positions—a model of leadership that is more empathetic, able to build a workplace based on trust, genuine collaboration, and mutual respect. Some women have managed to do this (and it really is appropriate to call it an achievement), but they are still too few. We should probably ask them how they managed it—although I am convinced that the context in which one grows up plays a major role in this kind of development. <em><span style="color: #3366ff">If girls are trusted from a young age and encouraged to engage in constructive dialogue, they will have no difficulty, as adults, in embodying the role of a positive leader.</span></em></span></div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"> </div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><strong><span style="color: #000080">Harassment in academic environments is still widely underreported. In your view, what power dynamics or institutional factors make it so difficult for women to speak out? </span></strong></div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><span data-ogsc="rgb(12, 100, 192)">Quite clearly, the fear of losing one’s position—or, in the case of students, of failing an exam or not completing their thesis—often plays a major role. Universities are starting to put systems in place that allow harassment episodes to be reported and investigated more easily, but until we begin to see real consequences and sanctions for those who commit such behaviors, reports will always remain few. Universities carry a great responsibility in this regard.</span></div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"> </div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody">
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><strong><span style="color: #000080">How important are mentorship networks and allies in creating safer and more inclusive academic spaces, and how can they be strengthened? </span></strong></div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><span data-ogsc="rgb(12, 100, 192)">As I mentioned before, the system that I believe women should foster is one based on empathy, trust, and respect. From this perspective, mentorship networks and allies in creating safer and more inclusive academic spaces are clearly fundamental. Specifically, <em><span style="color: #3366ff">within our department, among female colleagues, we organize lunches together every 2–3 months. Starting these meetings has been very helpful, as it allowed us to discuss issues of discrimination and realize that some of the challenges we personally experienced are shared by other colleagues.</span></em>Talking and sharing experiences helped us understand that we were not alone and that, together, we could find solutions. Most importantly, <strong><span style="color: #800080">supporting each other makes us stronger</span></strong>. To strengthen these networks, it is important to engage in discussions with male colleagues as well, especially younger ones who are sensitive to the issue and can help drive change within the male sphere. It is essential, even if it seems obvious, that they point out to their peers when sexist jokes are inappropriate, and help highlight and overcome problematic or harmful behaviors. Intervening to defuse these behaviors even when no women are present is essential.</span></div>
</div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"> </div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody">
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><strong><span style="color: #000080">As a senior scientist, how do you think established academics can and should intervene when they witness discrimination, harassment, or abuse of power? </span></strong></div>
</div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody">
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><span data-ogsc="rgb(12, 100, 192)">They should definitely stand up for the person who is experiencing abuse and help them find the appropriate channels to report it. However, this is not always easy to do. Very often, <em><span style="color: #3366ff">people worry about the repercussions on their own careers</span></em>. Even with a tenured position at a university, there are many ways in which others can create obstacles; for example, <em><span style="color: #3366ff">by ensuring that one of your projects is not approved</span></em>. This is another example of how, <strong><span style="color: #800080">having a strong network behind you is essential, as it allows you to act with greater confidence and support</span></strong>.</span></div>
</div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"> </div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody">
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><strong><span style="color: #000080">What strategies can early-career women adopt to protect themselves from professional devaluation or hostile academic environments, without feeling that they are risking their careers? </span></strong></div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><span data-ogsc="rgb(12, 100, 192)">First of all, it is important for them to be aware of their own worth, even if someone tries to undermine it. I would advise them to familiarize with the resources and key contacts within their institution in case they witness or experience any form of harassment. However, <strong><span style="color: #800080">it is ultimately the responsibility of institutions to monitor these situations and provide people with the tools to protect themselves</span></strong>. As educators, it is our duty to educate.</span></div>
</div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"> </div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody">
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><strong><span style="color: #000080">Do you think formal equality and anti-harassment policies are sufficient, or is a deeper cultural change within academia still urgently needed? </span></strong></div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><span data-ogsc="rgb(12, 100, 192)">Anti-harassment policies are necessary, but not sufficient. <em><span style="color: #3366ff">A profound cultural change is required, which will take years, if not decades, and continuous efforts to raise awareness</span></em>. However, I have faith in the new generations.</span></div>
</div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"> </div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody">
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><span style="color: #000080"><strong>What message would you like to share with young women entering Earth Sciences who may already feel discouraged, marginalized, or unsure of their place in academia? </strong></span></div>
<div role="presentation" data-ogsc="" data-olk-copy-source="MessageBody"><span data-ogsc="rgb(12, 100, 192)">Remember what brought you to this career. If you have become Earth scientists, it is surely because, even from a young age, <em><span style="color: #3366ff">you felt a deep connection with our Planet</span></em>. Think about it—can anyone take that away from you? No.<em><span style="color: #3366ff"> This love is a part of you, and no one can take it away!</span></em></span></div>
</div>
<p style="text-align: justify"><!-- /wp:paragraph --></p>]]></content:encoded>
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					<title><![CDATA[Save the date: TopoToolbox Workshop, June 2-3]]></title>
					<link>https://blogs.egu.eu/divisions/gm/2026/05/19/save-the-date-topotoolbox-workshop-june-2-3/</link>
					<comments>https://blogs.egu.eu/divisions/gm/2026/05/19/save-the-date-topotoolbox-workshop-june-2-3/#comments</comments>
					<pubDate>Mon, 18 May 2026 23:37:41 +0000</pubDate>
					<dc:creator><![CDATA[Emma Lodes]]></dc:creator>
							<category><![CDATA[Announcement]]></category>
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		<category><![CDATA[terrain analysis]]></category>
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		<category><![CDATA[webinar]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Save the dates for our upcoming webinar series on TopoToolbox, organized by the GM ECS Team and convened by Wolfgang Schwanghart, Dirk Scherler, William Kearney, Boris Gailleton, and Bastien Mathieux. The webinar will take place on June 2 and 3, from 16:00 to 18:00 CEST, in a Zoom meetings format. The webinar will be a two-part event introducing TopoToolbox 3, its MATLAB and Python interfaces, and examples of topographic analysis workflows. The second session will be more practical, with demos showing how TopoToolbox can be integrated into broader data analysis and modelling workflows, together with a discussion on community contributions. Register here: Part 1: https://www.egu.eu/webinars/813/topographic-analysis-using-topotoolbox-in-matlab-and-python-session-1/ Part 2: https://www.egu.eu/webinars/781/topographic-analysis-using-topotoolbox-in-matlab-and-python-part-2/ More information from the registration page: During this webinar, attendees will learn how to address scientific problems by using TopoToolbox, an open-source platform for experimentation in quantitative geomorphology.  Across the two webinars, you will learn about the functionalities of TopoToolbox 3 and how it can be integrated into MATLAB and Python data analysis and modelling workflows. Hands-on programming activities will help participants get started with the MATLAB and Python interfaces. We will also demonstrate how simulation tools such as GraphFlood for flood simulation and MinVoellmy for landslide simulation can be run from TopoToolbox, and how TopoToolbox can interface with Landlab. TopoToolbox is developed openly on GitHub, and we would be glad for this webinar to also serve as an opportunity to discuss how the community can get involved in its ongoing development. More broadly, the event aims to present the new functionalities of TopoToolbox across different environments, show how users can contribute, explore what the community needs and expects, and bring users and developers together. Conveners Wolfgang Schwanghart, University of Potsdam, Germany Dirk Scherler, GFZ Potsdam, Germany William Kearney, University of Potsdam, Germany Boris Gailleton, Université de Rennes, France Bastien Mathieux, Université de Strasbourg, France Speaker Wolfgang Schwanghart (University of Potsdam, Germany) &#8211; Wolfgang is a geomorphologist at the University of Potsdam and the main developer of TopoToolbox. He studies Earth surface processes and their interactions with mountain environments across different time and spatial scales, combining digital terrain analysis, GIS, landscape evolution modelling, statistics, machine learning, and field-based geomorphology. To participate in the webinars, you must register in advance. Please note that this webinar will be recorded and published on the EGU YouTube channel the week after the event. Need help? If you have any questions about the webinar &#8220;Topographic analysis using TopoToolbox in MATLAB and Python &#8211; Session 1&#8221;, please contact us via webinars@egu.eu.]]></description>
													<content:encoded><![CDATA[Save the dates for our upcoming webinar series on TopoToolbox, organized by the GM ECS Team and convened by Wolfgang Schwanghart, Dirk Scherler, William Kearney, Boris Gailleton, and Bastien Mathieux. The webinar will take place on June 2 and 3, from 16:00 to 18:00 CEST, in a Zoom meetings format.

The webinar will be a two-part event introducing TopoToolbox 3, its MATLAB and Python interfaces, and examples of topographic analysis workflows. The second session will be more practical, with demos showing how TopoToolbox can be integrated into broader data analysis and modelling workflows, together with a discussion on community contributions.

Register here:

Part 1: <a href="https://www.egu.eu/webinars/813/topographic-analysis-using-topotoolbox-in-matlab-and-python-session-1/" target="_blank" rel="noopener" data-saferedirecturl="https://www.google.com/url?q=https://www.egu.eu/webinars/813/topographic-analysis-using-topotoolbox-in-matlab-and-python-session-1/&amp;source=gmail&amp;ust=1779217727505000&amp;usg=AOvVaw03_Q8X-Xykxw3-aEsNGRav">https://www.egu.eu/webinars/<wbr />813/topographic-analysis-<wbr />using-topotoolbox-in-matlab-<wbr />and-python-session-1/</a>

Part 2: <a href="https://www.egu.eu/webinars/781/topographic-analysis-using-topotoolbox-in-matlab-and-python-part-2/" target="_blank" rel="noopener" data-saferedirecturl="https://www.google.com/url?q=https://www.egu.eu/webinars/781/topographic-analysis-using-topotoolbox-in-matlab-and-python-part-2/&amp;source=gmail&amp;ust=1779217727505000&amp;usg=AOvVaw2LV8MNarZCk19KgcFE9Xa5">https://www.egu.eu/webinars/<wbr />781/topographic-analysis-<wbr />using-topotoolbox-in-matlab-<wbr />and-python-part-2/</a>
<h4>More information from the registration page:</h4>
During this webinar, attendees will learn how to address scientific problems by using TopoToolbox, an open-source platform for experimentation in quantitative geomorphology.  Across the two webinars, you will learn about the functionalities of TopoToolbox 3 and how it can be integrated into MATLAB and Python data analysis and modelling workflows. Hands-on programming activities will help participants get started with the MATLAB and Python interfaces. We will also demonstrate how simulation tools such as GraphFlood for flood simulation and MinVoellmy for landslide simulation can be run from TopoToolbox, and how TopoToolbox can interface with Landlab.

TopoToolbox is developed openly on GitHub, and we would be glad for this webinar to also serve as an opportunity to discuss how the community can get involved in its ongoing development. More broadly, the event aims to present the new functionalities of TopoToolbox across different environments, show how users can contribute, explore what the community needs and expects, and bring users and developers together.
<h4>Conveners</h4>
Wolfgang Schwanghart, University of Potsdam, Germany
Dirk Scherler, GFZ Potsdam, Germany
William Kearney, University of Potsdam, Germany
Boris Gailleton, Université de Rennes, France
Bastien Mathieux, Université de Strasbourg, France
<h4>Speaker</h4>
Wolfgang Schwanghart (University of Potsdam, Germany) - Wolfgang is a geomorphologist at the University of Potsdam and the main developer of TopoToolbox. He studies Earth surface processes and their interactions with mountain environments across different time and spatial scales, combining digital terrain analysis, GIS, landscape evolution modelling, statistics, machine learning, and field-based geomorphology.

To participate in the webinars, you must register in advance. Please note that this webinar will be recorded and published on the <a class="external" href="https://www.youtube.com/egu/" target="_blank" rel="noopener noreferrer" aria-label="EGU YouTube channel (link opens in new window/tab)">EGU YouTube channel</a> the week after the event.
<h3>Need help?</h3>
If you have any questions about the webinar "Topographic analysis using TopoToolbox in MATLAB and Python - Session 1", please contact us via <a href="mailto:webinars@egu.eu">webinars@egu.eu</a>.]]></content:encoded>
																<wfw:commentRss>https://blogs.egu.eu/divisions/gm/2026/05/19/save-the-date-topotoolbox-workshop-june-2-3/feed/</wfw:commentRss>
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					<title><![CDATA[A Brief Recap of EGU GA26]]></title>
					<link>https://blogs.egu.eu/divisions/g/2026/05/15/a-brief-recap-of-egu-ga26/</link>
					<comments>https://blogs.egu.eu/divisions/g/2026/05/15/a-brief-recap-of-egu-ga26/#comments</comments>
					<pubDate>Fri, 15 May 2026 12:00:03 +0000</pubDate>
					<dc:creator><![CDATA[Radosław Zajdel]]></dc:creator>
							<category><![CDATA[Division news]]></category>
		<category><![CDATA[EGU General Assembly]]></category>
		<category><![CDATA[GA26]]></category>
		<category><![CDATA[recap]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Thank you all for an amazing EGU General Assembly (GA) this year! If you missed EGU26 or some of the events we organised, here’s a recap so you can stop wondering how it went and get an idea of what to expect next year and connect with us through our channels to stay updated. As in the past years, we started our GA with the online division meeting before the general assembly to present the G-Division strucure and give an overview of our activities. We updated the division structure as the team is growing. We are excited to introduce our new ECS Co-representative, Michela Ravanelli, who has taken over the role from our outgoing ECS Co-representative, Öykü Koç. Here, we want to express our great gratitude to Öykü’s work over the past years within the Geodesy Division and their efforts for the ECS community union-wide. Öykü initiated many blog post series and implemented regular online and in-person events during the General Assembly, which strengthened our community and we will continue to organise in the future. We introduced the new ECS team members who have and will continue to write this blog, coordinate our social media, and host our regular campfires and onsite Pop-up networking events. Our representative, Marius, will continue to organize together with Michela and the entire team these events and extend our community efforts. In Vienna, we started the EGU26 week with the pre-icebreaker as usual, but this year we decided to expand the number of divisions involved a bit more, partly to engage with other fields and explore the interdisciplinarity of our division. It took place on Sunday, when early-career scientists from the Geodesy (G), Geodynamics (GD), Planetary Sciences (PS), and Solar-Terrestrial Sciences (ST) divisions gathered at CopaBeach. Yes, this spot became a kind of permanent location for our pre-GA meet-up. We plan to continue this event every year, so we would love to see you there next year. Let your colleagues know, especially those new to EGU, as it builds a great foundation for a successful and fun week. Following the icebreaker, many attendees headed to the EGU Opening Reception at the conference venue, marking the official start of EGU26. The momentum continued on Monday morning with the Geodesy Fika, a social gathering held in the EGU networking zone. Geodesy Early Career Scientists convened at the terrace G (our usual spot 🙂) to enjoy a coffee break and connect with each other. It was a vibrant atmosphere, with discussions ranging from research interests to expectations for the General Assembly. The short course Geodesy 101, convened by Rebekka Steffen, Eva Boergens, Martin Sehnal, and Anna Kłos, was on Monday lunchtime this year, and it was a great success as it attracted many researchers from all divisions, satisfying their hunger to get an overview of geodetic concepts ranging from GNSS and coordinate transformations to the analysis of gravity data. Have you thought about broadening your horizon across disciplines? The 101 short courses are offered by various divisions and can offer you easily understandable insights into many disciplines. If you are interested, we recommend you take the time to check them out at next year’s GA. Monday had even more events for the Geodesy ECS &#8211; a joint dinner. Fortunately, we were able to extend the number of spots available compared to last year, allowing us to fill an entire floor! Isn’t it fantastic to have so many ECSs together? If you attended, we would love to hear about your experience so we can work on improvements for next time and don’t forget to tell your new colleagues to join us next year! The first couple of days at the GA were packed with social events, from union-wide ECS networking events to division-specific ones. This year, the &#8220;Women in Geodesy” coffee break was quite a success on Tuesday, where we discussed equity, diversity, and inclusion in geodesy. We ended the day with the IAG reception, which has been a wonderful addition to the GA’s geodesy program for many years. If you missed registering, sign up to our mailing list to be informed immediately when the registration opens next year. Last year’s GA, we introduced a special session in Geodesy G0.1, in a panel discussion format, titled &#8220;Geodesy – From Invisible to Essential,&#8221; to raise awareness of the importance of geodetic products. After the great interest, we moved this year&#8217;s special session, G2.1 &#8220;Streamlining geodetic research for policy &#8211; how can we utilize the Essential Geodetic Variables (EGVs) for easier engagement and communication&#8220;, into a large room, where the community discussed how to take action, support and shape policy decision processes. This was an amazing highlight of the Geodesy community in this year’s GA week. Another highlight of the week was, of course, the medal lectures: the Vening Meinesz Medal Lecture by Frank Flechtner and the G Division Outstanding ECS Award Lecture by Eva Boergens. Bringing together the implementation of satellite gravimetry missions and their processing to userfriendly data products to a variaty of applications. These events, including this blog, are community efforts. Thank you very much to all of you who participated in these events, making the EGU26 a special experience for all of us. We want to continuously improve these events for the community, and it is important for us to give you an opportunity to participate actively and to receive feedback from you, the community. So please let us know if you have feedback on past events or suggestions for future events. Ideas are always welcome and with your support we can archieve great experiences together. One very sucessful example is the GeoVision which happened for the first time this year and attracted hundreds of people celebrating music together! This event idea grow from our Division and is implemented together with the ECS task group for outreach and communication! Reach us to contribute, give feedback, and give us new ideas! We are looking forward to seeing you again in Vienna next year. In the meantime, stay updated with us in the community via this blog and our social media channels, and listen to and discuss with us online in our monthly campfires. -Edited by Geodesy ECS Team]]></description>
													<content:encoded><![CDATA[Thank you all for an amazing EGU General Assembly (GA) this year! If you missed EGU26 or some of the events we organised, here’s a recap so you can stop wondering how it went and get an idea of what to expect next year and connect with us through <a href="https://linktr.ee/ecsg_egu">our channels</a> to stay updated.

[caption id="attachment_5629" align="alignleft" width="400"]<a href="https://blogs.egu.eu/divisions/g/files/2026/05/GA26_RECAP_FIG1-1.jpg"><img class="wp-image-5629" src="https://blogs.egu.eu/divisions/g/files/2026/05/GA26_RECAP_FIG1-1.jpg" alt="" width="400" height="300" /></a> Part of the ECS Team that attended the GA26 onsite. From left to right: Chethan Çağatay, Michela, Marius, Barbara, Leire, Kiana (Picture courtesy of Kiana Karimi)[/caption]

As in the past years, we started our GA with the online division meeting before the general assembly to present the G-Division strucure and give an overview of our activities. We updated the division structure as the team is growing. We are excited to introduce our new ECS Co-representative, Michela Ravanelli, who has taken over the role from our outgoing ECS Co-representative, Öykü Koç. Here, we want to express our great gratitude to Öykü’s work over the past years within the Geodesy Division and their efforts for the ECS community union-wide. Öykü initiated many blog post series and implemented regular online and in-person events during the General Assembly, which strengthened our community and we will continue to organise in the future. We introduced the new ECS team members who have and will continue to write this blog, coordinate our social media, and host our regular campfires and onsite Pop-up networking events. Our representative, Marius, will continue to organize together with Michela and the entire team these events and extend our community efforts.

In Vienna, we started the EGU26 week with the pre-icebreaker as usual, but this year we decided to expand the number of divisions involved a bit more, partly to engage with other fields and explore the interdisciplinarity of our division. It took place on Sunday, when early-career scientists from the Geodesy (G), Geodynamics (GD), Planetary Sciences (PS), and Solar-Terrestrial Sciences (ST) divisions gathered at CopaBeach.

[caption id="attachment_5630" align="alignnone" width="1600"]<a href="https://blogs.egu.eu/divisions/g/files/2026/05/GA26_RECAP_FIG2_3-1.jpg"><img class="wp-image-5630 size-full" src="https://blogs.egu.eu/divisions/g/files/2026/05/GA26_RECAP_FIG2_3-1.jpg" alt="" width="1600" height="558" /></a> Left: Pre-icebreqker at Copa Beach (Picture courtesy of Marius Schlaak); Right: Geodesy Fika on terrace G (Picture courtesy of Barbara Jenny)[/caption]

Yes, this spot became a kind of permanent location for our pre-GA meet-up. We plan to continue this event every year, so we would love to see you there next year. Let your colleagues know, especially those new to EGU, as it builds a great foundation for a successful and fun week. Following the icebreaker, many attendees headed to the EGU Opening Reception at the conference venue, marking the official start of EGU26.

The momentum continued on Monday morning with the Geodesy Fika, a social gathering held in the EGU networking zone. Geodesy Early Career Scientists convened at the terrace G (our usual spot 🙂) to enjoy a coffee break and connect with each other. It was a vibrant atmosphere, with discussions ranging from research interests to expectations for the General Assembly.

[caption id="attachment_5633" align="alignleft" width="400"]<a href="https://blogs.egu.eu/divisions/g/files/2026/05/IMG-20260504-WA0033.jpg"><img class="wp-image-5633" src="https://blogs.egu.eu/divisions/g/files/2026/05/IMG-20260504-WA0033.jpg" alt="" width="400" height="300" /></a> Short Course Geodesy 101 (Picture courtesy of Barbara Jenny)[/caption]

The short course Geodesy 101, convened by Rebekka Steffen, Eva Boergens, Martin Sehnal, and Anna Kłos, was on Monday lunchtime this year, and it was a great success as it attracted many researchers from all divisions, satisfying their hunger to get an overview of geodetic concepts ranging from GNSS and coordinate transformations to the analysis of gravity data. Have you thought about broadening your horizon across disciplines? The 101 short courses are offered by various divisions and can offer you easily understandable insights into many disciplines. If you are interested, we recommend you take the time to check them out at next year’s GA.

[caption id="attachment_5636" align="alignright" width="400"]<a href="https://blogs.egu.eu/divisions/g/files/2026/05/GA26_RECAP_FIG5-1.jpg"><img class="wp-image-5636" src="https://blogs.egu.eu/divisions/g/files/2026/05/GA26_RECAP_FIG5-1.jpg" alt="" width="400" height="300" /></a> ECS Dinner on Monday night (Picture courtesy of Michela Ravanelli)[/caption]

Monday had even more events for the Geodesy ECS - a joint dinner. Fortunately, we were able to extend the number of spots available compared to last year, allowing us to fill an entire floor! Isn’t it fantastic to have so many ECSs together? If you attended, we would love to hear about your experience so we can work on improvements for next time and don’t forget to tell your new colleagues to join us next year!

<span style="background-color: transparent">The first couple of days at the GA were packed with social events, from union-wide ECS networking events to division-specific ones. This year, the "Women in Geodesy” coffee break was quite a success on Tuesday, where we discussed equity, diversity, and inclusion in geodesy. We ended the day with the IAG reception, which has been a wonderful addition to the GA’s geodesy program for many years. If you missed registering, sign up to our </span><a style="font-style: italic;background-color: transparent" href="https://linktr.ee/ecsg_egu">mailing list</a><span style="background-color: transparent"> to be informed immediately when the registration opens next year.</span>

[caption id="attachment_5642" align="alignnone" width="1600"]<a href="https://blogs.egu.eu/divisions/g/files/2026/05/GA26_RECAP_FIG6-1.jpg"><img class="wp-image-5642 size-full" src="https://blogs.egu.eu/divisions/g/files/2026/05/GA26_RECAP_FIG6-1.jpg" alt="" width="1600" height="1200" /></a> IAG Reception on the top floor of the BEV in Vienna (Picture courtesy of Barbara Jenny)[/caption]

<div style="text-align: left;margin-top: 1em">

Last year’s GA, we introduced a special session in Geodesy G0.1, in a panel discussion format, titled "Geodesy – From Invisible to Essential," to raise awareness of the importance of geodetic products. After the great interest, we moved this year's special session, G2.1 "<a href="https://www.egu26.eu/session/58223">Streamlining geodetic research for policy - how can we utilize the Essential Geodetic Variables (EGVs) for easier engagement and communication</a>", into a large room, where the community discussed how to take action, support and shape policy decision processes. This was an amazing highlight of the Geodesy community in this year’s GA week.

Another highlight of the week was, of course, the medal lectures: the <a href="https://www.egu.eu/awards-medals/vening-meinesz/2026/frank-flechtner/">Vening Meinesz Medal Lecture by Frank Flechtner</a> and the G Division Outstanding <a href="https://www.egu.eu/awards-medals/division-outstanding-ecs-award/2026/eva-borgens/">ECS Award Lecture by Eva Boergens</a>. Bringing together the implementation of satellite gravimetry missions and their processing to userfriendly data products to a variaty of applications.

[caption id="attachment_5637" align="alignnone" width="1600"]<a href="https://blogs.egu.eu/divisions/g/files/2026/05/GA26_RECAP_FIG7-1.jpg"><img class="wp-image-5637 size-full" src="https://blogs.egu.eu/divisions/g/files/2026/05/GA26_RECAP_FIG7-1.jpg" alt="" width="1600" height="1124" /></a> Top left: ECS award lecture of Eva Boergens; Bottom left: Medal lecture of Vening Meinesz medalist Frank Flechtner; Right: Frank Flechtner and Eva Boergens (Pictures courtesy of Holger Steffen)[/caption]

These events, including this blog, are community efforts. Thank you very much to all of you who participated in these events, making the EGU26 a special experience for all of us. We want to continuously improve these events for the community, and it is important for us to give you an opportunity to participate actively and to receive feedback from you, the community. So please let us know if you have <a href="mailto:ecs-g@egu.eu">feedback </a>on past events or suggestions for future events.

[caption id="attachment_5646" align="alignright" width="400"]<a href="https://blogs.egu.eu/divisions/g/files/2026/05/GA26_RECAP_FIG8.jpg"><img class="wp-image-5646" src="https://blogs.egu.eu/divisions/g/files/2026/05/GA26_RECAP_FIG8-1024x768.jpg" alt="" width="400" height="300" /></a> Snapshots from GeoVision (Picture courtesy of Christina Orieschnig)[/caption]

Ideas are always welcome and with your support we can archieve great experiences together. One very sucessful example is the GeoVision which happened for the first time this year and attracted hundreds of people celebrating music together! This event idea grow from our Division and is implemented together with the ECS task group for outreach and communication! <a href="mailto:ecs-g@egu.eu">Reach us </a>to contribute, give feedback, and give us new ideas!

We are looking forward to seeing you again in Vienna next year. In the meantime, stay updated with us in the community via this blog and our social media <a href="https://linktr.ee/ecsg_egu">channels</a>, and listen to and discuss with us online in our monthly campfires.
<p style="text-align: right"><span style="color: #333333"><em>-Edited by Geodesy ECS Team</em></span></p>

</div>]]></content:encoded>
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					<title><![CDATA[What can Greenland ice cores tell us about winter extreme events over Europe?]]></title>
					<link>https://blogs.egu.eu/divisions/cl/2026/05/15/ice_cores/</link>
					<comments>https://blogs.egu.eu/divisions/cl/2026/05/15/ice_cores/#comments</comments>
					<pubDate>Fri, 15 May 2026 11:00:40 +0000</pubDate>
					<dc:creator><![CDATA[Ceren Moral]]></dc:creator>
							<category><![CDATA[Climate of the Past]]></category>
		<category><![CDATA[Greenland Ice cores]]></category>
		<category><![CDATA[stable oxygen isotope ratios]]></category>
		<category><![CDATA[winter extreme events]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Introduction Human-caused climate change is increasing the frequency of extreme weather events around the world, and Europe is no exception. These events typically last from a few days to several weeks or even months. Using climate models and reanalysis products, scientists are studying how extreme weather events will evolve and where they are likely to become more frequent and intense in a warming world, particularly in vulnerable regions. Paleoclimate research makes an important contribution to this effort. Changes in global and regional climate leave traces in physical and biological materials called proxies, which are preserved in natural archives such as trees, corals, speleothems, and ice cores. Scientists have overcome numerous technical and methodological challenges to extract these proxies and use them as a valuable source of information about past climate changes. The type and resolution of information available depends on the nature of the proxy and the archive in which it is stored. In our study, we use the stable oxygen isotope ratios δ18O recorded from 16 Greenland ice cores combined into a single composite record called a stacked record (Figure 1a). This proxy reflects the relative abundance of heavy and light oxygen isotopes in the ice compared to a predetermined sample. Variations in this ratio are primarily driven by the local temperature at which precipitation forms and moisture source conditions. The variation of the stable oxygen isotope ratios is a widely used proxy of past climate temperature changes, but it is also a very good proxy of large-scale atmospheric and oceanic anomaly patterns. While some studies have as well linked variations of the stable oxygen isotope ratios to weather regimes and atmospheric blocking, our study examines its relationship with extreme hydroclimatic events across Europe. How does stable oxygen isotope ratios in Greenland ice cores capture extreme events over Europe? Our study first links stable oxygen isotope ratios variability in the stacked record to a specific atmospheric phenomenon: atmospheric blocking. Blocking occurs when a persistent high-pressure system persists over a region deviating the jet stream, a narrow band of strong winds in the upper atmosphere that flows around the globe. The meandering of the jet stream creates favorable conditions for extreme weather events such as cold spells, heatwaves, and heavy precipitation. Our hypothesis is that when atmospheric blocking occurs over Europe, the circulation over the North Atlantic prevents relatively warm and humid mid-latitude air masses from reaching Greenland, resulting in precipitation with less heavy stable isotope of oxygen, which in turn affects the stable oxygen isotope ratios signal recorded as anomalously low values in the ice cores. To test this hypothesis, we divided the stacked ice core record into two periods: an observational period (1920 – 2011) and a long-term perspective period (1602 – 2003) (Figure 1b &amp; c). We focused first on the observational period, where data availability is greater. Within this period, we identified years with particularly low stable oxygen isotope ratios values and examined the average large-scale atmospheric circulation patterns during those years (Figure 2a). The resulting circulation pattern provides empirical support for our hypothesis, showing that the atmospheric configuration prevents mid-latitude air masses from reaching Greenland (Figure 2b). Importantly, we found that atmospheric blocking occurs four times more frequently during low stable oxygen isotope ratios years compared to all other years. A similar pattern is also observed over the long-term period (Figure 3a). How does atmospheric blocking shape temperature and precipitation across Europe? During the observational period, the blocking events are associated with a high-pressure system stretching from the Azores toward northern and central Europe. This drives increased moisture transport toward northern Europe, particularly along the Norwegian coast, resulting in wetter conditions there (Figures 2d). Southern Europe, by contrast, tends to be drier. Blocking also reshapes temperature patterns across the continent (Figure 2c). By drawing cold air masses southward from the Nordic region, it drives notable cooling in western Turkey and Greece, and to a lesser extent in southern Italy and the Iberian Peninsula. Central Europe, however, experiences relatively warmer conditions, as Atlantic air masses can still reach these regions. The overall picture is a clear spatial contrast: cooling in the southeast and warming in the centre and northwest. Over the long-term period, the relationship between Greenland stable oxygen isotope ratios and European hydroclimate remains remarkably consistent. Lower stable oxygen isotope ratios values are again associated with circulation patterns resembling persistent blocking over Europe (Figure 3a), producing warmer and wetter conditions in northern Europe and cooler and drier conditions in the south. Comparing the distributions of temperature and precipitation changes between low and high stable oxygen isotope ratios years (Figure 3b, c &amp; d) reveals that the effects of the blocking are most pronounced in the tails of these distributions, pointing to a greater likelihood of extreme wet and warm conditions in northern Europe, and extreme cold and dry conditions in the south. This recurring pattern suggests that the link between stable oxygen isotope ratios variability and European hydroclimate is stable over centuries. Our results show that Greenland ice cores record atmospheric blocking activity over Europe, which plays a key role in shaping hydroclimatic extremes across the continent. To read more about our research you can access the article here. This post has been edited by the editorial board References: Gagliardi, A., Rimbu, N., Lohmann, G., and Ionita, M.: Northern Greenland transect stacked ice cores as a proxy for winter extreme events in Europe, Clim. Past, 22, 935–955, https://doi.org/10.5194/cp-22-935-2026, 2026. IPCC: Climate Change 2021: The Physical Science Basis. Contribution of Working Group I to the Sixth Assessment Report of the Intergovernmental Panel on Climate Change, vol. In Press, Cambridge University Press, Cambridge, United Kingdom and New York, NY, USA, https://doi.org/10.1017/9781009157896, 2021. Hörhold, M., Münch, T., Weißbach, S., Kipfstuhl, S., Freitag, J., Sasgen, I., Lohmann, G., Vinther, B., and Laepple, T.: Modern temperatures in central–north Greenland warmest in past millennium, Nature, 613, 503–507, https://doi.org/10.1038/s41586-022-05517-z, 2023. &nbsp;]]></description>
													<content:encoded><![CDATA[<strong>Introduction</strong>

Human-caused climate change is increasing the frequency of extreme weather events around the world, and Europe is no exception. These events typically last from a few days to several weeks or even months. Using climate models and reanalysis products, scientists are studying how extreme weather events will evolve and where they are likely to become more frequent and intense in a warming world, particularly in vulnerable regions.

Paleoclimate research makes an important contribution to this effort. Changes in global and regional climate leave traces in physical and biological materials called proxies, which are preserved in natural archives such as trees, corals, speleothems, and ice cores. Scientists have overcome numerous technical and methodological challenges to extract these proxies and use them as a valuable source of information about past climate changes. The type and resolution of information available depends on the nature of the proxy and the archive in which it is stored.

[caption id="attachment_5559" align="alignright" width="1024"]<a href="https://blogs.egu.eu/divisions/cl/files/2026/04/f1.png"><img class="wp-image-5559 size-large" src="https://blogs.egu.eu/divisions/cl/files/2026/04/f1-1024x569.png" alt="" width="1024" height="569" /></a> <strong>Figure 1</strong> Ice cores locations (dots) and weather stations (diamonds) used in stacked ice cores (a). The detrended anomalies of δ18O series over the period 1920− 2011 and 1602− 2003 (b, c). The upward-pointing red triangles refer to years whenever the δ18O is above the threshold 1σ (pos. years) (σ = standard deviation). Similarly, downward-pointing blue triangles refer to years below the threshold −1σ (neg. years).[/caption]

<a href="https://cp.copernicus.org/articles/22/935/2026/">In our study</a>, we use the stable oxygen isotope ratios δ<sup>18</sup>O recorded from 16 Greenland ice cores combined into a single composite record called a stacked record (<strong>Figure 1a</strong>). This proxy reflects the relative abundance of heavy and light oxygen isotopes in the ice compared to a predetermined sample. Variations in this ratio are primarily driven by the local temperature at which precipitation forms and moisture source conditions. The variation of the stable oxygen isotope ratios is a widely used proxy of past climate temperature changes, but it is also a very good proxy of large-scale atmospheric and oceanic anomaly patterns. While some studies have as well linked variations of the stable oxygen isotope ratios to weather regimes and atmospheric blocking, our study examines its relationship with extreme hydroclimatic events across Europe.

<strong>How does stable oxygen isotope ratios in Greenland ice cores capture extreme events over Europe?</strong>

Our study first links stable oxygen isotope ratios variability in the stacked record to a specific atmospheric phenomenon: atmospheric blocking. Blocking occurs when a persistent high-pressure system persists over a region deviating the jet stream, a narrow band of strong winds in the upper atmosphere that flows around the globe. The meandering of the jet stream creates favorable conditions for extreme weather events such as cold spells, heatwaves, and heavy precipitation.

Our hypothesis is that when atmospheric blocking occurs over Europe, the circulation over the North Atlantic prevents relatively warm and humid mid-latitude air masses from reaching Greenland, resulting in precipitation with less heavy stable isotope of oxygen, which in turn affects the stable oxygen isotope ratios signal recorded as anomalously low values in the ice cores.

[caption id="attachment_5563" align="alignleft" width="1024"]<a href="https://blogs.egu.eu/divisions/cl/files/2026/04/f2.png"><img class="wp-image-5563 size-large" src="https://blogs.egu.eu/divisions/cl/files/2026/04/f2-1024x738.png" alt="" width="1024" height="738" /></a> <strong>Figure 2</strong> The composite maps of the detrended monthly anomalies of the geopotential height (shaded) at 500 hPa (Z500) and the wind (vector) at 500hPa (a), detrended integrated vapor transport (IVT) (b), detrended cool nights index TN10p (c), and detrended total precipitation index PRCPTOT (d) on the winter season (DJF) in the negative years the NGT stacked ice core record for the period 1920− 2011.[/caption]

To test this hypothesis, we divided the stacked ice core record into two periods: an observational period (1920 – 2011) and a long-term perspective period (1602 – 2003) (<strong>Figure 1b &amp; c</strong>). We focused first on the observational period, where data availability is greater. Within this period, we identified years with particularly low stable oxygen isotope ratios values and examined the average large-scale atmospheric circulation patterns during those years (<strong>Figure 2a</strong>). The resulting circulation pattern provides empirical support for our hypothesis, showing that the atmospheric configuration prevents mid-latitude air masses from reaching Greenland (<strong>Figure 2b</strong>). Importantly, we found that atmospheric blocking occurs four times more frequently during low stable oxygen isotope ratios years compared to all other years. A similar pattern is also observed over the long-term period (<strong>Figure 3a</strong>).

<strong>How does atmospheric blocking shape temperature and precipitation across Europe?</strong>

During the observational period, the blocking events are associated with a high-pressure system stretching from the Azores toward northern and central Europe. This drives increased moisture transport toward northern Europe, particularly along the Norwegian coast, resulting in wetter conditions there (<strong>Figures 2d</strong>). Southern Europe, by contrast, tends to be drier.

Blocking also reshapes temperature patterns across the continent (<strong>Figure 2c</strong>). By drawing cold air masses southward from the Nordic region, it drives notable cooling in western Turkey and Greece, and to a lesser extent in southern Italy and the Iberian Peninsula. Central Europe, however, experiences relatively warmer conditions, as Atlantic air masses can still reach these regions. The overall picture is a clear spatial contrast: cooling in the southeast and warming in the centre and northwest.

[caption id="attachment_5565" align="alignright" width="965"]<a href="https://blogs.egu.eu/divisions/cl/files/2026/04/f3.png"><img class="wp-image-5565 size-full" src="https://blogs.egu.eu/divisions/cl/files/2026/04/f3.png" alt="" width="965" height="932" /></a> <strong>Figure 3</strong> Probability density functions of the standardized monthly field average for the following atmospheric variables: geopotential height at 500 hPa (Z500) (a), 2-meter temperature over the selected box (b), and precipitation (c, d)). All indices are calculated for winter (DJF) during the negative years of the NGT-stacked ice core δ18O record, covering the period 1602–2003. The shaded bands represent the 90% confidence intervals. The corresponding analysis boxes are shown with solid red lines in the upper-right map of each panel. See the main text for the coordinates used for the NGT-stacked ice record.[/caption]

Over the long-term period, the relationship between Greenland stable oxygen isotope ratios and European hydroclimate remains remarkably consistent. Lower stable oxygen isotope ratios values are again associated with circulation patterns resembling persistent blocking over Europe (<strong>Figure 3a</strong>), producing warmer and wetter conditions in northern Europe and cooler and drier conditions in the south. Comparing the distributions of temperature and precipitation changes between low and high stable oxygen isotope ratios years (<strong>Figure 3b, c &amp; d</strong>) reveals that the effects of the blocking are most pronounced in the tails of these distributions, pointing to a greater likelihood of extreme wet and warm conditions in northern Europe, and extreme cold and dry conditions in the south. This recurring pattern suggests that the link between stable oxygen isotope ratios variability and European hydroclimate is stable over centuries.

Our results show that Greenland ice cores record atmospheric blocking activity over Europe, which plays a key role in shaping hydroclimatic extremes across the continent.

To read more about our research you can access the article <a href="https://cp.copernicus.org/articles/22/935/2026/">here</a>.
<p style="text-align: right"><strong>This post has been edited by the editorial board</strong></p>

<pre style="font-weight: 400">References:
Gagliardi, A., Rimbu, N., Lohmann, G., and Ionita, M.: Northern Greenland transect stacked ice cores as a proxy for winter extreme events in Europe, Clim. Past, 22, 935–955, <a href="https://cp.copernicus.org/articles/22/935/2026/">https://doi.org/10.5194/cp-22-935-2026</a>, 2026.

IPCC: Climate Change 2021: The Physical Science Basis. Contribution of Working Group I to the Sixth Assessment Report of the Intergovernmental Panel on Climate Change, vol. In Press, Cambridge University Press, Cambridge, United Kingdom and New York, NY, USA, <a href="https://doi.org/10.1017/9781009157896">https://doi.org/10.1017/9781009157896</a>, 2021.

Hörhold, M., Münch, T., Weißbach, S., Kipfstuhl, S., Freitag, J., Sasgen, I., Lohmann, G., Vinther, B., and Laepple, T.: Modern temperatures in central–north Greenland warmest in past millennium, Nature, 613, 503–507, <a href="https://doi.org/10.1038/s41586-022-05517-z">https://doi.org/10.1038/s41586-022-05517-z</a>, 2023.</pre>
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					<title><![CDATA[Dialogues between glaciers and humans]]></title>
					<link>https://blogs.egu.eu/divisions/cr/2026/05/15/glacier-and-humans-dialogue-between-art-and-science/</link>
					<comments>https://blogs.egu.eu/divisions/cr/2026/05/15/glacier-and-humans-dialogue-between-art-and-science/#comments</comments>
					<pubDate>Fri, 15 May 2026 08:03:04 +0000</pubDate>
					<dc:creator><![CDATA[Sophie Berger]]></dc:creator>
							<category><![CDATA[Cryoscience & Art]]></category>
		<category><![CDATA[Art-science]]></category>
		<category><![CDATA[field stories]]></category>
		<category><![CDATA[glacier]]></category>
		<category><![CDATA[outreach]]></category>
		<category><![CDATA[Svalbard]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[At the edge of the world, a voice tries to make itself heard, a whisper slipping between the threads of an unstable reality. In the remote lands of Svalbard, a few hundred miles from the North Pole, lie millennia-old entities, relics of a disappearing species. They murmur in a language that humans today no longer know how to decipher. And yet, it is in this deafness to the voices around them that the climate crisis triggered by humans takes root. In an attempt to reconnect through listening and communication, a small group of humans sets out to meet these entities, the glaciers, listening to their murmurs. It is in this encounter that the research project Glacier Lamentations is born. Research project The research project Glacier Lamentations is led by the Norwegian Academy of Music and the University Centre in Svalbard. Over three years, it brings together three musicians and two glaciologists to address a central question: what if listening to the Earth could push us to act in order to protect it? By combining acoustic and seismological approaches to record different glacier sounds in Svalbard, the project aims to study the impact of these sounds on the perception of the climate crisis and to create musical compositions by exploring the links between humans and non-humans. Beyond listening to glaciers and raising awareness, this project aims at creating embodied, affective, and multisensory forms of engagement with climate change. By developing artistic methods of inquiry through improvisation, field recording, sonification, scientific collaboration and public representation, Glacier Lamentations is thus not only thematic but also methodological, opening a space of discussion between humans and non-humans. Want to listen in? Listen here with this link. Research team The team of Glacier Lamentations is composed of three musicians and two glaciologists. This composition aims at going beyond the binary relation between art and science, exploring how field knowledge, scientific methods, listening practices and artistic transformation inform one another, rather than standing in simple opposition. The three musicians, Torben Snekkestad, Anja Lauvdal and Morten Qvenild, are also researchers in musicology, specialized in the practice and study of free improvisation. They consider exploring the glacier as an improvisation partner. Torben is a saxophonist, he grew up on an island, where he spent a lot of time underwater, free-diving, listening. His approach is to try to reproduce and create multiphonic sounds inspired by nature with different wind instruments. Today, he is reaching the foot of glaciers to continue this technical and spiritual quest. Anja is a pianist, her topics of reflection are aligned with her personality, she works on notions of improvisation, primary creative energy, imperfection. Approaching the glaciers, she continues to explore the responsibility implied by the project, both collectively and as a person carrying important messages. Morten is also a pianist, with one difference: his piano is augmented. When he started thinking about how to lose control in musical creation, he introduced electronic randomness into his compositions. Today, he continues this desire to play on an equal footing with non-humans. The two glaciologists are Andy Hodson and myself, Ugo Nanni. Andy is a researcher and professor of glaciology at UNIS. After working on several glaciers around the world, he has been based in Svalbard for ten years now, a demanding life that quickly tires the body. As a child, he liked being outside, fishing and spending time by the river. Now, he studies ecosystems linked to glaciers and their meltwaters. This career path keeps him almost always outside and on the field with his students. He strongly believes in interdisciplinarity and enjoys transmitting his knowledge to his students. In the Glacier Lamentations project, he is both the Svalbard expert and the field guide. Since my first meeting with Andy on one of his trips to the glaciers in 2017, I have studied glaciers from the Alps to the Arctic, through the Himalayas. In my travels I have recorded their vibrations using seismometers to understand how they respond to melting, how they fracture, how they collapse. I listen to glaciers, as they tell, in their own way, the brutal response of the Earth to what we impose on it, to what we impose on ourselves. As Torben says, glaciers are not only voices or metaphorical interlocutors, but also material, acoustic and temporal phenomena, perhaps even, at times, partners for listening and performance. I deeply believe in the scientific approach, I know its rigor, its beauty, the long time it requires, but I have also understood that it must find other forms to be heard. I have started to look for a bit of poetry in a world that, caught by other narratives, no longer hears scientists. It is not about giving up rigor or simplifying discourse, but about imagining forms where sensitivity finds again its place and its usefulness. This questioning now runs through my practice, and this is why, after three years of living and working in Norway, I joined the Glacier Lamentations project. Listening to glaciers The central perspective of Glacier Lamentations is based on field recording, articulated with a technical and philosophical reflection on situated listening. The musicians bring microphones and hydrophones to collect glacier sounds. The glaciologists bring methods, instruments, and field knowledge. Then, we listen: to each other, to the people living by the glaciers, to the glaciers, and to ourselves. From these audio recordings, we compose a sensitive musical work to raise awareness of global warming. Through an approach rooted in free improvisation, the project explores links between humans and non-humans, sounds and silences, past and future, in order to make the invisible heard. Without aiming at simplification or illustration, this approach proposes a productive tension. On one side, the rigor of the scientific method, based on measurement and repeatability; on the other, the openness of listening, which welcomes unpredictability and emotion. For our group, listening to a glacier is not only collecting sounds, it is recognizing an active otherness, a presence with which we share a fragile world. Our field campaigns are not only documentation trips, but deeply shape the scientific and musical work. In that sense, our shared encounter with place, instability, sound, and environment draws an experiential score. The encounter between humans and glaciers begins in Longyearbyen (Svalbard), the northernmost town in the world and where Andy now calls home. On this island, discovered by whalers and trappers, then populated by coal miners and academics, the population sees its environment changing, too much, too fast. Snow, once cold and light, becomes filled with water and causes deadly avalanches; glaciers, millennia-old entities, will have left the island within a few hundred years. As glaciers retreat, methane reserves buried in the ground are released, initiating a climate feedback process that Andy studies. These changes result from atmospheric warming caused by human activity, in particular the burning of fossil fuels. In Svalbard, temperatures have increased almost seven times faster than elsewhere; by coming to these lands, the Glacier Lamentations research group is not only making a journey to the edge of the world, but also into a potential future for our mid-latitudes, if the voices of this island are not heard. Facing uncertainties and anxiety The climate crisis, and the narratives associated with it, tend to provoke fear and anxiety, which is understandable, but these are paralyzing emotions, not driving ones. We want to encourage engagement by creating emotions such as joy and wonder, by proposing an immersive narrative, and by suggesting adopting the perspective of non-humans, through that of the glacier. The central place of improvisation reflects such a perspective, it is not only an artistic response or aesthetic language, but also a way of exploring relation, attention, contingency, embodiment, and shared experience. Beyond fear, beyond anxiety, beyond paralysis or cynicism, we try to bring out a form of curiosity, a joy, that allows engagement and the belief in a more just future, for humans as well as non-humans. This is why our project crosses genres, opens doors and adopts a vast ecology of forms, a broad constellation of practices. The team from the Norwegian Academy of Music organizes workshops with students, to create these encounters between humans and non-humans, to question our relationships to the world and help them face their anxiety. We share, during concert-lectures and through tactile sound objects, the voices of glaciers and of those who listen to them, whether in political, entrepreneurial, or public spheres.  Sharing beyond academia In line with this constellation, we are currently making a documentary, with Erwan Le Cornec and Chloe Reymond, his partner. Our documentary aims to open a reflection on our relationship to the Other — human as well as non-human. By mixing our approaches, we want to represent the link between the perspective of the expert and that of the citizen, facing subjects that sometimes seem complex to approach and to make one’s own. Our documentary aims to make the research process accessible, through the questions, doubts, and failures that are part of researchers’ daily lives. We have chosen a form in which these questions are also present, with a balance between human and non-human presence, a balance between different forms of language, and a use of fiction storytelling tools to tell reality. Our documentary is therefore grounded in listening, and in particular in listening to those who are not listened to. The narrative arc follows these first encounters between the human group and the glaciers, the search for a dialogue through sound and music, and the sharing of their research through a concert. This documentary is now an integral part of the Glacier Lamentations project and allows this research to reach beyond academic circles. Through these encounters, between scientists and musicians, between humans and non-humans, between voice, sound, and music, we explore, with Glacier Lamentations, the question of our relationship to the Other. Acknowledgements Such a project is never done by a small group; while acknowledging all of our inspirations and the people that contributed would become very long, I wanted to acknowledge some of the one that greatly contributed to this project: Ingrid Ballari Nilssen (Communications Adviser at UNIS), Fred Skancke Hansen (Director of HSE and Quality at UNIS), Julia Freeman (artist), Clovis Tisserand (sound engineer), the Norwegian Research Council and the French Embassy in Norway. Torben Snekkestad and Chloé Reymond have significantly contributed to this article. Torben Snekkestad and Chloé Reymond have significantly contributed to this article.  Further reading Listening to the glacier: www.kraks.fr (website in french, but the whispers of glaciers are universal) The roots of listening in ecology: https://en.wikipedia.org/wiki/Songs_of_the_Humpback_Whale_(album) and https://en.wikipedia.org/wiki/Silent_Spring  About the poetics and the improvisation approaches: https://www.researchcatalogue.net/view/518792/522412  Two authors that inspired this project: https://en.wikipedia.org/wiki/Donna_Haraway and https://en.wikipedia.org/wiki/Hartmut_Rosa  How climate change affect glaciers stability in the Arctic: https://www.nature.com/articles/s41467-025-66349-9 Edited by Emma Pearce and Mack Baysinger]]></description>
													<content:encoded><![CDATA[<i><span style="font-weight: 400">At the edge of the world, a voice tries to make itself heard, a whisper slipping between the threads of an unstable reality. In the remote lands of Svalbard, a few hundred miles from the North Pole, lie millennia-old entities, relics of a disappearing species. They murmur in a language that humans today no longer know how to decipher. And yet, it is in this deafness to the voices around them that the climate crisis triggered by humans takes root. In an attempt to reconnect through listening and communication, a small group of humans sets out to meet these entities, the glaciers, listening to their murmurs. It is in this encounter that the research project </span></i><b><i>Glacier Lamentations</i></b><i><span style="font-weight: 400"> is born.</span></i>

<hr />

<h3><span style="font-weight: 400">Research project</span></h3>
<span style="font-weight: 400">The research project </span><a href="https://nmh.no/en/research/projects/glacier-lamentation"><i><span style="font-weight: 400">Glacier</span></i></a> <a href="https://nmh.no/en/research/projects/glacier-lamentation"><i><span style="font-weight: 400">Lamentations</span></i></a><span style="font-weight: 400"> is led by the Norwegian Academy of Music and the </span><a href="https://www.unis.no/"><span style="font-weight: 400">University Centre in Svalbard</span></a><span style="font-weight: 400">. Over three years, it brings together three musicians and two glaciologists to address a central question: what if listening to the Earth could push us to act in order to protect it? By combining acoustic and seismological approaches to record different glacier sounds in Svalbard, the project aims to study the impact of these sounds on the perception of the climate crisis and to create musical compositions by exploring the links between humans and non-humans. Beyond </span><i><span style="font-weight: 400">listening to glaciers </span></i><span style="font-weight: 400">and </span><i><span style="font-weight: 400">raising awareness</span></i><span style="font-weight: 400">, this project aims at creating embodied, affective, and multisensory forms of engagement with climate change. By developing artistic methods of inquiry through improvisation, field recording, sonification, scientific collaboration and public representation, </span><i><span style="font-weight: 400">Glacier Lamentations</span></i><span style="font-weight: 400"> is thus not only thematic but also methodological, opening a space of discussion between humans and non-humans.</span>

Want to listen in? <a href="https://w.soundcloud.com/player/?url=https%3A//api.soundcloud.com/tracks/soundcloud%253Atracks%253A2230828904&amp;color=%231551c6&amp;auto_play=false&amp;hide_related=true&amp;show_comments=false&amp;show_user=true&amp;show_reposts=false&amp;show_teaser=false">Listen here with this link.</a>
<h3><span style="font-weight: 400">Research team</span></h3>
<span style="font-weight: 400">The team of Glacier Lamentations is composed of three musicians and two glaciologists. This composition aims at going beyond the binary relation between art and science, exploring how field knowledge, scientific methods, listening practices and artistic transformation inform one another, rather than standing in simple opposition. The three musicians, </span><a href="https://trostrecords.bandcamp.com/album/another-way-of-the-heart"><span style="font-weight: 400">Torben Snekkestad</span></a><span style="font-weight: 400">, </span><a href="https://anjalauvdal.bandcamp.com/album/from-a-story-now-lost"><span style="font-weight: 400">Anja Lauvdal</span></a><span style="font-weight: 400"> and </span><a href="https://mortenqvenvild.bandcamp.com/album/personal-piano"><span style="font-weight: 400">Morten Qvenild</span></a><span style="font-weight: 400">, are also researchers in musicology, specialized in the practice and study of free improvisation. They consider exploring the glacier as an improvisation partner. Torben is a saxophonist, he grew up on an island, where he spent a lot of time underwater, free-diving, listening. His approach is to try to reproduce and create multiphonic sounds inspired by nature with different wind instruments. Today, he is reaching the foot of glaciers to continue this technical and spiritual quest. Anja is a pianist, her topics of reflection are aligned with her personality, she works on notions of improvisation, primary creative energy, imperfection. Approaching the glaciers, she continues to explore the responsibility implied by the project, both collectively and as a person carrying important messages. Morten is also a pianist, with one difference: his piano is augmented. When he started thinking about how to lose control in musical creation, he introduced electronic randomness into his compositions. Today, he continues this desire to play on an equal footing with non-humans. The two glaciologists are </span><a href="https://www.unis.no/staff/andy-hodson/"><span style="font-weight: 400">Andy Hodson</span></a><span style="font-weight: 400"> and myself, </span><a href="https://www.ugonanni.fr/"><span style="font-weight: 400">Ugo Nanni</span></a><span style="font-weight: 400">. Andy is a researcher and professor of glaciology at UNIS. After working on several glaciers around the world, he has been based in Svalbard for ten years now, a demanding life that quickly tires the body. As a child, he liked being outside, fishing and spending time by the river. Now, he studies ecosystems linked to glaciers and their meltwaters. This career path keeps him almost always outside and on the field with his students. He strongly believes in interdisciplinarity and enjoys transmitting his knowledge to his students. In the </span><i><span style="font-weight: 400">Glacier Lamentations</span></i><span style="font-weight: 400"> project, he is both the Svalbard expert and the field guide.</span>

<span style="font-weight: 400">Since my first meeting with Andy on one of his trips to the glaciers in 2017, I have studied glaciers from the Alps to the Arctic, through the Himalayas. In my travels I have recorded their vibrations using seismometers to understand how they respond to melting, how they fracture, how they collapse. I </span><a href="https://blogs.egu.eu/divisions/cr/2022/06/03/cryoseismology/"><span style="font-weight: 400">listen to glaciers</span></a><span style="font-weight: 400">, as they tell, in their own way, the brutal response of the Earth to what we impose on it, to what we impose on ourselves. As Torben says, glaciers are not only </span><i><span style="font-weight: 400">voices</span></i><span style="font-weight: 400"> or metaphorical interlocutors, but also material, acoustic and temporal phenomena, perhaps even, at times, partners for listening and performance. I deeply believe in the scientific approach, I know its rigor, its beauty, the long time it requires, but I have also understood that it must find other forms to be heard. I have started to look for a bit of poetry in a world that, caught by other narratives, no longer </span><a href="https://standupforscience.fr/"><span style="font-weight: 400">hears scientists</span></a><span style="font-weight: 400">. It is not about giving up rigor or simplifying discourse, but about imagining forms where sensitivity finds again its place and its usefulness. This questioning now runs through my practice, and this is why, after three years of living and working in Norway, I joined the </span><i><span style="font-weight: 400">Glacier Lamentations</span></i><span style="font-weight: 400"> project.</span>

[caption id="attachment_17415" align="aligncenter" width="1600"]<a href="https://blogs.egu.eu/divisions/cr/files/2026/05/Still-2025-03-24-080527_1.59.1.png"><img class="size-full wp-image-17415" src="https://blogs.egu.eu/divisions/cr/files/2026/05/Still-2025-03-24-080527_1.59.1.png" alt="scattered equipment lays in a windswept, snow covered landscape " width="1600" height="900" /></a> Human presence on the top of the Adventalen pingos. Microphones, jerrycans, drillers. Svalbard, March 2025. Credits E. Le Cornec and C. Reymond. CC BY-NC-ND.[/caption]
<h3><span style="font-weight: 400">Listening to glaciers</span></h3>
<span style="font-weight: 400">The central perspective of </span><i><span style="font-weight: 400">Glacier Lamentations</span></i><span style="font-weight: 400"> is based on field recording, articulated with a technical and philosophical reflection on situated listening. The musicians bring microphones and hydrophones to collect glacier sounds. The glaciologists bring methods, instruments, and field knowledge. Then, we listen: to each other, to the people living by the glaciers, to the glaciers, and to ourselves. From these audio recordings, we compose a sensitive musical work to raise awareness of global warming. Through an approach rooted in free improvisation, the project explores links between humans and non-humans, sounds and silences, past and future, in order to make the invisible heard. Without aiming at simplification or illustration, this approach proposes a productive tension. On one side, the rigor of the scientific method, based on measurement and repeatability; on the other, the openness of listening, which welcomes unpredictability and emotion. For our group, listening to a glacier is not only collecting sounds, it is recognizing an active otherness, a presence with which we share a fragile world. Our field campaigns are not only documentation trips, but deeply shape the scientific and musical work. In that sense, our shared encounter with place, instability, sound, and environment draws an </span><i><span style="font-weight: 400">experiential score</span></i><span style="font-weight: 400">.</span>

[caption id="attachment_17417" align="aligncenter" width="1600"]<a href="https://blogs.egu.eu/divisions/cr/files/2026/05/Still-2025-04-11-001439_1.15.11.png"><img class="size-full wp-image-17417" src="https://blogs.egu.eu/divisions/cr/files/2026/05/Still-2025-04-11-001439_1.15.11.png" alt="two researchers in full arctic gear huddle over a piece of scientific instrumentation in intense wind" width="1600" height="900" /></a> Retrieving seismometers at the front of the surging Paulabreen, Svalbard, March 2025. Credits E. Le Cornec and C. Reymond. CC BY-NC-ND.[/caption]

<span style="font-weight: 400">The encounter between humans and glaciers begins in Longyearbyen (Svalbard), the northernmost town in the world and where Andy now calls home. On this island, discovered by whalers and trappers, then populated by coal miners and academics, the population sees its environment changing, too much, </span><a href="https://northernstories.no/books/63-line-nagell-ylvisaker-my-world-is-melting"><span style="font-weight: 400">too fast</span></a><span style="font-weight: 400">. Snow, once cold and light, becomes filled with water and causes deadly avalanches; glaciers, millennia-old entities, will have left the island within a few hundred years. As glaciers retreat, methane reserves buried in the ground are released, initiating a climate feedback process that Andy studies. These changes result from atmospheric warming caused by human activity, in particular the burning of fossil fuels. In Svalbard, temperatures have increased almost </span><a href="https://www.amap.no/documents/doc/amap-arctic-climate-change-update-2024-key-trends-and-impacts/3851"><span style="font-weight: 400">seven times faster</span></a><span style="font-weight: 400"> than elsewhere; by coming to these lands, the </span><i><span style="font-weight: 400">Glacier Lamentations</span></i><span style="font-weight: 400"> research group is not only making a journey to the edge of the world, but also into a potential future for our mid-latitudes, if the voices of this island are not heard.</span>
<h3><span style="font-weight: 400">Facing uncertainties and anxiety</span></h3>
<span style="font-weight: 400">The climate crisis, and the narratives associated with it, tend to provoke fear and anxiety, which is understandable, but these are paralyzing emotions, not driving ones. We want to encourage engagement by creating emotions such as joy and wonder, by proposing an immersive narrative, and by suggesting adopting the perspective of non-humans, through that of the glacier. The central place of improvisation reflects such a perspective, it is not only an artistic response or aesthetic language, but also a way of exploring relation, attention, contingency, embodiment, and shared experience. Beyond fear, beyond anxiety, beyond paralysis or cynicism, we try to bring out a form of curiosity, a joy, that allows engagement and the belief in a more just future, for humans as well as non-humans. This is why our project crosses genres, </span><a href="https://vimeo.com/1068032392"><span style="font-weight: 400">opens doors</span></a><span style="font-weight: 400"> and adopts a vast ecology of forms, a broad constellation of practices. The team from the Norwegian Academy of Music organizes workshops with students, to create these encounters between humans and non-humans, to question our relationships to the world and help them face their anxiety. We share, during concert-lectures and through </span><a href="https://braiduk.org/artist-julie-freeman"><span style="font-weight: 400">tactile sound objects</span></a><span style="font-weight: 400">, the voices of glaciers and of those who listen to them, whether in </span><a href="https://vimeo.com/1068032392"><span style="font-weight: 400">political</span></a><span style="font-weight: 400">, entrepreneurial, or </span><a href="https://www.articasvalbard.no/2026/glacier-lamentation"><span style="font-weight: 400">public</span></a><span style="font-weight: 400"> spheres. </span>

[caption id="attachment_17419" align="aligncenter" width="1600"]<a href="https://blogs.egu.eu/divisions/cr/files/2026/05/Still-2025-03-24-080527_1.8.2.png"><img class="size-full wp-image-17419" src="https://blogs.egu.eu/divisions/cr/files/2026/05/Still-2025-03-24-080527_1.8.2.png" alt="the photo is almost completely black, except for small spots of light from snow machines in the snow, as seen from a distance" width="1600" height="900" /></a> Night and lights at the edges of Paulabreen. Svalbard, March 2025. Credits E. Le Cornec and C. Reymond. CC BY-NC-ND.[/caption]
<h3><span style="font-weight: 400">Sharing beyond academia</span></h3>
<span style="font-weight: 400">In line with this constellation, we are currently making a documentary, with Erwan Le Cornec and Chloe Reymond, his partner. Our </span><a href="https://www.ugonanni.fr/lechantduglacier.html"><span style="font-weight: 400">documentary</span></a><span style="font-weight: 400"> aims to open a reflection on our relationship to the Other — human as well as non-human. By mixing our approaches, we want to represent the link between the perspective of the expert and that of the citizen, facing subjects that sometimes seem complex to approach and to make one’s own. Our documentary aims to make the research process accessible, through the questions, doubts, and failures that are part of researchers’ daily lives. We have chosen a form in which these questions are also present, with a balance between human and non-human presence, a balance between different forms of language, and a use of fiction storytelling tools to tell reality. Our documentary is therefore grounded in listening, and in particular in listening to those who are not listened to. The narrative arc follows these first encounters between the human group and the glaciers, the search for a dialogue through sound and music, and the sharing of their research through a concert. This documentary is now an integral part of the </span><i><span style="font-weight: 400">Glacier Lamentations</span></i><span style="font-weight: 400"> project and allows this research to reach beyond academic circles.</span>

<span style="font-weight: 400">Through these encounters, between scientists and musicians, between humans and non-humans, between voice, sound, and music, we explore, with </span><i><span style="font-weight: 400">Glacier Lamentations</span></i><span style="font-weight: 400">, the question of our relationship to the Other.</span>
<h3><span style="font-weight: 400">Acknowledgements</span></h3>
<span style="font-weight: 400">Such a project is never done by a small group; while acknowledging all of our inspirations and the people that contributed would become very long, I wanted to acknowledge some of the one that greatly contributed to this project: Ingrid Ballari Nilssen (</span><i><span style="font-weight: 400">Communications Adviser at UNIS</span></i><span style="font-weight: 400">), Fred Skancke Hansen (</span><i><span style="font-weight: 400">Director of HSE and Quality at UNIS</span></i><span style="font-weight: 400">), </span><a href="https://en.wikipedia.org/wiki/Julie_Freeman_(artist)"><span style="font-weight: 400">Julia Freeman</span></a><span style="font-weight: 400"> (artist), </span><a href="https://www.clovistisserand.fr/"><span style="font-weight: 400">Clovis Tisserand</span></a><span style="font-weight: 400"> (sound engineer), the Norwegian Research Council and the French Embassy in Norway. <i>Torben Snekkestad and Chloé Reymond have significantly contributed to this article.</i></span>

<i><span style="font-weight: 400">Torben Snekkestad and Chloé Reymond have significantly contributed to this article. </span></i>
<h3><span style="font-weight: 400">Further reading</span></h3>
<ul>
 	<li style="font-weight: 400"><span style="font-weight: 400">Listening to the glacier: </span><a href="http://www.kraks.fr"><span style="font-weight: 400">www.kraks.fr</span></a><span style="font-weight: 400"> (website in french, but the whispers of glaciers are universal)</span></li>
 	<li style="font-weight: 400"><span style="font-weight: 400">The roots of listening in ecology: </span><a href="https://en.wikipedia.org/wiki/Songs_of_the_Humpback_Whale_(album)"><span style="font-weight: 400">https://en.wikipedia.org/wiki/Songs_of_the_Humpback_Whale_(album)</span></a><span style="font-weight: 400"> and </span><a href="https://en.wikipedia.org/wiki/Silent_Spring"><span style="font-weight: 400">https://en.wikipedia.org/wiki/Silent_Spring</span></a><span style="font-weight: 400"> </span></li>
 	<li style="font-weight: 400"><span style="font-weight: 400">About the poetics and the improvisation approaches: </span><a href="https://www.researchcatalogue.net/view/518792/522412"><span style="font-weight: 400">https://www.researchcatalogue.net/view/518792/522412</span></a><span style="font-weight: 400"> </span></li>
 	<li style="font-weight: 400"><span style="font-weight: 400">Two authors that inspired this project: </span><a href="https://en.wikipedia.org/wiki/Donna_Haraway"><span style="font-weight: 400">https://en.wikipedia.org/wiki/Donna_Haraway</span></a><span style="font-weight: 400"> and </span><a href="https://en.wikipedia.org/wiki/Hartmut_Rosa"><span style="font-weight: 400">https://en.wikipedia.org/wiki/Hartmut_Rosa</span></a><span style="font-weight: 400"> </span></li>
 	<li><span style="font-weight: 400">How climate change affect glaciers stability in the Arctic: </span><a href="https://www.nature.com/articles/s41467-025-66349-9"><span style="font-weight: 400">https://www.nature.com/articles/s41467-025-66349-9</span></a>

<hr />

<h5 style="text-align: right"><em><strong>Edited by Emma Pearce and Mack Baysinger</strong></em></h5>
</li>
</ul>]]></content:encoded>
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					<title><![CDATA[HydroTalks: Prof. Laura Richards and Ajmal Roshan on groundwater quality, arsenic, and citizen science]]></title>
					<link>https://blogs.egu.eu/divisions/hs/2026/05/14/hydrotalks-prof-laura-richards-and-ajmal-roshan-on-groundwater-quality-arsenic-and-citizen-science/</link>
					<comments>https://blogs.egu.eu/divisions/hs/2026/05/14/hydrotalks-prof-laura-richards-and-ajmal-roshan-on-groundwater-quality-arsenic-and-citizen-science/#comments</comments>
					<pubDate>Thu, 14 May 2026 14:00:00 +0000</pubDate>
					<dc:creator><![CDATA[Archita Bhattacharyya]]></dc:creator>
							<category><![CDATA[Contaminant hydrology]]></category>
		<category><![CDATA[Early Career Scientists]]></category>
		<category><![CDATA[Groundwater]]></category>
		<category><![CDATA[Subsurface hydrology]]></category>
		<category><![CDATA[Contamination]]></category>
		<category><![CDATA[groundwater]]></category>
		<category><![CDATA[Water quality]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[For this month’s episode of HydroTalks, we’re thrilled to welcome Prof. Laura Richards and Ajmal Roshan. Laura is a UKRI Future Leaders Fellow and Professor of Water Resources and Environmental Geochemistry at the University of Manchester. Laura is also the project lead of the AQUAROAD Programme on groundwater quality in the Global South. Ajmal is a Cookson Awardee PhD scholar, and he&#8217;s working within Laura&#8217;s group as a joint PhD student between the University of Manchester and University of Melbourne. You can check out the full episode here read the interview summary in this blog! To kick off, can you quickly tell us about your current research focus? Laura: My work sits between environmental engineering and environmental geochemistry. I study how contaminants move through groundwater, how human activities affect water quality, and how we can choose better remediation strategies. A lot of my research is field-based, and I&#8217;ve had the opportunity to work extensively in South and Southeast Asia, East Africa, and South America. Ajmal: I work on groundwater arsenic contamination in Bihar, India. My research focuses on improving water security by identifying and managing suitable arsenic remediation options. What pollutants of concern do you find in the aquifers of the Gangetic Plain? Ajmal: The Gangetic Plain is quite densely populated. And the groundwater can be contaminated with different geogenic contaminants such as arsenic, fluoride, uranium, and manganese and sometimes microbial contamination. Since many households in Bihar rely on groundwater for drinking, contamination can becomes a public health issue. Since contaminants like arsenic are colourless and odourless, many residents are consuming it without knowing. Laura: We also find anthropogenic contaminants from human activities, including pharmaceuticals, fertilisers, industrial chemicals, and personal care products. In Patna, one commonly detected emerging contaminant was sucralose, an artificial sweetener. Many of these chemicals still lack guideline values, so their risks are not always clear. Why is arsenic contamination such a concern? Laura: Arsenic is naturally present in some aquifer sediments and can be released into groundwater under reducing conditions, often through the breakdown of iron and manganese minerals. It is dangerous because chronic exposure can lead to numerous health effects, and awareness can be low because people cannot see, smell, or taste it in water. Estimates suggest that about 220 million people worldwide are potentially exposed to high concentrations of arsenic in groundwater, and around 94% of them are in Asia. A statewide survey as part of our Far-Ganga project, showed that in Bihar alone, 16% of the samples had elevated Arsenic. Ajmal:  Arsenic is highly variable, even over short distances. Two wells only a few hundred metres apart can have very different arsenic levels, even if they are similar depths. Local geology and redox conditions play a major role. Do you see any promising arsenic remediation technologies? Ajmal: In our recent paper we explored different technologies.  Filter-based, sorption-based, membrane-based options can be capable, but there is no gold-standard across different regions. The best option depends on effectiveness, local conditions, cost, maintenance needs, material availability, and whether the community is willing to use it. Do you anticipate that increasing floods and droughts due to climate change can have a cascade effect on arsenic pollution? Laura: Possibly. Arsenic release is linked to microbial activity, iron minerals, and organic carbon, all of which may respond to changing flood and drought patterns. However, the links are complex and highly redox-sensitive. In our research in Cambodia, we have seen seasonal changes in redox conditions, organic matter and microbes, but not strong seasonal changes in arsenic. So, spatial and depth controls may be more important than seasonal patterns. But  it&#8217;s a really important area for future research. How are you using AI and citizen science to tackle water quality issues? Laura: Citizen science can support both data collection and public engagement. In Bihar, around 600 students helped collect groundwater samples, which greatly expanded the scale of sampling. It also helped raise awareness and show young people different pathways into STEM. Ajmal: AI tools need good data. In many low- and middle-income regions, groundwater data are limited or uneven. Citizen science can help generate better datasets, which may later support AI-based decision tools. What is the aim of AQUAROAD? Laura: AQUAROAD aims to develop a roadmap for better groundwater quality management in the Global South. We are starting with Bihar and Uganda as contrasting case studies. The project brings together experts in groundwater science, remediation, decision science, social science, machine learning, and modelling. This breadth of expertise is needed to tackle some pressing issues, and trans-disciplinary global challenges. What are the biggest breakthroughs in the past 10 years and what are the biggest trends in upcoming years? Laura: Over the past decade, water research has increasingly moved beyond disciplinary and sectoral silos. Future progress will depend on connecting groundwater, surface water, engineering, and social science perspectives, while using tools like AI responsibly to address complex water and climate challenges. Finally, what is the career advice that you&#8217;ve received and want to share with early-career scientists? Laura: Do not let naysayers define what you can do. Embrace opportunities, be persistent, and find the path that works for your own priorities and values. Ajmal: Be flexible. Research and career paths do not always go as planned, so it helps to have a broad blueprint rather than a rigid plan. Check out the full episode here.]]></description>
													<content:encoded><![CDATA[For this month’s episode of HydroTalks, we’re thrilled to welcome <a href="https://research.manchester.ac.uk/en/persons/laura.richards">Prof. Laura Richards</a> and <a href="https://research.manchester.ac.uk/en/persons/ajmal-roshan/">Ajmal Roshan</a>. Laura is a UKRI Future Leaders Fellow and Professor of Water Resources and Environmental Geochemistry at the University of Manchester. Laura is also the project lead of the <a href="https://www.aquaroad.org/">AQUAROAD</a> Programme on groundwater quality in the Global South. Ajmal is a Cookson Awardee PhD scholar, and he's working within Laura's group as a joint PhD student between the University of Manchester and University of Melbourne.

You can check out the <a href="https://youtu.be/6lJ3kxpAZC4?si=s80LDa5QAz7_efKL">full episode here</a> read the interview summary in this blog!
<h2>To kick off, can you quickly tell us about your current research focus?</h2>
<u>Laura:</u> My work sits between environmental engineering and environmental geochemistry. I study how contaminants move through groundwater, how human activities affect water quality, and how we can choose better remediation strategies. A lot of my research is field-based, and I've had the opportunity to work extensively in South and Southeast Asia, East Africa, and South America.

<u>Ajmal:</u> I work on groundwater arsenic contamination in Bihar, India. My research focuses on improving water security by identifying and managing suitable arsenic remediation options.
<h2>What pollutants of concern do you find in the aquifers of the Gangetic Plain?</h2>
<u>Ajmal:</u> The Gangetic Plain is quite densely populated. And the groundwater can be contaminated with different geogenic contaminants such as arsenic, fluoride, uranium, and manganese and sometimes microbial contamination. Since many households in Bihar rely on groundwater for drinking, contamination can becomes a public health issue. Since contaminants like arsenic are colourless and odourless, many residents are consuming it without knowing.

<u>Laura:</u> We also find anthropogenic contaminants from human activities, including pharmaceuticals, fertilisers, industrial chemicals, and personal care products. In Patna, one commonly detected emerging contaminant was sucralose, an artificial sweetener. Many of these chemicals still lack guideline values, so their risks are not always clear.
<h2>Why is arsenic contamination such a concern?</h2>
<u>Laura:</u> Arsenic is naturally present in some aquifer sediments and can be released into groundwater under reducing conditions, often through the breakdown of iron and manganese minerals. It is dangerous because chronic exposure can lead to numerous health effects, and awareness can be low because people cannot see, smell, or taste it in water. Estimates suggest that about 220 million people worldwide are potentially exposed to high concentrations of arsenic in groundwater, and around 94% of them are in Asia. A statewide survey as part of our <a href="https://www.farganga.org/"><u>Far-Ganga project,</u></a> showed that in Bihar alone, 16% of the samples had elevated Arsenic.

<u>Ajmal</u><u>:</u>  Arsenic is highly variable, even over short distances. Two wells only a few hundred metres apart can have very different arsenic levels, even if they are similar depths. Local geology and redox conditions play a major role.
<h2>Do you see any promising arsenic remediation technologies?</h2>
Ajmal: In our <a href="https://www.sciencedirect.com/science/article/pii/S2352801X26000226"><u>recent paper</u></a> we explored different technologies.  Filter-based, sorption-based, membrane-based options can be capable, but there is no gold-standard across different regions. The best option depends on effectiveness, local conditions, cost, maintenance needs, material availability, and whether the community is willing to use it.
<h2>Do you anticipate that increasing floods and droughts due to climate change can have a cascade effect on arsenic pollution?</h2>
<u>Laura:</u> Possibly. Arsenic release is linked to microbial activity, iron minerals, and organic carbon, all of which may respond to changing flood and drought patterns. However, the links are complex and highly redox-sensitive. In <a href="https://www.sciencedirect.com/science/article/pii/S0048969718353336?via%3Dihub"><u>our research</u></a> in Cambodia, we have seen seasonal changes in redox conditions, organic matter and microbes, but not strong seasonal changes in arsenic. So, spatial and depth controls may be more important than seasonal patterns. But  it's a really important area for future research.
<h2>How are you using AI and citizen science to tackle water quality issues?</h2>
<u>Laura:</u> Citizen science can support both data collection and public engagement. In Bihar, around 600 students helped collect groundwater samples, which greatly expanded the scale of sampling. It also helped raise awareness and show young people different pathways into STEM.

<u>Ajmal: </u>AI tools need good data. In many low- and middle-income regions, groundwater data are limited or uneven. Citizen science can help generate better datasets, which may later support AI-based decision tools.
<h2>What is the aim of AQUAROAD?</h2>
<u>Laura:</u> <a href="https://www.aquaroad.org/"><u>AQUAROAD</u></a> aims to develop a roadmap for better groundwater quality management in the Global South. We are starting with Bihar and Uganda as contrasting case studies. The project brings together experts in groundwater science, remediation, decision science, social science, machine learning, and modelling. This breadth of expertise is needed to tackle some pressing issues, and trans-disciplinary global challenges.
<h2>What are the biggest breakthroughs in the past 10 years and what are the biggest trends in upcoming years?</h2>
<u>Laura:</u> Over the past decade, water research has increasingly moved beyond disciplinary and sectoral silos. Future progress will depend on connecting groundwater, surface water, engineering, and social science perspectives, while using tools like AI responsibly to address complex water and climate challenges.
<h2>Finally, what is the career advice that you've received and want to share with early-career scientists?</h2>
<u>Laura:</u> Do not let naysayers define what you can do. Embrace opportunities, be persistent, and find the path that works for your own priorities and values.

<u>Ajmal</u>: Be flexible. Research and career paths do not always go as planned, so it helps to have a broad blueprint rather than a rigid plan.

Check out the <a href="https://youtu.be/6lJ3kxpAZC4?si=s80LDa5QAz7_efKL">full episode here</a>.]]></content:encoded>
																<wfw:commentRss>https://blogs.egu.eu/divisions/hs/2026/05/14/hydrotalks-prof-laura-richards-and-ajmal-roshan-on-groundwater-quality-arsenic-and-citizen-science/feed/</wfw:commentRss>
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					<title><![CDATA[Destruction of North China Craton: through the chronotunnel of time]]></title>
					<link>https://blogs.egu.eu/divisions/gd/2026/05/13/destruction-of-north-china-craton-through-the-chronotunnel-of-time/</link>
					<comments>https://blogs.egu.eu/divisions/gd/2026/05/13/destruction-of-north-china-craton-through-the-chronotunnel-of-time/#comments</comments>
					<pubDate>Wed, 13 May 2026 07:00:05 +0000</pubDate>
					<dc:creator><![CDATA[Editorial Team 2]]></dc:creator>
							<category><![CDATA[Remarkable Regions]]></category>
		<category><![CDATA[asia]]></category>
		<category><![CDATA[china]]></category>
		<category><![CDATA[china tectonics]]></category>
		<category><![CDATA[cratons]]></category>
		<category><![CDATA[decratonization]]></category>
		<category><![CDATA[geodynamic]]></category>
		<category><![CDATA[north china craton]]></category>
		<category><![CDATA[orogen]]></category>
		<category><![CDATA[tectonics]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[The Asian continent has fascinated the world for at least 3,000 years with its music, food, and discoveries, as well as its breathtaking landscapes. Most of these incredible landscapes are formed by mountains that can be considered geologically &#8220;recent&#8221; (such as the Cenozoic formation of the Himalayas). However, there are also ancient terrains, pre-dating the Mesozoic, that pose intriguing questions for geoscientists. Today, Professor Yu Wang (王瑜) from the Institute of Earth Sciences (Beijing) at the Chinese University of Geosciences (中国地质大学(北京)) will take us on a geological tour through the history of one of these ancient terrains: the North China Craton! This portion of the Chinese landmass is located between the Yangtze Craton (also known as the South China Craton) and the Central Asian Orogenic Belt—a giant tectonic domain—and hosts the Cenozoic basins of China’s northern coast (Figure 1). The formation, evolution, and destruction of the North China Craton (NCC) are highly complex and remain a subject of active debate, as modern geoscience continually brings forward new data and theories regarding the region. Now that we have a brief introduction, let us examine it more closely. Several proposed models The lithospheric thinning of the North China Craton (NCC) by ~100–120 km was initially deduced from early Paleozoic kimberlite intrusions (~480 Ma) in eastern China (Figure 1). Therefore, the destruction of the NCC has been attributed to multiple cycles of delamination associated with magmatic ascent, rifting, and extension. Typically, cratonic destruction was considered to have occurred predominantly around 130–120 Ma, resulting from multiple magmatic intrusions and coinciding with the formation of many metamorphic core complexes. Driven by this timeline, different geodynamic hypotheses have been put forward, such as cratonic delamination and the subduction rollback of the paleo-Pacific plate. Following a comprehensive review of the NCC&#8217;s tectonic evolution, the current consensus is that the so-called destruction of the craton was actually a long-term evolutionary process in the region. Age data indicate distinct structural and magmatic stages occurring at ~1600–1500, 1300–1100, 445–315, 270–200, 170–155, 130–110, 75–65, and 25–20 Ma. These distinct stages correlate directly with episodes of basin formation, continental uplift, and lithospheric collapse. 1. Cratonization and Decratonization The NCC formed prior to ~1.8–1.9 Ga. Although its oldest Archean rocks date back to 3.8 Ga, the majority of its crustal growth occurred between 2.9 and 2.5 Ga. From 1.8 Ga onwards, subsequent sedimentation covered the entirety of the craton. During the Mesoproterozoic (at ~1.6–1.4 Ga), following the break-up of the Columbia (also known as the Nuna) supercontinent, intense magmatic activity took place, resulting in the formation of a major unconformity along the northern margin of the NCC. Similar tectonic features are observed at the southern margin, evidenced by records of volcanic eruptions dating to ~1.6–1.5 Ga.  From 1,300 to ~445 Ma, the cratonic crust remained relatively stable, as indicated by the shallow marine sediments covering the basement rocks. This earlier stage of marginal rifting and extension can be characterised as a period of &#8216;proto-destruction&#8217;, serving as a prelude to the craton&#8217;s later, more severe decratonization. 2. De-rooting of the NCC (~445–315 Ma) A sudden shift in sedimentary sequences during the Late Ordovician reflects a period of significant regional uplift, which persisted until the Middle–Late Carboniferous. Although this uplift event affected the entirety of the NCC, it was most pronounced in the central region, with absolute ages constraining the tectonic activity to between 445 and 315 Ma. Stratigraphic and petrological evidence supports this timeline. For instance, early Paleozoic kimberlite intrusions (488–465 Ma) predate the formation of the zircon-bearing bauxites associated with the uplift. Because these kimberlites indicate an intact lithospheric thickness of approximately 200 km during the early Paleozoic, researchers infer that the NCC only became detached from its lithospheric root subsequently (around 480–460 Ma). Over time, the lithosphere thinned by as much as 100 to 120 km. This extensive continental uplift was most likely driven by the craton detaching from its deep root, resulting in a fundamental loss of tectonic stability. 3. Marginal reactivation and subsequent orogeny (~320–200 Ma) Along the northern and southern margins of the NCC, episodes of deformation and magmatism occurred between ~320 and 200 Ma (Figure 2). Petrology suggests that these magmatic rocks originated from the partial melting of pre-existing gneiss and granulite. At the northern margin, E-W trending ductile shear zones accommodated this strain, producing prominent southward-verging inclined and recumbent folds. This indicates that the de-rooting of the craton likely initiated at its margins before progressively migrating towards the cratonic interior. Ultimately, these marginal areas lost their inherent cratonic stability and fluid-depleted characteristics. Having shed their cratonic signature, they transitioned entirely into active orogenic belts. Following this stage of marginal reactivation, the stable, rigid core of the North China Craton was significantly reduced in size and continued to progressively shrink over time. 4. Tectonic transformation and complete reactivation (170–155 Ma) Beginning at ~170–165 Ma, a fundamental transformation of the regional tectonic domain completely reconfigured the eastern Chinese landmass (Figure 3). During this period, the structural regime of the NCC underwent a major kinematic shift, transitioning from an E–W trend to a N-S trend. Correspondingly, the overarching tectonic setting shifted from an association with the Eurasian domain to being governed by the western Pacific plate boundary. Deformation during this transitional stage was both intensive and widespread. Lower crustal materials were exhumed to the surface, accompanied by substantial volcanic activity and crust–mantle interaction, predominantly localised within regions undergoing active tectonic transformation. Continued orogenesis at the cratonic margins resulted in a further reduction in the size of the stable cratonic core. Ultimately, under the influence of the western Pacific tectonic setting, the NCC transitioned entirely into an active continental margin 5. Removal of the lithospheric root: the North China cratonic margin (130–110 Ma) It has been suggested that the main period of destruction of the NCC was at ~130–110 Ma. Studies indicate that deformation, magmatism and basin formation during this period represent strong evidence for the destruction of the North China craton. Between 130 and 110 Ma, de-rooting of the craton had occurred along the northern margin, and likely also the southern margin. Either lithospheric de-rooting must have occurred, or a new lithospheric root must have grown. There is no evidence of regional extensional tectonics at this time. The rollback of the Western Pacific Plate may have been controlled by the extension of a large area of Eastern Asia. The best explanation so far is that mantle extrusion occurred across the entire Eastern Asian continent. 6. Partial removal of continental lithospheric mantle (75–65 Ma) This stage of deformation only affected the eastern segment of the northern North China Craton, and in the northeast and southeast of eastern China. High-angle normal faults define the boundaries of the eastern part of the NCC, or the boundaries of the North China Basin. At 75–65 Ma, the Taihang Mountain Belt underwent rapid uplift and exhumation, and the eastern China continental margin opened. Since then, the North China continental lithospheric mantle changed as the oceanic lithospheric mantle feature. 7. Deformation and differential mountain uplift (25–20 Ma) Deformation and volcanic activity during this stage occurred in localised areas, generally along the north of the North China Basin. Basaltic activity occurred along the eastern Asian continental margin and in the interior. Later rifting, up to eight million years younger, took place at the margins of the Ordos Basin. At this stage, the western Pacific plate was being subducted westward beneath the eastern Asian continent. The South China Sea opened up during this time, while the Japan Sea began to close. Collision-related uplift of the Tibetan Plateau controlled this deformation within the Chinese continent, including volcanic activity at 24–20 Ma. The stable craton relict comprised the southern part of the North China Basin, the centre of the Ordos Basin and the Shanxi Plateau The Challenges Persist In summary, the lithosphere remained thicker than 150–170 km under most of the NCC, and the lithosphere was thinnest along the northern Taihang Mountain Belt and the Bohai Bay Basin, being less than ~75 km. The total amount of lithospheric thinning was ~120 km, given an original thickness of ~200 km. The processes of destruction of the NCC have been suggested and discussed, but there are still many unknowns: whether cratonic stability was lost in a single event or over time, and whether deformation was overprinted by subsequent thermal events or simply by plate subduction. In addition, it is unclear whether intracontinental deformation resulted from asthenospheric upwelling, continental marginal subduction and collision, or a combination of these processes (Figure 4). Besides, the question of whether a craton that has lost its stability can still be considered a craton, should be reconsidered. References: Wang Yu, Zhou Liyun and Li Jinyi, 2011, Intracontinental superimposed tectonics — A case study in the Western Hills of Beijing, eastern China. Geological Society of America Bulletin, 123, 1033-1055. Wang Yu, Zhou Liyun, Zhao Lijun, 2013, Cratonic reactivation and orogeny: An example from the northern margin of the North China Craton. Gondwana Research, 24，1203-1222. Wang, Y., Zhou, L. Y., Luo, Z. H., 2017, Kinematics and timing of continental block deformation from margins to interiors. Terra Nova, 29, 253-263. Wang, Y., 2025, Intracontinental tectonics and orogeny. Cambridge Scholars Publishing, pp. 435]]></description>
													<content:encoded><![CDATA[The Asian continent has fascinated the world for at least 3,000 years with its music, food, and discoveries, as well as its breathtaking landscapes. Most of these incredible landscapes are formed by mountains that can be considered geologically "recent" (such as the Cenozoic formation of the Himalayas). However, there are also ancient terrains, pre-dating the Mesozoic, that pose intriguing questions for geoscientists. Today, <strong>Professor Yu Wang (<span class="qu yKyxu" role="gridcell"><span class="gD" data-hovercard-id="wangy@cugb.edu.cn" data-hovercard-owner-id="17">王瑜)</span></span></strong> from the Institute of Earth Sciences (Beijing) at the Chinese University of Geosciences (中国地质大学(北京)) will take us on a geological tour through the history of one of these ancient terrains: the North China Craton!

[caption id="attachment_42788" align="alignleft" width="196"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/05/yuwang.png"><img class=" wp-image-42788" src="https://blogs.egu.eu/divisions/gd/files/2026/05/yuwang.png" alt="Professor Yu Wang. Chinese man with rectangular glasses, short black hair and wearing a dark blue shirt." width="196" height="284" /></a> Yu Wang (<span class="qu yKyxu" role="gridcell"><span class="gD" data-hovercard-id="wangy@cugb.edu.cn" data-hovercard-owner-id="17">王瑜</span></span>) is a professor of structural geology, tectonics, and tectonochronology at the Institute of Earth Sciences, China University of Geosciences (Beijing), China. His current research involves intracontinental tectonics and orogens. He completed his PhD in tectonics at the Chinese Academy of Geological Sciences, Beijing, in 1994.[/caption]

This portion of the Chinese landmass is located between the Yangtze Craton (also known as the South China Craton) and the Central Asian Orogenic Belt—a giant tectonic domain—and hosts the Cenozoic basins of China’s northern coast (Figure 1). The formation, evolution, and destruction of the North China Craton (NCC) are highly complex and remain a subject of active debate, as modern geoscience continually brings forward new data and theories regarding the region. Now that we have a brief introduction, let us examine it more closely.
<h1><b>Several proposed models </b></h1>
<span style="font-weight: 400">The lithospheric thinning of the North China Craton (NCC) by ~100–120 km was initially deduced from early Paleozoic kimberlite intrusions (~480 Ma) in eastern China (Figure 1). Therefore, the destruction of the NCC has been attributed to multiple cycles of delamination associated with magmatic ascent, rifting, and extension. Typically, cratonic destruction was considered to have occurred predominantly around 130–120 Ma, resulting from multiple magmatic intrusions and coinciding with the formation of many metamorphic core complexes. Driven by this timeline, different geodynamic hypotheses have been put forward, such as cratonic delamination and the subduction rollback of the paleo-Pacific plate.</span>

<span style="font-weight: 400">Following a comprehensive review of the NCC's tectonic evolution, the current consensus is that the so-called destruction of the craton was actually a long-term evolutionary process in the region. Age data indicate distinct structural and magmatic stages occurring at ~1600–1500, 1300–1100, 445–315, 270–200, 170–155, 130–110, 75–65, and 25–20 Ma. These distinct stages correlate directly with episodes of basin formation, continental uplift, and lithospheric collapse.</span>

[caption id="attachment_42790" align="aligncenter" width="701"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/05/figure-1.jpg"><img class="wp-image-42790 size-large" src="https://blogs.egu.eu/divisions/gd/files/2026/05/figure-1-701x1024.jpg" alt="" width="701" height="1024" /></a> Figure 1: Regional tectonics of northern eastern China (Wang et al., 2011). North China Craton is between the two E-W orogenic belts.[/caption]
<h2>1. Cratonization and Decratonization</h2>
<span style="font-weight: 400">The NCC formed prior to ~1.8–1.9 Ga. Although its oldest Archean rocks date back to 3.8 Ga, the majority of its crustal growth occurred between 2.9 and 2.5 Ga. From 1.8 Ga onwards, subsequent sedimentation covered the entirety of the craton. During the Mesoproterozoic (at ~1.6–1.4 Ga), following the break-up of the Columbia (also known as the Nuna) supercontinent, intense magmatic activity took place, resulting in the formation of a major unconformity along the northern margin of the NCC. Similar tectonic features are observed at the southern margin, evidenced by records of volcanic eruptions dating to ~1.6–1.5 Ga. </span>

<span style="font-weight: 400">From 1,300 to ~445 Ma, the cratonic crust remained relatively stable, as indicated by the shallow marine sediments covering the basement rocks. This earlier stage of marginal rifting and extension can be characterised as a period of 'proto-destruction', serving as a prelude to the craton's later, more severe decratonization.</span>
<h2><b>2. De-rooting of the NCC (~445–315 Ma)</b><b></b></h2>
<b></b><span style="font-weight: 400">A sudden shift in sedimentary sequences during the Late Ordovician reflects a period of significant regional uplift, which persisted until the Middle–Late Carboniferous. Although this uplift event affected the entirety of the NCC, it was most pronounced in the central region, with absolute ages constraining the tectonic activity to between 445 and 315 Ma. </span><span style="font-weight: 400">Stratigraphic and petrological evidence supports this timeline. For instance, early Paleozoic kimberlite intrusions (488–465 Ma) predate the formation of the zircon-bearing bauxites associated with the uplift. Because these kimberlites indicate an intact lithospheric thickness of approximately 200 km during the early Paleozoic, researchers infer that the NCC only became detached from its lithospheric root subsequently (around 480–460 Ma). Over time, the lithosphere thinned by as much as 100 to 120 km. This extensive continental uplift was most likely driven by the craton detaching from its deep root, resulting in a fundamental loss of tectonic stability.</span>
<h2><b>3. Marginal reactivation and subsequent orogeny (~320–200 Ma)</b></h2>
<span style="font-weight: 400">Along the northern and southern margins of the NCC, episodes of deformation and magmatism occurred between ~320 and 200 Ma (Figure 2). Petrology </span><span style="font-weight: 400">suggests</span><span style="font-weight: 400"> that these magmatic rocks originated from the partial melting of pre-existing gneiss and granulite. At the northern margin, E-W trending ductile shear zones accommodated this strain, producing prominent southward-verging inclined and recumbent folds. This indicates that the de-rooting of the craton likely initiated at its margins before progressively migrating towards the cratonic interior.</span>

[caption id="attachment_42793" align="aligncenter" width="1024"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/05/figure-2.jpg"><img class="wp-image-42793 size-large" src="https://blogs.egu.eu/divisions/gd/files/2026/05/figure-2-1024x554.jpg" alt="" width="1024" height="554" /></a> Figure 2: (A) Combined structural–chronological section from north to south portion of NCC. (B) Kinematic features of the Inner Mongolian Orogenic Belt southward to the North China Craton (Wang et al., 2013).[/caption]

<span style="font-weight: 400">Ultimately, these marginal areas lost their inherent cratonic stability and fluid-depleted characteristics. Having shed their cratonic signature, they transitioned entirely into active orogenic belts. Following this stage of marginal reactivation, the stable, rigid core of the North China Craton was significantly reduced in size and continued to progressively shrink over time.</span>
<h2><b>4. Tectonic transformation and complete reactivation (170–155 Ma)</b></h2>
<span style="font-weight: 400">Beginning at ~170–165 Ma, a fundamental transformation of the regional tectonic domain completely reconfigured the eastern Chinese landmass (Figure 3). During this period, the structural regime of the NCC underwent a major kinematic shift, transitioning from an E–W trend to a N-S trend. Correspondingly, the overarching tectonic setting shifted from an association with the Eurasian domain to being governed by the western Pacific plate boundary.</span>

[caption id="attachment_42794" align="aligncenter" width="1024"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/05/Figure-3.jpg"><img class="wp-image-42794 size-large" src="https://blogs.egu.eu/divisions/gd/files/2026/05/Figure-3-1024x523.jpg" alt="" width="1024" height="523" /></a> Summary lithological profile and structural cross-section of the North China Craton during the 180–150 Ma interval (Wang et al., 2017). This section represents an E-W slice of Figure 1 (ENCC: East North China Craton; WNCC: West North China Craton).[/caption]

<span style="font-weight: 400">Deformation during this transitional stage was both intensive and widespread. Lower crustal materials were exhumed to the surface, accompanied by substantial volcanic activity and crust–mantle interaction, predominantly localised within regions undergoing active tectonic transformation. Continued orogenesis at the cratonic margins resulted in a further reduction in the size of the stable cratonic core. Ultimately, under the influence of the western Pacific tectonic setting, the NCC transitioned entirely into an active continental margin</span>
<h2><b>5. Removal of the lithospheric root: the North China cratonic margin (130–110 Ma)</b></h2>
<span style="font-weight: 400">It has been suggested that the main period of destruction of the NCC was at ~130–110 Ma. Studies indicate that deformation, magmatism and basin formation during this period represent strong evidence for the destruction of the North China craton. Between 130 and 110 Ma, de-rooting of the craton had occurred along the northern margin, and likely also the southern margin. Either lithospheric de-rooting must have occurred, or a new lithospheric root must have grown. There is no evidence of regional extensional tectonics at this time. The rollback of the Western Pacific Plate may have been controlled by the extension of a large area of Eastern Asia. The best explanation so far is that mantle extrusion occurred across the entire Eastern Asian continent.</span>
<h2><b>6. Partial removal of continental lithospheric mantle (75–65 Ma)</b></h2>
<span style="font-weight: 400">This stage of deformation only affected the eastern segment of the northern North China Craton, and in the northeast and southeast of eastern China. High-angle normal faults define the boundaries of the eastern part of the NCC, or the boundaries of the North China Basin. At 75–65 Ma, the Taihang Mountain Belt underwent rapid uplift and exhumation, and the eastern China continental margin opened. Since then, the North China continental lithospheric mantle changed as the oceanic lithospheric mantle feature. </span>
<h2><b>7. Deformation and differential mountain uplift (25–20 Ma)</b></h2>
<span style="font-weight: 400">Deformation and volcanic activity during this stage occurred in localised areas, generally along the north of the North China Basin. Basaltic activity occurred along the eastern Asian continental margin and in the interior. Later rifting, up to eight million years younger, took place at the margins of the Ordos Basin. At this stage, the western Pacific plate was being subducted westward beneath the eastern Asian continent. The South China Sea opened up during this time, while the Japan Sea began to close. Collision-related uplift of the Tibetan Plateau controlled this deformation within the Chinese continent, including volcanic activity at 24–20 Ma. The stable craton relict comprised the southern part of the North China Basin, the centre of the Ordos Basin and the Shanxi Plateau</span>
<h1>The Challenges Persist</h1>
<span style="font-weight: 400">In summary, the lithosphere remained thicker than 150–170 km under most of the NCC, and the lithosphere was thinnest along the northern Taihang Mountain Belt and the Bohai Bay Basin, being less than ~75 km. The total amount of lithospheric thinning was ~120 km, given an original thickness of ~200 km. The processes of destruction of the NCC have been suggested and discussed, but there are still many unknowns: whether cratonic stability was lost in a single event or over time, and whether deformation was overprinted by subsequent thermal events or simply by plate subduction. In addition, it is unclear whether intracontinental deformation resulted from asthenospheric upwelling, continental marginal subduction and collision, or a combination of these processes (Figure 4). Besides, the question of whether a craton that has lost its stability can still be considered a craton, should be reconsidered.</span>

[caption id="attachment_42797" align="aligncenter" width="1024"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/05/Figure-4.jpg"><img class="wp-image-42797 size-large" src="https://blogs.egu.eu/divisions/gd/files/2026/05/Figure-4-1024x647.jpg" alt="" width="1024" height="647" /></a> Frameworks and mechanisms at the crust, lithosphere, and mantle levels, based on the case of North China Craton destruction (Wang, 2025). Layered crustal shear, mantle shear, mantle flow, and syn-tectonic magmatic flow from continental margins to interiors are also involved.[/caption]
<pre><b>References:</b>
<span style="font-weight: 400">  Wang Yu, Zhou Liyun and Li Jinyi, 2011, Intracontinental superimposed tectonics — A case study in the Western Hills of Beijing, eastern China. Geological Society of America Bulletin, 123, 1033-1055. </span>
<span style="font-weight: 400">  Wang Yu, Zhou Liyun, Zhao Lijun, 2013, Cratonic reactivation and orogeny: An example from the northern margin of the North China Craton. Gondwana Research, 24，1203-1222.</span>
<span style="font-weight: 400">  Wang, Y., Zhou, L. Y., Luo, Z. H., 2017, Kinematics and timing of continental block deformation from margins to interiors. Terra Nova, 29, 253-263.</span>
<span style="font-weight: 400">  Wang, Y., 2025, Intracontinental tectonics and orogeny. Cambridge Scholars Publishing, pp. 435</span></pre>]]></content:encoded>
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					<title><![CDATA[Knowing better, but still losing more: why disaster risk reduction breaks down]]></title>
					<link>https://blogs.egu.eu/divisions/nh/2026/05/11/knowing-better-but-still-losing-more-why-disaster-risk-reduction-breaks-down/</link>
					<comments>https://blogs.egu.eu/divisions/nh/2026/05/11/knowing-better-but-still-losing-more-why-disaster-risk-reduction-breaks-down/#comments</comments>
					<pubDate>Mon, 11 May 2026 08:00:14 +0000</pubDate>
					<dc:creator><![CDATA[hediehsoltanpour]]></dc:creator>
							<category><![CDATA[Disaster Risk Reduction]]></category>
		<category><![CDATA[EGU Natural Hazards Division]]></category>
		<category><![CDATA[Non Climatic Risk Drivers]]></category>
		<category><![CDATA[#DRR]]></category>
		<category><![CDATA[#naturalhazards]]></category>
		<category><![CDATA[disaster risk reduction]]></category>
		<category><![CDATA[NonClimaticRiskDrivers #NaturalHazards #Adaptation #EGUblogs]]></category>
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											<description><![CDATA[The surviving house in Pacific Palisades became one of the most discussed images from the 2025 California wildfires (Fig. 1). What makes it scientifically interesting, though, is not that it survived. It is that many of the features associated with the house’s survival – a more fire-resistant exterior, stronger windows, and details that reduce ember entry – are already well known. This case points to a broader problem explored in our paper: disaster losses remain high, not simply because knowledge is missing, but because existing knowledge is still not consistently implemented in planning, building practice, and policy. This issue sits at the heart of our recent Invited Perspective in Natural Hazards and Earth System Sciences. Using the 2025 California wildfires as a starting point, we argue that the problem is often not a lack of scientific or technical knowledge. In many cases, the necessary knowledge and solutions already exist. What fails, however, is the translation of that knowledge into land-use planning, building practice, public communication, and policy. Disaster risk reduction is not only a technical challenge but also a social, institutional, and political one. In the paper, we identify four key failures that undermine the effectiveness of disaster risk reduction: limited awareness, limited capacities, weak incentives, and governance barriers. These failures are interconnected. They interact and reinforce one another (Fig. 2), making it harder to reduce future losses before the next event. &nbsp; Key failure 1: limited awareness Living with risk does not automatically mean high risk awareness. Hazard information may well exist, but it is not always easy to understand, reliable, or straightforward to act upon. During the 2025 California wildfires, limits in risk communication, evacuation guidance, and access to hazard information constrained people’s ability to interpret what was happening and respond in time. More broadly, awareness is shaped by familiar human tendencies: underestimating future danger, focusing on immediate costs, or assuming that someone else will take responsibility. Key failure 2: capacity deficits Even when risk awareness in society is high, a lack of money, time, technical knowledge, or institutional support can undermine preparedness. This is evident at different scales: from single households to local authorities and organisations. Rules and standards may exist on paper, but they still require staff, expertise, coordination, and funding to be sufficiently implemented. In wildfire-prone areas, this challenge is especially clear: responsibility often falls to local governments and residents, even though their capacity to act is uneven. Voluntary programmes can help, but they also implicitly shift responsibility for risk reduction onto individuals by often assuming that households already have the resources needed to respond. Key failure 3: lack of incentives Knowledge of appropriate preparedness, response and recovery actions does not necessarily translate into action. In California, rebuilding after wildfire often takes place in the same risky places instead of encouraging settlement and development away from hazardous areas. Recovery systems frequently support rapid reconstruction more than long-term risk reduction. That means the easiest path is often to rebuild exposure rather than reduce it. The paper points to evidence showing that rebuilding in place remains common after destructive fires, with little shift toward lower-risk locations. Key failure 4: inadequate governance Responsibilities are often fragmented across several actors such as agencies, levels of government, and sectors. As a result, coordination becomes difficult and accountability unclear. In the case of California, wildfire suppression and emergency response operate within a complex multi-level system, while land-use planning and building practice depend heavily on state and local authorities. The result is a fragmented landscape in which prevention can easily fall between institutions. The paper also points out that some proposed wildfire safety regulations in California had stalled in bureaucratic processes, even after years of discussion. Crucially, these four failures are not isolated from one another – they interact in ways that reinforce and intensify each other, creating a cycle that perpetuates disaster losses. Limited awareness weakens public demand for change. Limited capacity means even good intentions may not be translated into action. Weak incentives can encourage rebuilding in risky places. Governance barriers can delay or dilute action. Together, they constrain the ability of institutions and communities to reduce risk in a sustainable way. In our paper, we show these challenges as a connected system: these linked barriers contribute to continued exposure, poor adaptation choices, and socially unequal outcomes. Therefore, our perspective goes beyond wildfire. Although the California fires provide the entry point, the same pattern appears across many hazards and contexts. The 2023 Turkey–Syria earthquakes, the 2024 Valencia flood, and the 2025 Texas floods all show versions of the same broader problem: existing risk knowledge not translated effectively into action. Across these cases, failures in communication, weak enforcement, fragmented responsibilities, and limited institutional capacity shaped the severity of impacts. This broader perspective is crucial because it reshapes how we think about solutions.If disasters were mainly a problem of weak scientific capacities, lack of technology and missing knowledge, the answer would simply be more research. Research remains essential, of course, but it is not enough. The greater challenge is making risk reduction work in the real world, under real political pressures, unequal resources, and competing priorities. That means improving not only scientific understanding, but also the ways that knowledge is communicated, funded, regulated, and embedded into everyday decisions. Moreover, we have to acknowledge that disaster losses are deeply shaped by inequality. Risk is not shared evenly, and neither is the ability to prepare, recover, or relocate. When adaptation depends heavily on private resources, some people can protect themselves more easily than others. When rebuilding is encouraged without changing the underlying conditions of exposure, future losses remain locked in. Disaster risk reduction is therefore not only about safety. It is also about equity. So what lesson should we draw from the surviving house in Pacific Palisades? Surely not that solely risk-aware building design can solve the problem. Nor is that people simply need better technical advice. The real lesson is broader and demands immediate action. Knowledge to reduce hazard impacts is available. However, unless societies address awareness, capacity, incentives, and governance together, that knowledge will continue to be applied unevenly and ineffectively. When that happens, disaster losses remain high not because risk cannot be reduced, but because risk reduction breaks down between science and action. In that sense, the challenge is not only to know better but to act better, together. Reference (s) [1] Fuchs, S., Karagiorgos, K., Keiler, M., Nyberg, L., Papathoma-Köhle, M., and Polderman, A.: Four reasons DRR does not work as intended – lessons from the 2025 California wildfires and beyond, Natural Hazards and Earth System Sciences, 26, 1785-1794, https://doi.org/10.5194/nhess-26-1785-2026, 2026. Post edited by: Hedieh Soltanpour and Navakanesh M Batmanathan ]]></description>
													<content:encoded><![CDATA[<span style="font-weight: 400">The surviving house in Pacific Palisades became one of the most discussed images from the 2025 California wildfires (Fig. 1). What makes it scientifically interesting, though, is not that it survived. It is that many of the </span><a href="https://doi.org/10.1038/s41598-022-10479-3"><span style="font-weight: 400">features associated with the house’s survival</span></a><span style="font-weight: 400"> – a more fire-resistant exterior, stronger windows, and details that reduce ember entry – are already well known. This case points to a broader problem explored in our </span><a href="https://doi.org/10.5194/nhess-26-1785-2026"><span style="font-weight: 400">paper</span></a><span style="font-weight: 400">: disaster losses remain high, not simply because knowledge is missing, but because existing knowledge is still not consistently implemented in planning, building practice, and policy.</span>

[caption id="attachment_11055" align="aligncenter" width="499"]<img class="wp-image-11055" src="https://blogs.egu.eu/divisions/nh/files/2026/05/Fig_1-300x200.png" alt="" width="499" height="333" /> Figure 1. A house in Pacific Palisades that survived the 2025 wildfire events. Its design included a fire-resistant exterior, heat-resistant windows, sealed openings, and details intended to reduce ember entry and debris build-up. The point is not that the house was “miraculous”, but that many of the protective principles were already known. Image credit the authors based on a Google Street View scene (02/2025)[/caption]

<span style="font-weight: 400">This issue sits at the heart of our recent Invited Perspective in</span> <a href="https://doi.org/10.5194/nhess-26-1785-2026"><i><span style="font-weight: 400">Natural Hazards and Earth System Sciences</span></i></a><span style="font-weight: 400">. Using the 2025 California wildfires as a starting point, we argue that the problem is often not a lack of scientific or technical knowledge. In many cases, </span><span style="font-weight: 400">the</span><a href="https://www.nfpa.org/Education-and-Research/Wildfire/Firewise-USA"> <span style="font-weight: 400">necessary knowledge and solutions already exist</span></a><span style="font-weight: 400">. </span><span style="font-weight: 400">What fails, however, is the translation of that knowledge into land-use planning, building practice, public communication, and policy. Disaster risk reduction is not only a technical challenge but also a social, institutional, and political one. In the paper, we identify four key failures that undermine the effectiveness of disaster risk reduction: limited awareness, limited capacities, weak incentives, and governance barriers. These failures are interconnected. They interact and reinforce one another (Fig. 2), making it harder to reduce future losses before the next event.</span>

&nbsp;
<h2><strong>Key failure 1: limited awareness</strong></h2>
<span style="font-weight: 400">Living with risk does not automatically mean high risk awareness. Hazard information may well exist, but it is not always easy to understand, reliable, or straightforward to act upon. During the 2025 California wildfires, limits in risk communication, evacuation guidance, and access to hazard information constrained people’s ability to interpret what was happening and respond in time. More broadly, awareness is shaped by familiar human tendencies: underestimating future danger, focusing on immediate costs, or assuming that someone else will take responsibility.</span>
<h2><strong>Key failure 2: capacity deficits</strong></h2>
<span style="font-weight: 400">Even when risk awareness in society is high, a lack of money, time, technical knowledge, or institutional support can undermine preparedness. This is evident at different scales: from single households to local authorities and organisations. Rules and standards may exist on paper, but they still require staff, expertise, coordination, and funding to be sufficiently implemented. In wildfire-prone areas, this challenge is especially clear: responsibility often falls to local governments and residents, even though their capacity to act is uneven. Voluntary programmes can help, but they also implicitly shift responsibility for risk reduction onto individuals by often assuming that households already have the resources needed to respond.</span>
<h2><strong>Key failure 3: lack of incentives</strong></h2>
<span style="font-weight: 400">Knowledge of appropriate preparedness, response and recovery actions does not necessarily translate into action. In California, rebuilding after wildfire often takes place in the same risky places instead of encouraging settlement and development away from hazardous areas. Recovery systems frequently support rapid reconstruction more than long-term risk reduction. That means the easiest path is often to rebuild exposure rather than reduce it. The paper points to evidence showing that rebuilding in place remains common after destructive fires, with little shift toward lower-risk locations.</span>
<h2><strong>Key failure 4: inadequate governance</strong></h2>
<span style="font-weight: 400">Responsibilities are often fragmented across several actors such as agencies, levels of government, and sectors. As a result, coordination becomes difficult and accountability unclear. In the case of California, wildfire suppression and emergency response operate within a complex multi-level system, while land-use planning and building practice depend heavily on state and local authorities. The result is a fragmented landscape in which prevention can easily fall between institutions. The paper also points out that some proposed wildfire safety regulations in California had stalled in bureaucratic processes, even after years of discussion.</span>

<span style="font-weight: 400">Crucially, these four failures are not isolated from one another – they interact in ways that reinforce and intensify each other, creating a cycle that perpetuates disaster losses. Limited awareness weakens public demand for change. Limited capacity means even good intentions may not be translated into action. Weak incentives can </span><a href="https://doi.org/10.1016/j.landusepol.2021.105502"><span style="font-weight: 400">encourage rebuilding</span></a><span style="font-weight: 400"> in risky places</span><span style="font-weight: 400">. Governance barriers can delay or dilute action. Together, they constrain the ability of institutions and communities to reduce risk in a sustainable way. In our paper, we show these challenges as a connected system: these linked barriers contribute to continued exposure, poor adaptation choices, and socially unequal outcomes.</span>

<span style="font-weight: 400">Therefore, our perspective goes beyond wildfire. Although the California fires provide the entry point, the same pattern appears across many hazards and contexts. The 2023 Turkey–Syria earthquakes, the 2024 Valencia flood, and the 2025 Texas floods all show versions of the same broader problem: existing risk knowledge not translated effectively into action. Across these cases, failures in communication, weak enforcement, fragmented responsibilities, and limited institutional capacity shaped the severity of impacts.</span>

<span style="font-weight: 400">This broader perspective is crucial because it reshapes how we think about solutions.If disasters were mainly a problem of weak scientific capacities, lack of technology and missing knowledge, the answer would simply be more research. Research remains essential, of course, but it is not enough. The greater challenge is making risk reduction work in the real world, under real political pressures, unequal resources, and competing priorities. That means improving not only scientific understanding, but also the ways that knowledge is communicated, funded, regulated, and embedded into everyday decisions.</span>

<span style="font-weight: 400">Moreover, we have to acknowledge that disaster losses are deeply shaped by inequality. Risk is not shared evenly, and neither is the ability to prepare, recover, or relocate. When adaptation depends heavily on private resources, some people can protect themselves more easily than others. When rebuilding is encouraged without changing the underlying conditions of exposure, future losses remain locked in. Disaster risk reduction is therefore not only about safety. It is also about equity.</span>

<span style="font-weight: 400">So what lesson should we draw from the surviving house in Pacific Palisades?</span>

<span style="font-weight: 400">Surely not that solely risk-aware building design can solve the problem. Nor is that people simply need better technical advice. The real lesson is broader and demands immediate action. Knowledge to reduce hazard impacts is available. However, unless societies address awareness, capacity, incentives, and governance together, that knowledge will continue to be applied unevenly and ineffectively. When that happens, disaster losses remain high not because risk cannot be reduced, but because risk reduction breaks down between science and action.</span>

<span style="font-weight: 400">In that sense, the challenge is not only to know better but to act better, together.</span>
<h2><strong>Reference (s)</strong></h2>
<span style="font-weight: 400">[1] </span><span style="font-weight: 400">Fuchs, S., Karagiorgos, K., Keiler, M., Nyberg, L., Papathoma-Köhle, M., and Polderman, A.: Four reasons DRR does not work as intended – lessons from the 2025 California wildfires and beyond, Natural Hazards and Earth System Sciences, 26, 1785-1794, https://doi.org/10.5194/nhess-26-1785-2026, 2026.</span>

Post edited by: <em>Hedieh Soltanpour and Navakanesh M Batmanathan </em>]]></content:encoded>
																<wfw:commentRss>https://blogs.egu.eu/divisions/nh/2026/05/11/knowing-better-but-still-losing-more-why-disaster-risk-reduction-breaks-down/feed/</wfw:commentRss>
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					<title><![CDATA[EGU26 Friday Highlights]]></title>
					<link>https://blogs.egu.eu/divisions/gmpv/2026/05/08/egu26-friday-highlights/</link>
					<comments>https://blogs.egu.eu/divisions/gmpv/2026/05/08/egu26-friday-highlights/#comments</comments>
					<pubDate>Fri, 08 May 2026 03:00:13 +0000</pubDate>
					<dc:creator><![CDATA[PIYAL HALDER]]></dc:creator>
							<category><![CDATA[EGU]]></category>
		<category><![CDATA[EGU GMPV]]></category>
		<category><![CDATA[Uncategorized]]></category>
		<category><![CDATA[EGU26]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Hey folks, Today is the last day of the EGU26. Let&#8217;s have a quick look at today&#8217;s GMPV sessions- Session Code Time &amp; Place Session Title Convenor &amp; Co-Convenors Session Overview GMPV4.3 Oral: 08:30–12:30 Room: K1 What Makes Earth So Special: Global Cycles of Volatiles Convener: Alessia Borghini; Co-conveners: Carla Tiraboschi, Sally Gibson, Michał Bukała The Session will particularly focus on- (i) deep volatile cycles of H₂O, CO₂, halogens and sulphur; (ii) volatile mobilisation and transfer during subduction in COHNS fluids and silicate melts; (iii) roles of volatiles in metamorphic and metasomatic processes; (iv) physical and chemical properties of volatiles in melts and fluids; (v) volatile storage in the lithospheric mantle; (vi) emissions and reservoirs in volcanic systems. GMPV8.2 Oral: 08:30–10:10 Room: 0.96/97 From Earth to Exoplanets: Exploring deep planetary interiors through advances in modelling and experiments Convener: Lélia Libon Co-conveners: Amrita Chakraborti, Renaud Deguen, Clemens Prescher The session will enlighten on- (i) understanding of materials and processes under extreme conditions; (ii) mineral physics properties, interior structure and dynamics, and the chemical and physical evolution of Earth and exoplanets; (iii) novel experimental techniques, innovative synchrotron and FEL approaches, and cutting-edge modelling methods to reveal the complex interplay of chemistry, physics, and dynamics within Earth and planetary interiors. GMPV10.9  Oral: 10:45–12:20 Room: 0.96/97 Poster: 14:00–15:45 Hall X2 &nbsp; Tectonic, eruptive and geomorphological processes in volcanic areas The Session will deal with- (i) multidisciplinary approaches, including field studies, remote sensing, geophysical methods and laboratory analyses, to capture the complexities of volcanic systems throughout their lifecycle. (ii) influence of the volcanotectonic processes on volcanic landform evolution and its implications for hazard assessment and risk reduction. &nbsp; GMPV2.1 Oral: 14:00–15:45 Room: K1 Solving geoscience problems using mineralogy and mineral’s inclusions Convener: Jannick Ingrin Co-conveners: Lea Pennacchioni, Mara Murri, Stylianos Aspiotis, Marta Berkesi   &nbsp; The session will address- (i) issues that involve the use and development of spectroscopic techniques; (ii) the relevant ab initio simulations beyond current applications in metamorphic and magmatic petrology applied to the Earth and other planetary bodies. GMPV3.1  Oral: 6:15–18:00 &nbsp; Understanding fluid-rock interactions of ultramafic rocks for CO2 mineralization, natural H2 resources and critical element mobility Convener: Manuel Menzel Co-conveners: Katrin Steinthorsdottir, Frank Zwaan, Francesco Giuntoli &nbsp; &nbsp; The session will focus on advancement of the understanding of the conditions, mechanisms and rates of CO2 mineralization, H2 generation and element mobility during fluid-rock interactions in peridotites and serpentinites from microscopic to industrial and tectonic scales, including studies of natural analogues, field surveys, pilot injection sites, laboratory experiments and theoretical simulations. &nbsp; GD4.2 Oral: 8:30–10:10 Room: 2.93 &nbsp; Unveiling Earth&#8217;s critical resources: Advances in numerical modelling and inversion in support of the energy transition &nbsp; Convener: Andrew Valentine Co-conveners: Alberto García González, Macarena Amaya The session will focus on- (i) the computational and methodological developments necessary for progress towards more sustainable energy; &nbsp; (ii) a diverse range of topics &#8212; including simulation, e.g. of thermo-chemical flow processes, subsurface imaging, data fusion and AI &#8212; with their application to critical resources as a unifying theme. GI2.1 Oral: 08:30–12:30 Room: 2.62 Poster: 14:00–15:45 Hall X4 &nbsp; Artificial Intelligence in Geosciences: applications, innovative approaches and new frontiers Convener: Andrea Vitale Co-conveners: Luigi Bianco, Ivana Ventola, Giacomo Roncoroni &nbsp; By leveraging algorithms and machine learning, AI empowers geoscientists to uncover intricate patterns and relationships within complex data sources, ultimately advancing our understanding of the Earth&#8217;s dynamic systems. In essence, artificial intelligence has become an indispensable tool for achieving quantitative precision and deeper insights in the fascinating world of geosciences. Poster-only Sessions: Session Code Time &amp; Place Session Title Convenor &amp; Co-Convenors Session Overview GMPV10.4 10:45–12:30 Hall X2 &nbsp; Understanding magmatic plumbing systems via multidisciplinary approaches: from petrology and geochemistry to remote sensing, geophysics and modelling Convener: Martin Oeser Co-conveners: Felix Marxer, Uddalak Biswas, Ségolène Rabin, Daniele Maestrelli, Benjamin Klein, Domenico Montanari &nbsp; This session aims to investigate the multitude of key processes operating in magmatic systems at all scales, from source to surface, including: magma generation and transport, mixing, storage, and the resulting deformation; mineral–melt–fluid reactions and fractionation; and kinetic and equilibrium elemental and isotopic exchange. GMPV10.10 10:45–12:30 Hall X2 Mud Volcanoes as Natural Laboratories: Dynamics, Monitoring, and Impacts on the Environment and Society Convener: Paola Cusano Co-conveners: Alessandra Sciarra, Simona Petrosino, Mariarosaria Falanga, Enza De Lauro This session will address- (i) the reconstruction of the deep engine dynamics of MV activity and their stratigraphic structure; (ii) the processes that form mud volcanoes and drive material migration to the surface; (iii) the hydrological regime and its influence on MV activity; (iv) outcomes from long-term monitoring and spot surveys; (v) the interplay between the regional/local seismicity and MV activity, as manifestation of crustal dynamics; (vi) the remote sensing, terrain and surface modelling, and geophysical imaging; (vii) the impact of MVs&#8217; activity on ecosystems and climate. (viii) Multidisciplinary approaches to the MVs study, aimed at identifying reliable indicators of their activity state, are welcome. GMPV11.3 10:45–12:30 Hall X2 &nbsp; Volcano Seismology and Acoustics Convener: Miriam Christina Reiss; Co-conveners: Anna Perttu, Corentin Caudron, Ivan Lokmer, Chris Bean &nbsp; The Session will focus on- (i) seismicity and infrasound catalogues and their spatio-temporal evolution, (ii) wave propagation, scattering, and atmospheric effects, (iii) high-resolution imaging of volcanic structures, (iv) joint seismic–acoustic source inversions, and (v) time-lapse monitoring and forecasting. Studies on geothermal analogues, novel instrumentation, and emerging analysis methodologies (e.g., machine learning). GMPV11.5 10:45–12:30 Hall X2 &nbsp; Volcanic Eruptions and Climate: Observations, Modeling, and Impacts Convener: Vito Zago; Co-conveners: Eleonora Amato, Federica Torrisi, Ciro Del Negro &nbsp; This session will focus on how volcanic processes influence the climate system and thus deal with- (i)  forward-looking strategies that combine multi-source data, real-time monitoring, and advanced modeling—including hybrid and data-driven approaches—to enhance ability to monitor, interpret, and anticipate the climate impacts of volcanic activity. (ii) Integration of satellite, in situ, and paleo records with physical models and computational techniques. (iii) Detection of anomalies, identifying patterns, and quantifying both short- and long-term effects. (iv) Case studies of recent or historical major eruptions and the use of innovative analytical or simulation methods. &nbsp; SM6.4 Advances in Seismic Attenuation, Scattering, and Absorption Convener: Mirko Bracale Co-conveners: Lian Feng Zhao, Simona Gabrielli, Miriam Christina Reiss, Luca De Siena The session will deal with- (i) Theoretical advancements that improve understanding of attenuation processes, including scattering and intrinsic absorption; (ii) Resolve Earth’s internal structure through analysis of attenuation data; (iii) Numerical simulations of the relevant equations for seismic wave propagation in heterogeneous media and attenuation; (iv) Applications to the study and characterization of seismic sources; (v) Attenuation studies in seismic hazard and damage assessment, including ground motion models and the effects of shaking on structures and infrastructure; (vi) Energy dispersion from geological heterogeneities, such as faults, fractures, and variations in rock properties; (vii) Attenuation as an indicator of energy conversion into heat, with applications to geothermal exploration and volcanic hazard assessment; (viii) Tomographic imaging that integrates attenuation, scattering, and absorption to investigate Earth’s structure from crust to core; (ix) Planetary science investigations that use seismic attenuation to probe the internal structure and dynamics of other planetary bodies. SM6.4 Advances in Seismic Attenuation, Scattering, and Absorption Convener: Mirko Bracale Co-conveners: Lian Feng Zhao, Simona Gabrielli, Miriam Christina Reiss, Luca De Siena The session will deal with- (i) Theoretical advancements that improve understanding of attenuation processes, including scattering and intrinsic absorption; (ii) Resolve Earth’s internal structure through analysis of attenuation data; (iii) Numerical simulations of the relevant equations for seismic wave propagation in heterogeneous media and attenuation; (iv) Applications to the study and characterization of seismic sources; (v) Attenuation studies in seismic hazard and damage assessment, including ground motion models and the effects of shaking on structures and infrastructure; (vi) Energy dispersion from geological heterogeneities, such as faults, fractures, and variations in rock properties; (vii) Attenuation as an indicator of energy conversion into heat, with applications to geothermal exploration and volcanic hazard assessment; (viii) Tomographic imaging that integrates attenuation, scattering, and absorption to investigate Earth’s structure from crust to core; (ix) Planetary science investigations that use seismic attenuation to probe the internal structure and dynamics of other planetary bodies. PICO Sessions: Session Code Time &amp; Place Session Title Convenor &amp; Co-Co nvenors Session Overview  GD1.3 08:30–10:15 PICO spot 2 &nbsp; Geochemical and geodynamic perspectives on the origin and evolution of deep-seated mantle melts and their interaction with the lithosphere Convener: Igor Ashchepkov Co-conveners: Sonja Aulbach, Natalia Lebedeva, Rohit Pandey &nbsp; The session will deal with- (i) Reconstructions of the structure and composition of the lithospheric mantle, and the influence of plumes and subduction zones on root construction; (ii) Interactions of plume- and subduction-derived melts and fluids with the continental lithosphere, and the nature and development of metasomatic agents; (iii) Source rocks, formation conditions (P-T-fO2) and evolution of mantle melts originating below or in the mantle lithosphere; (iv) Deep source regions, melting processes and phase transformation in mantle plumes and their fluids; (v) Modes of melt migration and ascent, as constrained from numerical modelling and microstructures of natural mantle samples; (vi) Role of mantle melts and fluids in the generation of hybrid and acid magmas. &nbsp; Keep in touch with EGU GMPV&#8230;..See you next year&#8230;..]]></description>
													<content:encoded><![CDATA[Hey folks,

Today is the last day of the EGU26.

Let's have a quick look at today's GMPV sessions-
<table style="height: 1642px" width="747">
<tbody>
<tr>
<td width="121">
<h3 style="text-align: center"><strong>Session Code</strong></h3>
<h3 style="text-align: center"><strong>Time &amp; Place</strong></h3>
</td>
<td style="text-align: center" width="224">
<h3><strong>Session Title</strong></h3>
<h3><strong>Convenor </strong><strong>&amp; </strong><strong>Co-Convenors</strong></h3>
</td>
<td width="278">
<h3 style="text-align: center"><strong>Session Overview</strong></h3>
</td>
</tr>
<tr>
<td width="121">
<p style="text-align: left"><a href="https://www.egu26.eu/pg/GMPV_080526">GMPV4.3</a></p>
<p style="text-align: left"><strong>O</strong><strong>ral: </strong>08:30–12:30</p>
<p style="text-align: left"><strong>Room: </strong>K1</p>
<p style="text-align: left"></p>
</td>
<td style="text-align: left" width="224">What Makes Earth So Special: Global Cycles of Volatiles

<strong>Convener:</strong> Alessia Borghini;

<strong>Co-conveners:</strong> Carla Tiraboschi, Sally Gibson, Michał Bukała</td>
<td width="278">
<p style="text-align: left">The Session will particularly focus on-</p>
<p style="text-align: left">(i) deep volatile cycles of H₂O, CO₂, halogens and sulphur;</p>
<p style="text-align: left">(ii) volatile mobilisation and transfer during subduction in COHNS fluids and silicate melts;</p>
<p style="text-align: left">(iii) roles of volatiles in metamorphic and metasomatic processes;</p>
<p style="text-align: left">(iv) physical and chemical properties of volatiles in melts and fluids;</p>
<p style="text-align: left">(v) volatile storage in the lithospheric mantle;</p>
<p style="text-align: left">(vi) emissions and reservoirs in volcanic systems.</p>
</td>
</tr>
<tr>
<td width="121"><a href="https://www.egu26.eu/pg/GMPV_080526">GMPV8.2</a>

<strong>O</strong><strong>ral: </strong>08:30–10:10

<strong>Room: </strong>0.96/97</td>
<td width="224">From Earth to Exoplanets: Exploring deep planetary interiors through advances in modelling and experiments

<strong>Convener: </strong>Lélia Libon

<strong>Co-conveners:</strong>

Amrita Chakraborti, Renaud Deguen, Clemens Prescher</td>
<td width="278">The session will enlighten on-

(i) understanding of materials and processes under extreme conditions;

(ii) mineral physics properties, interior structure and dynamics, and the chemical and physical evolution of Earth and exoplanets;

(iii) novel experimental techniques, innovative synchrotron and FEL approaches, and cutting-edge modelling methods to reveal the complex interplay of chemistry, physics, and dynamics within Earth and planetary interiors.</td>
</tr>
<tr>
<td width="121"><a href="https://www.egu26.eu/pg/GMPV_080526">GMPV10.9  </a>

<strong>Oral: </strong>10:45–12:20

<strong>Room: </strong>0.96/97

<strong>Poster: </strong>14:00–15:45

Hall X2

&nbsp;</td>
<td width="224">Tectonic, eruptive and geomorphological processes in volcanic areas</td>
<td width="278">The Session will deal with-

(i) multidisciplinary approaches, including field studies, remote sensing, geophysical methods and laboratory analyses, to capture the complexities of volcanic systems throughout their lifecycle.

(ii) influence of the volcanotectonic processes on volcanic landform evolution and its implications for hazard assessment and risk reduction.

&nbsp;</td>
</tr>
</tbody>
</table>
<table style="height: 1491px" width="749">
<tbody>
<tr>
<td width="121"><a href="https://www.egu26.eu/pg/GMPV_080526">GMPV2.1</a>

<strong>O</strong><strong>ral: </strong>14:00–15:45

<strong>Room:</strong> K1</td>
<td width="224">Solving geoscience problems using mineralogy and mineral’s inclusions

<strong>Convener:</strong> Jannick Ingrin

<strong>Co-conveners:</strong> Lea Pennacchioni, Mara Murri, Stylianos Aspiotis, Marta Berkesi

<strong> </strong>

&nbsp;</td>
<td width="278">The session will address-

(i) issues that involve the use and development of spectroscopic techniques;

(ii) the relevant ab initio simulations beyond current applications in metamorphic and magmatic petrology applied to the Earth and other planetary bodies.</td>
</tr>
<tr>
<td width="121"><a href="https://www.egu26.eu/pg/GMPV_080526">GMPV3.1 </a>

<strong>Oral: </strong>6:15–18:00

&nbsp;</td>
<td width="224">Understanding fluid-rock interactions of ultramafic rocks for CO<sub>2</sub> mineralization, natural H<sub>2</sub> resources and critical element mobility

<strong>Convener:</strong> Manuel Menzel

<strong>Co-conveners: </strong>Katrin Steinthorsdottir, Frank Zwaan, Francesco Giuntoli

&nbsp;

&nbsp;</td>
<td width="278">The session will focus on advancement of the understanding of the conditions, mechanisms and rates of CO<sub>2 </sub>mineralization, H<sub>2</sub> generation and element mobility during fluid-rock interactions in peridotites and serpentinites from microscopic to industrial and tectonic scales, including studies of natural analogues, field surveys, pilot injection sites, laboratory experiments and theoretical simulations.

&nbsp;</td>
</tr>
<tr>
<td width="121"><a href="https://www.egu26.eu/pg/GMPV_080526">GD4.2</a>

<strong>Oral: </strong>8:30–10:10

<strong>Room:</strong> 2.93

&nbsp;</td>
<td width="224">Unveiling Earth's critical resources: Advances in numerical modelling and inversion in support of the energy transition

&nbsp;

<strong>Convener:</strong> Andrew Valentine

<strong>Co-conveners:</strong> Alberto García González, Macarena Amaya</td>
<td width="278">The session will focus on-

(i) the computational and methodological developments necessary for progress towards more sustainable energy;

&nbsp;

(ii) a diverse range of topics -- including simulation, e.g. of thermo-chemical flow processes, subsurface imaging, data fusion and AI -- with their application to critical resources as a unifying theme.</td>
</tr>
<tr>
<td width="121"><a href="https://www.egu26.eu/pg/GMPV_080526">GI2.1</a>

<strong>Oral: </strong>08:30–12:30

<strong>Room:</strong> 2.62

<strong>Poster: </strong>14:00–15:45

Hall X4

&nbsp;</td>
<td width="224">Artificial Intelligence in Geosciences: applications, innovative approaches and new frontiers

<strong>Convener:</strong> Andrea Vitale

<strong>Co-conveners:</strong> Luigi Bianco, Ivana Ventola, Giacomo Roncoroni

&nbsp;</td>
<td width="278">By leveraging algorithms and machine learning, AI empowers geoscientists to uncover intricate patterns and relationships within complex data sources, ultimately advancing our understanding of the Earth's dynamic systems. In essence, artificial intelligence has become an indispensable tool for achieving quantitative precision and deeper insights in the fascinating world of geosciences.</td>
</tr>
</tbody>
</table>
<h2><strong>Poster-only Sessions:</strong></h2>
<table style="height: 3642px" width="751">
<tbody>
<tr>
<td width="97">
<h3 style="text-align: center"><strong>Session Code</strong></h3>
<h3 style="text-align: center"><strong>Time &amp; Place</strong></h3>
</td>
<td style="text-align: center" width="225">
<h3><strong>Session Title</strong></h3>
<h3><strong>Convenor</strong></h3>
<h3><strong>&amp;</strong></h3>
<h3><strong>Co-Convenors</strong></h3>
</td>
<td width="298">
<h3 style="text-align: center"><strong>Session Overview</strong></h3>
</td>
</tr>
<tr>
<td width="97"><a href="https://www.egu26.eu/pg/GMPV_080526">GMPV10.4</a>

10:45–12:30

Hall X2

&nbsp;</td>
<td width="225">Understanding magmatic plumbing systems via multidisciplinary approaches: from petrology and geochemistry to remote sensing, geophysics and modelling

<strong>Convener: </strong>Martin Oeser

<strong>Co-conveners:</strong> Felix Marxer, Uddalak Biswas, Ségolène Rabin, Daniele Maestrelli, Benjamin Klein, Domenico Montanari

&nbsp;</td>
<td width="298">This session aims to investigate the multitude of key processes operating in magmatic systems at all scales, from source to surface, including: magma generation and transport, mixing, storage, and the resulting deformation; mineral–melt–fluid reactions and fractionation; and kinetic and equilibrium elemental and isotopic exchange.</td>
</tr>
<tr>
<td width="97"><a href="https://www.egu26.eu/pg/GMPV_080526">GMPV10.10</a>

10:45–12:30

Hall X2</td>
<td width="225">Mud Volcanoes as Natural Laboratories: Dynamics, Monitoring, and Impacts on the Environment and Society

<strong>Convener: </strong>Paola Cusano

<strong>Co-conveners: </strong>Alessandra Sciarra, Simona Petrosino, Mariarosaria Falanga, Enza De Lauro</td>
<td width="298">This session will address-

(i) the reconstruction of the deep engine dynamics of MV activity and their stratigraphic structure;

(ii) the processes that form mud volcanoes and drive material migration to the surface;

(iii) the hydrological regime and its influence on MV activity;

(iv) outcomes from long-term monitoring and spot surveys;

(v) the interplay between the regional/local seismicity and MV activity, as manifestation of crustal dynamics;

(vi) the remote sensing, terrain and surface modelling, and geophysical imaging;

(vii) the impact of MVs' activity on ecosystems and climate.

(viii) Multidisciplinary approaches to the MVs study, aimed at identifying reliable indicators of their activity state, are welcome.</td>
</tr>
<tr>
<td width="97"><a href="https://www.egu26.eu/pg/GMPV_080526">GMPV11.3</a>

10:45–12:30

Hall X2

&nbsp;</td>
<td width="225">Volcano Seismology and Acoustics

<strong>Convener: </strong>Miriam Christina Reiss;

<strong>Co-conveners:</strong> Anna Perttu, Corentin Caudron, Ivan Lokmer, Chris Bean

&nbsp;</td>
<td width="298">The Session will focus on-

(i) seismicity and infrasound catalogues and their spatio-temporal evolution,

(ii) wave propagation, scattering, and atmospheric effects,

(iii) high-resolution imaging of volcanic structures,

(iv) joint seismic–acoustic source inversions, and

(v) time-lapse monitoring and forecasting. Studies on geothermal analogues, novel instrumentation, and emerging analysis methodologies (e.g., machine learning).</td>
</tr>
<tr>
<td width="97"><a href="https://www.egu26.eu/pg/GMPV_080526">GMPV11.5</a>

10:45–12:30

Hall X2

&nbsp;</td>
<td width="225">Volcanic Eruptions and Climate: Observations, Modeling, and Impacts

<strong>Convener: </strong>Vito Zago;

<strong>Co-conveners: </strong>Eleonora Amato, Federica Torrisi, Ciro Del Negro

&nbsp;</td>
<td width="298">This session will focus on how volcanic processes influence the climate system and thus deal with-

(i)  forward-looking strategies that combine multi-source data, real-time monitoring, and advanced modeling—including hybrid and data-driven approaches—to enhance ability to monitor, interpret, and anticipate the climate impacts of volcanic activity.

(ii) Integration of satellite, in situ, and paleo records with physical models and computational techniques.

(iii) Detection of anomalies, identifying patterns, and quantifying both short- and long-term effects.

(iv) Case studies of recent or historical major eruptions and the use of innovative analytical or simulation methods.

&nbsp;</td>
</tr>
<tr>
<td width="97"><a href="https://www.egu26.eu/pg/GMPV_080526">SM6.4</a></td>
<td width="225">Advances in Seismic Attenuation, Scattering, and Absorption

<strong>Convener:</strong> Mirko Bracale

<strong>Co-conveners: </strong>Lian Feng Zhao, Simona Gabrielli, Miriam Christina Reiss, Luca De Siena</td>
<td width="298">The session will deal with-

(i) Theoretical advancements that improve understanding of attenuation processes, including scattering and intrinsic absorption;

(ii) Resolve Earth’s internal structure through analysis of attenuation data;

(iii) Numerical simulations of the relevant equations for seismic wave propagation in heterogeneous media and attenuation;

(iv) Applications to the study and characterization of seismic sources;

(v) Attenuation studies in seismic hazard and damage assessment, including ground motion models and the effects of shaking on structures and infrastructure;

(vi) Energy dispersion from geological heterogeneities, such as faults, fractures, and variations in rock properties;

(vii) Attenuation as an indicator of energy conversion into heat, with applications to geothermal exploration and volcanic hazard assessment;

(viii) Tomographic imaging that integrates attenuation, scattering, and absorption to investigate Earth’s structure from crust to core;

(ix) Planetary science investigations that use seismic attenuation to probe the internal structure and dynamics of other planetary bodies.</td>
</tr>
</tbody>
</table>
<table style="height: 1041px" width="750">
<tbody>
<tr>
<td width="97"><a href="https://www.egu26.eu/pg/GMPV_080526">SM6.4</a></td>
<td width="225">Advances in Seismic Attenuation, Scattering, and Absorption

<strong>Convener:</strong> Mirko Bracale

<strong>Co-conveners: </strong>Lian Feng Zhao, Simona Gabrielli, Miriam Christina Reiss, Luca De Siena</td>
<td width="298">The session will deal with-

(i) Theoretical advancements that improve understanding of attenuation processes, including scattering and intrinsic absorption;

(ii) Resolve Earth’s internal structure through analysis of attenuation data;

(iii) Numerical simulations of the relevant equations for seismic wave propagation in heterogeneous media and attenuation;

(iv) Applications to the study and characterization of seismic sources;

(v) Attenuation studies in seismic hazard and damage assessment, including ground motion models and the effects of shaking on structures and infrastructure;

(vi) Energy dispersion from geological heterogeneities, such as faults, fractures, and variations in rock properties;

(vii) Attenuation as an indicator of energy conversion into heat, with applications to geothermal exploration and volcanic hazard assessment;

(viii) Tomographic imaging that integrates attenuation, scattering, and absorption to investigate Earth’s structure from crust to core;

(ix) Planetary science investigations that use seismic attenuation to probe the internal structure and dynamics of other planetary bodies.</td>
</tr>
</tbody>
</table>
<h2><strong>PICO Sessions:</strong></h2>
<table style="height: 972px" width="748">
<tbody>
<tr>
<td width="97">
<h3 style="text-align: center"><strong>Session Code</strong></h3>
<h3 style="text-align: center"><strong>Time &amp; Place</strong></h3>
</td>
<td style="text-align: center" width="225">
<h3><strong>Session Title</strong></h3>
<h3><strong>Convenor</strong></h3>
<h3><strong>&amp;</strong></h3>
<h3><strong>Co-Co</strong></h3>

<hr />

<h3><strong>nvenors</strong></h3>
</td>
<td width="298">
<h3 style="text-align: center"><strong>Session Overview</strong></h3>
</td>
</tr>
<tr>
<td width="97"> <a href="https://www.egu26.eu/session/55702">GD1.3</a>

08:30–10:15

PICO spot 2

&nbsp;</td>
<td width="225">Geochemical and geodynamic perspectives on the origin and evolution of deep-seated mantle melts and their interaction with the lithosphere

<strong>Convener:</strong> Igor Ashchepkov

<strong>Co-conveners: </strong>Sonja Aulbach, Natalia Lebedeva, Rohit Pandey

&nbsp;</td>
<td width="298">The session will deal with-

(i) Reconstructions of the structure and composition of the lithospheric mantle, and the influence of plumes and subduction zones on root construction;

(ii) Interactions of plume- and subduction-derived melts and fluids with the continental lithosphere, and the nature and development of metasomatic agents;

(iii) Source rocks, formation conditions (P-T-fO<sub>2</sub>) and evolution of mantle melts originating below or in the mantle lithosphere;

(iv) Deep source regions, melting processes and phase transformation in mantle plumes and their fluids;

(v) Modes of melt migration and ascent, as constrained from numerical modelling and microstructures of natural mantle samples;

(vi) Role of mantle melts and fluids in the generation of hybrid and acid magmas.</td>
</tr>
</tbody>
</table>
&nbsp;

Keep in touch with EGU GMPV.....See you next year.....]]></content:encoded>
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					<title><![CDATA[EGU26 Thursday Highlights]]></title>
					<link>https://blogs.egu.eu/divisions/gmpv/2026/05/07/egu26-thursday-highlights/</link>
					<comments>https://blogs.egu.eu/divisions/gmpv/2026/05/07/egu26-thursday-highlights/#comments</comments>
					<pubDate>Thu, 07 May 2026 00:49:35 +0000</pubDate>
					<dc:creator><![CDATA[Samira Yalla]]></dc:creator>
							<category><![CDATA[Conferences]]></category>
		<category><![CDATA[EGU]]></category>
		<category><![CDATA[EGU GMPV]]></category>
		<category><![CDATA[Session in the Spotlight]]></category>
		<category><![CDATA[Uncategorized]]></category>
		<category><![CDATA[#EGU_GMPV]]></category>
		<category><![CDATA[conference]]></category>
		<category><![CDATA[EGU26]]></category>
		<category><![CDATA[Highlights]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Four days in, and the week isn&#8217;t done yet! Thursday is shaping up to be one of the most eventful days of the assembly for the GMPV community. Grab your badge and let&#8217;s walk you through it. Morning orals — Room K1 [08:30–12:30 (CEST)] Kick off your Thursday in Room K1 with GMPV2.2 – Advances in Geochronology and Thermochronology: from traditional methods to avant-garde applications (co-org TS). This is a full morning of talks covering the latest in dating methods — from improved U-Pb, Rb-Sr and Lu-Hf protocols to new thermochronological approaches and thermal history modelling — applied across timescales from deep mantle dynamics to surface evolution. Coffee break — Poster Hall X2 [display 08:30, attendance 10:45–12:30 (CEST)] While the geochronology orals are running, Hall X2 is already filling up with posters across four sessions worth exploring: GMPV4.1 – Decoding Earth&#8217;s Crustal Engine: Integrated Petrochronology and Structural Constraints on 4-D Tectono-Metamorphic Evolution (co-org TS) — contributions linking microscale rock records to planetary-scale geodynamics through petrochronology, structural geology, and metamorphic petrology. GMPV4.3 – What Makes Earth So Special: Global Cycles of Volatiles — how volatiles and incompatible elements are transferred between Earth&#8217;s surface and deep interior through subduction, melts, and fluids. Orals are tomorrow, but the posters are today. GMPV8.2 – From Earth to Exoplanets: Deep Planetary Interiors through advances in modelling and experiments (co-org GD/PS) — experimental and modelling work on mineral physics under extreme pressure-temperature conditions, bridging Earth science and planetary exploration. Orals tomorrow, posters today. GMPV10.8 – Volcano–Glacier Interactions on Earth and Beyond: polar perspectives from land to seafloor (co-org GM/NH) — from subglacial eruptions to tephra deposition and ice mass balance, covering some of the most remote and dynamic volcanic environments on the planet. Also worth checking: ERE4.4 (co-org GMPV6) on geophysical imaging for critical minerals, natural hydrogen and geothermal resources has posters in Hall X4 (attendance 10:45–12:30). Lunchtime — Room D2 [12:45–13:45 (CEST)] Don&#8217;t skip the GMPV Division Meeting (DM12), convened by division president Holly Stein. This is where you hear division updates, ongoing activities, and plans for the year ahead — and have your say as part of the GMPV community. Afternoon orals Two sessions are lined up this afternoon: GMPV7.4 – Structure, origin, and evolution of anomalous magmatism: models for intraplate and unusual plate boundary volcanism (co-org GD/NH) — Room K1, 14:00–15:45. This session tackles intraplate volcanism and unusual plate boundary magmatism: hotspots, mantle plumes, LIPs, and everything that doesn&#8217;t fit neatly into standard plate tectonics. Convened by Gillian Foulger, a prominent name in this debate. ERE4.4/GMPV6 – Geophysical Imaging of the Lithosphere for Critical Minerals, Natural H2 and Geothermal Resources (co-org GD) — Room -2.43, 16:15–18:00. This session connects lithospheric structure to the resources that matter most for the energy transition. Afternoon poster hall — Hall X2 [display 14:00, attendance 16:15–18:00 (CEST)] The afternoon shift in Hall X2 brings a new wave of poster sessions: GMPV1.1 – Looking into the unreachable: Inclusions as snapshots into Earth processes, from the Crust to the deep Mantle and beyond — fluid, melt and mineral inclusions from magmatic and metamorphic settings to deep mantle dynamics, with cutting-edge micro- to nano-scale analytics on display. GMPV2.1 – Solving Geoscience Problems Using Mineralogy and Mineral Inclusions — a broad session on the diversity of mineralogical methods, from spectroscopy to inclusions. Orals are tomorrow. GMPV2.2 posters (Geochronology &amp; Thermochronology — companion to the morning orals) GMPV7.4 posters (companion to the afternoon orals on anomalous magmatism). Virtual posters — Zoom, vPoster spot 3 [14:00–15:45, discussion 16:15–18:00 (CEST)] A rich afternoon of virtual presentations awaits online, including contributions from GMPV2.2 (14:24), GMPV2.1 (14:27), GMPV4.1 (14:36), GMPV5.2 – Formation of metal ore deposits during fluid-rock interactions: from physical patterns, chemical reaction to numerical modelling (14:48), GMPV8.2 (14:54), and GMPV10.12 – Volcanic Processes: Tectonics, Deformation and Unrest (15:06). If you&#8217;re attending online or want to catch up with virtual presenters, this is the place to be. Evening — Room -2.33 [19:00–20:00 (CEST)] End your Thursday on a high note with the Robert Wilhelm Bunsen Medal Lecture by Giovanni Chiodini (MAL30-GMPV), convened by Holly Stein. The 2026 Bunsen Medal honours Chiodini for his transformative contributions to volcanology and gas geochemistry, particularly his work on Earth&#8217;s degassing processes and long-term global volcano monitoring. A landmark lecture — don&#8217;t miss it. Have a great penultimate day at #EGU26 :)]]></description>
													<content:encoded><![CDATA[Four days in, and the week isn't done yet! Thursday is shaping up to be one of the most eventful days of the assembly for the GMPV community. Grab your badge and let's walk you through it.

<strong>Morning orals — Room K1 [08:30–12:30 (CEST)]</strong>

Kick off your Thursday in Room K1 with <strong>GMPV2.2 – </strong><a href="https://meetingorganizer.copernicus.org/EGU26/session/57228">Advances in Geochronology and Thermochronology: from traditional methods to avant-garde applications</a> (co-org TS). This is a full morning of talks covering the latest in dating methods — from improved U-Pb, Rb-Sr and Lu-Hf protocols to new thermochronological approaches and thermal history modelling — applied across timescales from deep mantle dynamics to surface evolution.

<strong>Coffee break — Poster Hall X2 [display 08:30, attendance 10:45–12:30 (CEST)]</strong>

While the geochronology orals are running, Hall X2 is already filling up with posters across four sessions worth exploring:
<ul>
 	<li><strong>GMPV4.1 – </strong><a href="https://meetingorganizer.copernicus.org/EGU26/session/57234">Decoding Earth's Crustal Engine: Integrated Petrochronology and Structural Constraints on 4-D Tectono-Metamorphic Evolution</a> (co-org TS) — contributions linking microscale rock records to planetary-scale geodynamics through petrochronology, structural geology, and metamorphic petrology.</li>
 	<li><strong>GMPV4.3 – </strong><a href="https://meetingorganizer.copernicus.org/EGU26/session/57235">What Makes Earth So Special: Global Cycles of Volatiles</a> — how volatiles and incompatible elements are transferred between Earth's surface and deep interior through subduction, melts, and fluids. Orals are tomorrow, but the posters are today.</li>
 	<li><strong>GMPV8.2 – </strong><a href="https://meetingorganizer.copernicus.org/EGU26/session/57794">From Earth to Exoplanets: Deep Planetary Interiors through advances in modelling and experiments</a> (co-org GD/PS) — experimental and modelling work on mineral physics under extreme pressure-temperature conditions, bridging Earth science and planetary exploration. Orals tomorrow, posters today.</li>
 	<li><strong>GMPV10.8 </strong><a href="https://meetingorganizer.copernicus.org/EGU26/session/57800"><strong>– </strong>Volcano–Glacier Interactions on Earth and Beyond: polar perspectives from land to seafloor</a> (co-org GM/NH) — from subglacial eruptions to tephra deposition and ice mass balance, covering some of the most remote and dynamic volcanic environments on the planet.</li>
</ul>
Also worth checking: <strong>ERE4.4 (co-org GMPV6)</strong> on <a href="https://meetingorganizer.copernicus.org/EGU26/session/58030">geophysical imaging for critical minerals, natural hydrogen and geothermal resources</a> has posters in Hall X4 (attendance 10:45–12:30).

<strong>Lunchtime — Room D2 [12:45–13:45 (CEST)]</strong>

Don't skip the <strong>GMPV Division Meeting (DM12)</strong>, convened by division president Holly Stein. This is where you hear division updates, ongoing activities, and plans for the year ahead — and have your say as part of the GMPV community.

<strong>Afternoon orals</strong>

Two sessions are lined up this afternoon:
<ul>
 	<li><strong>GMPV7.4 – </strong><a href="https://meetingorganizer.copernicus.org/EGU26/session/57226">Structure, origin, and evolution of anomalous magmatism: models for intraplate and unusual plate boundary volcanism</a> (co-org GD/NH) — Room K1, 14:00–15:45. This session tackles intraplate volcanism and unusual plate boundary magmatism: hotspots, mantle plumes, LIPs, and everything that doesn't fit neatly into standard plate tectonics. Convened by Gillian Foulger, a prominent name in this debate.</li>
 	<li><strong>ERE4.4/GMPV6 – </strong><a href="https://meetingorganizer.copernicus.org/EGU26/session/58030">Geophysical Imaging of the Lithosphere for Critical Minerals, Natural H2 and Geothermal Resources</a> (co-org GD) — Room -2.43, 16:15–18:00. This session connects lithospheric structure to the resources that matter most for the energy transition.</li>
</ul>
<strong>Afternoon poster hall — Hall X2 [display 14:00, attendance 16:15–18:00 (CEST)]</strong>

The afternoon shift in Hall X2 brings a new wave of poster sessions:
<ul>
 	<li><strong>GMPV1.1 – </strong><a href="https://meetingorganizer.copernicus.org/EGU26/session/57076">Looking into the unreachable: Inclusions as snapshots into Earth processes, from the Crust to the deep Mantle and beyond</a> — fluid, melt and mineral inclusions from magmatic and metamorphic settings to deep mantle dynamics, with cutting-edge micro- to nano-scale analytics on display.</li>
 	<li><strong>GMPV2.1 – </strong><a href="https://meetingorganizer.copernicus.org/EGU26/session/57230">Solving Geoscience Problems Using Mineralogy and Mineral Inclusions</a> — a broad session on the diversity of mineralogical methods, from spectroscopy to inclusions. Orals are tomorrow.</li>
 	<li><a href="https://meetingorganizer.copernicus.org/EGU26/session/57228"><strong>GMPV2.2</strong></a> posters (Geochronology &amp; Thermochronology — companion to the morning orals)</li>
 	<li><a href="https://meetingorganizer.copernicus.org/EGU26/session/57226"><strong>GMPV7.4</strong></a> posters (companion to the afternoon orals on anomalous magmatism).</li>
</ul>
<strong>Virtual posters — Zoom, vPoster spot 3 [14:00–15:45, discussion 16:15–18:00 (CEST)]</strong>

A rich afternoon of virtual presentations awaits online, including contributions from <a href="https://meetingorganizer.copernicus.org/EGU26/session/57228"><strong>GMPV2.2</strong></a> (14:24), <a href="https://meetingorganizer.copernicus.org/EGU26/session/57230"><strong>GMPV2.1</strong></a> (14:27), <a href="https://meetingorganizer.copernicus.org/EGU26/session/57234"><strong>GMPV4.1</strong></a> (14:36), <strong>GMPV5.2 – </strong><a href="https://meetingorganizer.copernicus.org/EGU26/session/57232">Formation of metal ore deposits during fluid-rock interactions: from physical patterns, chemical reaction to numerical modelling</a> (14:48), <a href="https://meetingorganizer.copernicus.org/EGU26/session/57794"><strong>GMPV8.2</strong></a> (14:54), and <strong>GMPV10.12 – </strong><a href="https://meetingorganizer.copernicus.org/EGU26/session/58066">Volcanic Processes: Tectonics, Deformation and Unrest</a> (15:06). If you're attending online or want to catch up with virtual presenters, this is the place to be.

<strong>Evening — Room -2.33 [19:00–20:00 (CEST)]</strong>

End your Thursday on a high note with the <strong>Robert Wilhelm Bunsen Medal Lecture by Giovanni Chiodini</strong> (MAL30-GMPV), convened by Holly Stein. The 2026 Bunsen Medal honours Chiodini for his transformative contributions to volcanology and gas geochemistry, particularly his work on Earth's degassing processes and long-term global volcano monitoring. A landmark lecture — don't miss it.

Have a great penultimate day at #EGU26 :)]]></content:encoded>
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					<title><![CDATA[Meet Thomas S. Bianchi, Vladimir Ivanovich Vernadsky Medallist 2026]]></title>
					<link>https://blogs.egu.eu/divisions/bg/2026/05/06/meet-thomas-s-bianchi-vladimir-ivanovich-vernadsky-medallist-2026/</link>
					<comments>https://blogs.egu.eu/divisions/bg/2026/05/06/meet-thomas-s-bianchi-vladimir-ivanovich-vernadsky-medallist-2026/#comments</comments>
					<pubDate>Wed, 06 May 2026 21:42:53 +0000</pubDate>
					<dc:creator><![CDATA[Ana Bastos]]></dc:creator>
							<category><![CDATA[Uncategorized]]></category>
		<category><![CDATA[Awards and Medals]]></category>
		<category><![CDATA[blue carbon]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Thomas S. Bianchi is the 2026 Vladimir Ivanovich Vernadsky medallist of the Biogeosciences Division. The BG team congratulates Thomas and celebrates this well deserved recognition! We talked with Thomas to learn more about his career, research interests and advice for early career scientists Could you tell us a bit about yourself and what inspired you to pursue a career in biogeosciences? I grew up in a blue-collar family in Holbrook, NY—then a one–traffic-light town on eastern Long Island surrounded by woodlands. I spent my time playing basketball, diving, drumming, and exploring the coast. Long Island offered a remarkable range of shorelines, the Long Island Sound estuary, Peconic Bay, the Great South Bay barrier-island lagoon, the Atlantic Ocean, and extensive marshes, which fueled my fascination with coastal environments. From an early age I collected shoreline organisms, watched Cousteau specials, and read science books. I became captivated by marshes and invertebrates after spending countless hours diving and exploring diverse coastal habitats. I actually came into biogeochemistry through oceanography. Back then, biogeochemistry wasn&#8217;t a recognized field, at least not in the U.S. While Vernadsky understood the concept, it wasn&#8217;t on our radar yet, and I was too junior to even use the terminology. As a high school senior, a friend and I even built a small artificial reef in about 15 m of water in Long Island Sound and documented its colonization; we briefly tried (unsuccessfully) to publish the results. An inspiring oceanography teacher, Dennis Hirsch, further encouraged my interests. As an undergraduate, I joined several local research projects with faculty and was selected for a 10-day natural history field trip to Gran Canaria in the Canary Islands. This was my first trip abroad, and it had a huge impact on me. Another big influence for me as a potential scientist was the fact that I lived close to many research institutes that held open science events. I had the opportunity to attend seminars and tours at Brookhaven National Laboratory, Cold Spring Harbor Laboratory, the American Museum of Natural History, and Columbia University’s Lamont-Doherty Core Repository. All these experiences broadened my interests beyond oceanography into chemistry and genetics, and further confirmed my desire to become a scientist. Could you briefly describe your research area and your specific contributions to the field? My research career began, and largely continues, in muddy environments. Aside from a brief period studying sand flats in Delaware Bay during my Ph.D., my work started with mud in my M.S. research and has stayed there ever since. It is perhaps no surprise, then, that I am now writing a book about Earth’s mud. A reason for my interest in muddy environments is that over 90% of all the organic carbon in the ocean gets buried in the coastal margins. So, these small fringes have a huge importance in the ocean carbon cycling. Like many academics, my work has evolved in stages. In graduate school at Stony Brook University with Jeff Levinton, and later at the University of Maryland with Don Rice, I focused on animal–sediment interactions—specifically the nutritional ecology of mud-dwelling macroinvertebrates and their influence on sediment geochemistry. These processes are important to both paleontologists and marine ecologists. A postdoc fellowship at the Cary Institute of Ecosystem Studies allowed me to extend this work in mud habitats at the Hudson River estuarine boundary. To better understand which types of organic matter are processed in mud, I needed tools to trace the many organic sources in coastal sediments to the organisms that use them. This is where Rodger Dawson, a member of my Ph.D. committee and fellow band member, influenced my work through his expertise in chemical biomarkers. That collaboration led me to plant pigments and other molecular tracers, which I have used throughout my career to distinguish algae, terrestrial plants, and soil-derived organic matter in sediments. With these tools, I expanded my research to broader questions about how terrestrial organic matter connects with the coastal ocean, eventually focusing on the biogeochemical dynamics of mud in coastal marshes and estuaries. In terms of contributions, some of our key findings have helped clarify how organic carbon is processed and transported along the land–ocean continuum. I say “our” deliberately, in gratitude to the graduate students, postdocs, and visiting scholars who conducted much of the field and laboratory work; without them, there would be little for me to discuss. Here are a few examples: When we started analyzing river inputs in the Gulf of Mexico around 1997, we were surprised find less terrestrial organic matter from land plants than what was expected from known river inputs. It turns out that this comes back to suspensions of mud where river waters mix with Gulf waters. Mud is composed of very fine particles of silt and clay, which bind the terrestrial organic matter allowing it to stay resuspended for long periods which enhanced export to other regions. More specifically, using chemical biomarkers, we showed that some of the “missing” terrestrial organic carbon in shelf sediments was exported offshore as particulate organic carbon (POC) in the benthic boundary layer, or bottom waters. This further supported recent work, by Miguel Goni and Tim Eglinton, on the distribution of terrestrial organic matter in surface sediments of the Gulf. This work illustrated the importance in distinguishing marine vs. terrestrial buried carbon for understanding coastal carbon sequestration amid rising atmospheric CO₂ (364 ppm in 1997 to ca. 429 ppm in 2026). Upon moving to Sweden on a Fulbright scholarship, I found the local community deeply concerned with the problematic cyanobacterial blooms in the Baltic Sea. Although research focused heavily on identifying the region&#8217;s main nutrient sources, it was unclear whether such massive algal blooms existed before human-induced impacts. Diatoms were known to exhibit significant population shifts over thousands of years, which were well-documented through their preserved silica frustules, or exoskeletons. In contrast, cyanobacteria lack such structures, decompose rapidly, and leave no microfossil record. We demonstrated that cyanobacterial blooms comparable to modern events occurred over 7,000 years ago in the Baltic Sea, driven by eustatic and isostatic changes, linking modern ecosystem dynamics with long-term environmental history. While this does not rule out the role of recent anthropogenic nutrient inputs in driving blooms, it indicated that such blooms had occurred much earlier, driven by large nutrient pulses from the ocean during distinct geological phases of the Baltic&#8217;s formation. Another important contribution was to extend the concept of the microbial “priming effect,” previously known from soils to aquatic environments, as previously noted by Bertrand Guenet and others, showing how labile carbon inputs can stimulate degradation of refractory carbon across diverse ecosystem gradients. Given my past experience working on coastal river deltas and estuaries, it was a logical path to explore priming across the land-ocean margin. For example, we analyzed river confluences in tributaries of the Amazon, where the green and brown waters, comprised of phytoplankton and mud, mix. Together with Nick Ward, a postdoc in my group, and Jeff Richey, we used labeled isotopes to detect the priming effect at these interfaces. There are many fascinating topics in this domain and I have dedicated significant effort to synthesizing research in this field in 10 books I authored or co-authored, most notably through Biogeochemistry of Estuaries (2007) and Chemical Biomarkers in Aquatic Ecosystems (2011).&#8221; What key knowledge gaps still need to be addressed in this area? As we continue to explore how carbon is sequestered on the planet, we need to return to two topics that had received considerable 30 to 50 years ago, the role of sulfur cycling and the importance of petrogenic organic carbon burial. While there have been some new and exciting studies on these topics over the past decade or so, there remain significant gaps in their roles in organic carbon burial. A better understanding of these pathway will continue to prove useful in exploring the mechanisms of the short and long-term carbon cycle. There also remain many gaps in our understanding of priming, particularly in aquatic systems. New isotopic probing and omics techniques continue to provide innovative ways to trace the mechanisms involved priming, particularly as new aquatic critical zones are created from global change. What have been the biggest challenges and the greatest opportunities in your career? Early on, my biggest challenge was simply paying for college. My family could offer little financial support, so I worked about 40 hours a week unloading trucks while completing my undergraduate degree. Balancing work with coursework, like tending Drosophila crosses in genetics lab at odd hours in the evening, was demanding. I had to get special keys to go in the middle of the night and do these things. My books were thrown in the back seat, and I largely worked independently. So I never really experienced the idea of a “study group.” I never knew what a study group was. I have no idea how I did it, but I managed to get through it. Later, like many early-career academics, I faced the usual challenges of balancing teaching and research while building a lab with limited funding and no technician. Then an extraordinary challenge arose: Hurricane Katrina. At the time I was a professor at Tulane University in New Orleans. I had been working on the Mississippi River and the Gulf of Mexico, and had so many ideas for future research. Everything just vanished. My family—my wife Jo Ann and son Christopher—and I lost our home and everything in it. Professionally, the colleagues I was collaborating with dispersed across the country with no certainty of returning. Ultimately, we did not go back, and I moved to Texas A&amp;M University. Losing years of research at Tulane was devastating, but my family&#8217;s safety and support gave me the strength to rebuild. Some of my most rewarding opportunities came through two Fulbright Program scholarships, the first in Sweden and later in Cyprus. These experiences opened doors to collaborations with regional research groups, leading to long-term partnerships and rich cultural exchanges. Later in my career, visiting research appointments during sabbaticals also proved highly productive. How do you think the scientific field has changed since you started your career? Universities have embraced a business model far more aggressively than in the past, placing intense pressure on young faculty to secure funding and publish more papers. University rankings now play a central role, further shifting the burden onto faculty. At the same time, classrooms have increasingly become “safe spaces”. A lot of the bullies are gone and that&#8217;s great, but students are often less challenged, something that, in my view, has also weakened academia. Meanwhile, the number of journals has grown at an astonishing rate, making it easier to place publications, while publishing costs have soared with little solution in sight. Yet the real elephant in the room is AI. Yuval Noah Harari has written eloquently, and pessimistically, about its trajectory. AI has already proven to be a remarkable tool for scientists, helping recent Nobel laureates make major advances. But like any powerful invention, it brings risks and complex implications that we still need to confront. What general advice would you give to early-career scientists? These are challenging times, particularly in the United States. Attacks on academia have led to severe funding cuts, denial of climate change, threats to scholars’ privacy, and restrictions on international collaboration. Our government’s irresponsibility has also contributed to global instability. My advice is to stay focused on your work, this period will pass, perhaps sooner than expected. Reflecting back on Vladimir Vernadsky, it is well-known that he worked under intense political pressure during the Russian Revolution and the Stalinist era. Rather than disengaging, he navigated these constraints by focusing deeply on his science. For young scientists, it’s important to contribute to large interdisciplinary projects while still seeking opportunities to publish first-authored papers, even when projects are led by graduate students, postdocs, or collaborators. This helps maintain your original passion and creativity. Finally, stay open to shifting research directions as funding or new opportunities arise, inside and outside of academia, and surround yourself with good people.]]></description>
													<content:encoded><![CDATA[<p style="text-align: justify"><strong>Thomas S. Bianchi is the 2026 Vladimir Ivanovich Vernadsky medallist of the Biogeosciences Division. The BG team congratulates Thomas and celebrates this well deserved recognition! We talked with Thomas to learn more about his career, research interests and advice for early career scientists</strong></p>
<strong>Could you tell us a bit about yourself and what inspired you to pursue a career in biogeosciences?</strong>
<p style="text-align: justify"><span style="font-weight: 400">I grew up in a blue-collar family in Holbrook, NY—then a one–traffic-light town on eastern Long Island surrounded by woodlands. I spent my time playing basketball, diving, drumming, and exploring the coast. Long Island offered a remarkable range of shorelines, the Long Island Sound estuary, Peconic Bay, the Great South Bay barrier-island lagoon, the Atlantic Ocean, and extensive marshes, which fueled my fascination with coastal environments. From an early age I collected shoreline organisms, watched Cousteau specials, and read science books. I became captivated by marshes and invertebrates after spending countless hours diving and exploring diverse coastal habitats.</span></p>
<p style="text-align: justify"><span style="font-weight: 400">I actually came into biogeochemistry through oceanography. Back then, biogeochemistry wasn't a recognized field, at least not in the U.S. While Vernadsky understood the concept, it wasn't on our radar yet, and I was too junior to even use the terminology. As a high school senior, a friend and I even built a small artificial reef in about 15 m of water in Long Island Sound and documented its colonization; we briefly tried (unsuccessfully) to publish the results. An inspiring oceanography teacher, Dennis Hirsch, further encouraged my interests. As an undergraduate, I joined several local research projects with faculty and was selected for a 10-day natural history field trip to Gran Canaria in the Canary Islands. This was my first trip abroad, and it had a huge impact on me.
Another big influence for me as a potential scientist was the fact that I lived close to many research institutes that held open science events. I had the opportunity to attend seminars and tours at Brookhaven National Laboratory, Cold Spring Harbor Laboratory, the American Museum of Natural History, and Columbia University’s Lamont-Doherty Core Repository. All these experiences broadened my interests beyond oceanography into chemistry and genetics, and further confirmed my desire to become a scientist.</span></p>
<strong>Could you briefly describe your research area and your specific contributions to the field?</strong>
<p style="text-align: justify"><span style="font-weight: 400">My research career began, and largely continues, in muddy environments. Aside from a brief period studying sand flats in Delaware Bay during my Ph.D., my work started with mud in my M.S. research and has stayed there ever since. It is perhaps no surprise, then, that I am now writing a book about Earth’s mud. A reason for my interest in muddy environments is that over 90% of all the organic carbon in the ocean gets buried in the coastal margins. So, these small fringes have a huge importance in the ocean carbon cycling.
Like many academics, my work has evolved in stages. In graduate school at Stony Brook University with Jeff Levinton, and later at the University of Maryland with Don Rice, I focused on animal–sediment interactions—specifically the nutritional ecology of mud-dwelling macroinvertebrates and their influence on sediment geochemistry. These processes are important to both paleontologists and marine ecologists. A postdoc fellowship at the Cary Institute of Ecosystem Studies allowed me to extend this work in mud habitats at the Hudson River estuarine boundary.</span></p>


[caption id="attachment_4020" align="aligncenter" width="300"]<a href="https://blogs.egu.eu/divisions/bg/files/2026/05/Picture4.jpg"><img class="alignnone size-medium wp-image-4022" src="https://blogs.egu.eu/divisions/bg/files/2026/05/Picture4-300x209.jpg" alt="" width="300" height="209" /></a> <br />Box core of mud off the Mississippi river delta in the Gulf of Mexico (2002).[/caption]
<p style="text-align: justify"><span style="font-weight: 400">To better understand which types of organic matter are processed in mud, I needed tools to trace the many organic sources in coastal sediments to the organisms that use them. This is where Rodger Dawson, a member of my Ph.D. committee and fellow band member, influenced my work through his expertise in chemical biomarkers. That collaboration led me to plant pigments and other molecular tracers, which I have used throughout my career to distinguish algae, terrestrial plants, and soil-derived organic matter in sediments.
With these tools, I expanded my research to broader questions about how terrestrial organic matter connects with the coastal ocean, eventually focusing on the biogeochemical dynamics of mud in coastal marshes and estuaries. In terms of contributions, some of our key findings have helped clarify how organic carbon is processed and transported along the land–ocean continuum. I say “our” deliberately, in gratitude to the graduate students, postdocs, and visiting scholars who conducted much of the field and laboratory work; without them, there would be little for me to discuss. </span></p>
Here are a few examples:
<p style="text-align: justify"><span style="font-weight: 400">When we started analyzing river inputs in the Gulf of Mexico around 1997, we were surprised find less terrestrial organic matter from land plants than what was expected from known river inputs. It turns out that this comes back to suspensions of mud where river waters mix with Gulf waters. Mud is composed of very fine particles of silt and clay, which bind the terrestrial organic matter allowing it to stay resuspended for long periods which enhanced export to other regions. More specifically, using chemical biomarkers, we showed that some of the “missing” terrestrial organic carbon in shelf sediments was exported offshore as particulate organic carbon (POC) in the benthic boundary layer, or bottom waters. This further supported recent work, by Miguel Goni and Tim Eglinton, on the distribution of terrestrial organic matter in surface sediments of the Gulf. This work illustrated the importance in distinguishing marine vs. terrestrial buried carbon for understanding coastal carbon sequestration amid rising atmospheric CO₂ (364 ppm in 1997 to ca. 429 ppm in 2026).</span></p>
<p style="text-align: justify"><span style="font-weight: 400">Upon moving to Sweden on a Fulbright scholarship, I found the local community deeply concerned with the problematic cyanobacterial blooms in the Baltic Sea. Although research focused heavily on identifying the region's main nutrient sources, it was unclear whether such massive algal blooms existed before human-induced impacts. Diatoms were known to exhibit significant population shifts over thousands of years, which were well-documented through their preserved silica frustules, or exoskeletons. In contrast, cyanobacteria lack such structures, decompose rapidly, and leave no microfossil record. We demonstrated that cyanobacterial blooms comparable to modern events occurred over 7,000 years ago in the Baltic Sea, driven by eustatic and isostatic changes, linking modern ecosystem dynamics with long-term environmental history. While this does not rule out the role of recent anthropogenic nutrient inputs in driving blooms, it indicated that such blooms had occurred much earlier, driven by large nutrient pulses from the ocean during distinct geological phases of the Baltic's formation.</span></p>


[caption id="attachment_4020" align="aligncenter" width="300"]<a href="https://blogs.egu.eu/divisions/bg/files/2026/05/Picture1.png"><img class="alignnone size-medium wp-image-4014" src="https://blogs.egu.eu/divisions/bg/files/2026/05/Picture1-300x243.png" alt="" width="300" height="243" /></a> <br />Thomas holding a sediment core with beautiful layers from their bloom work in the Baltic Sea (2000).[/caption]
<p style="text-align: justify"><span style="font-weight: 400">Another important contribution was to extend the concept of the microbial “priming effect,” previously known from soils to aquatic environments, as previously noted by Bertrand Guenet and others, showing how labile carbon inputs can stimulate degradation of refractory carbon across diverse ecosystem gradients. Given my past experience working on coastal river deltas and estuaries, it was a logical path to explore priming across the land-ocean margin. For example, we analyzed river confluences in tributaries of the Amazon, where the green and brown waters, comprised of phytoplankton and mud, mix. Together with Nick Ward, a postdoc in my group, and Jeff Richey, we used labeled isotopes to detect the priming effect at these interfaces.
There are many fascinating topics in this domain and I have dedicated significant effort to synthesizing research in this field in 10 books I authored or co-authored, most notably through Biogeochemistry of Estuaries (2007) and Chemical Biomarkers in Aquatic Ecosystems (2011)."</span></p>


[caption id="attachment_4020" align="aligncenter" width="300"]<a href="https://blogs.egu.eu/divisions/bg/files/2026/05/Picture3.jpg"><img class="size-medium wp-image-4020" src="https://blogs.egu.eu/divisions/bg/files/2026/05/Picture3-300x225.jpg" alt="" width="300" height="225" /></a> Confluence of green tributary water with brown mainstream amazon water. Photo by Nick Ward.[/caption]
<p style="text-align: justify"><strong>What key knowledge gaps still need to be addressed in this area?</strong>
<span style="font-weight: 400">As we continue to explore how carbon is sequestered on the planet, we need to return to two topics that had received considerable 30 to 50 years ago, the role of sulfur cycling and the importance of petrogenic organic carbon burial. While there have been some new and exciting studies on these topics over the past decade or so, there remain significant gaps in their roles in organic carbon burial. A better understanding of these pathway will continue to prove useful in exploring the mechanisms of the short and long-term carbon cycle.
There also remain many gaps in our understanding of priming, particularly in aquatic systems. New isotopic probing and omics techniques continue to provide innovative ways to trace the mechanisms involved priming, particularly as new aquatic critical zones are created from global change. </span></p>
<strong>What have been the biggest challenges and the greatest opportunities in your career?</strong>
<p style="text-align: justify"><span style="font-weight: 400">Early on, my biggest challenge was simply paying for college. My family could offer little financial support, so I worked about 40 hours a week unloading trucks while completing my undergraduate degree. Balancing work with coursework, like tending Drosophila crosses in genetics lab at odd hours in the evening, was demanding. I had to get special keys to go in the middle of the night and do these things. My books were thrown in the back seat, and I largely worked independently. So I never really experienced the idea of a “study group.” I never knew what a study group was. I have no idea how I did it, but I managed to get through it. </span></p>
<p style="text-align: justify"><span style="font-weight: 400">Later, like many early-career academics, I faced the usual challenges of balancing teaching and research while building a lab with limited funding and no technician. Then an extraordinary challenge arose: Hurricane Katrina. At the time I was a professor at Tulane University in New Orleans. I had been working on the Mississippi River and the Gulf of Mexico, and had so many ideas for future research. Everything just vanished. My family—my wife Jo Ann and son Christopher—and I lost our home and everything in it. Professionally, the colleagues I was collaborating with dispersed across the country with no certainty of returning. Ultimately, we did not go back, and I moved to Texas A&amp;M University. Losing years of research at Tulane was devastating, but my family's safety and support gave me the strength to rebuild.
Some of my most rewarding opportunities came through two Fulbright Program scholarships, the first in Sweden and later in Cyprus. These experiences opened doors to collaborations with regional research groups, leading to long-term partnerships and rich cultural exchanges. Later in my career, visiting research appointments during sabbaticals also proved highly productive.</span></p>
<strong>How do you think the scientific field has changed since you started your career?</strong>
<p style="text-align: justify"><span style="font-weight: 400">Universities have embraced a business model far more aggressively than in the past, placing intense pressure on young faculty to secure funding and publish more papers. University rankings now play a central role, further shifting the burden onto faculty. At the same time, classrooms have increasingly become “safe spaces”. A lot of the bullies are gone and that's great, but students are often less challenged, something that, in my view, has also weakened academia.</span></p>
<p style="text-align: justify"><span style="font-weight: 400">Meanwhile, the number of journals has grown at an astonishing rate, making it easier to place publications, while publishing costs have soared with little solution in sight. Yet the real elephant in the room is AI. Yuval Noah Harari has written eloquently, and pessimistically, about its trajectory. AI has already proven to be a remarkable tool for scientists, helping recent Nobel laureates make major advances. But like any powerful invention, it brings risks and complex implications that we still need to confront.</span></p>
<strong>What general advice would you give to early-career scientists?</strong>
<p style="text-align: justify"><span style="font-weight: 400">These are challenging times, particularly in the United States. Attacks on academia have led to severe funding cuts, denial of climate change, threats to scholars’ privacy, and restrictions on international collaboration. Our government’s irresponsibility has also contributed to global instability. My advice is to stay focused on your work, this period will pass, perhaps sooner than expected.</span></p>
<p style="text-align: justify"><span style="font-weight: 400">Reflecting back on Vladimir Vernadsky, it is well-known that he worked under intense political pressure during the Russian Revolution and the Stalinist era. Rather than disengaging, he navigated these constraints by focusing deeply on his science.
For young scientists, it’s important to contribute to large interdisciplinary projects while still seeking opportunities to publish first-authored papers, even when projects are led by graduate students, postdocs, or collaborators. This helps maintain your original passion and creativity. Finally, stay open to shifting research directions as funding or new opportunities arise, inside and outside of academia, and surround yourself with good people.</span></p>]]></content:encoded>
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					<title><![CDATA[Social Dinner GMPV is at capacity!]]></title>
					<link>https://blogs.egu.eu/divisions/gmpv/2026/05/06/social-dinner-gmpv-is-at-capacity/</link>
					<comments>https://blogs.egu.eu/divisions/gmpv/2026/05/06/social-dinner-gmpv-is-at-capacity/#comments</comments>
					<pubDate>Wed, 06 May 2026 13:03:13 +0000</pubDate>
					<dc:creator><![CDATA[Agata Poganj]]></dc:creator>
							<category><![CDATA[Uncategorized]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Thank you for the increased interest, our reservation is at capacity! We will see everyone who filled the form at Plutzer Bräu at 8 pm! Please note: This event is being held at an off-site location chosen by the event organisers, not at the Austria Centre Vienna. Copernicus Meetings and EGU cannot accept any liability for networking events held outside the Austria Centre Vienna.]]></description>
													<content:encoded><![CDATA[<strong>Thank you for the increased interest, our reservation is at capacity!</strong>

We will see everyone who filled the form at Plutzer Bräu at 8 pm!

Please note: This event is being held at an off-site location chosen by the event organisers, not at the Austria Centre Vienna. Copernicus Meetings and EGU cannot accept any liability for networking events held outside the Austria Centre Vienna.]]></content:encoded>
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					<title><![CDATA[Fluid injection-induced seismicity: the case of hydrofracking]]></title>
					<link>https://blogs.egu.eu/divisions/gd/2026/05/06/fluid-injection-induced-seismicity-the-case-of-hydrofracking/</link>
					<comments>https://blogs.egu.eu/divisions/gd/2026/05/06/fluid-injection-induced-seismicity-the-case-of-hydrofracking/#comments</comments>
					<pubDate>Wed, 06 May 2026 08:00:13 +0000</pubDate>
					<dc:creator><![CDATA[Editorial Team 3]]></dc:creator>
							<category><![CDATA[Geodynamics 101]]></category>
		<category><![CDATA[Hydraulic fracturing]]></category>
		<category><![CDATA[Induced-seismicity]]></category>
		<category><![CDATA[Microseismicity]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Seismicity is undoubtedly an integral part of Geodynamics, since seismic data, from large-scale geophysical monitoring, can provide many valuable insights regarding the state of the Earth’s crust; seismicity, however, is not always natural, it can also be induced. In this week’s blog, we explored the subject of fluid injection-induced seismicity mainly through the lens of hydraulic fracturing (HF; hydrofracking or simply fracking), a process used in the petroleum industry to extract oil and gas from tight rock formations (e.g., shales – schists); brief discussions were facilitated pertaining to the two primary modern conundrums concerning the induced seismicity from hydrofracking operations, namely, the dominant crack source mechanisms, as well as the differentiation of the so-called ‘’wet’’ and ‘’dry’’ seismic events, along with their implications in the accurate estimation of the stimulated reservoir volume (SRV). Induced vs natural seismicity; what’s the difference and should we even care? Induced seismicity, often referred to as induced microseisms, is a phenomenon where microearthquakes (i.e., seismic events of low magnitude) are triggered due to man-related activities that affect the natural stress – strain fields of the Earth, in comparison, natural earthquakes can be caused by geological processes, such as tectonic plate movements. Originally, the scientific community was interested in induced seismicity due to mining activities (e.g., rock blasting etc.); however, in the past few decades, this interest was rekindled through the scope of fluid injection-induced seismicity, given the abrupt rise of (a) enhanced geothermal systems (EGS), (b) injection of CO2 for permanent carbon capture and storage, (c) HF for oil and gas recovery, (d) injection of either water or CO2 into depleted reservoirs for enhanced oil recovery, and (e) disposal of waste water into deep formations, due to the global sustainability goals for renewable geothermal energy, environmental protection, economic optimization, amongst others. Zang et al. (2014) classified injection operations into two separate categories, based on their time-scale and total injected volumes, i.e., long-term injection operations (b) and (e) (where the injected volumes &gt; 100,000 m3), and short-term injection operations (a), (c), and (d) (where the injected volumes &lt; 100,000 m3); today we will mainly discuss the latter class of injection operations, and particularly, the process of HF. In contrast to popular belief, hydrofracking, or the ‘’hydrafrac job/process’’ as it was referred in the original publication of Clark (1949), is an old school method for increasing the productivity of oil and gas wells in ultra tight rock formations, such as schists, that dates back to the late 40s. The HF method requires the drilling of a well in an oil-bearing formation of low permeability, and the subsequent pressurization of a sealed-off section of the borehole until the rock formation fails and ruptures abruptly. During the pressurization process, which causes the progressive failure of the surrounding rock, microcracks (which eventually lead to macrocracks) form that generate elastic acoustic waves, that can have a varying degree of energy, these elastic waves, that propagate through the rock medium, are often denoted as acoustic emission (AE) events; they essentially represent induced microseismic events, that can be effectively captured via the usage of specialized high frequency AE sensors with typical frequency bandwidths ranging from 100 kHz to 1 MHz. Overall, the induced seismicity from hydrofracking operations lies in the micro scale, i.e., it has very low recorded moment magnitudes (as low as -8 – -6 up to -3 – -1); it has been shown, however, that the scale of the induced seismicity can drastically increase across multiple orders of magnitude provided that active, or even passive, faults exist in the near vicinity of the HF. For instance, Bao and Eaton (2016) observed that a fault was reactivated during a shale gas stimulation due to the conduction of HFs. Generally, apart from the implications of microseismicity regarding the potential to create large-scale hazardous earthquakes, microseismic data can provide a great variety of insightful information relating to the fracturing process of the pressurized rock, as well as the SRV. Crack source mechanisms; how does the pressurized rock fail? Crack source mechanism analysis (or focal mechanism analysis) of microseismic data can provide a clear picture of the dominant fracture type of the rock, meaning tensile, shear, compressive, and/or mix-mode. This information can have great implications towards mitigating microseismicity, since tensile microcracks (type I) radiate elastic waves with substantially less energy relative to shearing microcracks (type II); very often researchers aim to generate an abundance of type I microcracks and as few type II microcracks as possible. For the most part, it appears that the dominant cracking mode is heavily dependent on the method used for the determination of the crack source mechanisms (e.g., moment tensor analysis, polarity, tensile angle etc.), the examined rock type (e.g., shale – metamorphic, granite – crystalline igneous, sandstone – sedimentary), and the density of pre-existing micro- or macrocracks in the rock volume, amongst other factors. For instance, Butt et al. (2024) performed true-triaxial HF tests on cubical granite rock specimens, they generally observed tensile dominated events using both a low and a high viscosity fracturing fluid. Moreover, Naoi et al. (2020) conducted simple uniaxial HF tests on Eagle Ford shale specimens, they noticed an extreme domination of tensile events. These conclusions, come into contrast with the more commonly encountered shear dominated events observed in actual production fields (e.g., Maxwell and Cipolla 2011) and large-scale in situ experiments (e.g., Ishida et al. 2019). Overall, by uncovering the influence of each parameter on the derived focal mechanisms a deeper understanding can be gained towards the necessary steps to decrease the larger magnitude shear events. Wet and dry microseismic events; towards an accurate estimation of the SRV Microseismicity induced by HF stimulations can be mainly attributed to either pressure or mechanical changes/perturbations; given this simple distinction, the seismic events can be divided into: ‘’wet’’ microseismic events, which are caused due to fluid-flow related pressure changes (they are directly connected with the main HF), and remote ‘’dry’’ microseismic events, which are a product of stress changes at considerable distances away from the borehole (they are usually not connected with the main HF). Provided that for many years, it is a common practice to estimate the SRV by inferring to the AE cloud, the inclusion of isolated and distant ‘’dry’’ events, which are not actually connected with the main HF and hence do not really contribute to the SRV, into the AE seismic cloud can result in significant overestimations of the SRV. Although there exists no unified way to directly differentiate between ‘’wet’’ and ‘’dry’’ events, one of the following two paths is usually adopted; namely, Maxwell et al. (2015a,b) observed that ‘’dry’’ and ‘’wet’’ events have noticeably different b-values, with former having a b-value of around 1, whereas the latter has a b-value of around 2. Finally, a less effective way is to create a distance – time from injection plot, in an attempt to locate early-stage distant events. A method capable of precisely distinguishing between ‘’dry’’ and ‘’wet’’ microseismic events can be truly beneficial to the progression of the field, since it will allow for the accurate determination of the SRV using the derived microseismic data. References Bao X, Eaton DW (2016) Fault activation by hydraulic fracturing in western Canada. Science 354(6318): 1406 – 1409. Butt A, Hedayat A, Moradian O (2024) Microseismic Monitoring of Laboratory Hydraulic Fracturing Experiments in Granitic Rocks for Different Fracture Propagation Regimes. Rock Mech Rock Eng 57: 2035 – 2059. Clark JB (1949) A Hydraulic Process for Increasing the Productivity of Wells. J Pet Technol 1(1): 1 – 8. Ishida T, Fujito W, Yamashita H, Naoi M, Fuji H, Suzuki K, Matsui H (2019) Crack expansion and fracturing mode of hydraulic refracturing from acoustic emission monitoring in a small-scale field experiment. Rock Mech Rock Eng 52: 543 – 553. Maxwell SC, Cipolla C (2011) What does microseismicity tell us about hydraulic fracturing? In: SPE Annual Technical Conference and Exhibition, Denver, Colorado, SPE146932. Maxwell SC, Mack M, Zhang F, Chorney D, Goodfellow SD, Grob M (2015a) Differentiating Wet and Dry Microseismic Events Induced During Hydraulic Fracturing. In: SPE/AAPG/SEG Unconventional Resources Technology Conference, San Antonio, Texas, USA. Maxwell SC, Chorney D, Goodfellow SD (2015b) Microseismic geomechanics of hydraulic-fracture networks: Insights into mechanisms of microseismic sources. The Leading Edge 34(8): 904 – 910. Naoi M, Chen Y, Yamamoto K, Morishige Y, Imakita K, Tsutumi N, Kawakata H, Ishida T, Tanaka H, Arima Y, Kitamura S, Hyodo D (2020) Tensile-dominant fractures observed in hydraulic fracturing laboratory experiment using eagle ford shale. Geophys J Inter 222: 769 – 780. Zang A, Oye V, Jousset P, Deichmann N, Gritto R, McGarr A, Majer E, Bruhn D (2014) Analysis of induced seismicity in geothermal reservoirs – an overview. Anal Induc Seism Geotherm Oper 52: 6 – 21.]]></description>
													<content:encoded><![CDATA[<p style="font-weight: 400"><strong>Seismicity is undoubtedly an integral part of Geodynamics, since seismic data, from large-scale geophysical monitoring, can provide many valuable insights regarding the state of the Earth’s crust; seismicity, however, is not always natural, it can also be induced. In this week’s blog, we explored the subject of fluid injection-induced seismicity mainly through the lens of hydraulic fracturing (HF; hydrofracking or simply fracking), a process used in the petroleum industry to extract oil and gas from tight rock formations (e.g., shales – schists); brief discussions were facilitated pertaining to the two primary modern conundrums concerning the induced seismicity from hydrofracking operations, namely, the dominant crack source mechanisms, as well as the differentiation of the so-called ‘’wet’’ and ‘’dry’’ seismic events, along with their implications in the accurate estimation of the stimulated reservoir volume (SRV).</strong></p>


[caption id="attachment_42768" align="alignleft" width="368"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/05/Fig_1.jpg"><img class=" wp-image-42768" src="https://blogs.egu.eu/divisions/gd/files/2026/05/Fig_1.jpg" alt="" width="368" height="488" /></a> Dimitrios just wrapped up his bachelor in mining engineering from NTUA; in the next few months he will begin his PhD journey in the Department of Geology &amp; Geological Engineering of the Colorado School of Mines.[/caption]
<h4 style="font-weight: 400"><strong>Induced vs natural seismicity; what’s the difference and should we even care?</strong></h4>
<p style="font-weight: 400">Induced seismicity, often referred to as induced microseisms, is a phenomenon where microearthquakes (i.e., seismic events of low magnitude) are triggered due to man-related activities that affect the natural stress – strain fields of the Earth, in comparison, natural earthquakes can be caused by geological processes, such as tectonic plate movements. Originally, the scientific community was interested in induced seismicity due to mining activities (e.g., rock blasting etc.); however, in the past few decades, this interest was rekindled through the scope of fluid injection-induced seismicity, given the abrupt rise of (a) enhanced geothermal systems (EGS), (b) injection of CO<sub>2</sub> for permanent carbon capture and storage, (c) HF for oil and gas recovery, (d) injection of either water or CO<sub>2</sub> into depleted reservoirs for enhanced oil recovery, and (e) disposal of waste water into deep formations, due to the global sustainability goals for renewable geothermal energy, environmental protection, economic optimization, amongst others.</p>
<p style="font-weight: 400">Zang et al. (2014) classified injection operations into two separate categories, based on their time-scale and total injected volumes, i.e., long-term injection operations (b) and (e) (where the injected volumes &gt; 100,000 m<sup>3</sup>), and short-term injection operations (a), (c), and (d) (where the injected volumes &lt; 100,000 m<sup>3</sup>); today we will mainly discuss the latter class of injection operations, and particularly, the process of HF. In contrast to popular belief, hydrofracking, or the ‘’hydrafrac job/process’’ as it was referred in the original publication of Clark (1949), is an old school method for increasing the productivity of oil and gas wells in ultra tight rock formations, such as schists, that dates back to the late 40s. The HF method requires the drilling of a well in an oil-bearing formation of low permeability, and the subsequent pressurization of a sealed-off section of the borehole until the rock formation fails and ruptures abruptly.</p>
<p style="font-weight: 400">During the pressurization process, which causes the progressive failure of the surrounding rock, microcracks (which eventually lead to macrocracks) form that generate elastic acoustic waves, that can have a varying degree of energy, these elastic waves, that propagate through the rock medium, are often denoted as acoustic emission (AE) events; they essentially represent induced microseismic events, that can be effectively captured via the usage of specialized high frequency AE sensors with typical frequency bandwidths ranging from 100 kHz to 1 MHz.</p>
<p style="font-weight: 400">Overall, the induced seismicity from hydrofracking operations lies in the micro scale, i.e., it has very low recorded moment magnitudes (as low as -8 – -6 up to -3 – -1); it has been shown, however, that the scale of the induced seismicity can drastically increase across multiple orders of magnitude provided that active, or even passive, faults exist in the near vicinity of the HF. For instance, Bao and Eaton (2016) observed that a fault was reactivated during a shale gas stimulation due to the conduction of HFs. Generally, apart from the implications of microseismicity regarding the potential to create large-scale hazardous earthquakes, microseismic data can provide a great variety of insightful information relating to the fracturing process of the pressurized rock, as well as the SRV.</p>

<h4 style="font-weight: 400"><strong>Crack source mechanisms; how does the pressurized rock fail?</strong></h4>
<p style="font-weight: 400">Crack source mechanism analysis (or focal mechanism analysis) of microseismic data can provide a clear picture of the dominant fracture type of the rock, meaning tensile, shear, compressive, and/or mix-mode. This information can have great implications towards mitigating microseismicity, since tensile microcracks (type I) radiate elastic waves with substantially less energy relative to shearing microcracks (type II); very often researchers aim to generate an abundance of type I microcracks and as few type II microcracks as possible. For the most part, it appears that the dominant cracking mode is heavily dependent on the method used for the determination of the crack source mechanisms (e.g., moment tensor analysis, polarity, tensile angle etc.), the examined rock type (e.g., shale – metamorphic, granite – crystalline igneous, sandstone – sedimentary), and the density of pre-existing micro- or macrocracks in the rock volume, amongst other factors.</p>
<p style="font-weight: 400">For instance, Butt et al. (2024) performed true-triaxial HF tests on cubical granite rock specimens, they generally observed tensile dominated events using both a low and a high viscosity fracturing fluid. Moreover, Naoi et al. (2020) conducted simple uniaxial HF tests on Eagle Ford shale specimens, they noticed an extreme domination of tensile events. These conclusions, come into contrast with the more commonly encountered shear dominated events observed in actual production fields (e.g., Maxwell and Cipolla 2011) and large-scale <em>in situ</em> experiments (e.g., Ishida et al. 2019). Overall, by uncovering the influence of each parameter on the derived focal mechanisms a deeper understanding can be gained towards the necessary steps to decrease the larger magnitude shear events.</p>

<h4 style="font-weight: 400"><strong>Wet and dry microseismic events; towards an accurate estimation of the SRV</strong></h4>
<p style="font-weight: 400">Microseismicity induced by HF stimulations can be mainly attributed to either pressure or mechanical changes/perturbations; given this simple distinction, the seismic events can be divided into: ‘’wet’’ microseismic events, which are caused due to fluid-flow related pressure changes (they are directly connected with the main HF), and remote ‘’dry’’ microseismic events, which are a product of stress changes at considerable distances away from the borehole (they are usually not connected with the main HF). Provided that for many years, it is a common practice to estimate the SRV by inferring to the AE cloud, the inclusion of isolated and distant ‘’dry’’ events, which are not actually connected with the main HF and hence do not really contribute to the SRV, into the AE seismic cloud can result in significant overestimations of the SRV.</p>
<span style="font-weight: 400">Although there exists no unified way to directly differentiate between ‘’wet’’ and ‘’dry’’ events, one of the following two paths is usually adopted; namely, Maxwell et al. (2015a,b) observed that ‘’dry’’ and ‘’wet’’ events have noticeably different <em>b</em>-values, with former having a <em>b</em>-value of around 1, whereas the latter has a <em>b</em>-value of around 2. Finally, a less effective way is to create a distance – time from injection plot, in an attempt to locate early-stage distant events. A method capable of precisely distinguishing between ‘’dry’’ and ‘’wet’’ microseismic events can be truly beneficial to the progression of the field, since it will allow for the accurate determination of the SRV using the derived microseismic data. </span>
<pre><strong>References</strong>
Bao X, Eaton DW (2016) Fault activation by hydraulic fracturing in western Canada. Science 354(6318): 1406 – 1409. 

Butt A, Hedayat A, Moradian O (2024) Microseismic Monitoring of Laboratory Hydraulic Fracturing Experiments in Granitic Rocks for Different Fracture Propagation Regimes. Rock Mech Rock Eng 57: 2035 – 2059. 

Clark JB (1949) A Hydraulic Process for Increasing the Productivity of Wells. J Pet Technol 1(1): 1 – 8. 

Ishida T, Fujito W, Yamashita H, Naoi M, Fuji H, Suzuki K, Matsui H (2019) Crack expansion and fracturing mode of hydraulic refracturing from acoustic emission monitoring in a small-scale field experiment. Rock Mech Rock Eng 52: 543 – 553. 

Maxwell SC, Cipolla C (2011) What does microseismicity tell us about hydraulic fracturing? In: SPE Annual Technical Conference and Exhibition, Denver, Colorado, SPE146932. 

Maxwell SC, Mack M, Zhang F, Chorney D, Goodfellow SD, Grob M (2015a) Differentiating Wet and Dry Microseismic Events Induced During Hydraulic Fracturing. In: SPE/AAPG/SEG Unconventional Resources Technology Conference, San Antonio, Texas, USA. 

Maxwell SC, Chorney D, Goodfellow SD (2015b) Microseismic geomechanics of hydraulic-fracture networks: Insights into mechanisms of microseismic sources. The Leading Edge 34(8): 904 – 910. 

Naoi M, Chen Y, Yamamoto K, Morishige Y, Imakita K, Tsutumi N, Kawakata H, Ishida T, Tanaka H, Arima Y, Kitamura S, Hyodo D (2020) Tensile-dominant fractures observed in hydraulic fracturing laboratory experiment using eagle ford shale. Geophys J Inter 222: 769 – 780. 

Zang A, Oye V, Jousset P, Deichmann N, Gritto R, McGarr A, Majer E, Bruhn D (2014) Analysis of induced seismicity in geothermal reservoirs – an overview. Anal Induc Seism Geotherm Oper 52: 6 – 21.</pre>]]></content:encoded>
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					<title><![CDATA[EGU26 Wednesday Highlights]]></title>
					<link>https://blogs.egu.eu/divisions/gmpv/2026/05/06/egu26-wednesday-highlights/</link>
					<comments>https://blogs.egu.eu/divisions/gmpv/2026/05/06/egu26-wednesday-highlights/#comments</comments>
					<pubDate>Wed, 06 May 2026 00:13:30 +0000</pubDate>
					<dc:creator><![CDATA[Guto Paiva-Silva]]></dc:creator>
							<category><![CDATA[Conferences]]></category>
		<category><![CDATA[EGU]]></category>
		<category><![CDATA[EGU GMPV]]></category>
		<category><![CDATA[#EGU_GMPV]]></category>
		<category><![CDATA[EGU26]]></category>
		<category><![CDATA[General Assembly]]></category>
		<category><![CDATA[Highlights]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[We are midway through the General Assembly, and for those of us obsessed with the &#8220;unreachable&#8221; parts of our planet, Wednesday is the day to be in Vienna! While the GMPV division is busy monitoring active volcanoes, many of us will be found in the cross-listed sessions where Geochemistry meets Geodynamics and Tectonics. Whether you are a geochemist, a mineralogist, a petrologist, or a volcanologist, today’s program is packed with opportunities to dive deep into the data. Starting at 08:30, grab your morning coffee or beverage of choice and choose between the volcanic surface or the metamorphic depths: head to Room K1 for the &#8216;Monitoring active volcanoes&#8216; session (GMPV11.7). A huge highlight here: at 10:45, our newest GMPV Blog Editor-in-Chief, Agata Poganj, will be presenting her work on how hydrothermal alteration influences permeability (EGU26-341). It’s a great opportunity to see her latest field study and congratulate her on the new role! But if you prefer the high-pressure world, go to Room G2 for the &#8216;Fluid-rock interactions&#8216; session (TS1.5). At 08:30, Anna Rogowitz (solicited) kicks off with a look at HP-metamorphism induced porosity in mafic rocks (EGU26-9041). Immediately after, at 08:45, Andrew Smye will discuss linking reactive fluid flow to the rheology of eclogite-facies oceanic crust (EGU26-15970). Back from the break, the &#8220;unreachable&#8221; becomes accessible through two brilliant sessions: In Room 0.16: The session &#8216;Looking into the unreachable: Inclusions as snapshots&#8216; (GMPV1.1) begins. At 15:00, Alexander Pengg discusses methane and hydrogen in fluid inclusions (EGU26-6278), followed at 15:10 by Guangming Su, who presents a reconstruction of paleo-atmospheric nitrogen pressure using quartz-hosted inclusions (EGU26-5575). In Room G2: If you are interested in how grains influence plates, don’t miss &#8216;Fluid Flow and Rock Interaction Across Scales&#8216; (TS1.6). Catch Oliver Plümper (solicited) at 14:05 showcasing AI-driven permeability reconstruction (EGU26-3949), and Alessandro Petroccia at 14:15 on tracking dehydration in exhuming shear zones (EGU26-331). From 16:15, the poster halls become the focal point of the division. In Hall X1, you can dive deeper into the magmatic and volcanic flagship sessions: Monitoring active volcanoes (GMPV11.7), Magmatic textures: petrological insights into igneous processes (GMPV10.2), and Understanding magmatic processes: from magma storage to eruptive behaviour, and implications for volcanic hazard (GMPV10.3). You should also check out the latest work on Advances in understanding fluid migration systems and their surface manifestations: integrated, multidisciplinary data acquisition and interpretation (GMPV10.5), Volcanic degassing (GMPV10.6), and Volcanoes and their geothermal systems: Properties, risks and resources (GMPV10.7). If you can tear yourself away from the poster boards in Hall X1 for a quick deviation, head back to Room G2 for the Brittle and ductile deformation of Earth’s lithosphere: Mechanisms governing deformation style session (TS1.1) at 17:40 to catch Alessia Tagliaferri discuss the &#8220;memory of crystals&#8221; and microstructures in UHP garnets from Dora Maira (EGU26-9776). Finally, after a day of exploring everything from magmatic storage to mantle inclusions, it&#8217;s time to enjoy a night out in Vienna. Join the community for the Pride &amp; Allies Reception (NET13) from 18:00–19:30 at the Rooftop Foyer. It’s a wonderful space to celebrate diversity in geosciences and reflect on the day&#8217;s discussions before heading out for some traditional Viennese Schnitzel as we gear up for the final stretch of the conference!  Have a great Wednesday at #EGU26 and check out our blog tomorrow for tips for Thursday!]]></description>
													<content:encoded><![CDATA[<span style="font-weight: 400">We are midway through the General Assembly, and for those of us obsessed with the "unreachable" parts of our planet, Wednesday is the day to be in Vienna!
</span>

<span style="font-weight: 400">While the GMPV division is busy monitoring active volcanoes, many of us will be found in the cross-listed sessions where Geochemistry meets Geodynamics and Tectonics. Whether you are a geochemist, a mineralogist, a petrologist, or a volcanologist, today’s program is packed with opportunities to dive deep into the data.</span>

<span style="font-weight: 400">Starting at 08:30, grab your morning coffee or beverage of choice and choose between the volcanic surface or the metamorphic depths: h</span><span style="font-weight: 400">ead to </span><strong>Room K1</strong><span style="font-weight: 400"> for the </span><b>'<a href="https://www.egu26.eu/session/57808#Orals">Monitoring active volcanoes</a>'</b><span style="font-weight: 400"> session (</span><strong>GMPV11.7</strong><span style="font-weight: 400">). A huge highlight here: at </span>10:45<span style="font-weight: 400">, our newest </span><strong>GMPV Blog Editor-in-Chief, Agata Poganj</strong><span style="font-weight: 400">, will be presenting her work on how hydrothermal alteration influences permeability (</span>EGU26-341<span style="font-weight: 400">). It’s a great opportunity to see her latest field study and congratulate her on the new role! </span>

<span style="font-weight: 400">But if you prefer the high-pressure world, go to </span><strong>Room G2</strong><span style="font-weight: 400"> for the </span><b>'<a href="https://www.egu26.eu/session/56639#Orals">Fluid-rock interactions</a>'</b><span style="font-weight: 400"> session (</span><strong>TS1.5</strong><span style="font-weight: 400">). At </span>08:30, Anna Rogowitz (solicited) kicks off with a look at HP-metamorphism induced porosity in mafic rocks (EGU26-9041). Immediately after, at 08:45, Andrew Smye will discuss linking reactive fluid flow to the rheology of eclogite-facies oceanic crust (EGU26-15970).

<span style="font-weight: 400">Back from the break, the "unreachable" becomes accessible through two brilliant sessions:</span>
<ul>
 	<li style="font-weight: 400"><b>In </b><strong>Room 0.16</strong><b>:</b><span style="font-weight: 400"> The session </span><b>'<a href="https://www.egu26.eu/session/57076#Orals">Looking into the unreachable: Inclusions as snapshots</a>'</b><span style="font-weight: 400"> (</span><strong>GMPV1.1</strong><span style="font-weight: 400">) begins. At </span>15:00, Alexander Pengg discusses methane and hydrogen in fluid inclusions (EGU26-6278), followed at 15:10 by Guangming Su, who presents a reconstruction of paleo-atmospheric nitrogen pressure using quartz-hosted inclusions (EGU26-5575).</li>
 	<li style="font-weight: 400"><b>In </b><strong>Room G2</strong><b>:</b><span style="font-weight: 400"> If you are interested in how grains influence plates, don’t miss </span><b>'<a href="https://www.egu26.eu/session/56661#Orals">Fluid Flow and Rock Interaction Across Scales</a>'</b><span style="font-weight: 400"> (</span><strong>TS1.6</strong><span style="font-weight: 400">). Catch </span>Oliver Plümper (solicited) at 14:05 showcasing AI-driven permeability reconstruction (EGU26-3949), and Alessandro Petroccia at 14:15 on tracking dehydration in exhuming shear zones (EGU26-331).</li>
</ul>
<p data-path-to-node="5">From <b data-path-to-node="5" data-index-in-node="59">16:15</b>, the poster halls become the focal point of the division. In <strong>Hall X1</strong>, you can dive deeper into the magmatic and volcanic flagship sessions: <a href="https://www.egu26.eu/session/57808#Posters_on_site"><b data-path-to-node="0" data-index-in-node="151">Monitoring active volcanoes</b></a> (<strong>GMPV11.7</strong>), <a href="https://www.egu26.eu/session/57801#Posters_on_site"><b data-path-to-node="0" data-index-in-node="191">Magmatic textures: petrological insights into igneous processes</b></a> (<strong>GMPV10.2</strong>), and <a href="https://www.egu26.eu/session/57803#Posters_on_site"><b data-path-to-node="0" data-index-in-node="271">Understanding magmatic processes: from magma storage to eruptive behaviour, and implications for volcanic hazard</b></a> (<strong>GMPV10.3</strong>).</p>
<p data-path-to-node="5">You should also check out the latest work on <a href="https://www.egu26.eu/session/57802#Posters_on_site"><b data-path-to-node="1" data-index-in-node="45">Advances in understanding fluid migration systems and their surface manifestations: integrated, multidisciplinary data acquisition and interpretation</b></a> (<strong>GMPV10.5</strong>), <a href="https://www.egu26.eu/session/57810#Posters_on_site"><b data-path-to-node="1" data-index-in-node="207">Volcanic degassing</b></a> (<strong>GMPV10.6</strong>), and <a href="https://www.egu26.eu/session/57811#Posters_on_site"><b data-path-to-node="1" data-index-in-node="242">Volcanoes and their geothermal systems: Properties, risks and resources</b></a> (<strong>GMPV10.7</strong>).</p>
<p data-path-to-node="6">If you can tear yourself away from the poster boards in Hall X1 for a quick deviation, head back to <strong>Room G2</strong> for the <a href="https://www.egu26.eu/session/56119">Brittle and ductile deformation of Earth’s lithosphere: Mechanisms governing deformation style</a> session (<strong>TS1.1</strong>) at 17:40 to catch Alessia Tagliaferri discuss the "memory of crystals" and microstructures in UHP garnets from Dora Maira (EGU26-9776).</p>
<span style="font-weight: 400">Finally, after a day of exploring everything from magmatic storage to mantle inclusions, it's time to enjoy a night out in Vienna. Join the community for the </span><strong>Pride &amp; Allies Reception (NET13)</strong><span style="font-weight: 400"> from </span>18:00–19:30 at the Rooftop Foyer<span style="font-weight: 400">. It’s a wonderful space to celebrate diversity in geosciences and reflect on the day's discussions before heading out for some traditional Viennese Schnitzel as we gear up for the final stretch of the conference! </span>

<span style="font-weight: 400">Have a great Wednesday at #EGU26 and check out our blog tomorrow for tips for Thursday!</span>]]></content:encoded>
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					<title><![CDATA[Meet Tillys Petit, EGU Ocean Sciences' 2026 Outstanding Early Career Scientist Award Winner!]]></title>
					<link>https://blogs.egu.eu/divisions/os/2026/05/05/meet-tillys-petit-egu-ocean-sciences-2026-outstanding-early-career-scientist-award-winner/</link>
					<comments>https://blogs.egu.eu/divisions/os/2026/05/05/meet-tillys-petit-egu-ocean-sciences-2026-outstanding-early-career-scientist-award-winner/#comments</comments>
					<pubDate>Tue, 05 May 2026 21:33:20 +0000</pubDate>
					<dc:creator><![CDATA[Maurie Keppens]]></dc:creator>
							<category><![CDATA[News]]></category>
		<category><![CDATA[OS Announcements]]></category>
		<category><![CDATA[OS Research]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[On Monday 4 May, Tillys Petit delivered the OS Division Outstanding Early Career Scientist Award Lecture at EGU 2026 in Vienna. We chatted with her about the hidden engines driving the Atlantic Meridional Overturning Circulation, and why that matters for the future of our climate. Spoiler: it&#8217;s not just about the Labrador Sea! 🌊 Can you share your career journey with us? Did you always dream of becoming an oceanographer, and what inspired you to pursue this path? Growing up, I was always fascinated by research and understanding the natural world — particularly in areas like climate, the ocean, and health sciences. My aunt, a research scientist in microbiology, gave me an early glimpse into what a scientific career could look like, and that really stuck with me. That said, my path into oceanography wasn&#8217;t entirely straightforward. I initially studied biology before developing a stronger interest in Earth processes, which led me to geology. It was really during my master&#8217;s degree that I discovered a passion for ocean sciences and decided to specialise. After a PhD in France on the large-scale Atlantic Meridional Overturning Circulation (AMOC) in the subpolar North Atlantic, I moved to the US for my first postdoctoral position on the OSNAP project, where I focused on the mechanisms driving AMOC variability using observation-based datasets. Building on that experience, I joined the SNAP-DRAGON project in the UK to work on the intercomparison of key parameters across climate models. I&#8217;m currently at the National Oceanography Centre (NOC) in the UK, where I&#8217;m a co-investigator on the international RAPID project — which monitors ocean circulation at 26°N. 🌊 Could you describe the research that led to you receiving this award? My research focuses on improving our understanding of the AMOC: a system of ocean currents that plays a crucial role in our climate by transporting heat, freshwater, carbon, and nutrients throughout the Atlantic Ocean. For Europe in particular, it acts as a kind of heat pump, redistributing warmth from lower to higher latitudes and influencing everything from sea level to the weather patterns we experience day to day. To investigate this, I combine observational datasets and climate models, which allows me to cross-check findings and build a more complete picture. The core of my work has been to help shift the perspective on where and how dense waters are formed in the subpolar North Atlantic — a process that is a crucial driver of the AMOC. Before the OSNAP programme, the field was largely dominated by a Labrador-centric view. But results from the OSNAP observing system revealed that deep water production in the Labrador Sea is actually quite small, raising the question of where these waters are actually formed. My 2020 paper — which built directly on the landmark Lozier et al. 2019 OSNAP results — showed that these dense waters are largely formed outside the Labrador Sea, primarily through buoyancy forcing in the Irminger and Iceland basins. This implies that atmospheric forcing over these basins is likely a more important predictor of AMOC variability than forcing over the Labrador Sea, at least on observational timescales. That has significant implications — for climate modellers trying to improve projections of AMOC evolution, and for palaeoceanographers interpreting records of past AMOC variability who have so far focused mainly on the Labrador Sea. 🌊 What does this recognition mean to you, both personally and professionally? I was surprised and truly delighted to receive this award! On a personal level, it feels like a reflection not just of my own work, but of the many collaborations and interactions that have shaped it over the years, through my PhD, my postdocs, and my current position. Research is very much a collective effort, and I&#8217;ve been fortunate to work with supportive colleagues, mentors, and collaborators who have all contributed in different ways. Professionally, it is both encouraging and motivating at this stage of my career. It provides visibility within the ocean sciences community and reinforces the importance of the research we are doing at the NOC. 🌊 What have been some of the biggest challenges in your career, and were there key moments that shaped your path? One of the main challenges has been working on a system as complex as ocean circulation, where processes occur across a wide range of spatial and temporal scales and are inherently difficult to observe directly. This requires combining different approaches — models, observations, reanalyses — while constantly navigating and communicating uncertainty. My answer to that has largely been collaboration: seeking out colleagues with complementary expertise and learning from them. I&#8217;ve been fortunate in that respect. The AMOC research community, while specialised, is one where people know each other well. There are many workshops and conferences where you can build new connections, and that culture of openness has been invaluable to me. In many ways, the collaborations I&#8217;ve built across my postdoctoral positions have been the defining thread of my career so far. 🌊 Looking ahead, what are the most important questions about the Atlantic overturning circulation that you are excited to tackle? One of the most pressing open questions (and one that has been making headlines in recent years) is whether the AMOC could undergo a significant, or even abrupt, weakening as a result of anthropogenic climate change. This has been suggested by many climate models, but it remains difficult to observe directly. The longest continuous record we have is the RAPID time series, spanning the last 20 years, which is still not long enough to detect a statistically robust trend. And yet the stakes are high: even a relatively modest weakening of the AMOC could have substantial impacts on climate in Europe and beyond. Understanding by how much, and on what timescale, this weakening might occur is therefore one of the most urgent questions in our field. Answering it requires sustained, reliable observations. Arrays like RAPID and OSNAP are essential infrastructure. They allow us to monitor changes in real time, deepen our understanding of this complex system, and better assess potential risks. That is why I am genuinely excited to contribute to this effort through my role as co-investigator on the RAPID project. 🌊 What advice would you give to young scientists who want to make a difference in ocean circulation and the wider ocean sciences? Stay open to new ideas and don&#8217;t be afraid to follow an unconventional path. Ocean science is highly collaborative, and there is a real need for fresh perspectives and diverse skills. Fields like machine learning and AI are increasingly finding their way into ocean sciences, and that creates exciting opportunities for scientists who are willing to be curious and bring their own ideas to the table. I would also encourage early career researchers to seek out international experiences where possible. Immersing yourself in different scientific environments and ways of thinking can be genuinely transformative. It often leads to the collaborations that end up shaping your research for years to come! Thank you, Tillys, for the interview and for sharing your career insights and advice! Read more: Google Scholar profile of Tillys Petit Interviewed and edited by M. Keppens]]></description>
													<content:encoded><![CDATA[<span style="font-weight: 400">On Monday 4 May, Tillys Petit delivered the OS Division Outstanding Early Career Scientist Award Lecture at EGU 2026 in Vienna. We chatted with her about the hidden engines driving the Atlantic Meridional Overturning Circulation, and why that matters for the future of our climate. Spoiler: it's not just about the Labrador Sea!</span>

<h5>🌊<strong> Can you share your career journey with us? Did you always dream of becoming an oceanographer, and what inspired you to pursue this path? </strong></h5>

<span style="font-weight: 400">Growing up, I was always fascinated by research and understanding the natural world — particularly in areas like climate, the ocean, and health sciences. My aunt, a research scientist in microbiology, gave me an early glimpse into what a scientific career could look like, and that really stuck with me.</span>

<span style="font-weight: 400">That said, my path into oceanography wasn't entirely straightforward. I initially studied biology before developing a stronger interest in Earth processes, which led me to geology. It was really during my master's degree that I discovered a passion for ocean sciences and decided to specialise.</span>

<span style="font-weight: 400">After a PhD in France on the large-scale Atlantic Meridional Overturning Circulation (AMOC) in the subpolar North Atlantic, I moved to the US for my first postdoctoral position on the <a href="https://www.o-snap.org/">OSNAP </a>project, where I focused on the mechanisms driving AMOC variability using observation-based datasets. Building on that experience, I joined the SNAP-DRAGON project in the UK to work on the intercomparison of key parameters across climate models. I'm currently at the National Oceanography Centre (NOC) in the UK, where I'm a co-investigator on the international <a href="https://rapid.ac.uk/">RAPID </a>project — which monitors ocean circulation at 26°N.</span>

<h5>🌊<strong> Could you describe the research that led to you receiving this award? </strong></h5>

<span style="font-weight: 400">My research focuses on improving our understanding of the AMOC: a system of ocean currents that plays a crucial role in our climate by transporting heat, freshwater, carbon, and nutrients throughout the Atlantic Ocean. For Europe in particular, it acts as a kind of heat pump, redistributing warmth from lower to higher latitudes and influencing everything from sea level to the weather patterns we experience day to day.</span>

<span style="font-weight: 400">To investigate this, I combine observational datasets and climate models, which allows me to cross-check findings and build a more complete picture. The core of my work has been to help shift the perspective on where and how dense waters are formed in the subpolar North Atlantic — a process that is a crucial driver of the AMOC. Before the OSNAP programme, the field was largely dominated by a Labrador-centric view. But results from the OSNAP observing system revealed that deep water production in the Labrador Sea is actually quite small, raising the question of where these waters are actually formed.</span>

[caption id="attachment_2932" align="aligncenter" width="500"]<a href="https://blogs.egu.eu/divisions/os/files/2026/05/aa2dfdf5-455e-4581-b51f-451f5613358a.jpg"><img class="wp-image-2932 " src="https://blogs.egu.eu/divisions/os/files/2026/05/aa2dfdf5-455e-4581-b51f-451f5613358a.jpg" alt="" width="1000" height="900" /></a> Image: Tillys on a field campaign.[/caption]

<span style="font-weight: 400"><a href="https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2020GL091028">My 2020 paper</a> — which built directly on the landmark <a href="https://www.science.org/doi/10.1126/science.aau6592">Lozier et al. 2019</a> OSNAP results — showed that these dense waters are largely formed outside the Labrador Sea, primarily through buoyancy forcing in the Irminger and Iceland basins. This implies that atmospheric forcing over these basins is likely a more important predictor of AMOC variability than forcing over the Labrador Sea, at least on observational timescales. That has significant implications — for climate modellers trying to improve projections of AMOC evolution, and for palaeoceanographers interpreting records of past AMOC variability who have so far focused mainly on the Labrador Sea.</span>

<h5>🌊<strong> What does this recognition mean to you, both personally and professionally? </strong></h5>

<span style="font-weight: 400">I was surprised and truly delighted to receive this award! On a personal level, it feels like a reflection not just of my own work, but of the many collaborations and interactions that have shaped it over the years, through my PhD, my postdocs, and my current position. Research is very much a collective effort, and I've been fortunate to work with supportive colleagues, mentors, and collaborators who have all contributed in different ways.</span>

<span style="font-weight: 400">Professionally, it is both encouraging and motivating at this stage of my career. It provides visibility within the ocean sciences community and reinforces the importance of the research we are doing at the NOC.</span>

[caption id="attachment_2932" align="aligncenter" width="500"]<a href="https://blogs.egu.eu/divisions/os/files/2026/05/c01ccd51-6fbe-4d65-8a8f-cfaf48b2bedc-2.jpg"><img class="wp-image-2932 " src="https://blogs.egu.eu/divisions/os/files/2026/05/c01ccd51-6fbe-4d65-8a8f-cfaf48b2bedc-2.jpg" alt="" width="1000" height="900" /></a> Image: Tillys on a field campaign.[/caption]

<h5>🌊<strong> What have been some of the biggest challenges in your career, and were there key moments that shaped your path? </strong></h5>

<span style="font-weight: 400">One of the main challenges has been working on a system as complex as ocean circulation, where processes occur across a wide range of spatial and temporal scales and are inherently difficult to observe directly. This requires combining different approaches — models, observations, reanalyses — while constantly navigating and communicating uncertainty. My answer to that has largely been collaboration: seeking out colleagues with complementary expertise and learning from them.</span>

<span style="font-weight: 400">I've been fortunate in that respect. The AMOC research community, while specialised, is one where people know each other well. There are many workshops and conferences where you can build new connections, and that culture of openness has been invaluable to me. In many ways, the collaborations I've built across my postdoctoral positions have been the defining thread of my career so far.</span>

<h5>🌊<strong> Looking ahead, what are the most important questions about the Atlantic overturning circulation that you are excited to tackle? </strong></h5>

<span style="font-weight: 400">One of the most pressing open questions (and one that has been making headlines in recent years) is whether the AMOC could undergo a significant, or even abrupt, weakening as a result of anthropogenic climate change. This has been suggested by many climate models, but it remains difficult to observe directly. The longest continuous record we have is the RAPID time series, spanning the last 20 years, which is still not long enough to detect a statistically robust trend.</span>

<span style="font-weight: 400">And yet the stakes are high: even a relatively modest weakening of the AMOC could have substantial impacts on climate in Europe and beyond. Understanding by how much, and on what timescale, this weakening might occur is therefore one of the most urgent questions in our field.</span>

<span style="font-weight: 400"> Answering it requires sustained, reliable observations. Arrays like RAPID and OSNAP are essential infrastructure. They allow us to monitor changes in real time, deepen our understanding of this complex system, and better assess potential risks. That is why I am genuinely excited to contribute to this effort through my role as co-investigator on the RAPID project.</span>

<h5>🌊<strong> What advice would you give to young scientists who want to make a difference in ocean circulation and the wider ocean sciences? </strong></h5>

<span style="font-weight: 400"> Stay open to new ideas and don't be afraid to follow an unconventional path. Ocean science is highly collaborative, and there is a real need for fresh perspectives and diverse skills. Fields like machine learning and AI are increasingly finding their way into ocean sciences, and that creates exciting opportunities for scientists who are willing to be curious and bring their own ideas to the table.</span>

<span style="font-weight: 400"> I would also encourage early career researchers to seek out international experiences where possible. Immersing yourself in different scientific environments and ways of thinking can be genuinely transformative. It often leads to the collaborations that end up shaping your research for years to come! </span>

<h5><strong> Thank you, Tillys, for the interview and for sharing your career insights and advice! </strong></h5>

[caption id="attachment_2932" align="aligncenter" width="500"]<a href="https://blogs.egu.eu/divisions/os/files/2026/05/Screenshot-2026-05-05-223243.png"><img class="wp-image-2932 " src="https://blogs.egu.eu/divisions/os/files/2026/05/Screenshot-2026-05-05-223243.png" alt="" width="1400" height="1000" /></a> Image: Tillys giving her award lecture and receiving the OS Division Outstanding ECS Award![/caption]

<h5><strong> Read more: </strong></h5>

<a href="https://scholar.google.com/citations?user=S559Z9UAAAAJ&amp;hl=fr">Google Scholar profile of Tillys Petit</a> 

<span style="font-weight: 400"><em>Interviewed and edited by M. Keppens</em> </span>



]]></content:encoded>
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					<title><![CDATA[EGU26 Tuesday Highlights]]></title>
					<link>https://blogs.egu.eu/divisions/gmpv/2026/05/05/egu26-tuesday-highlights/</link>
					<comments>https://blogs.egu.eu/divisions/gmpv/2026/05/05/egu26-tuesday-highlights/#comments</comments>
					<pubDate>Tue, 05 May 2026 04:35:41 +0000</pubDate>
					<dc:creator><![CDATA[Agata Poganj]]></dc:creator>
							<category><![CDATA[Conferences]]></category>
		<category><![CDATA[EGU]]></category>
		<category><![CDATA[EGU GMPV]]></category>
		<category><![CDATA[Session in the Spotlight]]></category>
		<category><![CDATA[#EGU_GMPV]]></category>
		<category><![CDATA[EGU26]]></category>
		<category><![CDATA[General Assembly]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Welcome all to the second day of the EGU26 General Assembly! If you are still trying to figure out what sessions not to miss, help yourself with a quick summary tailored for a GMPV crowd! Morning sessions Start your day with a joint TS1.6/EMRP1/GD5/GMPV7 poster session titled &#8221;Fluid Flow and Rock Interaction Across Scales: From Grains to Plates&#8221;. Or choose from many of the morning short courses: &#8221;Best Practices for Early Career Researcher (ECR) Engagement and Empowerment&#8221; is ideal for PhDs or first-time PostDocs &#8221;European Research Council (ERC) Funding Opportunities&#8221; is ideal for more seasoned researchers &#8221;The LGBT Pride group at EGU: How to find and build your community&#8221; for the LGBT community and allies alike After the ECS Coffee break catch-up in the EGU booth, Hall X2, be sure to stop by the GMPV10.3 session, where presentations will focus on explosive vs effusive eruption styles and magma plumbing systems. An alternative is to come learn from other people&#8217;s mistakes in a fun and innovative session co-organised across 14 divisions, titled &#8221;BUGS: Blunders, Unexpected Glitches, and Surprises&#8221; where big ideas turned out to be less than ideal. Afternoon session Early afternoon, from 14:00 to 15:45, can be blocked out for a GMPV5.1. session focused on magmatic volcanism and magmatic ore deposits, &#8221;Magmas, volatiles, and triggers of volcanism and ore mineralisation&#8221;. From 16:20 to 16:40, Mathieu Colombier will present a combined image and chemistry analysis addressing the 2022 Honga eruption, in his &#8221;Ash generation and transport during explosive submarine eruptions&#8221; talk. Simultaneously, GMPV10.2 session &#8221;Magmatic textures: petrological insights into igneous processes&#8221; highlights presentations from Janine Birbaum &#8221;Addressing the elephant in the room: combined experimental and numerical approaches for scaling to volcanic conditions&#8221; and Lydéric France &#8221;Chemical maps as a memory of magma solidification: from crystallization onset to trapped melt&#8221;. Don&#8217;t forget to enjoy yourself and finish off the day with the ECS Networking Reception at the Rooftop Foyer and Foyer C from 18:00 to 19:30!]]></description>
													<content:encoded><![CDATA[Welcome all to the second day of the EGU26 General Assembly!

If you are still trying to figure out what sessions not to miss, help yourself with a quick summary tailored for a GMPV crowd!

<strong>Morning sessions</strong>

Start your day with a joint TS1.6/EMRP1/GD5/GMPV7 poster session titled ''<strong><a href="https://www.egu26.eu/session/56661" data-id="56661">Fluid Flow and Rock Interaction Across Scales: From Grains to Plates</a></strong>''. Or choose from many of the morning short courses:
<ul>
 	<li>''<strong><a href="https://www.egu26.eu/session/57786" data-id="57786">Best Practices for Early Career Researcher (ECR) Engagement and Empowerment</a></strong>'' is ideal for PhDs or first-time PostDocs</li>
 	<li>''<a href="https://www.egu26.eu/session/57868" data-id="57868"><strong>European Research Council (ERC) Funding Opportunities</strong></a>'' is ideal for more seasoned researchers</li>
 	<li>''<strong><a href="https://www.egu26.eu/session/57777" data-id="57777">The LGBT Pride group at EGU: How to find and build your community</a></strong>'' for the LGBT community and allies alike</li>
</ul>
After the <strong>ECS </strong><span style="margin: 0px;padding: 0px"><strong>Coffee break catch-up </strong>in the EGU booth, Hall X2, be sure to stop by the <a href="https://meetingorganizer.copernicus.org/EGU26/session/57803" target="_blank" rel="noopener"><strong>GMPV10.3 </strong></a>session, where presentations will focus on explosive vs effusive eruption styles</span> and magma plumbing systems. An alternative is to come learn from other people's mistakes in a fun and innovative session co-organised across 14 divisions, titled ''<strong><a href="https://www.egu26.eu/session/56997" data-id="56997">BUGS: Blunders, Unexpected Glitches, and Surprises</a></strong>'' where big ideas turned out to be less than ideal.

<strong>Afternoon session</strong>

Early afternoon, from 14:00 to 15:45, can be blocked out for a GMPV5.1. session focused on magmatic volcanism and magmatic ore deposits, ''<strong><a href="https://meetingorganizer.copernicus.org/EGU26/session/57074" data-id="57074">Magmas, volatiles, and triggers of volcanism and ore mineralisation</a></strong>''.

From 16:20 to 16:40, Mathieu Colombier will present a combined image and chemistry analysis addressing the 2022 Honga eruption, in his ''<a class="co_mto_abstractHTML-html-toggler" href="https://meetingorganizer.copernicus.org/EGU26/EGU26-13749.html" target="#" data-id="36916662"><strong>Ash generation and transport during explosive submarine eruptions</strong></a>'' talk. Simultaneously, GMPV10.2 session ''<a href="https://meetingorganizer.copernicus.org/EGU26/session/57801"><strong class="link-coloured">Magmatic textures: petrological insights into igneous processes</strong></a>'' highlights presentations from Janine Birbaum ''<a class="co_mto_abstractHTML-html-toggler" href="https://meetingorganizer.copernicus.org/EGU26/EGU26-14160.html" target="#" data-id="380135"><strong>Addressing the elephant in the room: combined experimental and numerical approaches for scaling to volcanic conditions</strong></a>'' and Lydéric France ''<a class="co_mto_abstractHTML-html-toggler" href="https://meetingorganizer.copernicus.org/EGU26/EGU26-2830.html" target="#" data-id="368791"><strong>Chemical maps as a memory of magma solidification: from crystallization onset to trapped melt</strong></a>''.

Don't forget to enjoy yourself and finish off the day with the <strong><a href="https://www.egu26.eu/pg/NET_050526#:~:text=NET10,ECS%20Networking%20Reception">ECS Networking Reception</a></strong> at the Rooftop Foyer and Foyer C from 18:00 to 19:30!]]></content:encoded>
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