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			<title>EGU Blogs - Recent Division Posts</title>
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					<title><![CDATA[Meet your ECS Rep – Archita Bhattacharyya]]></title>
					<link>https://blogs.egu.eu/divisions/hs/2026/06/19/meet-your-ecs-rep-archita-bhattacharyya/</link>
					<comments>https://blogs.egu.eu/divisions/hs/2026/06/19/meet-your-ecs-rep-archita-bhattacharyya/#comments</comments>
					<pubDate>Fri, 19 Jun 2026 13:21:00 +0000</pubDate>
					<dc:creator><![CDATA[Annegret Roessler]]></dc:creator>
							<category><![CDATA[Early Career Scientists]]></category>
		<category><![CDATA[ECS]]></category>
		<category><![CDATA[ECS rep]]></category>
		<category><![CDATA[HS Division]]></category>
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											<description><![CDATA[Archita Bhattacharyya is an Environmental Scientist and a research and development fellow at the Department of Environment, Food and Rural affairs, England. For 2026, she is the Early Career Scientist Representative for the Hydrological Sciences division. Can you tell us about the focus of your research? In my PhD, I focused on groundwater microbiology, especially how microbial communities change across space and time in different aquifer geologies. This involved studying the aquifer microbiology using flow cytometry and DNA sequencing and relating the microbiology data to aquifer type, and environmental factors like groundwater recharge and chemistry. After my PhD, I moved into a policy fellowship role, where I looked into the applications of engineering biology for sludge and soil remediation, particularly for emerging contaminants like plastics and PFAS. Recently, I have started another job where I’ll use my science skills to monitor, evaluate and report on the effectiveness of nature restoration policies. So although the research topic has changed, I am still interested in how science can help us better understand and manage environmental systems. What originally inspired you to go into this field? I first became interested in this field during my Master’s dissertation on groundwater quality, where I learnt about all the unknowns in the subsurface world. When I came across a PhD project on groundwater microbiology, I was immediately drawn to how novel it felt. I was excited by the idea of learning about subsurface life and combining my hydrogeological background with molecular biology methods.  Looking back, what was the most challenging aspect of your PhD and what was the most enjoyable? The most challenging part was definitely the time management. It was a large project with several workstreams, and at times I pushed myself too hard trying to keep everything moving.  The most enjoyable part was the fieldwork. I loved travelling to new places and towns, and making memories along the way. I also really enjoyed working with my datasets. Every time I learned a new piece of code or created a figure that clearly showed something meaningful, it gave me a real sense of accomplishment. How was your experience of post-PhD life so far? After PhD, I have been working in policy roles, quite different from a typical academic career trajectory. Straight after finishing the PhD, I started an R&amp;D fellowship in the Department of Environment, Food and Rural Affairs, England, where I worked on a project involving engineering biology for sludge treatment, another very novel and exciting topic. After the end of this fellowship, now I am working on another policy role, where I’ll use my science skills to monitor and evaluate nature restoration policies. Overall, these roles allowed me to see how science translates into real-life decisions and shapes regional and national policies. What advice would you give to an Early Career Researcher about the challenges they might face in academic life? This is advice I also have to remind myself of: not every research career is linear. Everyone faces difficult phases. That is why celebrating small wins really matters. It will help you keep going. I would also say that science is not strictly limited to academia. The skills we develop as researchers are valuable in many other spaces, including policy and industry. My own move from academia into policy has been eye-opening, and it has made me think more openly and flexibly about what a scientific career can look like. Why did you decide to become an Early Career Scientist Representative and how has being a part of the ECS team impacted you? At first, I joined because I wanted to build my skills in organisation, project management, and team-management, while also becoming part of a wider scientific network. Over time, though, my motivation changed and I genuinely enjoy being part of the ECS team. It has given me opportunities to do creative things like podcasting and blog writing, and it has connected me with a wonderful group of people. It has also helped me grow in confidence, especially in communication. Coming from a non-English-medium school, that has been a very meaningful experience for me. What do you plan to achieve as the ECS rep this year? This year, I would really like to maintain and enhance the great work our team is already doing. We run a lot of valuable activities, so one of my priorities is to streamline processes and improve how we manage ongoing projects. I would like us to minimise workload where possible while still maximising the impact of what we produce. What do you like about the role? What I like most is the chance to work with talented, motivated, and genuinely inspiring people. The ECS team is full of brilliant scientists, but also kind and creative individuals. Through the podcast, I have had the opportunity to speak with many hydrologists about their research and career experiences, and I have found those conversations incredibly engaging. What advice would you give to other early career scientists who perhaps want to contribute to the ECS network but are hesitant? I would say: join us and contribute whatever you can. There is space for different kinds of involvement, from scientific blog writing and podcasting to more creative or organisational activities. You can be involved a little or a lot. It is a great way to build skills outside your own research, meet new people, and be part of a broader community. ]]></description>
													<content:encoded><![CDATA[<span style="font-weight: 400">Archita Bhattacharyya is an Environmental Scientist and a research and development fellow at the Department of Environment, Food and Rural affairs, England. For 2026, she is the Early Career Scientist Representative for the Hydrological Sciences division.</span>
<h1><span style="font-weight: 400">Can you tell us about the focus of your research?</span></h1>
<span style="font-weight: 400">In my PhD, I focused on groundwater microbiology, especially how microbial communities change across space and time in different aquifer geologies. This involved studying the aquifer microbiology using flow cytometry and DNA sequencing and relating the microbiology data to aquifer type, and environmental factors like groundwater recharge and chemistry.</span>

<span style="font-weight: 400">After my PhD, I moved into a policy fellowship role, where I looked into the applications of engineering biology for sludge and soil remediation, particularly for emerging contaminants like plastics and PFAS. </span><span style="font-weight: 400">Recently, I have started another job where I’ll use my science skills to monitor, evaluate and report on the effectiveness of nature restoration policies.</span><span style="font-weight: 400"> So although the research topic has changed, I am still interested in how science can help us better understand and manage environmental systems.</span>
<h1><span style="font-weight: 400">What originally inspired you to go into this field?</span></h1>
<span style="font-weight: 400">I first became interested in this field during my Master’s dissertation on groundwater quality, where I learnt about all the unknowns in the subsurface world. When I came across a PhD project on groundwater microbiology, I was immediately drawn to how novel it felt. I was excited by the idea of learning about subsurface life and combining my hydrogeological background with molecular biology methods.  </span>
<h1><span style="font-weight: 400">Looking back, what was the most challenging aspect of your PhD and what was the most enjoyable?</span></h1>
<span style="font-weight: 400">The most challenging part was definitely the time management. It was a large project with several workstreams, and at times I pushed myself too hard trying to keep everything moving. </span>

<span style="font-weight: 400">The most enjoyable part was the fieldwork. I loved travelling to new places and towns, and making memories along the way. I also really enjoyed working with my datasets. Every time I learned a new piece of code or created a figure that clearly showed something meaningful, it gave me a real sense of accomplishment.</span>
<h1><span style="font-weight: 400">How was your experience of post-PhD life so far?</span></h1>
<span style="font-weight: 400">After PhD, I have been working in policy roles, quite different from a typical academic career trajectory</span><span style="font-weight: 400">. Straight after finishing the PhD, I started an R&amp;D fellowship in the Department of Environment, Food and Rural Affairs, England, where I worked on a project involving engineering biology for sludge treatment, another very novel and exciting topic. </span><span style="font-weight: 400">After the end of this fellowship, now I am working on another policy role, where I’ll use my science skills to monitor and evaluate nature restoration policies. Overall, these roles allowed me to see how science translates into real-life decisions and shapes regional and national policies.</span>

[caption id="attachment_13957" align="aligncenter" width="534"]<img class="size-full wp-image-13957" src="https://blogs.egu.eu/divisions/hs/files/2026/06/Archita_cake.jpg" alt="" width="534" height="540" /> Feeling absolutely stoked by the Sludge-cake, customised by a colleague, on Defra R&amp;D fellowship ending day.[/caption]
<h1><span style="font-weight: 400">What advice would you give to an Early Career Researcher about the challenges they might face in academic life?</span></h1>
<span style="font-weight: 400">This is advice I also have to remind myself of: not every research career is linear. Everyone faces difficult phases. That is why celebrating small wins really matters. It will help you keep going.</span>

<span style="font-weight: 400">I would also say that science is not strictly limited to academia. The skills we develop as researchers are valuable in many other spaces, including policy and industry. My own move from academia into policy has been eye-opening, and it has made me think more openly and flexibly about what a scientific career can look like.</span>
<h1><span style="font-weight: 400">Why did you decide to become an Early Career Scientist Representative and how has being a part of the ECS team impacted you?</span></h1>
<span style="font-weight: 400">At first, I joined because I wanted to build my skills in organisation, project management, and team-management, while also becoming part of a wider scientific network. Over time, though, my motivation changed and I genuinely enjoy being part of the ECS team.</span>

<span style="font-weight: 400">It has given me opportunities to do creative things like podcasting and blog writing, and it has connected me with a wonderful group of people. It has also helped me grow in confidence, especially in communication. Coming from a non-English-medium school, that has been a very meaningful experience for me.</span>

[caption id="attachment_13958" align="aligncenter" width="508"]<img class="size-full wp-image-13958" src="https://blogs.egu.eu/divisions/hs/files/2026/06/Archita_hydromeet.png" alt="" width="508" height="540" /> With the outgoing and incoming ECS reps at the Hydromeet event of GA 2025 (from left: Archita, Melissa and Christina)[/caption]
<h1><span style="font-weight: 400">What do you plan to achieve as the ECS rep this year?</span></h1>
<span style="font-weight: 400">This year, I would really like to maintain and enhance the great work our team is already doing. We run a lot of valuable activities, so one of my priorities is to streamline processes and improve how we manage ongoing projects. I would like us to minimise workload where possible while still maximising the impact of what we produce.</span>
<h1><span style="font-weight: 400">What do you like about the role?</span></h1>
<span style="font-weight: 400">What I like most is the chance to work with talented, motivated, and genuinely inspiring people. The ECS team is full of brilliant scientists, but also kind and creative individuals. Through the podcast, I have had the opportunity to speak with many hydrologists about their research and career experiences, and I have found those conversations incredibly engaging.</span>
<h1><span style="font-weight: 400">What advice would you give to other early career scientists who perhaps want to contribute to the ECS network but are hesitant?</span></h1>
<span style="font-weight: 400">I would say: join us and contribute whatever you can. There is space for different kinds of involvement, from scientific blog writing and podcasting to more creative or organisational activities. You can be involved a little or a lot. It is a great way to build skills outside your own research, meet new people, and be part of a broader community. </span>]]></content:encoded>
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					<title><![CDATA[Dialogue is essential for advancing hydrological science]]></title>
					<link>https://blogs.egu.eu/divisions/hs/2026/06/18/dialogue-is-essential-for-advancing-hydrological-science/</link>
					<comments>https://blogs.egu.eu/divisions/hs/2026/06/18/dialogue-is-essential-for-advancing-hydrological-science/#comments</comments>
					<pubDate>Thu, 18 Jun 2026 08:00:14 +0000</pubDate>
					<dc:creator><![CDATA[Bettina Schaefli]]></dc:creator>
							<category><![CDATA[Conference highlights]]></category>
		<category><![CDATA[EGU]]></category>
		<category><![CDATA[Opinion]]></category>
		<category><![CDATA[Dalton Medal]]></category>
		<category><![CDATA[EGU2026]]></category>
		<category><![CDATA[EGU26]]></category>
		<category><![CDATA[hydrology]]></category>
		<category><![CDATA[modelling]]></category>
		<category><![CDATA[water resources]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[A little over a decade ago, a group of us argued that “it takes a village to raise a hydrologist”. The skills and knowledge any hydrologist should be exposed to during their training goes far beyond what a single person can do and know. Even more, the experience of how water shapes and interacts with diverse landscapes all around the world cannot be obtained by a single person. This is true especially today, when human activity interacts with this landscape and the water cycle almost everywhere on our planet. But, you might argue, we also have more data than ever before – more satellites circle and observe the Earth, and more powerful AI methods and diverse models analyse, utilize and produce data at incredible speed. Our main knowledge repository, in which we record our hydrological experiences, meaning the papers we publish in our journals, is growing so rapidly that we now publish about 10,000 papers a year just in the main water journals. Should we just rely on AI? Some argue that knowledge accumulation alone equals scientific advancement, but it is increasingly difficult – and maybe impossible – to know what knowledge we jointly possess and where our knowledge gaps lie. If you think of our knowledge as pieces in a puzzle, then any new student of hydrology would typically start by finding the pieces that make up the edges of the puzzle. Once you have the outside frame of the puzzle, you slowly work inwards because now you can better see where further pieces belong – you have a frame of reference. In hydrology, our puzzle pieces have become so numerous that it is becoming impossible to find the edges. Certainly, for any single person. We can use AI to help us find and organize the puzzle pieces – e.g. Stein et al. used natural language processing to find and geolocate several hundred thousand papers on hydro-hazards out of a corpus of millions. But we are still figuring out how to do this, and it is not satisfying to have our knowledge organized and gaps identified by AI. At least not alone, among other reasons because current AI systems lack epistemic humility, meaning that they are confident even when they are wrong or when the existing database is insufficient. Scientific dialogue is a complementary path An important complementary path is dialogue. Scientific dialogue is essential for any scientific community, especially for hydrology where we deal with an incredibly diverse subject – water on our planet. What do I mean by scientific dialogue? Well, underlying all of science is a scientific method in which we use our current understanding to develop new theory, from which we derive testable hypotheses, which we compare with available evidence. If hypotheses and evidence are consistent, then the theory is corroborated, if not, then we have to modify the theory. Every scientific dialogue between two researchers is a small-scale application of this scientific method. In this way, we continuously debate whether our ideas and opinions withstand exposure to evidence. This is often not straightforward given the large uncertainties and biases in our observations. They leave room for debate on whether inconsistencies between hypotheses and evidence should be attributed to poor theory or poor data. Scientific dialogue is also a great equalizer in science. Standing at your poster at a scientific conference, it does not matter whether you are a first year PhD student or a senior professor – both must equally defend their work with reference to available evidence, not based on opinion or authority. Such dialogue within our community is key to identifying the puzzle pieces that make up the edges of our knowledge, and to decide where new pieces should go. It should help us to identify which puzzle pieces are truly new, which provide further corroboration for previous findings, or which synthesize multiple earlier puzzle pieces into a single new one. It is critically important that this dialogue happens across different generations of hydrologists. When I finished my PhD – about 25 years ago – the amount of literature was dramatically smaller. I could actually read a significant fraction of it and establish the edges of the puzzle I was trying to put together. Thus, adding new pieces was easier then, and it has remained easier for me since because of this original framing. It is vastly more difficult to achieve this framing today. Not because we were smarter then (of course not), but because the puzzle was so much smaller. So, dialogue is more essential today if we want to ensure that our community puzzle is becoming more and more complete, and more transparent to everybody. And finally, some words about the role of this dialogue beyond science. Outside of science, civilized dialogue is increasingly in decline. While this trend is depressing, I am encouraged by seeing that I can still have scientific dialogues even with people I strongly disagree with. Because we have a dialogue on the same terms. And maybe also because we have &#8216;epistemic humility&#8217;, which means we are aware of the limitations of our knowledge and that our &#8216;truths&#8217; are tentative &#8211; they may be falsified in the future by the emergence of new evidence. I believe that this is an important message we should share with the public. A dialogue that is focused on testing ideas and opinions against evidence – as difficult as this is – is a way to communicate and maybe even advance joint knowledge. &nbsp; Acknowledgements: Some of these thoughts originate from my Dalton Medal Lecture at EGU 2026. Thanks to Francesca Pianosi for the reference to epistemic humility and critical comments on a previous draft of this blog entry.]]></description>
													<content:encoded><![CDATA[A little over a decade ago, a group of us argued that “<a href="https://hess.copernicus.org/articles/16/3405/2012/">it takes a village to raise a hydrologist</a>”. The skills and knowledge any hydrologist should be exposed to during their training goes far beyond what a single person can do and know. Even more, the experience of how water shapes and interacts with diverse landscapes all around the world cannot be obtained by a single person. This is true especially today, when human activity interacts with this landscape and the water cycle almost everywhere on our planet.

But, you might argue, we also have more data than ever before – more satellites circle and observe the Earth, and more powerful AI methods and diverse models analyse, utilize and produce data at incredible speed. Our main knowledge repository, in which we record our hydrological experiences, meaning the papers we publish in our journals, is growing so rapidly that we now<a href="https://onlinelibrary.wiley.com/doi/full/10.1002/hyp.14742"> publish about 10,000 papers a year just in the main water journals</a>.
<h3>Should we just rely on AI?</h3>
Some argue that <a href="https://onlinelibrary.wiley.com/doi/10.1111/j.1468-0068.2007.00638.x">knowledge accumulation alone equals scientific advancement,</a> but it is increasingly difficult – and maybe impossible – to know what knowledge we jointly possess and where our knowledge gaps lie. If you think of our knowledge as pieces in a puzzle, then any new student of hydrology would typically start by finding the pieces that make up the edges of the puzzle. Once you have the outside frame of the puzzle, you slowly work inwards because now you can better see where further pieces belong – you have a frame of reference. In hydrology, our puzzle pieces have become so numerous that it is becoming impossible to find the edges. Certainly, for any single person. We can use AI to help us find and organize the puzzle pieces – e.g. <a href="https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2024EF004590">Stein et al.</a> used natural language processing to find and geolocate several hundred thousand papers on hydro-hazards out of a corpus of millions. But we are still figuring out how to do this, and it is not satisfying to have our knowledge organized and gaps identified by AI. At least not alone, among other reasons because current <a href="https://www.nature.com/articles/s41591-025-04013-x">AI systems lack epistemic humility</a>, meaning that they are confident even when they are wrong or when the existing database is insufficient.
<h3>Scientific dialogue is a complementary path</h3>
An important complementary path is <strong><em>dialogue</em></strong>. Scientific dialogue is essential for any scientific community, especially for hydrology where we deal with an incredibly diverse subject – water on our planet. What do I mean by scientific dialogue? Well, underlying all of science is a <strong>scientific method</strong> in which we use our current understanding to develop <strong>new theory,</strong> from which we derive <strong>testable hypotheses</strong>, which we compare with available <strong>evidence</strong>. If hypotheses and evidence are consistent, then the theory is corroborated, if not, then we have to modify the theory. Every scientific dialogue between two researchers is a small-scale application of this scientific method. In this way, we continuously debate whether our ideas and opinions withstand exposure to evidence. This is often not straightforward given the large uncertainties and biases in our observations. They leave room for debate on whether inconsistencies between hypotheses and evidence should be attributed to poor theory or poor data. Scientific dialogue is also a great equalizer in science. Standing at your poster at a scientific conference, it does not matter whether you are a first year PhD student or a senior professor – both must equally defend their work with reference to available evidence, not based on opinion or authority.

Such dialogue within our community is key to identifying the puzzle pieces that make up the edges of our knowledge, and to decide where new pieces should go. It should help us to identify which puzzle pieces are truly new, which provide further corroboration for previous findings, or which synthesize multiple earlier puzzle pieces into a single new one. It is critically important that this dialogue happens across different generations of hydrologists. When I finished my PhD – about 25 years ago – the amount of literature was dramatically smaller. I could actually read a significant fraction of it and establish the edges of the puzzle I was trying to put together. Thus, adding new pieces was easier then, and it has remained easier for me since because of this original framing. It is vastly more difficult to achieve this framing today. Not because we were smarter then (of course not), but because the puzzle was so much smaller. So, dialogue is more essential today if we want to ensure that our community puzzle is becoming more and more complete, and more transparent to everybody.

And finally, some words about the role of this dialogue beyond science. Outside of science, civilized dialogue is increasingly in decline. While this trend is depressing, I am encouraged by seeing that I can still have scientific dialogues even with people I strongly disagree with. Because we have a dialogue on the same terms. And maybe also because we have 'epistemic humility', which means we are aware of the limitations of our knowledge and that our 'truths' are tentative - they may be falsified in the future by the emergence of new evidence. I believe that this is an important message we should share with the public. A dialogue that is focused on testing ideas and opinions against evidence – as difficult as this is – is a way to communicate and maybe even advance joint knowledge.

&nbsp;

<em><strong>Acknowledgements: </strong></em>Some of these thoughts originate from my<a href="https://www.egu.eu/awards-medals/john-dalton/2026/thorsten-wagener/"> Dalton Medal Lecture at EGU 2026</a>. Thanks to Francesca Pianosi for the reference to epistemic humility and critical comments on a previous draft of this blog entry.]]></content:encoded>
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					<slash:comments>1</slash:comments>
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					<title><![CDATA[Modeling the full spectrum of observed seismicity: Insights from friction laws, fault instability, and fault-zone mechanics]]></title>
					<link>https://blogs.egu.eu/divisions/gd/2026/06/17/modeling-the-full-spectrum-of-observed-seismicity-insights-from-friction-laws-fault-instability-and-fault-zone-mechanics/</link>
					<comments>https://blogs.egu.eu/divisions/gd/2026/06/17/modeling-the-full-spectrum-of-observed-seismicity-insights-from-friction-laws-fault-instability-and-fault-zone-mechanics/#comments</comments>
					<pubDate>Wed, 17 Jun 2026 08:44:53 +0000</pubDate>
					<dc:creator><![CDATA[Editorial Team 2]]></dc:creator>
							<category><![CDATA[Geodynamics 101]]></category>
		<category><![CDATA[News & Views]]></category>
		<category><![CDATA[Earthquake]]></category>
		<category><![CDATA[fault mechanics]]></category>
		<category><![CDATA[friction]]></category>
		<category><![CDATA[rate-and-state friction]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Introduction Despite advances in our understanding of rock mechanics, the frictional behavior of rocks, and the physics of instability in geological materials, the coexistence of slow and fast earthquakes, as well as various types of fault-zone seismic radiation such as tremor, remains enigmatic. Can fault mechanics and friction laws reproduce the full spectrum of observed seismicity? In this week’s blog post, Navid Kheirdast takes us through the fundamentals of fault mechanics and frictional behavior before introducing a simple yet powerful mechanical model composed of a main fault interacting with a population of off-fault fractures. Despite its simplicity, the model captures a remarkable range of behaviors observed in nature, reproducing the spectrum of fault slip from slow slip events to fast, dynamic earthquakes. Faults are interfaces in Earth&#8217;s crust—boundaries between tectonic plates or between blocks within a plate—that are permanently subjected to background stress driven by plate tectonics and environmental loading (tides, fluid pressure, and so on). In response to this stress, the two sides of a fault slide past each other: this sliding motion is called slip. To describe fault slip mechanically, we need two families of variables: Dynamic variables — the traction (force per unit area) acting on the fault surface, including frictional resistance and pore-fluid pressure. Kinematic variables — the relative displacement (slip) and slip rate across the fault. The fault-slip problem is a boundary-value problem: knowing one set of variables (say, the background stress) allows us to solve for the other (slip rate). The relationship between stress and slip is governed by a friction law. Slip on natural faults spans an enormous range of speeds, from a few millimeters per year all the way to several meters per second. Three end-member behaviors stand out. Creep Creep is aseismic, quasi-static sliding at roughly the tectonic loading rate — that is, the fault slides continuously at the same speed that the two tectonic plates move relative to each other. No earthquakes occur on creeping faults. Famous examples include the Parkfield segment of the San Andreas Fault and parts of the North Anatolian Fault near the Sea of Marmara. Slow Earthquakes Sometimes slip is faster than the tectonic loading rate but far too slow to radiate significant seismic waves in the classical seismic stations, and only very accurate GNSS stations can record them. Such events — slow earthquakes (also called slow-slip events or SSEs) — may unfold over weeks to months rather than seconds. They are commonly observed in subduction zones: Cascadia, Nankai, Mexico, and Chile all host periodic slow-slip events. Regular (Fast) Earthquakes At the other extreme, slip accelerates to meters per second in a matter of seconds, releasing energy as the seismic waves we feel as earthquakes. The central question is: what controls which of these behaviors a given fault segment will exhibit? There exists a critical stiffness for any fault segment under tectonic loading. If the fault is &#8220;stiff enough,&#8221; any small perturbation in slip rate dies out—the fault creeps stably. If the fault stiffness is below the critical value, perturbations grow, and an earthquake results. Computing this instability threshold is an eigenvalue problem: the critical eigenvalue depends on the frictional properties of the fault surface. This insight was established experimentally by Brace &amp; Byerlee (1966), who showed through triaxial rock-mechanics tests that laboratory rock samples under confining pressure produce stick-slip cycles — the laboratory analogue of repeated earthquakes. Two friction laws dominate earthquake modeling, each capturing a different aspect of fault behavior. 4.1 Linear Slip-Weakening Friction The simplest physically motivated friction law expresses resistance as a function of cumulative slip alone: At the onset of slip, friction equals the static strength τs = μsσ. As slip accumulates, resistance decreases linearly until it reaches a dynamic (residual) strength τd = μdσ after a characteristic slip distance Dc. Beyond Dc, friction stays constant at τd. Limitations of the slip-weakening law: No mechanism for friction recovery, or healing — once the fault has slipped past Dc, it cannot restore its previous strength. No rate dependence — friction does not depend on how fast the fault is sliding. This means that on a fault at the brink of instability, any infinitesimal increase in slip rate immediately triggers an earthquake, with no intermediate regime. Laboratory experiments, however, show that real surfaces resist sudden speed changes — they do not break instantly. 4.2 Rate-and-State Friction Rate-and-state friction (RSF), formulated by Dieterich (1979) and Ruina (1983) on the basis of laboratory experiments, addresses both limitations. It expresses the friction coefficient as a function of slip rate v and a state variable φ: μ = f* + a ln(v/v*) + b ln(θ/θ*) where a is a constant related to the direct strength increase due to a jump in velocity, v* is a reference slip rate, and θ encodes the history of contact. The state variable evolves with slip and time, providing the fault with memory. Two evolution equations for θ are widely used: Aging law — state evolves both with slip and with time (contacts strengthen even when stationary). Slip law — state evolves only when slip occurs; no healing without motion. Key insight from RSF: If you suddenly increase the slip rate, friction immediately increases (the &#8220;direct effect&#8221;), but then slowly decreases back to a new steady-state value as θ evolves. The long-term (steady-state) friction level at speed v is: τss(v) = μss(v) · σ, where Δμss = (a−b) ln(v2/v1) If a − b &lt; 0: steady-state friction decreases with increasing slip rate → velocity-weakening behavior → potentially unstable. If a − b &gt; 0: steady-state friction increases with increasing slip rate → velocity-strengthening behavior → inherently stable. Limitation of RSF: It was calibrated in laboratory experiments at low slip rates (micrometers to millimeters per second), far below the meters-per-second speeds reached during large earthquakes. At coseismic rates, slip-weakening is thought to take over. The Burridge-Knopoff spring-slider is the simplest mechanical system that reproduces stick-slip cycles. A block rests on a frictional surface and is connected by a spring to a loading point that moves at a constant velocity vpl, representing the far-field tectonic loading rate. Two outcomes are possible: Stable sliding (creep): If the spring is stiff enough, the block slides at exactly vpl, smoothly and continuously. Stick-slip (earthquake cycles): If the spring stiffness falls below a critical value kc, the block sticks while the spring stretches, then suddenly lurches forward when the spring force exceeds static friction — mimicking an earthquake. 6. Critical Stiffness — Why Each Behavior Occurs Linear Stability Analysis To find the threshold between stable and unstable slip, Ruina (1983) performed a quasi-static linear stability analysis around the steady-state sliding solution of a slider on a rate and state surface. The method is to perturb the slip rate slightly away from steady state and ask whether the perturbation grows or decays. Details of this analysis is well explained by Segall (2010), therefore we recommend the interested reader to follow from the text book. The critical stiffness gives: kc = σ(b − a) / Dc Physical Interpretation The critical stiffness kc has a transparent physical meaning: Parameter Role σ Normal stress — higher confining stress makes slip harder to control b − a Net velocity-weakening tendency — larger means more destabilizing Dc Characteristic slip distance — larger Dc means the fault &#8220;forgets&#8221; its history more slowly, which is stabilizing The Two Regimes at a Glance Condition Behavior Geological analog k &gt; kc (stiff) Stable sliding Aseismic creep k &lt; kc (compliant) Stick-slip Earthquake cycles 7. Numerical Example — Pseudo-Dynamic Simulation To see both regimes in action, we solve the spring-slider equations numerically, including a radiation-damping term ηv that approximates elastic wave effects without a full dynamic calculation: σ(f* + a ln(v/v*) + b ln(v*θ/Dc)) = k(vplt − δ) − ηv with the aging law θ̇ = 1 − vθ/Dc. With parameters chosen so that a/b = 0.9 (velocity-weakening) and k/kc = 0.95 (the spring is just below the critical stiffness), the simulation produces periodic stick-slip cycles: Increasing the spring stiffness slightly so that k/kc &gt; 1 immediately switches the system to stable sliding: These two simulations illustrate the core message: the same friction law and the same fault, but a single parameter crossing a threshold, separate creeping from seismogenic behavior. 8. Lack of Key Observations The spring-slider model, which resembles a single fault, captures key features of seismic cycles, such as stick-slip and creep-like fault behavior, interseismic and coseismic phases, and periodic ruptures, but it misses some important features, such as the Gutenberg–Richter magnitude-frequency relation, the coexistence of slow and fast ruptures, aftershock sequences, and the localization of seismic activity. In a recent paper by Almakari, Kheirdast et al. (2026), the authors showed that considering the size distribution of off-fault fractures around a main fault produces all of these features. The results of this model interestingly reproduce all statistical properties observed in real catalogs, including the Omori and inverse Omori laws, the Gutenberg–Richter law, and scaling of fast ruptures as M ∼ T³ and slow events as M ∼ T. An intriguing result of the fault-volume model is the migration of events in the fault zone as time approaches the main shock; after the main shock, events tend to return to background seismicity: 9. Conclusion Fault slip is one of the most unpredictable processes in nature. Yet, as this post has shown, much of its complexity can be traced back to a surprisingly compact set of mechanical ingredients. The wide spectrum of observed fault behaviors — from quiet aseismic creep, through slow-slip events that unfold over months, to sudden earthquake ruptures — is not the result of fundamentally different physical processes. It emerges from the interplay between frictional properties and the elastic stiffness of the surrounding crust. Rate-and-state friction, calibrated from laboratory rock experiments, captures the two key ingredients: a fault&#8217;s immediate resistance to speed changes (the direct effect) and its gradual loss or recovery of strength over time (the evolving state variable). When these are combined with a simple spring-slider geometry, a single dimensionless ratio — k/kc — determines whether the fault creeps or earthquakes.   Yet the single-fault spring-slider model, elegant as it is, cannot explain the full texture of real seismicity: the statistical distribution of earthquake sizes, the complex migration of activity in space and time, the coexistence of slow and fast events on the same fault system. The fault-volume model of Almakari, Kheirdast et al. (2026) demonstrates that bringing in off-fault fractures with a power-law size distribution — each obeying the same rate-and-state friction, each interacting mechanically with the main fault — is sufficient to recover all of these features at once. The Gutenberg–Richter law, Omori-law aftershock decay, inverse-Omori foreshock acceleration, and the characteristic scaling differences between slow and fast ruptures all emerge naturally from a single, self-consistent mechanical framework.   The broader lesson is one of emergent complexity from simple rules: a friction law grounded in laboratory physics, applied consistently across a geometrically realistic fault zone, reproduces phenomena that have long resisted explanation. This suggests that the enigmatic coexistence of slow and fast earthquakes, and the apparently erratic migration of seismic activity, may not require exotic physics — only a more complete account of the fault&#8217;s mechanical environment.   Understanding these mechanics has direct implications for seismic hazard assessment. If slow-slip events and tremors are governed by the same friction physics as regular earthquakes, they are not merely curiosities &#8211; they are windows into the stress state of fault zones, and potentially precursors to larger events. The migration patterns revealed by the fault-volume model, in particular, may one day inform operational monitoring strategies.   Much remains to be done. Validating model statistics against dense seismic catalogs are all open challenges. But the foundation laid by decades of friction experiments, stability theory, and increasingly realistic mechanical models gives good reason for optimism that a unified physical picture of fault-zone seismicity is within reach. ReferencesAlmakari, M., Kheirdast, N., Villafuerte, C., Thomas, M. Y., Dubernet, P., Cheng, J., ... &amp; Bhat, H. S. (2026). Fault volume digital twin to reproduce the full slip spectrum, scaling, and statistical laws. Journal of Geophysical Research: Solid Earth, 131(5), e2025JB032915.Coffey, G. L., Savage, H. M., Polissar, P. J., Cox, S. E., Hemming, S. R., Winckler, G., &amp; Bradbury, K. K. (2022). History of earthquakes along the creeping section of the San Andreas Fault, California, USA. Geology, 50(4), 516–521.Becker, D., Martínez-Garzón, P., Wollin, C., Kılıç, T., &amp; Bohnhoff, M. (2023). Variation of fault creep along the overdue Istanbul–Marmara seismic gap in NW Türkiye. Geophysical Research Letters, 50. [doi.org](https://doi.org/10.1029/2022GL101471)Zhang, H., &amp; Li, F. (2024). A review of prediction methods for global buckling critical loads of pultruded FRP struts. Composite Structures, 329, 117752. [doi.org](https://doi.org/10.1016/j.compstruct.2023.117752)Brace, W. F., &amp; Byerlee, J. D. (1966). Stick-slip as a mechanism for earthquakes. Science, 153(3739), 990–992.Dieterich, J. H. (1979). Modeling of rock friction: 1. Experimental results and constitutive equations. Journal of Geophysical Research: Solid Earth, 84(B5), 2161–2168.Ruina, A. (1983). Slip instability and state variable friction laws. Journal of Geophysical Research: Solid Earth, 88(B12), 10,359–10,370.Rice, J. R. (1993). Spatio-temporal complexity of slip on a fault. Journal of Geophysical Research: Solid Earth, 98(B6), 9885–9907.Cochard, A., &amp; Madariaga, R. (1994). Dynamic faulting under rate-dependent friction. Pure and Applied Geophysics, 142(3–4), 419–445.Ben-Zion, Y., &amp; Zaliapin, I. (2020). Localization and coalescence of seismicity before large earthquakes. Geophysical Journal International, 223(1), 561–583.Segall, P. (2010). Earthquake and volcano deformation.]]></description>
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<h2><strong>Introduction</strong></h2>
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<p>Despite advances in our understanding of rock mechanics, the frictional behavior of rocks, and the physics of instability in geological materials, the coexistence of slow and fast earthquakes, as well as various types of fault-zone seismic radiation such as tremor, remains enigmatic.</p>
<p><strong>Can fault mechanics and friction laws reproduce the full spectrum of observed seismicity?</strong></p>
<p>In this week’s blog post, Navid Kheirdast takes us through the fundamentals of <strong>fault mechanics and frictional behavior</strong> before introducing a simple yet powerful mechanical model composed of a main fault interacting with a population of off-fault fractures. Despite its simplicity, the model captures a remarkable range of behaviors observed in nature, reproducing the spectrum of fault slip from <strong>slow slip events to fast, dynamic earthquakes</strong>.</p>
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<h2><strong>1. Faults and the Forces They Bear</strong></h2>
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<p>Faults are interfaces in Earth's crust—boundaries between tectonic plates or between blocks within a plate—that are permanently subjected to <strong>background stress</strong> driven by plate tectonics and environmental loading (tides, fluid pressure, and so on). In response to this stress, the two sides of a fault slide past each other: this sliding motion is called <strong>slip</strong>.</p>
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<p>To describe fault slip mechanically, we need two families of variables:</p>
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<ul>
<li><strong>Dynamic variables</strong> — the traction (force per unit area) acting on the fault surface, including frictional resistance and pore-fluid pressure.</li>
<li><strong>Kinematic variables</strong> — the relative displacement (slip) and slip rate across the fault.</li>
</ul>
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<p>The fault-slip problem is a <strong>boundary-value problem</strong>: knowing one set of variables (say, the background stress) allows us to solve for the other (slip rate). The relationship between stress and slip is governed by a friction law.</p>
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<h2><strong>2. The Wide Spectrum of Fault Slip</strong></h2>
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<p>Slip on natural faults spans an enormous range of speeds, from a few millimeters per year all the way to several meters per second. Three end-member behaviors stand out.</p>
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<h3><strong>Creep</strong></h3>
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<p><strong>Creep</strong> is aseismic, quasi-static sliding at roughly the tectonic loading rate — that is, the fault slides continuously at the same speed that the two tectonic plates move relative to each other. No earthquakes occur on creeping faults. Famous examples include the Parkfield segment of the San Andreas Fault and parts of the North Anatolian Fault near the Sea of Marmara.</p>
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<figure class="wp-block-image">
[caption id="attachment_43029" align="aligncenter" width="282"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/06/CreepSanAndreas.png"><img class="size-full wp-image-43029" src="https://blogs.egu.eu/divisions/gd/files/2026/06/CreepSanAndreas.png" alt="" width="282" height="228" /></a> Creep across the San Andreas Fault. Credit: Coffey et al. (2022).[/caption]
[caption id="attachment_43030" align="aligncenter" width="322"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/06/CreepNorthAnatolianFault.png"><img class="size-full wp-image-43030" src="https://blogs.egu.eu/divisions/gd/files/2026/06/CreepNorthAnatolianFault.png" alt="" width="322" height="167" /></a> Creep across the North Anatolian Fault. Credit: Becker et al. (2023).[/caption]
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<h3><strong>Slow Earthquakes</strong></h3>
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<p>Sometimes slip is faster than the tectonic loading rate but far too slow to radiate significant seismic waves in the classical seismic stations, and only very accurate GNSS stations can record them. Such events — <strong>slow earthquakes</strong> (also called slow-slip events or SSEs) — may unfold over weeks to months rather than seconds. They are commonly observed in subduction zones: Cascadia, Nankai, Mexico, and Chile all host periodic slow-slip events.</p>
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<h3><strong>Regular (Fast) Earthquakes</strong></h3>
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<p>At the other extreme, slip accelerates to meters per second in a matter of seconds, releasing energy as the seismic waves we feel as earthquakes.</p>
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<p>The central question is: <strong>what controls which of these behaviors a given fault segment will exhibit?</strong></p>
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<h2><strong>3. Fault Stability</strong></h2>
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<p>There exists a <strong>critical stiffness</strong> for any fault segment under tectonic loading. If the fault is "stiff enough," any small perturbation in slip rate dies out—the fault creeps stably. If the fault stiffness is below the critical value, perturbations grow, and an earthquake results.</p>
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<p>Computing this instability threshold is an <strong>eigenvalue problem</strong>: the critical eigenvalue depends on the frictional properties of the fault surface. This insight was established experimentally by Brace &amp; Byerlee (1966), who showed through triaxial rock-mechanics tests that laboratory rock samples under confining pressure produce <strong>stick-slip cycles</strong> — the laboratory analogue of repeated earthquakes.</p>
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<h2><strong>4. Two Friction Laws for Fault Mechanics</strong></h2>
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<p>Two friction laws dominate earthquake modeling, each capturing a different aspect of fault behavior.</p>
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<h3><strong>4.1 Linear Slip-Weakening Friction</strong></h3>
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<p>The simplest physically motivated friction law expresses resistance as a function of <strong>cumulative slip alone</strong>:</p>
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<ul>
<li>At the onset of slip, friction equals the <strong>static strength</strong> τ<sub>s</sub> = μ<sub>s</sub>σ.</li>
<li>As slip accumulates, resistance decreases linearly until it reaches a <strong>dynamic (residual) strength</strong> τ<sub>d</sub> = μ<sub>d</sub>σ after a characteristic slip distance D<sub>c</sub>.</li>
<li>Beyond D<sub>c</sub>, friction stays constant at τ<sub>d</sub>.</li>
</ul>
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<figure class="wp-block-image">
[caption id="attachment_43033" align="aligncenter" width="351"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/06/slip_weakening.png"><img class=" wp-image-43033" src="https://blogs.egu.eu/divisions/gd/files/2026/06/slip_weakening-1024x745.png" alt="" width="351" height="255" /></a> Slip-weakening diagram: τ vs. δ (slip), showing peak τs, linear weakening to τd over Dc, then flat residual.[/caption]
</figure>
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<p><strong>Limitations of the slip-weakening law:</strong></p>
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<ol>
<li>No mechanism for <strong>friction recovery, or healing</strong> — once the fault has slipped past D<sub>c</sub>, it cannot restore its previous strength.</li>
<li>No <strong>rate dependence</strong> — friction does not depend on how fast the fault is sliding. This means that on a fault at the brink of instability, <em>any</em> infinitesimal increase in slip rate immediately triggers an earthquake, with no intermediate regime. Laboratory experiments, however, show that real surfaces resist sudden speed changes — they do not break instantly.</li>
</ol>
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<h3><strong>4.2 Rate-and-State Friction</strong></h3>
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<p>Rate-and-state friction (RSF), formulated by Dieterich (1979) and Ruina (1983) on the basis of laboratory experiments, addresses both limitations. It expresses the friction coefficient as a function of <strong>slip rate</strong> v and a <strong>state variable</strong> φ:</p>
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<p style="text-align: center;font-size: 1.2em">μ = f* + a ln(v/v*) + b ln(θ/θ*)</p>
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<p>where <em>a</em> is a constant related to the direct strength increase due to a jump in velocity, <em>v*</em> is a reference slip rate, and <em>θ</em> encodes the history of contact. The state variable evolves with slip and time, providing the fault with <strong>memory</strong>.</p>
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<p>Two evolution equations for θ are widely used:</p>
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<ul>
<li><strong>Aging law</strong> — state evolves both with slip and with time (contacts strengthen even when stationary).</li>
<li><strong>Slip law</strong> — state evolves only when slip occurs; no healing without motion.</li>
</ul>
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<figure class="wp-block-image">
[caption id="attachment_43035" align="aligncenter" width="421"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/06/frictional_instability.png"><img class="wp-image-43035 " src="https://blogs.egu.eu/divisions/gd/files/2026/06/frictional_instability.png" alt="" width="421" height="301" /></a> Velocity-step experiment: the top panel shows slip rate jumping from v1 to v2; the bottom panel shows the immediate increase in the friction coefficient μ, followed by gradual relaxation to the new steady-state value μss.[/caption]
<figcaption></figcaption>
</figure>
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<p><strong>Key insight from RSF:</strong> If you suddenly increase the slip rate, friction <em>immediately</em> increases (the "direct effect"), but then <em>slowly decreases</em> back to a new steady-state value as θ evolves. The long-term (steady-state) friction level at speed v is:</p>
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<p style="text-align: center;font-size: 1.1em">τ<sub>ss</sub>(v) = μ<sub>ss</sub>(v) · σ, where Δμ<sub>ss</sub> = (a−b) ln(v<sub>2</sub>/v<sub>1</sub>)</p>
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<ul>
<li>If a − b &lt; 0: steady-state friction <strong>decreases</strong> with increasing slip rate → <strong>velocity-weakening</strong> behavior → <strong>potentially</strong> unstable.</li>
<li>If a − b &gt; 0: steady-state friction <strong>increases</strong> with increasing slip rate → <strong>velocity-strengthening</strong> behavior → inherently stable.</li>
</ul>
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<p><strong>Limitation of RSF:</strong> It was calibrated in laboratory experiments at low slip rates (micrometers to millimeters per second), far below the meters-per-second speeds reached during large earthquakes. At coseismic rates, slip-weakening is thought to take over.</p>
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<h2><strong>5. The Spring-Slider System — A Minimal Earthquake Cycle Model</strong></h2>
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<p>The <strong>Burridge-Knopoff spring-slider</strong> is the simplest mechanical system that reproduces stick-slip cycles. A block rests on a frictional surface and is connected by a spring to a loading point that moves at a constant velocity v<sub>pl</sub>, representing the far-field tectonic loading rate.</p>
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<figure class="wp-block-image">
[caption id="attachment_43036" align="aligncenter" width="379"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/06/spring_slider.png"><img class=" wp-image-43036" src="https://blogs.egu.eu/divisions/gd/files/2026/06/spring_slider.png" alt="" width="379" height="259" /></a> Spring-slider diagram: block on frictional surface, spring of stiffness k, loading point moving at v_pl; arrows showing slip δ, slip rate v, normal stress σ.[/caption]
</figure>
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<p>Two outcomes are possible:</p>
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<ol>
<li><strong>Stable sliding (creep):</strong> If the spring is stiff enough, the block slides at exactly v<sub>pl</sub>, smoothly and continuously.</li>
<li><strong>Stick-slip (earthquake cycles):</strong> If the spring stiffness falls below a critical value k<sub>c</sub>, the block sticks while the spring stretches, then suddenly lurches forward when the spring force exceeds static friction — mimicking an earthquake.</li>
</ol>
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<h2><strong>6. Critical Stiffness — Why Each Behavior Occurs</strong></h2>
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<h3><strong>Linear Stability Analysis</strong></h3>
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<p>To find the threshold between stable and unstable slip, Ruina (1983) performed a <strong>quasi-static linear stability analysis</strong> around the steady-state sliding solution of a slider on a rate and state surface. The method is to perturb the slip rate slightly away from steady state and ask whether the perturbation grows or decays. Details of this analysis is well explained by Segall (2010), therefore we recommend the interested reader to follow from the text book.</p>
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<p>The <strong>critical stiffness</strong> gives:</p>
<p style="text-align: center"><strong>k<sub>c</sub> = σ(b − a) / D<sub>c</sub></strong></p>
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<h3><strong>Physical Interpretation</strong></h3>
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<p>The critical stiffness k<sub>c</sub> has a transparent physical meaning:</p>
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<figure class="wp-block-table">
<table>
<thead>
<tr>
<th>Parameter</th>
<th>Role</th>
</tr>
</thead>
<tbody>
<tr>
<td>σ</td>
<td>Normal stress — higher confining stress makes slip harder to control</td>
</tr>
<tr>
<td>b − a</td>
<td>Net velocity-weakening tendency — larger means more destabilizing</td>
</tr>
<tr>
<td>D<sub>c</sub></td>
<td>Characteristic slip distance — larger D<sub>c</sub> means the fault "forgets" its history more slowly, which is stabilizing</td>
</tr>
</tbody>
</table>
</figure>
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<h3><strong>The Two Regimes at a Glance</strong></h3>
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<figure class="wp-block-table">
<table>
<thead>
<tr>
<th>Condition</th>
<th>Behavior</th>
<th>Geological analog</th>
</tr>
</thead>
<tbody>
<tr>
<td>k &gt; k<sub>c</sub> (stiff)</td>
<td>Stable sliding</td>
<td>Aseismic creep</td>
</tr>
<tr>
<td>k &lt; k<sub>c</sub> (compliant)</td>
<td>Stick-slip</td>
<td>Earthquake cycles</td>
</tr>
</tbody>
</table>
</figure>
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<h2><strong>7. Numerical Example — Pseudo-Dynamic Simulation</strong></h2>
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<p>To see both regimes in action, we solve the spring-slider equations numerically, including a <strong>radiation-damping</strong> term ηv that approximates elastic wave effects without a full dynamic calculation:</p>
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<p style="text-align: center;font-size: 1.1em">σ(f* + a ln(v/v*) + b ln(v*θ/D<sub>c</sub>)) = k(v<sub>pl</sub>t − δ) − ηv</p>
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<p>with the aging law θ̇ = 1 − vθ/D<sub>c</sub>.</p>
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<p>With parameters chosen so that a/b = 0.9 (velocity-weakening) and k/k<sub>c</sub> = 0.95 (the spring is just below the critical stiffness), the simulation produces periodic <strong>stick-slip cycles</strong>:</p>
<p>[embed]https://www.youtube.com/watch?v=-eJFD_BW920[/embed]</p>
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<figure class="wp-block-video">
<figcaption>
<figure class="wp-block-image"></figure>
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<p>Increasing the spring stiffness slightly so that k/k<sub>c</sub> &gt; 1 immediately switches the system to <strong>stable sliding</strong>:</p>
</figcaption>
</figure>
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<figure class="wp-block-video">
<p>[embed]https://youtu.be/6ZWbybQZwag[/embed]</p>
</figure>
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<p>These two simulations illustrate the core message: <strong>the same friction law and the same fault, but a single parameter crossing a threshold, separate creeping from seismogenic behavior.</strong></p>
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<h2><strong>8. Lack of Key Observations</strong></h2>
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<p>The spring-slider model, which resembles a single fault, captures key features of seismic cycles, such as stick-slip and creep-like fault behavior, interseismic and coseismic phases, and periodic ruptures, but it misses some important features, such as the Gutenberg–Richter magnitude-frequency relation, the coexistence of slow and fast ruptures, aftershock sequences, and the localization of seismic activity. In a recent paper by Almakari, Kheirdast et al. (2026), the authors showed that considering the size distribution of off-fault fractures around a main fault produces all of these features.</p>
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<figure class="wp-block-image">
<div class="mceTemp">
<div class="mceTemp"><br />
[caption id="attachment_43069" align="aligncenter" width="1024"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/06/jgrb70338-fig-0001-m.jpg"><img class="size-large wp-image-43069" src="https://blogs.egu.eu/divisions/gd/files/2026/06/jgrb70338-fig-0001-m-1024x814.jpg" alt="" width="1024" height="814" /></a> The fault-volume model as presented in Almakari et al. (2026). In this model, a main rough fault is embedded in a fault volume. Close to the main fault, there is a higher density of off-fault fractures; fracture density decreases with distance from the fault. The size distribution of off-fault fractures follows a power law. Off-fault fractures are oriented optimally with respect to the background stress loading, and all faults are strengthened by rate-and-state friction, with Dc scaling with fault length.[/caption]
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<figcaption></figcaption>
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<p>The results of this model interestingly reproduce all statistical properties observed in real catalogs, including the Omori and inverse Omori laws, the Gutenberg–Richter law, and scaling of fast ruptures as M ∼ T³ and slow events as M ∼ T.</p>
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<figure class="wp-block-image">
[caption id="attachment_43060" align="aligncenter" width="1024"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/06/GlobalStatistics.png"><img class="size-large wp-image-43060" src="https://blogs.egu.eu/divisions/gd/files/2026/06/GlobalStatistics-1024x992.png" alt="" width="1024" height="992" /></a> Statistics of fault-volume seismicity from Almakari et al. (2026): (a) Omori-law decay in seismic activity after mainshocks, (b) Gutenberg–Richter magnitude-frequency distribution, (c) inverse-Omori increase in seismic activity prior to the main rupture, and (d) scaling of the magnitude and distribution of events produced in the fault zone lies between the M ∼ T³ and M ∼ T limits.[/caption]
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<p>An intriguing result of the fault-volume model is the migration of events in the fault zone as time approaches the main shock; after the main shock, events tend to return to background seismicity:</p>
[caption id="attachment_43063" align="aligncenter" width="1024"]<a href="https://blogs.egu.eu/divisions/gd/files/2026/06/Migration.jpg"><img class="size-large wp-image-43063" src="https://blogs.egu.eu/divisions/gd/files/2026/06/Migration-1024x577.jpg" alt="" width="1024" height="577" /></a> Migration of seismicity: (a) prior to the main shock, off-fault events tend to migrate toward the future event's epicenter. (b) After the main rupture, activity returns to the fault volume, a process called delocalization (Ben-Zion and Zaliapin, 2020).[/caption]
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<h2><strong>9. Conclusion</strong></h2>
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<p>Fault slip is one of the most unpredictable processes in nature. Yet, as this post has shown, much of its complexity can be traced back to a surprisingly compact set of mechanical ingredients.</p>
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<p>The wide spectrum of observed fault behaviors — from quiet aseismic creep, through slow-slip events that unfold over months, to sudden earthquake ruptures — is not the result of fundamentally different physical processes. It emerges from the <strong>interplay between frictional properties and the elastic stiffness of the surrounding crust</strong>. Rate-and-state friction, calibrated from laboratory rock experiments, captures the two key ingredients: a fault's immediate resistance to speed changes (the direct effect) and its gradual loss or recovery of strength over time (the evolving state variable). When these are combined with a simple spring-slider geometry, a single dimensionless ratio — k/k<sub>c</sub> — determines whether the fault creeps or earthquakes.</p>
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<p>  Yet the single-fault spring-slider model, elegant as it is, cannot explain the full texture of real seismicity: the statistical distribution of earthquake sizes, the complex migration of activity in space and time, the coexistence of slow and fast events on the same fault system. The fault-volume model of Almakari, Kheirdast et al. (2026) demonstrates that bringing in <strong>off-fault fractures with a power-law size distribution</strong> — each obeying the same rate-and-state friction, each interacting mechanically with the main fault — is sufficient to recover all of these features at once. The Gutenberg–Richter law, Omori-law aftershock decay, inverse-Omori foreshock acceleration, and the characteristic scaling differences between slow and fast ruptures all emerge naturally from a single, self-consistent mechanical framework.</p>
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<p>  The broader lesson is one of <strong>emergent complexity from simple rules</strong>: a friction law grounded in laboratory physics, applied consistently across a geometrically realistic fault zone, reproduces phenomena that have long resisted explanation. This suggests that the enigmatic coexistence of slow and fast earthquakes, and the apparently erratic migration of seismic activity, may not require exotic physics — only a more complete account of the fault's mechanical environment.</p>
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<p>  Understanding these mechanics has direct implications for seismic hazard assessment. If slow-slip events and tremors are governed by the same friction physics as regular earthquakes, they are not merely curiosities - they are windows into the stress state of fault zones, and potentially precursors to larger events. The migration patterns revealed by the fault-volume model, in particular, may one day inform operational monitoring strategies.</p>
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<p>  Much remains to be done. Validating model statistics against dense seismic catalogs are all open challenges. But the foundation laid by decades of friction experiments, stability theory, and increasingly realistic mechanical models gives good reason for optimism that a unified physical picture of fault-zone seismicity is within reach.</p>
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<pre>References<br /><br />Almakari, M., Kheirdast, N., Villafuerte, C., Thomas, M. Y., Dubernet, P., Cheng, J., ... &amp; Bhat, H. S. (2026). Fault volume digital twin to reproduce the full slip spectrum, scaling, and statistical laws. <i>Journal of Geophysical Research: Solid Earth</i>, <i>131</i>(5), e2025JB032915.<br /><br />Coffey, G. L., Savage, H. M., Polissar, P. J., Cox, S. E., Hemming, S. R., Winckler, G., &amp; Bradbury, K. K. (2022). History of earthquakes along the creeping section of the San Andreas Fault, California, USA. <em>Geology</em>, 50(4), 516–521.<br /><br />Becker, D., Martínez-Garzón, P., Wollin, C., Kılıç, T., &amp; Bohnhoff, M. (2023). Variation of fault creep along the overdue Istanbul–Marmara seismic gap in NW Türkiye. <em>Geophysical Research Letters</em>, 50. <a href="//doi.org/10.1029/2022GL101471)">[doi.org](https://doi.org/10.1029/2022GL101471)</a><br /><br />Zhang, H., &amp; Li, F. (2024). A review of prediction methods for global buckling critical loads of pultruded FRP struts. <em>Composite Structures</em>, 329, 117752. <a href="//doi.org/10.1016/j.compstruct.2023.117752)">[doi.org](https://doi.org/10.1016/j.compstruct.2023.117752)</a><br /><br />Brace, W. F., &amp; Byerlee, J. D. (1966). Stick-slip as a mechanism for earthquakes. <em>Science</em>, 153(3739), 990–992.<br /><br />Dieterich, J. H. (1979). Modeling of rock friction: 1. Experimental results and constitutive equations. <em>Journal of Geophysical Research: Solid Earth</em>, 84(B5), 2161–2168.<br /><br />Ruina, A. (1983). Slip instability and state variable friction laws. <em>Journal of Geophysical Research: Solid Earth</em>, 88(B12), 10,359–10,370.<br /><br />Rice, J. R. (1993). Spatio-temporal complexity of slip on a fault. <em>Journal of Geophysical Research: Solid Earth</em>, 98(B6), 9885–9907.<br /><br />Cochard, A., &amp; Madariaga, R. (1994). Dynamic faulting under rate-dependent friction. <em>Pure and Applied Geophysics</em>, 142(3–4), 419–445.<br /><br />Ben-Zion, Y., &amp; Zaliapin, I. (2020). Localization and coalescence of seismicity before large earthquakes. <em>Geophysical Journal International</em>, 223(1), 561–583.<br /><br />Segall, P. (2010). Earthquake and volcano deformation.</pre>
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					<title><![CDATA[Book Review: The Swarm by Frank Schätzing]]></title>
					<link>https://blogs.egu.eu/divisions/os/2026/06/16/book-review-the-swarm-by-frank-schatzing/</link>
					<comments>https://blogs.egu.eu/divisions/os/2026/06/16/book-review-the-swarm-by-frank-schatzing/#comments</comments>
					<pubDate>Tue, 16 Jun 2026 08:18:31 +0000</pubDate>
					<dc:creator><![CDATA[Jacqueline Behncke]]></dc:creator>
							<category><![CDATA[Book Reviews]]></category>
		<category><![CDATA[book review]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[So far, our reading adventures have kept us close to reality with Blue Machine by Helen Czerski and Below the Edge of Darkness by Edith Widder. Now, we are turning to a work of fiction. The author did plenty of research and spoke with scientists, who even appear as characters in the book, resulting in the science-fiction eco-thriller The Swarm. For centuries, humans have treated the ocean as a resource to exploit. From whale hunting and overfishing to noise pollution, oil spills, plastic pollution and increasing CO₂ emissions, humankind has endangered whole species and ecosystems. But what if the ocean could fight back? What if the deep sea hid an intelligence capable of retaliation? The Swarm, a science-fiction eco-thriller by German author Frank Schätzing, explores this scenario. First published in 2004, the novel tells the story of an unknown intelligent life form in the deep sea that strikes back against humanity’s exploitation of marine resources.  There’s plenty of life down there. The trouble is, it sees us coming and steps aside. The first half of the book follows several scientists as they investigate unusual behaviors and anomalies in the world’s oceans. These include a new species of deep-sea worm with symbiotic bacteria colonizing the North Sea floor, destabilization of the Norwegian continental shelf, changes in whale behavior, and poisonous jellyfish. These strange phenomena observed worldwide accumulate into vividly described catastrophic natural events similar to the disaster scenes in movies like 2012 or The Day After Tomorrow. The second half focuses on the formation of an international scientific task force, bringing together experts from multiple fields to identify the threat and attempt communication with the unknown deep-sea intelligence. This team includes biologists, behavioral scientists, geologists, sonar experts, and SETI (Search for Extraterrestrial Intelligence) scientists, all working together under the lead of the US Navy and CIA. They identify the origin and purpose of the alien life form in the deep sea: a swarm-intelligence, which is aggressively fighting back and threatening all of humankind. They want us to know that we’re in the here and now, whereas they’re everywhere and forever. In the following chapters, scientists use newly developed technologies and risk their lives to counter the attacks and mitigate their effects. Others focus on understanding the swarm intelligence while trying to establish communication. At the same time, conflicts emerge between the scientists and the military leading the mission, creating tension and complicating their efforts. The Swarm is a thought-provoking and thrilling novel that explores environmental and ethical questions. It is both an entertaining read and a striking reminder of the importance of respecting and preserving our natural world. Read more: Interview with Gerhard Borhmann: https://up2date.uni-bremen.de/en/article/the-swarm-bremen-marine-geologist-gerhard-bohrmann-as-fictional-characte  ]]></description>
													<content:encoded><![CDATA[<p>So far, our reading adventures have kept us close to reality with <a href="https://blogs.egu.eu/divisions/os/2024/12/13/book-review-blue-machine/">Blue Machine by Helen Czerski</a> and <a href="https://blogs.egu.eu/divisions/os/2025/05/15/book-review-below-the-edge-of-darkness/">Below the Edge of Darkness by Edith Widder</a>. Now, we are turning to a work of fiction. The author did plenty of research and spoke with scientists, who even appear as characters in the book, resulting in the science-fiction eco-thriller <strong><em>The Swarm</em></strong>.</p>
<p style="font-weight: 400">For centuries, humans have treated the ocean as a resource to exploit. From whale hunting and overfishing to noise pollution, oil spills, plastic pollution and increasing CO₂ emissions, humankind has endangered whole species and ecosystems. <strong>But what if the ocean could fight back?</strong> What if the deep sea hid an intelligence capable of retaliation? <em data-start="442" data-end="453">The Swarm</em>, a science-fiction eco-thriller by German author Frank Schätzing, explores this scenario. First published in 2004, the novel tells the story of an unknown intelligent life form in the deep sea that strikes back against humanity’s exploitation of marine resources. </p>
<blockquote>
<p>There’s plenty of life down there. The trouble is, it sees us coming and steps aside.</p>
</blockquote>
<p style="font-weight: 400">The first half of the book follows several scientists as they investigate unusual behaviors and anomalies in the world’s oceans. These include a new species of deep-sea worm with symbiotic bacteria colonizing the North Sea floor, destabilization of the Norwegian continental shelf, changes in whale behavior, and poisonous jellyfish. These strange phenomena observed worldwide accumulate into vividly described catastrophic natural events similar to the disaster scenes in movies like <em>2012</em> or <em>The Day After Tomorrow</em>.</p>
<p style="font-weight: 400">The second half focuses on the formation of an international scientific task force, bringing together experts from multiple fields to identify the threat and attempt communication with the unknown deep-sea intelligence. This team includes biologists, behavioral scientists, geologists, sonar experts, and SETI (Search for Extraterrestrial Intelligence) scientists, all working together under the lead of the US Navy and CIA. They identify the origin and purpose of the alien life form in the deep sea: a swarm-intelligence, which is aggressively fighting back and threatening all of humankind.</p>
<blockquote>
<p>They want us to know that we’re in the here and now, whereas they’re everywhere and forever.</p>
</blockquote>
<p data-start="464" data-end="847">In the following chapters, scientists use newly developed technologies and risk their lives to counter the attacks and mitigate their effects. Others focus on understanding the swarm intelligence while trying to establish communication. At the same time, conflicts emerge between the scientists and the military leading the mission, creating tension and complicating their efforts.</p>
<p data-start="849" data-end="1078"><em data-start="849" data-end="860">The Swarm</em> is a thought-provoking and thrilling novel that explores environmental and ethical questions. It is both an entertaining read and a striking reminder of the importance of respecting and preserving our natural world.</p>
<p><strong>Read more:<br /></strong></p>
<ul>
<li>Interview with Gerhard Borhmann: <a href="https://up2date.uni-bremen.de/en/article/the-swarm-bremen-marine-geologist-gerhard-bohrmann-as-fictional-character">https://up2date.uni-bremen.de/en/article/the-swarm-bremen-marine-geologist-gerhard-bohrmann-as-fictional-characte</a></li>
</ul>
<p><strong> </strong></p>
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					<title><![CDATA[When multiple hazards interact and the data doesn’t: The multi-hazard modelling problem nobody wants to talk about]]></title>
					<link>https://blogs.egu.eu/divisions/nh/2026/06/15/when-multiple-hazards-interact-and-the-data-doesnt-the-multi-hazard-modelling-problem-nobody-wants-to-talk-about/</link>
					<comments>https://blogs.egu.eu/divisions/nh/2026/06/15/when-multiple-hazards-interact-and-the-data-doesnt-the-multi-hazard-modelling-problem-nobody-wants-to-talk-about/#comments</comments>
					<pubDate>Mon, 15 Jun 2026 08:06:45 +0000</pubDate>
					<dc:creator><![CDATA[Hedieh Soltanpour]]></dc:creator>
							<category><![CDATA[Disaster risk reduction]]></category>
		<category><![CDATA[Multihazard]]></category>
		<category><![CDATA[Natural hazard]]></category>
		<category><![CDATA[#EGUblogs]]></category>
		<category><![CDATA[#multihazards]]></category>
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											<description><![CDATA[There is a quiet contradiction at the heart of natural hazard science. The regions most exposed to multi-hazard events are precisely the regions where we know the least. The Global South (comprising lower- and middle-income countries in Africa, Asia, Latin America and the Caribbean) is disproportionately affected by climate-related natural hazards, yet it is largely underrepresented in climate research and published literature [1]. Flood-exposed populations in the Global South are projected to be nearly five times greater than in the Global North (comprising, high-income countries in Europe, North America, and Australasia) by the end of the century [2], and compound hot-dry extremes are rising fastest in Asia, the Middle East, and Africa, amplified by large populations, lower income levels, and socio-economic vulnerability [3]. Sparse gauge networks, coarse-resolution soil data, incomplete hazard inventories, and a lack of high-resolution topography data. And yet, climate extremes are intensifying in these regions faster than our data infrastructure can keep up. We have built sophisticated multi-hazard models. We just rarely have the data to run them with integrity. The multi-hazard problem is not what you think Multi-hazard modelling is often framed as a problem of complexity: how do you represent the interactions between hazards within a single coherent framework? That is a real challenge, and a well-documented one [4, 5, 6, 7, 8, 9]. But in data-scarce regions, the harder problem comes before the modelling even starts. Consider a post-wildfire catchment in coastal Chile (Fig. 1). The February 2024 mega-wildfire in the Marga-Marga catchment in Viña del Mar, one of the most destructive in Chilean history, burned through densely urbanised slopes and fundamentally altered the hazard setting [10]. A wildfire removes vegetation; changes soil hydrological and stability properties and dramatically alters infiltration and rainfall-runoff dynamics. The next rainfall event in the Marga-Marga catchment, increasingly intense under a changing climate, triggers erosion, shallow landslides, and hyper-concentrated flows simultaneously. These are not independent hazards. As described by [11] and [12], they interact in concurrent, compounding and cascading ways, amplifying their impacts when treated as single hazards. Treating them in isolation is not conservative; it is wrong. &nbsp; &nbsp; &nbsp; &nbsp; But to model these multi-hazard interactions jointly (Fig. 2), you need to know when and where they occur. This requires spatially distributed multi-hazard models, which are inherently complex due to high data demands, parameterisation requirements, and the need to represent spatially and temporally interacting physical processes. Therefore, to assess post-wildfire multi-hazard interactions we need high-resolution topography, pre- and post-fire soil properties, sub-hourly rainfall, and a multi-hazard inventory for validation. In data-scarce regions, you typically have none of these at the quality multi-hazard models demand. You have a 30-metre Digital Elevation Model (DEM), ERA5 reanalysis at 9 km, SoilGrids estimates derived from Machine Learning (ML) models trained elsewhere, and a landslide inventory assembled after the disaster from satellite imagery and newspaper reports, if anything exists at all. In Chile, as across much of the Global South, official hazard records are often discontinued, incomplete, or simply absent. Acknowledging these limitations is not a reason to stop modelling. It is the first step toward transparent modelling. But recognising the data problem is only half the story. The other half is understanding what happens inside the model once you ignore it. &nbsp; The uncertainty cascade The data problem in multi-hazard modelling is not only about gaps. It is also about how uncertainty propagates. Every step of the modelling process carries its own uncertainty: estimating soil properties, resampling spatial resolution, disaggregating daily rainfall to sub-hourly intervals, selecting the model structure and validating it against an incomplete hazard inventory. Crucially, these uncertainties do not simply add together; they multiply. In post-wildfire multi-hazard settings, where we want to understand the effects of hazard interactions on landslides, debris flows, and hillslope erosion, this uncertainty cascade misrepresents key processes such as infiltration, pore pressure, and shear strength, which are essential drivers of hydrology and slope stability, distorting both the predicted location and magnitude of each hazard and the interactions between them. [13] and [14] demonstrate that quantifying this rigorously requires an ensemble of simulations rather than a single model run, as formalised in the GLUE framework (Generalised Likelihood Uncertainty Estimation). That is, many different parameter sets can reproduce observed hazard behaviour equally well, a problem known as equifinality. In data-scarce regions, where observations are few and data are uncertain, this approach does not weaken the analysis; it is the only honest way to represent what the data actually tells us about the plausible range of hazard behaviour. What honest multi-hazard modelling looks like in practice A hazard map is a static product: a single model run and a single moment in time, with uncertainty hidden behind clean colour gradients. The answer to the uncertainty cascade is not to abandon physically-based modelling in data-scarce regions. It is to structure the modelling workflow around it. [15] argues that uncertainty-aware modelling in data-limited environments requires explicit decisions at every step: which data sources are used and what uncertainty they carry, which parameter ranges are physically plausible given the available data, which model runs are retained as behavioural and which are rejected, and how the resulting ensemble is communicated to decision-makers. But this does not stop here. Climate change introduces an additional dimension: The rainfall events that trigger post-wildfire multi-hazard events are becoming more intense and frequent. This means that the set of behavioural parameters identified through GLUE are not only a tool for reproducing past observations but also provides a basis for evaluating how hazard behaviour responds to future rainfall extremes. The workflow itself becomes the scientific contribution: it makes the path from uncertain data to decision-relevant output transparent and reproducible decision-making. My own work on post-wildfire hazard in the Marga-Marga catchment has made this concrete. Building on research conducted at CIGIDEN (National Research Centre for Integrated Natural Disaster Management, Chile).  I ran a physically-based multi-hazard model (OpenLISEM Hazard) across hundreds of parameter combinations. I varied soil cohesion, hydraulic conductivity, porosity and friction angle. I used Earth observation datasets as the best available proxy for unmeasured field conditions. The model produced hazard outputs that communicated confidence ranges rather than false certainty. This approach is more computationally demanding than a single model run, but it is the only defensible method given our current knowledge. This points toward a distinction the field rarely makes explicit. A hazard map is a static product: a single model run and a single moment in time, with uncertainty hidden behind clean colour gradients. What I am describing is different: geospatial hazard intelligence, which has the capacity to transform uncertain, spatially distributed data into honest, decision-relevant knowledge about where hazards occur, how they interact and how confident we are in that assessment. Confidence is not an afterthought; it is the core deliverable. The output is not designed for archiving, but for the person who has to decide whether to rebuild a school on a hillslope after a wildfire, or whether to evacuate a neighbourhood before the next one. In regions where data are scarce, that distinction is not academic. The mega-wildfire in the Marga-Marga catchment destroyed around 5,500 homes across the densely populated slopes of Viña del Mar and neighbouring municipalities, triggering a reconstruction process estimated to cost one billion dollars [16]. Decisions about where to rebuild, which slopes were safe to reoccupy and which sites posed an elevated risk of post-wildfire landslides and debris flows were made on the same burned terrain, with the same missing data and under enormous political and social pressure to act quickly. Most rebuilding was carried out through residents&#8217; self-reconstruction efforts, largely outside the scope of formal hazard assessment [10]. A multi-hazard assessment that communicated not just the level of risk, but also the reliability of the assessment, could have informed which sites were recoverable and which were not. Such an assessment did not exist. Honest communication of uncertainty is not a weakness; it is the most actionable thing a model can produce. Hiding uncertainty is what causes disasters to happen twice in the same place. The hazards compound. The data doesn&#8217;t. Our methods must close that gap, and our outputs must reflect this. References [1] N. Communications, “Climate research in the Global South,” Nat. Commun., vol. 16, no. 1, pp. 3–4, 2025, doi: 10.1038/s41467-025-63884-3. [2] Q.Zhang et al., “Global South shows higher urban flood exposures than the Global North under current and future scenarios,” Commun. Earth Environ., vol. 6, no. 1, pp. 1–13, 2025, doi: 10.1038/s43247-025-02585-7. [3] J. Guo et al., “Rising compound hot-dry extremes engendering more inequality in human exposure risks,” npj Natural Hazards, vol. 2, no. 1, pp. 1–11, 2025, doi: 10.1038/s44304-025-00119-x. [4] S. De Angeli, B. D. Malamud, L. Rossi, F. E. Taylor, E. Trasforini, and R. Rudari, “A multi-hazard framework for spatial-temporal impact analysis,” International Journal of Disaster Risk Reduction, vol. 73, p. 102829, Apr. 2022, doi: 10.1016/j.ijdrr.2022.102829. [5]  J. C. Gill and B. D. Malamud, “Hazard interactions and interaction networks (cascades) within multi-hazard methodologies,” Earth System Dynamics, vol. 7, no. 3, pp. 659–679, 2016, doi: 10.5194/esd-7-659-2016. [6] S. Hochrainer-Stigler et al., “Toward a framework for systemic multi-hazard and multi-risk assessment and management,” iScience, vol. 26, no. 5, p. 106736, May 2023, doi: 10.1016/j.isci.2023.106736. [7] M. Kappes, M. Keiler, K. von Elverfeldt, and T. Glade, “Challenges of analyzing multi-hazard risk: A review,” Nov. 31, 2012. doi: 10.1007/s11069-012-0294-2. [8] R. Š. Trogrlić et al., “Challenges in assessing and managing multi-hazard risks: A European stakeholders perspective,” Environ. Sci. Policy, vol. 157, no. August 2023, 2024, doi: 10.1016/j.envsci.2024.103774. [9] A. Tilloy, B. D. Malamud, H. Winter, and A. Joly-Laugel, “A review of quantification methodologies for multi-hazard interrelationships,” Sep. 01, 2019, Elsevier B.V. doi: 10.1016/j.earscirev.2019.102881. [10] Martínez et al., “Incendios 02 y 03 de febrero de 2024, Viña del Mar (Región de Valparaíso),” 2024. [Online]. Available: https://www.cigiden.cl/wp-content/uploads/2024/02/CIGIDEN_2024_IncendiosVinadelMar_v04.pdf [Accessed: 3 June 2026]. [11]  J. C. Gill and B. D. Malamud, “Reviewing and visualizing the interactions of natural hazards,” Reviews of Geophysics, vol. 52, no. 4, pp. 680–722, Dec. 2014, doi: 10.1002/2013RG000445. [12] J. Zscheischler et al., “A typology of compound weather and climate events,” Nat. Rev. Earth Environ., pp. 1–15, Jun. 2020, doi: 10.1038/s43017-020-0060-z. [13] K. Beven, “A manifesto for the equifinality thesis,” J. Hydrol. (Amst)., vol. 320, no. 1–2, pp. 18–36, Mar. 2006, doi: 10.1016/j.jhydrol.2005.07.007. [14] K. Beven and A. Binley, “The future of distributed models: Model calibration and uncertainty prediction,” Hydrol. Process., vol. 6, no. 3, pp. 279–298, Jul. 1992, doi: 10.1002/hyp.3360060305. [15] K. Beven et al., “Epistemic uncertainties and natural hazard risk assessment – Part 2: What should constitute good practice?,” Natural Hazards and Earth System Sciences, vol. 18, no. 10, pp. 2769–2783, Oct. 2018, doi: 10.5194/nhess-18-2769-2018. [16] UNICEF, “Chile Humanitarian Flash Report No.2 (Wildfires),” 2024. [Online]. Available: https://reliefweb.int/report/chile/unicef-chile-humanitarian-flash-report-no2-wildfires-07-march-2024 [Accessed: 3 June 2026]. &nbsp; Blog post edited by: Hedieh Soltanpour and Harriet Thampson]]></description>
													<content:encoded><![CDATA[<h6><em>There is a quiet contradiction at the heart of natural hazard science. The regions most exposed to multi-hazard events are precisely the regions where we know the least. The Global South (comprising lower- and middle-income countries in Africa, Asia, Latin America and the Caribbean) is disproportionately affected by climate-related natural hazards, yet it is largely underrepresented in climate research and published literature [1]. Flood-exposed populations in the Global South are projected to be nearly five times greater than in the Global North (comprising, high-income countries in Europe, North America, and Australasia) by the end of the century [2], and compound hot-dry extremes are rising fastest in Asia, the Middle East, and Africa, amplified by large populations, lower income levels, and socio-economic vulnerability [3]. Sparse gauge networks, coarse-resolution soil data, incomplete hazard inventories, and a lack of high-resolution topography data. And yet, climate extremes are intensifying in these regions faster than our data infrastructure can keep up. We have built sophisticated multi-hazard models. We just rarely have the data to run them with integrity.</em></h6>
<h3><strong>The multi-hazard problem is not what you think</strong></h3>
Multi-hazard modelling is often framed as a problem of complexity: how do you represent the interactions between hazards within a single coherent framework? That is a real challenge, and a well-documented one [4, 5, 6, 7, 8, 9]. But in data-scarce regions, the harder problem comes before the modelling even starts. Consider a post-wildfire catchment in coastal Chile (Fig. 1). The February 2024 mega-wildfire in the Marga-Marga catchment in Viña del Mar, one of the most destructive in Chilean history, burned through densely urbanised slopes and fundamentally altered the hazard setting [10]. A wildfire removes vegetation; changes soil hydrological and stability properties and dramatically alters infiltration and rainfall-runoff dynamics. The next rainfall event in the Marga-Marga catchment, increasingly intense under a changing climate, triggers erosion, shallow landslides, and hyper-concentrated flows simultaneously. These are not independent hazards. As described by [11] and [12], they interact in concurrent, compounding and cascading ways, amplifying their impacts when treated as single hazards. Treating them in isolation is not conservative; it is wrong.

[caption id="attachment_11125" align="alignleft" width="310"]<img class="wp-image-11125" src="https://blogs.egu.eu/divisions/nh/files/2026/06/Figure1b-300x252.png" alt="" width="310" height="260" /> Figure 1 (left to right). The Marga-Marga catchment in Viña del Mar: the effects of wildfires on urbanisation and hillslope vegetation, and wildfire-affected settlements[/caption]

&nbsp;

<img class="alignnone wp-image-11126" src="https://blogs.egu.eu/divisions/nh/files/2026/06/Figure1a_Featured_Image-1-300x198.png" alt="" width="320" height="211" />

&nbsp;

&nbsp;

&nbsp;

But to model these multi-hazard interactions jointly (Fig. 2), you need to know when and where they occur. This requires spatially distributed multi-hazard models, which are inherently complex due to high data demands, parameterisation requirements, and the need to represent spatially and temporally interacting physical processes. Therefore, to assess post-wildfire multi-hazard interactions we need high-resolution topography, pre- and post-fire soil properties, sub-hourly rainfall, and a multi-hazard inventory for validation. In data-scarce regions, you typically have none of these at the quality multi-hazard models demand. You have a 30-metre Digital Elevation Model (DEM), ERA5 reanalysis at 9 km, SoilGrids estimates derived from Machine Learning (ML) models trained elsewhere, and a landslide inventory assembled after the disaster from satellite imagery and newspaper reports, if anything exists at all. In Chile, as across much of the Global South, official hazard records are often discontinued, incomplete, or simply absent. Acknowledging these limitations is not a reason to stop modelling. It is the first step toward transparent modelling. But recognising the data problem is only half the story. The other half is understanding what happens inside the model once you ignore it.

&nbsp;

[caption id="attachment_11129" align="aligncenter" width="530"]<img class="wp-image-11129" src="https://blogs.egu.eu/divisions/nh/files/2026/06/Figure2-1-300x200.png" alt="" width="530" height="353" /> Figure 2. Conceptual representation of post-wildfire cascading hazards (landslide, debris flow, and flooding) and associated data requirements for integrated multi-hazard modelling. Illustration generated using ChatGPT (Open AI).[/caption]
<h2></h2>
<h3><strong>The uncertainty cascade</strong></h3>
The data problem in multi-hazard modelling is not only about gaps. It is also about how uncertainty propagates. Every step of the modelling process carries its own uncertainty: estimating soil properties, resampling spatial resolution, disaggregating daily rainfall to sub-hourly intervals, selecting the model structure and validating it against an incomplete hazard inventory. Crucially, these uncertainties do not simply add together; they multiply.

In post-wildfire multi-hazard settings, where we want to understand the effects of hazard interactions on landslides, debris flows, and hillslope erosion, this uncertainty cascade misrepresents key processes such as infiltration, pore pressure, and shear strength, which are essential drivers of hydrology and slope stability, distorting both the predicted location and magnitude of each hazard and the interactions between them. [13] and [14] demonstrate that quantifying this rigorously requires an ensemble of simulations rather than a single model run, as formalised in the GLUE framework (Generalised Likelihood Uncertainty Estimation). That is, many different parameter sets can reproduce observed hazard behaviour equally well, a problem known as equifinality. In data-scarce regions, where observations are few and data are uncertain, this approach does not weaken the analysis; it is the only honest way to represent what the data actually tells us about the plausible range of hazard behaviour.
<h3><strong>What honest multi-hazard modelling looks like in practice</strong></h3>
<blockquote>A hazard map is a static product: a single model run and a single moment in time, with uncertainty hidden behind clean colour gradients.</blockquote>
The answer to the uncertainty cascade is not to abandon physically-based modelling in data-scarce regions. It is to structure the modelling workflow around it. [15] argues that uncertainty-aware modelling in data-limited environments requires explicit decisions at every step: which data sources are used and what uncertainty they carry, which parameter ranges are physically plausible given the available data, which model runs are retained as behavioural and which are rejected, and how the resulting ensemble is communicated to decision-makers.

But this does not stop here. Climate change introduces an additional dimension: The rainfall events that trigger post-wildfire multi-hazard events are becoming more intense and frequent. This means that the set of behavioural parameters identified through GLUE are not only a tool for reproducing past observations but also provides a basis for evaluating how hazard behaviour responds to future rainfall extremes. The workflow itself becomes the scientific contribution: it makes the path from uncertain data to decision-relevant output transparent and reproducible decision-making.

My own work on post-wildfire hazard in the Marga-Marga catchment has made this concrete. Building on research conducted at CIGIDEN (National Research Centre for Integrated Natural Disaster Management, Chile).  I ran a physically-based multi-hazard model (OpenLISEM Hazard) across hundreds of parameter combinations. I varied soil cohesion, hydraulic conductivity, porosity and friction angle. I used Earth observation datasets as the best available proxy for unmeasured field conditions. The model produced hazard outputs that communicated confidence ranges rather than false certainty. This approach is more computationally demanding than a single model run, but it is the only defensible method given our current knowledge.

This points toward a distinction the field rarely makes explicit. A hazard map is a static product: a single model run and a single moment in time, with uncertainty hidden behind clean colour gradients. What I am describing is different: geospatial hazard intelligence, which has the capacity to transform uncertain, spatially distributed data into honest, decision-relevant knowledge about where hazards occur, how they interact and how confident we are in that assessment. Confidence is not an afterthought; it is the core deliverable. The output is not designed for archiving, but for the person who has to decide whether to rebuild a school on a hillslope after a wildfire, or whether to evacuate a neighbourhood before the next one.

In regions where data are scarce, that distinction is not academic. The mega-wildfire in the Marga-Marga catchment destroyed around 5,500 homes across the densely populated slopes of Viña del Mar and neighbouring municipalities, triggering a reconstruction process estimated to cost one billion dollars [16]. Decisions about where to rebuild, which slopes were safe to reoccupy and which sites posed an elevated risk of post-wildfire landslides and debris flows were made on the same burned terrain, with the same missing data and under enormous political and social pressure to act quickly. Most rebuilding was carried out through residents' self-reconstruction efforts, largely outside the scope of formal hazard assessment [10]. A multi-hazard assessment that communicated not just the level of risk, but also the reliability of the assessment, could have informed which sites were recoverable and which were not. Such an assessment did not exist. Honest communication of uncertainty is not a weakness; it is the most actionable thing a model can produce. Hiding uncertainty is what causes disasters to happen twice in the same place.

<em>The hazards compound. The data doesn't. Our methods must close that gap, and our outputs must reflect this.</em>
<h3><strong>References</strong></h3>
[1] N. Communications, “Climate research in the Global South,” <em>Nat. Commun.</em>, vol. 16, no. 1, pp. 3–4, 2025, doi: 10.1038/s41467-025-63884-3.

[2] Q.Zhang <em>et al.</em>, “Global South shows higher urban flood exposures than the Global North under current and future scenarios,” <em>Commun. Earth Environ.</em>, vol. 6, no. 1, pp. 1–13, 2025, doi: 10.1038/s43247-025-02585-7.

[3] J. Guo <em>et al.</em>, “Rising compound hot-dry extremes engendering more inequality in human exposure risks,” <em>npj Natural Hazards</em>, vol. 2, no. 1, pp. 1–11, 2025, doi: 10.1038/s44304-025-00119-x.

[4] S. De Angeli, B. D. Malamud, L. Rossi, F. E. Taylor, E. Trasforini, and R. Rudari, “A multi-hazard framework for spatial-temporal impact analysis,” <em>International Journal of Disaster Risk Reduction</em>, vol. 73, p. 102829, Apr. 2022, doi: 10.1016/j.ijdrr.2022.102829.

[5]  J. C. Gill and B. D. Malamud, “Hazard interactions and interaction networks (cascades) within multi-hazard methodologies,” <em>Earth System Dynamics</em>, vol. 7, no. 3, pp. 659–679, 2016, doi: 10.5194/esd-7-659-2016.

[6] S. Hochrainer-Stigler <em>et al.</em>, “Toward a framework for systemic multi-hazard and multi-risk assessment and management,” <em>iScience</em>, vol. 26, no. 5, p. 106736, May 2023, doi: 10.1016/j.isci.2023.106736.

[7] M. Kappes, M. Keiler, K. von Elverfeldt, and T. Glade, “Challenges of analyzing multi-hazard risk: A review,” Nov. 31, 2012. doi: 10.1007/s11069-012-0294-2.

[8] R. Š. Trogrlić <em>et al.</em>, “Challenges in assessing and managing multi-hazard risks: A European stakeholders perspective,” <em>Environ. Sci. Policy</em>, vol. 157, no. August 2023, 2024, doi: 10.1016/j.envsci.2024.103774.

[9] A. Tilloy, B. D. Malamud, H. Winter, and A. Joly-Laugel, “A review of quantification methodologies for multi-hazard interrelationships,” Sep. 01, 2019, <em>Elsevier B.V.</em> doi: 10.1016/j.earscirev.2019.102881.

[10] Martínez <em>et al.</em>, “Incendios 02 y 03 de febrero de 2024, Viña del Mar (Región de Valparaíso),” 2024. [Online]. Available: <a href="https://www.cigiden.cl/wp-content/uploads/2024/02/CIGIDEN_2024_IncendiosVinadelMar_v04.pdf">https://www.cigiden.cl/wp-content/uploads/2024/02/CIGIDEN_2024_IncendiosVinadelMar_v04.pdf</a> [Accessed: 3 June 2026].

[11]  J. C. Gill and B. D. Malamud, “Reviewing and visualizing the interactions of natural hazards,” <em>Reviews of Geophysics</em>, vol. 52, no. 4, pp. 680–722, Dec. 2014, doi: 10.1002/2013RG000445.

[12] J. Zscheischler <em>et al.</em>, “A typology of compound weather and climate events,” <em>Nat. Rev. Earth Environ.</em>, pp. 1–15, Jun. 2020, doi: 10.1038/s43017-020-0060-z.

[13] K. Beven, “A manifesto for the equifinality thesis,” <em>J. Hydrol. (Amst).</em>, vol. 320, no. 1–2, pp. 18–36, Mar. 2006, doi: 10.1016/j.jhydrol.2005.07.007.

[14] K. Beven and A. Binley, “The future of distributed models: Model calibration and uncertainty prediction,” <em>Hydrol. Process.</em>, vol. 6, no. 3, pp. 279–298, Jul. 1992, doi: 10.1002/hyp.3360060305.

[15] K. Beven <em>et al.</em>, “Epistemic uncertainties and natural hazard risk assessment – Part 2: What should constitute good practice?,” <em>Natural Hazards and Earth System Sciences</em>, vol. 18, no. 10, pp. 2769–2783, Oct. 2018, doi: 10.5194/nhess-18-2769-2018.

[16] UNICEF, “Chile Humanitarian Flash Report No.2 (Wildfires),” 2024. [Online]. Available: <a href="https://reliefweb.int/report/chile/unicef-chile-humanitarian-flash-report-no2-wildfires-07-march-2024">https://reliefweb.int/report/chile/unicef-chile-humanitarian-flash-report-no2-wildfires-07-march-2024</a> [Accessed: 3 June 2026].

&nbsp;

Blog post edited by: Hedieh Soltanpour and Harriet Thampson]]></content:encoded>
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					<title><![CDATA[The Arctic's Blind Spot: Why Satellites Struggle Where Ice Meets the Coast]]></title>
					<link>https://blogs.egu.eu/divisions/cr/2026/06/12/the-arctics-blind-spot-why-satellites-struggle-where-ice-meets-the-coast/</link>
					<comments>https://blogs.egu.eu/divisions/cr/2026/06/12/the-arctics-blind-spot-why-satellites-struggle-where-ice-meets-the-coast/#comments</comments>
					<pubDate>Fri, 12 Jun 2026 08:10:57 +0000</pubDate>
					<dc:creator><![CDATA[Leah Muhle]]></dc:creator>
							<category><![CDATA[Cryo Adventures]]></category>
		<category><![CDATA[Fieldwork]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[The first time I stood on sea ice, I could not tell which direction the coast was. A community member named Bryan could. That gap in situational awareness, between what a trained remote sensing scientist could read from the landscape and what a local hunter understood instinctively, turned out to mirror almost exactly the gap in our satellite data: ICESat-2 produces reliable freeboard across the central Arctic but goes systematically blind within 25 km of every coastline. This post traces that coastal data gap from its algorithmic roots through its ecological and human consequences, and asks what it would mean to build satellite products that close it on the terms of the communities who need them most. _____________________________________________________________________________________________________________________________________ I grew up in Bangladesh, a country defined by delta and monsoon, emphatically not by ice. So when I stepped onto the frozen surface of Hudson Bay near Churchill, Manitoba in December 2021, on my first Arctic field campaign, I was meeting sea ice for the first time outside of a textbook (Figure 1). I didn&#8217;t really understand what it meant to travel over sea ice until I was on the back of a skidoo driven by a community member named Bryan. It was early in the freeze up season, what locals sometimes call the &#8220;free up&#8221; season, in acknowledgement of how volatile the margins can be. At one point, standing on the ice, I could not tell which direction the coast lay. Bryan simply followed the faint lines left by other skidoos, navigational knowledge encoded in the landscape itself, invisible to me but perfectly legible to him. A short while later, hunters returning from the landfast ice edge warned us we were closer to it than we had realised. Almost on cue, a crack began to open in the surface nearby. Bryan turned us around. In that moment, the abstract vocabulary of my remote sensing work, freeboard, sea surface reference, landfast ice extent, collapsed into something urgent. Bryan needed to know how thick that ice was. The hunters needed to know whether the edge was stable. These are not research questions. They are safety questions. Satellites That Couldn&#8217;t See Near the Coast The campaign was meant to be a satellite validation exercise: coincident snow depth and ice thickness measurements supporting ICESat-2 and CryoSat-2 freeboard retrievals during my MSc at the University of Manitoba (freeboard is the part of the sea ice above the waterline). But after we collected the data, we discovered that ICESat-2 had produced almost no usable freeboard within the 25 km coastal buffer around our study area. The multiyear record showed the same pattern season after season: a persistent coastal blank (Figure 2). The satellite had been overhead and had properly collected photons. But the downstream algorithms could not establish a reliable sea surface reference, and the data were flagged or discarded before any calculation for freeboard was attempted. That distinction matters, because it tells us where the solution lies: not in the hardware, but in what we do with the signal (Kwok et al, 2019, Petty et al., 2020). If ICESat-2 could not deliver freeboard within 25 km of the coast, we had to go to get the data. The following year our team at Maryland and the University of Calgary chartered a helicopter to Cambridge Bay, Nunavut (Figure 3 shows the sites that were surveyed). Cambridge Bay is, in many ways, the textbook setting for the failure modes I had identified in Hudson Bay: narrow channels with strong tidal forcing, persistent landfast ice well into spring, heavily ridged shore fast ice, and the operational stakes of sitting on the Northwest Passage shipping corridor (Smith et al., 2013). All algorithmic problems described in the following occur here simultaneously. That image of clean central Arctic freeboard ringed by a stubborn coastal void became the puzzle driving my MSc thesis and now my PhD at the University of Maryland. How Altimeters Measure Ice A sea ice floe sits in seawater like an ice cube in a glass with the freeboard as the portion above the waterline. Given an independent estimate of snow depth and the densities of snow, ice, and seawater, freeboard converts to total thickness through hydrostatic balance. The two altimeters at the heart of this work see the floe differently. ICESat-2&#8217;s ATLAS photon counting lidar reflects from the air to snow interface and therefore measures total freeboard (snow plus ice above sea level). CryoSat-2&#8217;s Ku band radar is conventionally assumed to penetrate the dry snow column and reflect from the snow to ice interface, yielding ice freeboard, although the validity of that assumption is now under active scrutiny (Nandan et al., 2017). The difference between the two retrievals along nearly coincident ICESat-2 and Cryosat-2 orbits provides the basis for satellite snow depth on sea ice. It is also the reason coastal data loss is doubly costly: when the algorithms fail, we lose both freeboard and the dual altimeter snow depth product simultaneously. The hard part for either sensor is the reference. We need an accurate, instantaneous sea surface height beneath the satellite, which in practice means finding open water or thin ice leads (sea ice leads are long cracks formed when Arctic ice floes diverge or shear), measuring their elevation, and differencing it from the surrounding ice. In the central pack, where leads are abundant and geometrically clean, this works well (Kwok et al., 2015). However, near the coast the scarcity of open water leads in the landfast ice along with challenges poised by algorithmic limitations linked to interactions of lidar with the rugged landfast ice makes the traditional method of measuring freeboard and ice thickness difficult. ICESat-2’s lead classifier, built on a narrow set of photon descriptors, misreads the coastal lead population: refrozen and wind roughened leads are misclassified as ice and bias the sea surface reference upward, while dark leads are indistinguishable from low albedo thin ice and excluded by default (Petty et al., 2021, Liu et al., 2025). On top of this, the embedded global tide models carry large errors in shallow bays, fjords, and inter island channels, leaving residual biases sufficient to drive thin first year ice freeboard into physically implausible negative values (Saha et al., 2025, Stammer et al., 2014). Rescuing the Coastal Record This diagnosis points directly at where the rescue effort has to happen: the surface classifier. A growing body of work, including custom and machine learning classifiers operating on ICESat-2 photon clouds, has demonstrated that a meaningful fraction of voided coastal segments contains physically valid specular returns that the operational classifier discards as ‘dark’ leads (Liu et al., 2025). As part of my ongoing PhD research at the University of Maryland College Park, I’m working towards developing algorithmic improvements to the current fixed threshold based algorithm on ICEsat-2 to a deep learning based workflow for sea ice surface classification. The improvement also tries to address the dark lead misclassification issue and leads to rescue of leads that were labelled as “dark” by the algorithm and therefore not considered for subsequent freeboard measurements from ICESat-2. From Satellite Design to Community Design The Arctic&#8217;s coastal blind spot reflects genuine physical complexity at one of the hardest remote sensing environments on Earth, compounded by algorithms calibrated for the central pack and ancillary inputs (passive microwave sea ice thickness, global tide models) that degrade near the coast. The diagnosis is now clear, and filling the spatial gap is tractable with designing coastal specific classifiers, using multi sensor integration with NASA’s Surface Water and Ocean Topography (SWOT)/ NASA-ISRO Synthetic Aperture Radar (NISAR), and conducting validation campaigns around the near coastal zone. However, the near coastal zone is not just a remote scientific abstraction. It is the most socially and ecologically consequential strip of ice in the Arctic. Landfast ice is the platform from which Indigenous communities hunt, travel, and sustain cultural practices with millennial roots (Huntington et al., 2016). Across northern Alaska the landfast season has shortened markedly since the late 1990s, compressing the spring bearded seal hunting window and leaving no easy food system substitute (Mahoney &amp; Einhorn., 2026,  Druckenmiller et al., 2013). The landfast ice edge and adjacent coastal polynyas are also among the most biologically productive features in the polar ocean. They drive spring blooms and support ringed seal pups whose survival depends on snow loaded ice lairs (Stirling, 1997), an ecological dependency directly tied to the snow on sea ice product that coastal altimetry could deliver if the data gap were closed. A satellite freeboard product that systematically voids data across this zone is not a technical inconvenience. It is a missing observational record at exactly the place where human safety, Indigenous food security, coastal stability, and marine ecosystem dynamics converge. And exactly this social and ecological importance of the near coastal zone caused me to wonder what it would look like to build satellite data products around community need rather than asking communities to adapt to what satellites already produce. It would mean going to Churchill and Cambridge Bay not just to validate algorithms but to ask what information is actually missing, at what time of season, at what spatial resolution, and in what format it would be usable. It would mean near-real-time dissemination pipelines as a design requirement, not an afterthought. It would mean feedback loops where local observers, hunters, and rangers contribute ground truth that shapes not only algorithm validation but the variables the product prioritises in the first place. The technology to do much of this exists. What has been missing is the willingness to treat community knowledge as a design input rather than a communication challenge. Bryan knew the ice better than the satellite did. The right question is not how we explain our data to him, but how we build systems that learn from what he already knows. References Kwok et al., 2019: ATLAS/ICESat-2 L3A Sea Ice Freeboard, Version 1 Petty et al., 2020: Winter Arctic Sea Ice Thickness From ICESat-2 Freeboards Smith et al., 2013: New Trans-Arctic shipping routes navigable by midcentury Nandan et al., 2017: Effect of Snow Salinity on CryoSat-2 Arctic First-Year Sea Ice Freeboard Measurements Kwok et al, 2015: Variability of Arctic sea ice thickness and volume from CryoSat-2 Petty et al., 2021: Assessment of ICESat-2 Sea Ice Surface Classification with Sentinel-2 Imagery: Implications for Freeboard and New Estimates of Lead and Floe Geometry Liu et al, 2025: Enhanced sea ice classification for ICESat-2 using combined unsupervised and supervised machine learning Saha et al., 2025: Snow depth estimation on leadless landfast ice using Cryo2Ice satellite observations Stammer et al., 2014: Accuracy assessment of global barotropic ocean tide models Huntington et al., 2016: Effects of changing sea ice on marine mammals and subsistence hunters in northern Alaska from traditional knowledge interviews Mahoney &amp; Einhorn, 2026: The Evolving Decline of Landfast Sea Ice in Northern Alaska and Adjacent Waters: Results from an Updated Climatology Druckenmiller et al., 2013: Trails to the whale: reflections of change and choice on an Iñupiat icescape at Barrow, Alaska Stirling, 1997: The importance of polynyas, ice edges, and leads to marine mammals and birds Edited by Florina Schalamon and Leah Sophie Muhle ]]></description>
													<content:encoded><![CDATA[<p style="font-weight: 400"><em>The first time I stood on sea ice, I could not tell which direction the coast was. A community member named Bryan could. That gap in situational awareness, between what a trained remote sensing scientist could read from the landscape and what a local hunter understood instinctively, turned out to mirror almost exactly the gap in our satellite data: ICESat-2 produces reliable freeboard across the central Arctic but goes systematically blind within 25 km of every coastline. This post traces that coastal data gap from its algorithmic roots through its ecological and human consequences, and asks what it would mean to build satellite products that close it on the terms of the communities who need them most.</em></p>
<p style="font-weight: 400"><em>_____________________________________________________________________________________________________________________________________</em></p>
<p style="font-weight: 400">I grew up in Bangladesh, a country defined by delta and monsoon, emphatically not by ice. So when I stepped onto the frozen surface of Hudson Bay near Churchill, Manitoba in December 2021, on my first Arctic field campaign, I was meeting sea ice for the first time outside of a textbook (Figure 1).</p>
<p style="font-weight: 400">I didn't really understand what it meant to travel over sea ice until I was on the back of a skidoo driven by a community member named Bryan. It was early in the freeze up season, what locals sometimes call the "free up" season, in acknowledgement of how volatile the margins can be. At one point, standing on the ice, I could not tell which direction the coast lay. Bryan simply followed the faint lines left by other skidoos, navigational knowledge encoded in the landscape itself, invisible to me but perfectly legible to him. A short while later, hunters returning from the landfast ice edge warned us we were closer to it than we had realised. Almost on cue, a crack began to open in the surface nearby. Bryan turned us around.</p>
<p style="font-weight: 400">In that moment, the abstract vocabulary of my remote sensing work, freeboard, sea surface reference, landfast ice extent, collapsed into something urgent. Bryan needed to know how thick that ice was. The hunters needed to know whether the edge was stable. These are not research questions. They are safety questions.</p>

<h4 style="font-weight: 400"><strong>Satellites That Couldn't See Near the Coast</strong></h4>
<p style="font-weight: 400">The campaign was meant to be a satellite validation exercise: coincident snow depth and ice thickness measurements supporting ICESat-2 and CryoSat-2 freeboard retrievals during my MSc at the University of Manitoba (freeboard is the part of the sea ice above the waterline). But after we collected the data, we discovered that ICESat-2 had produced almost no usable freeboard within the 25 km coastal buffer around our study area. The multiyear record showed the same pattern season after season: a persistent coastal blank (Figure 2). The satellite had been overhead and had properly collected photons. But the downstream algorithms could not establish a reliable sea surface reference, and the data were flagged or discarded before any calculation for freeboard was attempted. That distinction matters, because it tells us where the solution lies: not in the hardware, but in what we do with the signal (<a href="https://doi.org/10.5067/ATLAS/ATL10.001">Kwok et al, 2019,</a> <a href="https://doi.org/10.1029/2019JC015764">Petty et al., 2020</a>). If ICESat-2 could not deliver freeboard within 25 km of the coast, we had to go to get the data. The following year our team at Maryland and the University of Calgary chartered a helicopter to Cambridge Bay, Nunavut (Figure 3 shows the sites that were surveyed). Cambridge Bay is, in many ways, the textbook setting for the failure modes I had identified in Hudson Bay: narrow channels with strong tidal forcing, persistent landfast ice well into spring, heavily ridged shore fast ice, and the operational stakes of sitting on the Northwest Passage shipping corridor (<a href="https://www.pnas.org/doi/10.1073/pnas.1214212110">Smith et al., 2013</a>). All algorithmic problems described in the following occur here simultaneously. That image of clean central Arctic freeboard ringed by a stubborn coastal void became the puzzle driving my MSc thesis and now my PhD at the University of Maryland.</p>

[caption id="attachment_17495" align="alignnone" width="1600"]<a href="https://blogs.egu.eu/divisions/cr/files/2026/06/Gaps.png"><img class="size-full wp-image-17495" src="https://blogs.egu.eu/divisions/cr/files/2026/06/Gaps.png" alt="" width="1600" height="1397" /></a> Figure 2. Monthly ICESat-2 ATL10 total freeboard, November 2023 to April 2024. The dark blue ring indicates the near coastal data gap that persists through the full winter growth season. [Credit: Monojit Saha][/caption]
<h4 style="font-weight: 400"><strong>How Altimeters Measure Ice</strong></h4>
<p style="font-weight: 400">A sea ice floe sits in seawater like an ice cube in a glass with the freeboard as the portion above the waterline. Given an independent estimate of snow depth and the densities of snow, ice, and seawater, freeboard converts to total thickness through hydrostatic balance.</p>
<p style="font-weight: 400">The two altimeters at the heart of this work see the floe differently. ICESat-2's ATLAS photon counting lidar reflects from the air to snow interface and therefore measures total freeboard (snow plus ice above sea level). CryoSat-2's Ku band radar is conventionally assumed to penetrate the dry snow column and reflect from the snow to ice interface, yielding ice freeboard, although the validity of that assumption is now under active scrutiny (<a href="https://doi.org/10.1002/2017GL074506">Nandan et al., 2017</a>). The difference between the two retrievals along nearly coincident ICESat-2 and Cryosat-2 orbits provides the basis for satellite snow depth on sea ice. It is also the reason coastal data loss is doubly costly: when the algorithms fail, we lose both freeboard and the dual altimeter snow depth product simultaneously.</p>
<p style="font-weight: 400">The hard part for either sensor is the reference. We need an accurate, instantaneous sea surface height beneath the satellite, which in practice means finding open water or thin ice leads (sea ice leads are long cracks formed when Arctic ice floes diverge or shear), measuring their elevation, and differencing it from the surrounding ice. In the central pack, where leads are abundant and geometrically clean, this works well (<a href="https://doi.org/10.1098/rsta.2014.0157">Kwok et al., 2015</a>). However, near the coast the scarcity of open water leads in the landfast ice along with challenges poised by algorithmic limitations linked to interactions of lidar with the rugged landfast ice makes the traditional method of measuring freeboard and ice thickness difficult. ICESat-2’s lead classifier, built on a narrow set of photon descriptors, misreads the coastal lead population: refrozen and wind roughened leads are misclassified as ice and bias the sea surface reference upward, while dark leads are indistinguishable from low albedo thin ice and excluded by default (<a href="https://doi.org/10.1029/2020EA001491">Petty et al., 2021</a>, <a href="https://doi.org/10.1016/j.rse.2025.114607">Liu et al., 2025</a>). On top of this, the embedded global tide models carry large errors in shallow bays, fjords, and inter island channels, leaving residual biases sufficient to drive thin first year ice freeboard into physically implausible negative values (<a href="https://doi.org/10.5194/tc-19-325-2025">Saha et al., 2025</a>, <a href="https://doi.org/10.1002/2014RG000450">Stammer et al., 2014</a>).</p>

[caption id="attachment_17498" align="alignnone" width="1600"]<a href="https://blogs.egu.eu/divisions/cr/files/2026/06/tc-19-325-2025-f01-web.png"><img class="size-full wp-image-17498" src="https://blogs.egu.eu/divisions/cr/files/2026/06/tc-19-325-2025-f01-web.png" alt="" width="1600" height="1457" /></a> Figure 3. Study sites at Cambridge Bay that were surveyed to understand the near-coastal ice along the Dease Strait [Credit: Saha et al., 2025][/caption]
<h4 style="font-weight: 400"><strong>Rescuing the Coastal Record</strong></h4>
<p style="font-weight: 400">This diagnosis points directly at where the rescue effort has to happen: the surface classifier. A growing body of work, including custom and machine learning classifiers operating on ICESat-2 photon clouds, has demonstrated that a meaningful fraction of voided coastal segments contains physically valid specular returns that the operational classifier discards as ‘dark’ leads (<a href="https://doi.org/10.1016/j.rse.2025.114607">Liu et al., 2025</a>).</p>
<p style="font-weight: 400">As part of my ongoing PhD research at the University of Maryland College Park, I’m working towards developing algorithmic improvements to the current fixed threshold based algorithm on ICEsat-2 to a deep learning based workflow for sea ice surface classification. The improvement also tries to address the dark lead misclassification issue and leads to rescue of leads that were labelled as “dark” by the algorithm and therefore not considered for subsequent freeboard measurements from ICESat-2.</p>

<h4 style="font-weight: 400"><strong>From Satellite Design to Community Design</strong></h4>
<p style="font-weight: 400">The Arctic's coastal blind spot reflects genuine physical complexity at one of the hardest remote sensing environments on Earth, compounded by algorithms calibrated for the central pack and ancillary inputs (passive microwave sea ice thickness, global tide models) that degrade near the coast. The diagnosis is now clear, and filling the spatial gap is tractable with designing coastal specific classifiers, using multi sensor integration with NASA’s Surface Water and Ocean Topography (SWOT)/ NASA-ISRO Synthetic Aperture Radar (NISAR), and conducting validation campaigns around the near coastal zone.</p>
However, the near coastal zone is not just a remote scientific abstraction. It is the most socially and ecologically consequential strip of ice in the Arctic. Landfast ice is the platform from which Indigenous communities hunt, travel, and sustain cultural practices with millennial roots (<a href="https://doi.org/10.1098/rsbl.2016.0198">Huntington et al., 2016</a>). Across northern Alaska the landfast season has shortened markedly since the late 1990s, compressing the spring bearded seal hunting window and leaving no easy food system substitute (<a href="https://doi.org/10.1029/2025JC022464">Mahoney &amp; Einhorn., 2026</a>,  <a href="https://doi.org/10.1080/1088937X.2012.724459">Druckenmiller et al., 2013</a>). The landfast ice edge and adjacent coastal polynyas are also among the most biologically productive features in the polar ocean. They drive spring blooms and support ringed seal pups whose survival depends on snow loaded ice lairs (<a href="https://doi.org/10.1016/S0924-7963(96)00054-1">Stirling, 1997</a>), an ecological dependency directly tied to the snow on sea ice product that coastal altimetry could deliver if the data gap were closed. A satellite freeboard product that systematically voids data across this zone is not a technical inconvenience. It is a missing observational record at exactly the place where human safety, Indigenous food security, coastal stability, and marine ecosystem dynamics converge.
<p style="font-weight: 400">And exactly this social and ecological importance of the near coastal zone caused me to wonder what it would look like to build satellite data products around community need rather than asking communities to adapt to what satellites already produce. It would mean going to Churchill and Cambridge Bay not just to validate algorithms but to ask what information is actually missing, at what time of season, at what spatial resolution, and in what format it would be usable. It would mean near-real-time dissemination pipelines as a design requirement, not an afterthought. It would mean feedback loops where local observers, hunters, and rangers contribute ground truth that shapes not only algorithm validation but the variables the product prioritises in the first place. The technology to do much of this exists. What has been missing is the willingness to treat community knowledge as a design input rather than a communication challenge. Bryan knew the ice better than the satellite did. The right question is not how we explain our data to him, but how we build systems that learn from what he already knows.</p>

<h4><strong>References</strong></h4>
<ul>
 	<li><strong>Kwok et al., 2019</strong>: <a href="https://nsidc.org/data/atl10/versions/1">ATLAS/ICESat-2 L3A Sea Ice Freeboard, Version 1</a></li>
 	<li><strong>Petty et al., 2020</strong>: <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2019JC015764">Winter Arctic Sea Ice Thickness From ICESat-2 Freeboards</a></li>
 	<li><strong>Smith et al., 2013</strong>: <a href="https://www.pnas.org/doi/10.1073/pnas.1214212110">New Trans-Arctic shipping routes navigable by midcentury</a></li>
 	<li><strong>Nandan et al., 2017</strong>: <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1002/2017GL074506">Effect of Snow Salinity on CryoSat-2 Arctic First-Year Sea Ice Freeboard Measurements</a></li>
 	<li><strong>Kwok et al, 2015</strong>: <a href="https://royalsocietypublishing.org/rsta/article/373/2045/20140157/114910/Variability-of-Arctic-sea-ice-thickness-and-volume">Variability of Arctic sea ice thickness and volume from CryoSat-2</a></li>
 	<li><strong>Petty et al., 2021</strong>: <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2020EA001491">Assessment of ICESat-2 Sea Ice Surface Classification with Sentinel-2 Imagery: Implications for Freeboard and New Estimates of Lead and Floe Geometry</a></li>
 	<li><strong>Liu et al, 2025</strong>: <a href="https://www.sciencedirect.com/science/article/pii/S0034425725000112?via%3Dihub">Enhanced sea ice classification for ICESat-2 using combined unsupervised and supervised machine learning</a></li>
 	<li><strong>Saha et al., 2025</strong>: <a href="https://tc.copernicus.org/articles/19/325/2025/">Snow depth estimation on leadless landfast ice using Cryo2Ice satellite observations</a></li>
 	<li><strong>Stammer et al., 2014</strong>: <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1002/2014RG000450">Accuracy assessment of global barotropic ocean tide models</a></li>
 	<li><strong>Huntington et al., 2016</strong>: <a href="https://royalsocietypublishing.org/rsbl/article/12/8/20160198/87893/Effects-of-changing-sea-ice-on-marine-mammals-and">Effects of changing sea ice on marine mammals and subsistence hunters in northern Alaska from traditional knowledge interviews</a></li>
 	<li><strong>Mahoney &amp; Einhorn, 2026</strong>: <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2025JC022464">The Evolving Decline of Landfast Sea Ice in Northern Alaska and Adjacent Waters: Results from an Updated Climatology</a></li>
 	<li><strong>Druckenmiller et al., 2013</strong>: <a href="https://doi.org/10.1080/1088937X.2012.724459">Trails to the whale: reflections of change and choice on an Iñupiat icescape at Barrow, Alaska</a></li>
 	<li><strong>Stirling, 1997</strong>: <a href="https://doi.org/10.1016/S0924-7963(96)00054-1">The importance of polynyas, ice edges, and leads to marine mammals and birds</a></li>
</ul>
<p style="text-align: right"><strong><em>Edited by Florina Schalamon and Leah Sophie Muhle </em></strong></p>]]></content:encoded>
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					<title><![CDATA[Geodesy Cartoons – A Creative Tool for Outreach and Education]]></title>
					<link>https://blogs.egu.eu/divisions/g/2026/06/12/geodesy-cartoons/</link>
					<comments>https://blogs.egu.eu/divisions/g/2026/06/12/geodesy-cartoons/#comments</comments>
					<pubDate>Fri, 12 Jun 2026 09:00:16 +0000</pubDate>
					<dc:creator><![CDATA[Leire Retegui-Schiettekatte]]></dc:creator>
							<category><![CDATA[Guest post]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Geodesy is fundamental to understanding our dynamic planet. From monitoring sea-level rise and glacier melt to maintaining precise terrestrial reference frames for GNSS and Earth observation, geodesy provides the scientific backbone for many disciplines represented within the EGU and beyond. Despite its importance, geodesy often remains invisible outside the scientific community. Even within geosciences, many people use geodetic products daily without fully realizing the complex infrastructure and science behind them. To help make geodesy more visible and accessible, the International Association of Geodesy (IAG) and its Global Geodetic Observing System (GGOS) launched the Geodesy Cartoon initiative in 2024. The idea is simple: use cartoons and illustrations to explain geodetic concepts in a creative, understandable, and visually engaging way. At first glance, cartoons may seem unusual in a scientific context. However, they can be remarkably effective tools for science communication. Concepts such as reference frames, GNSS positioning, gravity field modelling, VLBI, or satellite geodesy are often difficult to explain to non-specialists. Visual storytelling helps lower the entry barrier and creates intuitive connections between complex scientific methods and their real-world applications. The cartoons cover a broad spectrum of topics relevant to the geodetic and geospatial community, including: GNSS and precise positioning, Earth observation and climate monitoring, gravity field determination, geodetic infrastructure and reference frames, surveying and land administration, and the role of geodesy in daily life. Many of the cartoons are particularly useful for lectures, conference presentations, outreach events, teaching activities, and social media communication. They can also help Early Career Scientists communicate their work to broader audiences, an increasingly important skill in interdisciplinary science and public engagement. A major milestone for the initiative was the international Geodesy Cartoon Competition, whose winners were announced during the EGU General Assembly 2026 in Vienna. The competition attracted 274 submissions from 119 cartoonists across 46 countries, demonstrating strong international interest in creative geoscience communication. The best cartoons were exhibited at the IAG Geodesy Reception during EGU26 and sparked numerous discussions among scientists about new ways of communicating research and geodetic applications. One particularly encouraging aspect was the diversity of contributors. Alongside professional scientists, the competition also attracted students, educators, and professional cartoonists, highlighting how science communication can connect communities far beyond traditional academic boundaries. For the geodesy community, initiatives like this are about more than outreach alone. They are also about visibility. While disciplines such as meteorology or geology are widely recognized by the public, geodesy often remains unknown despite underpinning positioning, navigation, digital twins, and many Earth observation applications. Strengthening awareness of geodesy is therefore essential not only for education, but also for attracting future students, supporting scientific collaboration, and highlighting the societal relevance of geodetic research. All cartoons are openly available under a Creative Commons license and can be freely reused for educational and outreach purposes. Further information: https://geodesy.science/cartoon – Edited by Leire Retegui-Schiettekatte]]></description>
													<content:encoded><![CDATA[Geodesy is fundamental to understanding our dynamic planet. From monitoring sea-level rise and glacier melt to maintaining precise terrestrial reference frames for GNSS and Earth observation, geodesy provides the scientific backbone for many disciplines represented within the EGU and beyond. Despite its importance, geodesy often remains invisible outside the scientific community. Even within geosciences, many people use geodetic products daily without fully realizing the complex infrastructure and science behind them.

To help make geodesy more visible and accessible, the International Association of Geodesy (IAG) and its Global Geodetic Observing System (GGOS) launched the Geodesy Cartoon initiative in 2024. The idea is simple: use cartoons and illustrations to explain geodetic concepts in a creative, understandable, and visually engaging way.

[caption id="attachment_5711" align="aligncenter" width="1600"]<a href="https://blogs.egu.eu/divisions/g/files/2026/05/Cat1_small_cropped.jpg"><img class="wp-image-5711 size-full" src="https://blogs.egu.eu/divisions/g/files/2026/05/Cat1_small_cropped.jpg" alt="Top cartoons in Category 1 - Explaining Geodesy." width="1600" height="922" /></a> <strong>Top cartoons in Category 1 - Explaining Geodesy.</strong> Cartoons by Eda Uzunoglu and Atmaja Septa Miyosa, distributed by <a href="https://geodesy.science/cartoon" target="_blank" rel="noopener"><u>geodesy.science/cartoon.</u></a> <span style="text-decoration: underline"><a class="external text" href="http://creativecommons.org/licenses/by/2.0/" target="_blank" rel="nofollow noopener">CC BY</a></span>.[/caption]

At first glance, cartoons may seem unusual in a scientific context. However, they can be remarkably effective tools for science communication. Concepts such as reference frames, GNSS positioning, gravity field modelling, VLBI, or satellite geodesy are often difficult to explain to non-specialists. Visual storytelling helps lower the entry barrier and creates intuitive connections between complex scientific methods and their real-world applications.

The cartoons cover a broad spectrum of topics relevant to the geodetic and geospatial community, including:
<ul>
 	<li>GNSS and precise positioning,</li>
 	<li>Earth observation and climate monitoring,</li>
 	<li>gravity field determination,</li>
 	<li>geodetic infrastructure and reference frames,</li>
 	<li>surveying and land administration,</li>
 	<li>and the role of geodesy in daily life.</li>
</ul>
Many of the cartoons are particularly useful for lectures, conference presentations, outreach events, teaching activities, and social media communication. They can also help Early Career Scientists communicate their work to broader audiences, an increasingly important skill in interdisciplinary science and public engagement.

[caption id="attachment_5712" align="aligncenter" width="1600"]<a href="https://blogs.egu.eu/divisions/g/files/2026/05/Cat2_small_cropped.jpg"><img class="wp-image-5712 size-full" src="https://blogs.egu.eu/divisions/g/files/2026/05/Cat2_small_cropped.jpg" alt="Top cartoons in Category 2 - Observation Techniques." width="1600" height="899" /></a> <strong>Top cartoons in Category 2 - Observation Techniques.</strong> Cartoons by Doru Axinte and Tom Fiedler, distributed by <a href="https://geodesy.science/cartoon" target="_blank" rel="noopener"><u>geodesy.science/cartoon.</u></a> <span style="text-decoration: underline"><a class="external text" href="http://creativecommons.org/licenses/by/2.0/" target="_blank" rel="nofollow noopener">CC BY</a></span>.[/caption]

A major milestone for the initiative was the international <strong>Geodesy Cartoon Competition</strong>, whose winners were announced during the EGU General Assembly 2026 in Vienna. The competition attracted 274 submissions from 119 cartoonists across 46 countries, demonstrating strong international interest in creative geoscience communication. The best cartoons were exhibited at the IAG Geodesy Reception during EGU26 and sparked numerous discussions among scientists about new ways of communicating research and geodetic applications.

One particularly encouraging aspect was the diversity of contributors. Alongside professional scientists, the competition also attracted students, educators, and professional cartoonists, highlighting how science communication can connect communities far beyond traditional academic boundaries.

[caption id="attachment_5713" align="aligncenter" width="1600"]<a href="https://blogs.egu.eu/divisions/g/files/2026/05/Cat3_small_cropped.jpg"><img class="wp-image-5713 size-full" src="https://blogs.egu.eu/divisions/g/files/2026/05/Cat3_small_cropped.jpg" alt="Top cartoons in Category 3 - Geodetic Products." width="1600" height="854" /></a> <strong>Top cartoons in Category 3 - Geodetic Products.</strong> Cartoons by Friedrich Tasser and Tom Fiedler, distributed by <a href="https://geodesy.science/cartoon" target="_blank" rel="noopener"><u>geodesy.science/cartoon.</u></a> <span style="text-decoration: underline"><a class="external text" href="http://creativecommons.org/licenses/by/2.0/" target="_blank" rel="nofollow noopener">CC BY</a></span>.[/caption]

For the geodesy community, initiatives like this are about more than outreach alone. They are also about visibility. While disciplines such as meteorology or geology are widely recognized by the public, geodesy often remains unknown despite underpinning positioning, navigation, digital twins, and many Earth observation applications. Strengthening awareness of geodesy is therefore essential not only for education, but also for attracting future students, supporting scientific collaboration, and highlighting the societal relevance of geodetic research.

All cartoons are openly available under a Creative Commons license and can be freely reused for educational and outreach purposes.

Further information: <a href="https://geodesy.science/cartoon" target="_blank" rel="noopener"><u>https://geodesy.science/cartoon</u></a>
<p style="text-align: right"><em>– Edited by Leire Retegui-Schiettekatte</em></p>]]></content:encoded>
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					<title><![CDATA[HydroTalks podcast: Introducing Ilias Pechlivanidis, the HS Division President-elect]]></title>
					<link>https://blogs.egu.eu/divisions/hs/2026/06/11/hydrotalks-podcast-introducing-ilias-pechlivanidis-the-hs-division-president-elect/</link>
					<comments>https://blogs.egu.eu/divisions/hs/2026/06/11/hydrotalks-podcast-introducing-ilias-pechlivanidis-the-hs-division-president-elect/#comments</comments>
					<pubDate>Thu, 11 Jun 2026 17:00:00 +0000</pubDate>
					<dc:creator><![CDATA[Archita Bhattacharyya]]></dc:creator>
							<category><![CDATA[division president]]></category>
		<category><![CDATA[Extreme events]]></category>
		<category><![CDATA[Hydrological forecasting]]></category>
		<category><![CDATA[Talking hydrology]]></category>
		<category><![CDATA[forecasting]]></category>
		<category><![CDATA[HS Division]]></category>
		<category><![CDATA[hydrological extremes]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[For this  episode of HydroTalks, we’re thrilled to welcome Dr. Ilias Pechlivanidis, Senior Researcher and Associate Professor (Docent) in hydrology and water resources at the Swedish Meteorological and Hydrological Institute (SMHI), and Visiting Researcher at Uppsala University. He is currently the Vice President of the EGU Hydrological Sciences Division and will serve as Division President for the 2027–2029 term. His responsibilities will include representing the hydrological scientific community within EGU, and managing the administration of the division, especially arranging the programme at the General Assembly. You can check out the full episode here and read the interview summary in this blog! About Ilias’s research Please tell us about your research. A large part of my research focuses on improving hydrological predictions. I investigate forecasting systems across river basins, from hours and days ahead to seasonal timescales. I am particularly interested in hybrid modelling, which combines process-based hydrological models with artificial intelligence. The key focus is to predict different hydrological conditions, including extremes, and translate predictions into actionable decisions. How do hydrological forecasts work in simple terms? And have you seen these forecasting systems evolve over time? At its core, hydrological forecasting needs three things: knowledge of today’s river conditions, such as soil moisture, snowpack and lake/reservoir levels; access to meteorological forecasts; and a well-performing hydrological model. To get today’s river conditions, we run the model using historical and real-time observations. Having actual condition data is a benefit, and we can assimilate those data into the model. After that, we force the model with meteorological forecasts, from hours and days ahead to seasons ahead. There are more advanced methods nowadays. Thanks to satellite-based products and methods such as data simulation schemes and machine learning, we have experienced quite some evolution in forecasting systems. For example, flood early warning systems can sometimes predict floods up to eight days ahead, depending of course on the river system. (Read More) Do forecasting systems perform equally well everywhere? Slow-responding rivers, including systems strongly influenced by lakes, snow/ice accumulation and melting or baseflow, can be more predictable than fast-responding rivers that are controlled by rainfall. Accurate meteorological forecasts are essential however, with regions experiencing localised convective rainfall remain challenging to capture. However, forecast performance is not the same as forecast usability, because decisions are even made with biased and uncertain predictions. (Read more) How could AI transform hydrological forecasting? AI and machine learning can improve accuracy, reduce uncertainty, generate high-resolution forecasts and even help us understand the drivers of predictability. Explainable AI and hybrid models are promising, because they bring physical knowledge and data-driven insights together. I see opportunities in the next-generation early warning systems through AI, supporting citizen-centred communications and helping individuals respond to disasters. However, AI integration in early warning systems must be done carefully, ensuring transparency and robustness, and following standardised evaluation frameworks and data security protocols. (Read more) How can better forecasts support local communities? Better forecasts can provide earlier and more accurate warnings, giving communities time to prepare and respond. This can reduce loss of life, economic damage and long-term disruption, as seen in some European countries in 2021, 2023 and 2024. But producing an accurate forecast is only part of the challenge. Warnings need to be clear, communicating the impacts to the society,, while they should ideally be tailored to different groups, so that  everyone can to understand what the warning means for them. (Read more) About Ilias’s role as incoming President of HS Division When did you first become involved with EGU? I first attended EGU in 2007 and have remained actively involved since then. Over the years, I have convened sessions, contributed to community activities, and served as the scientific officer for the Hydrological Forecasting subdivision from 2020 to 2024. What is your vision for the Hydrological Sciences Division? I want the division to remain a global and inclusive home for hydrologists. This means bringing in more voices from outside Europe, supporting early-career scientists, and strengthening connections with international communities. I also want to promote innovation, and  ensure that science continues supporting real-life decisions. I want to foster an open and collaborative culture of sharing ideas. Which skills do you believe could help in your role? Both academic and non-academic skills are essential. This includes a broad understanding of hydrology and water resources, alongside skills such as leadership, efficient communication, international coordination and collaboration, and inclusivity across disciplines, institutions, and cultures. What do you expect to be the most challenging and rewarding parts of the role? One challenge will be balancing the priorities of a large and diverse international community. At the same time, that diversity is also the most rewarding part. Bringing together different perspectives, supporting collaboration, and seeing ideas develop into impactful science and services can be very fulfilling. What career advice would you share with early-career scientists? Stay focused on your ethics and long-term goals, but remain open to opportunities beyond your immediate field. A career path does not always need to be linear. Sometimes taking a thoughtful risk can lead to something innovative. Check out the full episode here.]]></description>
													<content:encoded><![CDATA[For this  episode of HydroTalks, we’re thrilled to welcome <a href="https://www.smhi.se/en/research/our-team/search-for-employees/ilias-pechlivanidis"><u>Dr. Ilias Pechlivanidis</u></a>, Senior Researcher and Associate Professor (Docent) in hydrology and water resources at the Swedish Meteorological and Hydrological Institute (SMHI), and Visiting Researcher at Uppsala University.

He is currently the <a href="https://www.egu.eu/elections/egu-election-autumn-2025/"><u>Vice </u><u>President</u></a> of the EGU Hydrological Sciences Division and will serve as Division President for the 2027–2029 term. His responsibilities will include representing the hydrological scientific community within EGU, and managing the administration of the division, especially arranging the programme at the General Assembly.

You can check out the <a href="https://youtu.be/w2ZQuOx6HmY?si=qB9A8dhipdxRm52e">full episode here</a> and read the interview summary in this blog!

[caption id="attachment_13947" align="alignnone" width="276"]<img class="wp-image-13947 size-medium" src="https://blogs.egu.eu/divisions/hs/files/2026/06/Ilias_photonew-276x300.jpg" alt="" width="276" height="300" /> Dr. Ilias Pechlivanidis[/caption]
<h1><strong>About Ilias’s research</strong></h1>
<strong>Please tell us about your research</strong><strong>.</strong>

A large part of my research focuses on improving hydrological predictions. I investigate forecasting systems across river basins, from hours and days ahead to seasonal timescales. I am particularly interested in hybrid modelling, which combines process-based hydrological models with artificial intelligence. The key focus is to predict different hydrological conditions, including extremes, and translate predictions into actionable decisions.

<strong>How do hydrological forecasts work in simple terms?</strong><strong> And </strong><strong>have you seen these forecasting systems </strong><strong>evolve over time?</strong>

At its core, hydrological forecasting needs three things: knowledge of today’s river conditions, such as soil moisture, snowpack and lake/reservoir levels; access to meteorological forecasts; and a well-performing hydrological model. To get today’s river conditions, we run the model using historical and real-time observations. Having actual condition data is a benefit, and we can assimilate those data into the model. After that, we force the model with meteorological forecasts, from hours and days ahead to seasons ahead. There are more advanced methods nowadays.

Thanks to satellite-based products and methods such as data simulation schemes and machine learning, we have experienced quite some evolution in forecasting systems. For example, flood early warning systems can sometimes predict floods up to eight days ahead, depending of course on the river system. (<a href="https://doi.org/10.1175/BAMS-D-24-0322.1"><u>Read More</u></a>)

<strong>Do forecasting systems perform equally well everywhere?</strong>

Slow-responding rivers, including systems strongly influenced by lakes, snow/ice accumulation and melting or baseflow, can be more predictable than fast-responding rivers that are controlled by rainfall. Accurate meteorological forecasts are essential however, with regions experiencing localised convective rainfall remain challenging to capture. However, forecast performance is not the same as forecast usability, because decisions are even made with biased and uncertain predictions. (<a href="https://doi.org/10.1029/2019WR026987"><u>Read more</u></a>)

<strong>How could AI transform hydrological forecasting?</strong>

AI and machine learning can improve accuracy, reduce uncertainty, generate high-resolution forecasts and even help us understand the drivers of predictability. Explainable AI and hybrid models are promising, because they bring physical knowledge and data-driven insights together. I see opportunities in the next-generation early warning systems through AI, supporting citizen-centred communications and helping individuals respond to disasters. However, AI integration in early warning systems must be done carefully, ensuring transparency and robustness, and following standardised evaluation frameworks and data security protocols. (<a href="https://doi.org/10.1038/s43247-025-02324-y"><u>Read more</u></a>)

<strong>How can better forecasts support local communities?</strong>

Better forecasts can provide earlier and more accurate warnings, giving communities time to prepare and respond. This can reduce loss of life, economic damage and long-term disruption, as seen in some European countries in 2021, 2023 and 2024. But producing an accurate forecast is only part of the challenge. Warnings need to be clear, communicating the impacts to the society,, while they should ideally be tailored to different groups, so that  everyone can to understand what the warning means for them. (<a href="https://doi.org/10.1038/s41562-026-02405-8"><u>Read more</u></a>)
<h1>About Ilias’s role as incoming President of HS Division</h1>
<strong>When did you first become involved with EGU?</strong>

I first attended EGU in 2007 and have remained actively involved since then. Over the years, I have convened sessions, contributed to community activities, and served as the scientific officer for the Hydrological Forecasting subdivision from 2020 to 2024.

[caption id="attachment_13950" align="alignnone" width="477"]<img class="wp-image-13950" src="https://blogs.egu.eu/divisions/hs/files/2026/06/EGU24_HS_Hydro_forecasting_meeting-300x225.jpg" alt="" width="477" height="358" /> Photo with colleagues from the Hydrological Forecasting HS subdivision at EGU24[/caption]

<strong>What is your vision for the Hydrological Sciences Division?</strong>

I want the division to remain a global and inclusive home for hydrologists. This means bringing in more voices from outside Europe, supporting early-career scientists, and strengthening connections with international communities. I also want to promote innovation, and  ensure that science continues supporting real-life decisions. I want to foster an open and collaborative culture of sharing ideas.

<strong>Which skills do you believe could help</strong><strong> in your role?</strong>

Both academic and non-academic skills are essential. This includes a broad understanding of hydrology and water resources, alongside skills such as leadership, efficient communication, international coordination and collaboration, and inclusivity across disciplines, institutions, and cultures.

<strong>What do you expect to be the most challenging and rewarding parts of the role?</strong>

One challenge will be balancing the priorities of a large and diverse international community. At the same time, that diversity is also the most rewarding part. Bringing together different perspectives, supporting collaboration, and seeing ideas develop into impactful science and services can be very fulfilling.

<strong>What career advice would you share with early-career scientists?</strong>

Stay focused on your ethics and long-term goals, but remain open to opportunities beyond your immediate field. A career path does not always need to be linear. Sometimes taking a thoughtful risk can lead to something innovative.

Check out the <a href="https://youtu.be/w2ZQuOx6HmY?si=qB9A8dhipdxRm52e">full episode here.</a>]]></content:encoded>
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					<title><![CDATA[(Almost) everything wrong with: Journey to the Centre of the Earth]]></title>
					<link>https://blogs.egu.eu/divisions/gd/2026/06/10/almost-everything-wrong-with-journey-to-the-centre-of-the-earth/</link>
					<comments>https://blogs.egu.eu/divisions/gd/2026/06/10/almost-everything-wrong-with-journey-to-the-centre-of-the-earth/#comments</comments>
					<pubDate>Wed, 10 Jun 2026 08:00:11 +0000</pubDate>
					<dc:creator><![CDATA[Editorial team 1]]></dc:creator>
							<category><![CDATA[Uncategorised]]></category>
		<category><![CDATA[Earth sciences]]></category>
		<category><![CDATA[geodynamics]]></category>
		<category><![CDATA[geology]]></category>
		<category><![CDATA[how science works]]></category>
		<category><![CDATA[movies]]></category>
		<category><![CDATA[science fiction]]></category>
		<category><![CDATA[tectonophysics]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[ Spoiler warning! &nbsp; Have you ever watched a science fiction movie and thought, huh, I wonder if that is actually possible? Now, I hope by the time the dinosaurs turned up during this film, that this transient thought had departed from your mind, but to satisfy the idle curiosity of those who wondered this during Journey to the Centre of the Earth, and perhaps even impart some geodynamical lessons, I delved into the cinematic world of the Jules Verne adaptation. &nbsp; In 2008, a science fiction action-adventure movie was released starring Brendan Fraser and Josh Hutcherson, adapted from the famous 1864 novel of the same name by Jules Verne. The movie follows the adventure of volcanologist Trevor Anderson and his nephew Sean as they search for Trevor’s missing brother. Their journey takes them to Iceland, to an old mine, and then down volcanic tubes into the mysterious, fantastic, and dangerous centre of the Earth. &nbsp; Of course, they were actors playing a part in a fictional movie; they didn’t really go there, and it is simply a fantastical tale that claims no truth in its telling. You might think it pedantic, fastidious, or pretentious to fact check such a story. You might even see it as a completely pointless endeavour. You could be right, yet I will do it anyway. For those who were mildly perturbed when Trevor Anderson whispered “muscovite” I present: (almost) everything wrong with Journey to the Centre of the Earth. &nbsp; &nbsp; &nbsp; Journey to the Centre of the Earth film poster, New Line Cinema &nbsp; Hollow Earth? Let’s start with the most obvious: the hollow Earth. The signal we receive from seismic waves (vibrations that transfer energy through the ground) immediately rules this out. What we see is only consistent with a layered planet, mostly solid with a liquid layer in the outer part of the core. If you want more information about what is really going on down there, check out Prachi Kar&#8217;s blog post on the giant blobs deep inside the Earth. Speaking of liquids inside the Earth, I refer to molten iron and nickel, and not an ocean of water. Despite how cool it would be to sail across an underground ocean while dodging piranhas, the water inside the Earth is mostly locked away as a solid inside minerals like ringwoodite, and liquid water is dispersed in the tiny cracks between rocks, not in giant bodies of water. &nbsp; Falling into the oven If you’ve ever been underground, you might have noticed: it gets hot quickly. A main antagonist of our heroes in Journey to the Centre of the Earth is the temperature. Yet, things would be even more drastic than is portrayed on film. When they fall down the lava tube, they travel for an uncertain but lengthy distance, so long in fact, that there is a transition implying the scene was shortened for us. Trevor shouts out that it could be hundreds of kilometres deep as they fall—which would be a death sentence in many ways. From the time spent falling on screen, a back of the envelope calculation tells us they are at minimum seven kilometres deep in the Earth. Even though the movie suggests they are actually somewhere much deeper, this depth is already impressive, and would be the deepest humans have ever been inside the Earth. We know that temperature increases with depth, and we call the rate at which it does it the geothermal gradient. Beneath a regular colder part of the Earth’s crust like Ireland, where the geothermal gradient is 25°C/km, the temperature at seven kilometres would be a sizzling 175°C, and our main characters would meet a crispy end. Beneath Iceland, things are much worse. Gradients between 50 and 150°C/km in Iceland would mean Trevor and company ride their lava tunnel water slide into an ocean around 600°C. For reference, that’s a touch warmer than the hot springs of Tuscany. On a side note: water boils at 100°C at the Earth’s surface, but at high pressures this reaches much higher—so the presence of liquid water is not the crazy part. I guess they most have packed SPF 50,000, because they shrug off the blistering heat and continue on. But wait—shouldn’t they be under some serious pressure? And I don’t mean because they are on a perilous quest, but rather the immense pressures that exist at depth in the Earth. At the surface of the Earth, the pressure is 1 atm, or 101,325 Pa. At seven kilometres depth, a cavern that size would be under immense differential pressure. Lithostatic pressure of 2000 times the Earth’s surface would instantly crush the cavern and poor Trevor. Fortunately, they must have fallen into a cave with magical properties because it manages to withstand the weight of the Earth’s crust. &nbsp; Suspicious rocks Before their great fall to their physically-assured deaths, our main characters find themselves in a lava tube. Now, lava tubes are a geological phenomenon that do in fact exist—we can see them in nature. However, lava tubes form during lava flows, and are therefore found near or at the surface. They can be very long, so the 7 km length of the lava tube in the film is not strange but its orientation very much is. They form from the flow of lava and thus form horizontally, not vertically! We haven’t yet addressed the elephant in the room: the muscovite. Muscovite is not a rock, as the film portrays it, but rather a thin platy mineral found in igneous and metamorphic rocks. It is very weak, and even if you somehow constructed a thin floor made of muscovite (a geologically nonsensical idea), it would certainly not support the weight of a human. Fortunately for the characters, the muscovite in the film has a sense of dramatic timing, and only follows the laws of physics when it chooses to! &nbsp; Thurston Lava Tube at Hawaii Volcanoes National Park, Big Island, Hawaii. Author: Frank Schulenburg &nbsp; At the end of the day, Journey to the Centre of the Earth may violate the laws of physics, contradict our understanding of geodynamics, and even show dinosaurs to be living inside the Earth, but it is a fun adventure, and worth a watch!]]></description>
													<content:encoded><![CDATA[<h3 style="text-align: center"><strong> </strong><strong>Spoiler warning!</strong></h3>
&nbsp;

<strong>Have you ever watched a science fiction movie and thought, huh, I wonder if that is actually possible? Now, I hope by the time the dinosaurs turned up during this film, that this transient thought had departed from your mind, but to satisfy the idle curiosity of those who wondered this during Journey to the Centre of the Earth, and perhaps even impart some geodynamical lessons, I delved into the cinematic world of the Jules Verne adaptation.</strong>

&nbsp;

In 2008, a science fiction action-adventure movie was released starring Brendan Fraser and Josh Hutcherson, adapted from the famous 1864 novel of the same name by Jules Verne. The movie follows the adventure of volcanologist Trevor Anderson and his nephew Sean as they search for Trevor’s missing brother. Their journey takes them to Iceland, to an old mine, and then down volcanic tubes into the mysterious, fantastic, and dangerous centre of the Earth.

<a href="https://blogs.egu.eu/divisions/gd/?attachment_id=42719" rel="attachment wp-att-42719">
<img class="size-medium wp-image-42719 alignleft" src="https://blogs.egu.eu/divisions/gd/files/2026/04/Center_of_the_earth_3d-203x300.jpg" alt="" width="203" height="300" /></a>

&nbsp;

Of course, they were actors playing a part in a fictional movie; they didn’t really go there, and it is simply a fantastical tale that claims no truth in its telling. You might think it pedantic, fastidious, or pretentious to fact check such a story. You might even see it as a completely pointless endeavour.

You could be right, yet I will do it anyway. For those who were mildly perturbed when Trevor Anderson whispered “muscovite” I present: (almost) everything wrong with Journey to the Centre of the Earth.

&nbsp;

&nbsp;

&nbsp;

Journey to the Centre of the Earth

film poster, New Line Cinema

&nbsp;
<h3><strong>Hollow Earth?</strong></h3>
Let’s start with the most obvious: the hollow Earth. The signal we receive from seismic waves (vibrations that transfer energy through the ground) immediately rules this out. What we see is only consistent with a layered planet, mostly solid with a liquid layer in the outer part of the core. If you want more information about what is really going on down there, check out Prachi Kar's blog post on the <a href="https://blogs.egu.eu/divisions/gd/2025/10/08/my-journey-towards-the-centre-of-the-earth/">giant blobs deep inside the Earth</a>.

Speaking of liquids inside the Earth, I refer to molten iron and nickel, and not an ocean of water. Despite how cool it would be to sail across an underground ocean while dodging piranhas, the water inside the Earth is mostly locked away as a solid inside minerals like ringwoodite, and liquid water is dispersed in the tiny cracks between rocks, not in giant bodies of water.

&nbsp;
<h3><strong>Falling into the oven</strong></h3>
If you’ve ever been underground, you might have noticed: it gets hot quickly. A main antagonist of our heroes in Journey to the Centre of the Earth is the temperature. Yet, things would be even more drastic than is portrayed on film. When they fall down the lava tube, they travel for an uncertain but lengthy distance, so long in fact, that there is a transition implying the scene was shortened for us. Trevor shouts out that it could be hundreds of kilometres deep as they fall—which would be a death sentence in many ways. From the time spent falling on screen, a back of the envelope calculation tells us they are at minimum seven kilometres deep in the Earth. Even though the movie suggests they are actually somewhere much deeper, this depth is already impressive, and would be the deepest humans have ever been inside the Earth.

We know that temperature increases with depth, and we call the rate at which it does it the geothermal gradient. Beneath a regular colder part of the Earth’s crust like Ireland, where the geothermal gradient is 25°C/km, the temperature at seven kilometres would be a sizzling 175°C, and our main characters would meet a crispy end. Beneath Iceland, things are much worse. Gradients between 50 and 150°C/km in Iceland would mean Trevor and company ride their lava tunnel water slide into an ocean around 600°C. For reference, that’s a touch warmer than the hot springs of Tuscany. On a side note: water boils at 100°C at the Earth’s surface, but at high pressures this reaches much higher—so the presence of liquid water is not the crazy part.

I guess they most have packed SPF 50,000, because they shrug off the blistering heat and continue on. But wait—shouldn’t they be under some serious pressure? And I don’t mean because they are on a perilous quest, but rather the immense pressures that exist at depth in the Earth. At the surface of the Earth, the pressure is 1 atm, or 101,325 Pa. At seven kilometres depth, a cavern that size would be under immense differential pressure. Lithostatic pressure of 2000 times the Earth’s surface would instantly crush the cavern and poor Trevor. Fortunately, they must have fallen into a cave with magical properties because it manages to withstand the weight of the Earth’s crust.

&nbsp;
<h3><strong>Suspicious rocks</strong></h3>
Before their great fall to their physically-assured deaths, our main characters find themselves in a lava tube. Now, lava tubes are a geological phenomenon that do in fact exist—we can see them in nature. However, lava tubes form during lava flows, and are therefore found near or at the surface. They can be very long, so the 7 km length of the lava tube in the film is not strange but its orientation very much is. They form from the flow of lava and thus form horizontally, not vertically!

We haven’t yet addressed the elephant in the room: the muscovite. Muscovite is not a rock, as the film portrays it, but rather a thin platy mineral found in igneous and metamorphic rocks. It is very weak, and even if you somehow constructed a thin floor made of muscovite (a geologically nonsensical idea), it would certainly not support the weight of a human. Fortunately for the characters, the muscovite in the film has a sense of dramatic timing, and only follows the laws of physics when it chooses to!

&nbsp;

<a href="https://blogs.egu.eu/divisions/gd/?attachment_id=42725" rel="attachment wp-att-42725"><img class="wp-image-42725 size-large aligncenter" src="https://blogs.egu.eu/divisions/gd/files/2026/04/Thurston_Lava_Tube_Big_Island-1024x685.jpg" alt="" width="1024" height="685" /></a>
<p style="text-align: center">Thurston Lava Tube at Hawaii Volcanoes National Park, Big Island, Hawaii. Author: Frank Schulenburg</p>
&nbsp;

At the end of the day, Journey to the Centre of the Earth may violate the laws of physics, contradict our understanding of geodynamics, and even show dinosaurs to be living inside the Earth, but it is a fun adventure, and worth a watch!]]></content:encoded>
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					<title><![CDATA[EGU General Assembly 2026 – A Hydrological Wrap Up]]></title>
					<link>https://blogs.egu.eu/divisions/hs/2026/06/05/egu-general-assembly-2026-a-hydrological-wrap-up/</link>
					<comments>https://blogs.egu.eu/divisions/hs/2026/06/05/egu-general-assembly-2026-a-hydrological-wrap-up/#comments</comments>
					<pubDate>Fri, 05 Jun 2026 09:10:00 +0000</pubDate>
					<dc:creator><![CDATA[Annegret Roessler]]></dc:creator>
							<category><![CDATA[Conference highlights]]></category>
		<category><![CDATA[EGU]]></category>
		<category><![CDATA[division president]]></category>
		<category><![CDATA[ECS]]></category>
		<category><![CDATA[EGU26]]></category>
		<category><![CDATA[General Assembly]]></category>
		<category><![CDATA[HS]]></category>
		<category><![CDATA[HS Division]]></category>
		<category><![CDATA[hydrology]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[The EGU General Assembly (GA) 2026 was an amazing success! Over the course of five sunny days in Vienna, 20,173 presentations were given across 1,014 sessions by the 20,027 on-site participants and 2,470 online attendees. There were plenty of events to choose from for the hydrologists attending. Across sessions, networking events, short courses, posters and medal lectures, we have put together some highlights for you to wrap up a fantastic GA 2026! HS Division highlights As every year, the Hydrological Sciences (HS) division was very active during the GA week hosting in total 120 scientific sessions and 2,911 abstracts. On Tuesday lunchtime (May 5th) in Room C, the Hydrological Sciences Division meeting (open to the entire community) was chaired by Division President Alberto Viglione. Attendees got updates about developments within the division over the past year, while we also got to celebrate some achievements from our division members. Christa Kelleher and Roger Moussa received the Hydrology and Earth System Sciences (HESS) Outstanding Editor Award for their excellent editorial work during 2025. Cyprien Louis, Landon Halloran and Clément Roques received the 2025 Jim Dooge award for their outstanding paper on Seasonal and diurnal freeze–thaw dynamics of a rock glacier and their impacts on mixing and solute transport In addition, we celebrated the recipients of the 2025 Outstanding Student and PhD candidate Presentation (OSPP) prizes. Ahmed El-Azhari, Anna Leuteritz, AntonKöhler, Fredrik Schück, Kansei Fujimoto, Malin Grosse-Heilmann, Malve Heinz, Palok Biswas, Peter Wagener and Sahar Jannesarahmadi were all recognised as very well-deserved recipients. Congratulations!! Medals and lectures On Tuesday afternoon, Wednesday afternoon and Thursday evening the recipients of this years medals from the HS division gave insightful presentations to the HS and GA community. This years awardees are: Sally Thompson who received the Henry Darcy medal Thorsten Wagener who was awarded the John Dalton Medal Larisa Tarasova who received the HS Division Outstanding Early Career Scientist Award Congratulations to you all!! Nominations for next years awards are open until June 15th, so please get your nominations in if you know of a researcher that deserves recognition for their exceptional contributions to hydrology. Early Career Scientists networking 2026 was the year of the Early Career Scientists (ECS) at the General Assembly! 62% of the abstracts at this years GA were contributed by ECS and it was fantastic to see so many in attendance at the different networking events and short courses throughout the week. At Monday lunchtime, the ECS team of the HS division, along with the International Association of Hydrological Sciences (IAHS) and Young Hydrological Society ran the increasingly-popular annual HydromMeet social gathering. With amazing weather, we were able to mingle and network in the sunshine and it was great to see so many new connections being made. Save the dates for the EGU General Assembly 2027! Let us know what you thought of this year’s General Assembly HERE. The EGU General Assembly 2026 will take place from 4 – 9th April 2027. Keep an eye out for key dates announced over summer and we cannot wait to see you all again next year! &nbsp;]]></description>
													<content:encoded><![CDATA[The EGU General Assembly (GA) 2026 was an amazing success! Over the course of five sunny days in Vienna, 20,173 presentations were given across 1,014 sessions by the 20,027 on-site participants and 2,470 online attendees. There were plenty of events to choose from for the hydrologists attending. Across sessions, networking events, short courses, posters and medal lectures, we have put together some highlights for you to wrap up a fantastic GA 2026!
<h2>HS Division highlights</h2>
As every year, the Hydrological Sciences (HS) division was very active during the GA week hosting in total 120 scientific sessions and 2,911 abstracts.

[caption id="attachment_13862" align="aligncenter" width="383"]<img class=" wp-image-13862" src="https://blogs.egu.eu/divisions/hs/files/2026/06/photo_2026-05-29-22.20.06-300x225.jpeg" alt="" width="383" height="287" /> Alberto Viglione, the Hydrological Sciences Division President, leading the Division’s annual meeting[/caption]

On Tuesday lunchtime (May 5th) in Room C, the Hydrological Sciences Division meeting (open to the entire community) was chaired by Division President <a title="https://blogs.egu.eu/divisions/hs/2024/08/01/meet-division-president-alberto-viglione/" href="https://blogs.egu.eu/divisions/hs/2024/08/01/meet-division-president-alberto-viglione/">Alberto Viglione</a>. Attendees got updates about developments within the division over the past year, while we also got to celebrate some achievements from our division members.

[caption id="attachment_13865" align="aligncenter" width="404"]<img class=" wp-image-13865" src="https://blogs.egu.eu/divisions/hs/files/2026/06/photo_2026-05-29-22.20.23-300x195.jpeg" alt="" width="404" height="263" /> Thom Bogaard (left) and Theresa Blume (centre) and Landon Halloran (right) at the Jim Dooge Award handover.[/caption]
<p 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">Christa Kelleher and Roger Moussa received the Hydrology and Earth System Sciences (HESS) Outstanding Editor Award for their excellent editorial work during 2025. Cyprien Louis, Landon Halloran and Clément Roques received the 2025 Jim Dooge award for their outstanding paper on <a href="https://hess.copernicus.org/articles/29/1505/2025/">Seasonal and diurnal freeze–thaw dynamics of a rock glacier and their impacts on mixing and solute transport</a></p>
In addition, we celebrated the recipients of the 2025 Outstanding Student and PhD candidate Presentation (OSPP) prizes. Ahmed El-Azhari, Anna Leuteritz, AntonKöhler, Fredrik Schück, Kansei Fujimoto, Malin Grosse-Heilmann, Malve Heinz, Palok Biswas, Peter Wagener and Sahar Jannesarahmadi were all recognised as very well-deserved recipients. Congratulations!!
<h2>Medals and lectures</h2>
[caption id="attachment_13899" align="alignnone" width="1024"]<img class="size-large wp-image-13899" src="https://blogs.egu.eu/divisions/hs/files/2026/06/EGU26_HS_awards_3-1024x404.jpg" alt="" width="1024" height="404" /> From left to right: Sally Thompson receives the Henry Darcy Medal remotely, Thorsten Wagener receives the John Dalton Meldal, and Larisa Tarasova receives HS Division Outstanding Early Career Scientist Award.[/caption]
<p 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">On Tuesday afternoon, Wednesday afternoon and Thursday evening the recipients of this years medals from the HS division gave insightful presentations to the HS and GA community. This years awardees are:</p>

<ul>
 	<li><a title="https://www.egu.eu/awards-medals/henry-darcy/2025/jan-seibert/" href="https://www.egu.eu/awards-medals/henry-darcy/2026/sally-e-thompson/">Sally Thompson</a> who received the Henry Darcy medal</li>
 	<li><a title="" href="https://www.egu.eu/awards-medals/john-dalton/2026/thorsten-wagener/">Thorsten Wagener</a> who was awarded the John Dalton Medal</li>
 	<li><a href="https://www.egu.eu/awards-medals/division-outstanding-ecs-award/2026/larisa-tarasova/">Larisa Tarasova</a> who received the HS Division Outstanding Early Career Scientist Award</li>
</ul>
Congratulations to you all!! <a title="https://www.egu.eu/awards-medals/proposal-and-selection-of-candidates/" href="https://www.egu.eu/awards-medals/nominations/">Nominations for next years awards</a> are open until June 15th, so please get your nominations in if you know of a researcher that deserves recognition for their exceptional contributions to hydrology.
<h2><b>E</b><b>arly </b><b>C</b><b>areer </b><b>S</b><b>cientists</b><b> networking</b></h2>
2026 was the year of the Early Career Scientists (ECS) at the General Assembly! 62% of the abstracts at this years GA were contributed by ECS and it was fantastic to see so many in attendance at the different networking events and short courses throughout the week.

[caption id="attachment_13869" align="aligncenter" width="420"]<img class=" wp-image-13869" src="https://blogs.egu.eu/divisions/hs/files/2026/06/EGU26_Hydromeet-300x160.jpg" alt="" width="420" height="224" /> Attendees of the 2026 Hydromeet[/caption]
<p 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AAFrAAAABAYSAAAATwBwAGUAbgAgAFMAYQBuAHMABQYSAAAATwBwAGUAbgAgAFMAYQBuAHMABwYSAAAATwBwAGUAbgAgAFMAYQBuAHMABgYSAAAATwBwAGUAbgAgAFMAYQBuAHMACAQUAAAACQMzMzMIWQAAAABUAAAAoAByAGEAbgAgAHQAaABlACAAaQBuAGMAcgBlAGEAcwBpAG4AZwBsAHkALQBwAG8AcAB1AGwAYQByACAAYQBuAG4AdQBhAGwAIABIAHkAZAByAG8ADBIBAAACBAAAAAEAAAAAJgAAAEkAbABpAGEAcwAgAFAAZQBjAGgAbABpAHYAYQBuAGkAZABpAHMAASgAAAAyADAAMgA2AC0AMAA1AC0AMwAxAFQAMQA1ADoAMwA0ADoANQA5AFoAAyYAAABvAGMAbQAzAG4AZQA3AGIAbAB5ADIAZABfADIANAA2ADkAMQA5AASBAAAABXwAAAABawAAAAQGEgAAAE8AcABlAG4AIABTAGEAbgBzAAUGEgAAAE8AcABlAG4AIABTAGEAbgBzAAcGEgAAAE8AcABlAG4AIABTAGEAbgBzAAYGEgAAAE8AcABlAG4AIABTAGEAbgBzAAgEFAAAAAkDMzMzCAcAAAAPAgAAAG0ADRIBAAACBAAAAAIAAAAAJgAAAEkAbABpAGEAcwAgAFAAZQBjAGgAbABpAHYAYQBuAGkAZABpAHMAASgAAAAyADAAMgA2AC0AMAA1AC0AMwAxAFQAMQA1ADoAMwA0ADoANQA5AFoAAyYAAABvAGMAbQAzAG4AZQA3AGIAbAB5ADIAZABfADIANAA2ADkAMQA5AASBAAAABXwAAAABawAAAAQGEgAAAE8AcABlAG4AIABTAGEAbgBzAAUGEgAAAE8AcABlAG4AIABTAGEAbgBzAAcGEgAAAE8AcABlAG4AIABTAGEAbgBzAAYGEgAAAE8AcABlAG4AIABTAGEAbgBzAAgEFAAAAAkDMzMzCAcAAAAAAgAAAE0ABYAAAAABawAAAAQGEgAAAE8AcABlAG4AIABTAGEAbgBzAAUGEgAAAE8AcABlAG4AIABTAGEAbgBzAAcGEgAAAE8AcABlAG4AIABTAGEAbgBzAAYGEgAAAE8AcABlAG4AIABTAGEAbgBzAAgEFAAAAAkDMzMzCAsAAAAABgAAAGUAZQB0AA0yAQAAAgQAAAADAAAAACYAAABJAGwAaQBhAHMAIABQAGUAYwBoAGwAaQB2AGEAbgBpAGQAaQBzAAEoAAAAMgAwADIANgAtADAANQAtADMAMQBUADEANQA6ADMANQA6ADAANQBaAAMmAAAAbwBjAG0AMwBuAGUANwBiAGwAeQAyAGQAXwAyADQANgA5ADEAOQAEoQAAAAWcAAAAAWsAAAAEBhIAAABPAHAAZQBuACAAUwBhAG4AcwAFBhIAAABPAHAAZQBuACAAUwBhAG4AcwAHBhIAAABPAHAAZQBuACAAUwBhAG4AcwAGBhIAAABPAHAAZQBuACAAUwBhAG4AcwAIBBQAAAAJAzMzMwgnAAAAACIAAAAgAHMAbwBjAGkAYQBsACAAZwBhAHQAaABlAHIAaQBuAGcABYYBAAABawAAAAQGEgAAAE8AcABlAG4AIABTAGEAbgBzAAUGEgAAAE8AcABlAG4AIABTAGEAbgBzAAcGEgAAAE8AcABlAG4AIABTAGEAbgBzAAYGEgAAAE8AcABlAG4AIABTAGEAbgBzAAgEFAAAAAkDMzMzCBEBAAAADAEAAC4AIABXAGkAdABoACAAYQBtAGEAegBpAG4AZwAgAHcAZQBhAHQAaABlAHIALAAgAHcAZQAgAHcAZQByAGUAIABhAGIAbABlACAAdABvACAAbQBpAG4AZwBsAGUAIABhAG4AZAAgAG4AZQB0AHcAbwByAGsAIABpAG4AIAB0AGgAZQAgAHMAdQBuAHMAaABpAG4AZQAgAGEAbgBkACAAaQB0ACAAdwBhAHMAIABnAHIAZQBhAHQAIAB0AG8AIABzAGUAZQAgAHMAbwAgAG0AYQBuAHkAIABuAGUAdwAgAGMAbwBuAG4AZQBjAHQAaQBvAG4AcwAgAGIAZQBpAG4AZwAgAG0AYQBkAGUALgAFCgAAAAEAAAAACAAAAAAFCgAAAAEAAAAACAAAAAAA+AQAAAHHAAAAFQYGAAAAOAAzADkAAQYSAAAAJAQAAAAAJQQAAAAAJgQAAAAACQYVAAAAJwQsAQAACwEAKAThAAAAKQThAAAAGgYAAAAAGwZ8AAAAABoAAAAAAwAAAAUEAAAAAAYEBAAAAAMB/wcE/////wEaAAAAAAMAAAAFBAAAAAAGBAQAAAADAf8HBP////8CGgAAAAADAAAABQQAAAAABgQEAAAAAwH/BwT/////AxoAAAAAAwAAAAUEAAAAAAYEBAAAAAMB/wcE/////wInBAAABbIAAAABawAAAAQGEgAAAE8AcABlAG4AIABTAGEAbgBzAAUGEgAAAE8AcABlAG4AIABTAGEAbgBzAAcGEgAAAE8AcABlAG4AIABTAGEAbgBzAAYGEgAAAE8AcABlAG4AIABTAGEAbgBzAAgEGAAAAAkDMzMzCD0AAAAAOAAAAFMAYQB2AGUAIAB0AGgAZQAgAGQAYQB0AGUAcwAgAGYAbwByACAAdABoAGUAIABFAEcAVQAgAEcADR4BAAACBAAAAAQAAAAAJgAAAEkAbABpAGEAcwAgAFAAZQBjAGgAbABpAHYAYQBuAGkAZABpAHMAASgAAAAyADAAMgA2AC0AMAA1AC0AMwAxAFQAMQA1ADoAMwA2ADoAMgA0AFoAAyYAAABvAGMAbQAzAG4AZQA3AGIAbAB5ADIAZABfADIANAA2ADkAMQA5AASNAAAABYgAAAABawAAAAQGEgAAAE8AcABlAG4AIABTAGEAbgBzAAUGEgAAAE8AcABlAG4AIABTAGEAbgBzAAcGEgAAAE8AcABlAG4AIABTAGEAbgBzAAYGEgAAAE8AcABlAG4AIABTAGEAbgBzAAgEGAAAAAkDMzMzCBMAAAAADgAAAGUAbgBlAHIAYQBsACAABXwAAAABawAAAAQGEgAAAE8AcABlAG4AIABTAGEAbgBzAAUGEgAAAE8AcABlAG4AIABTAGEAbgBzAAcGEgAAAE8AcABlAG4AIABTAGEAbgBzAAYGEgAAAE8AcABlAG4AIABTAGEAbgBzAAgEGAAAAAkDMzMzCAcAAAAAAgAAAEEADR4BAAACBAAAAAUAAAAAJgAAAEkAbABpAGEAcwAgAFAAZQBjAGgAbABpAHYAYQBuAGkAZABpAHMAASgAAAAyADAAMgA2AC0AMAA1AC0AMwAxAFQAMQA1ADoAMwA2ADoAMgA2AFoAAyYAAABvAGMAbQAzAG4AZQA3AGIAbAB5ADIAZABfADIANAA2ADkAMQA5AASNAAAABYgAAAABawAAAAQGEgAAAE8AcABlAG4AIABTAGEAbgBzAAUGEgAAAE8AcABlAG4AIABTAGEAbgBzAAcGEgAAAE8AcABlAG4AIABTAGEAbgBzAAYGEgAAAE8AcABlAG4AIABTAGEAbgBzAAgEGAAAAAkDMzMzCBMAAAAADgAAAHMAcwBlAG0AYgBsAHkABYYAAAABawAAAAQGEgAAAE8AcABlAG4AIABTAGEAbgBzAAUGEgAAAE8AcABlAG4AIABTAGEAbgBzAAcGEgAAAE8AcABlAG4AIABTAGEAbgBzAAYGEgAAAE8AcABlAG4AIABTAGEAbgBzAAgEGAAAAAkDMzMzCBEAAAAADAAAACAAMgAwADIANwAhAAUKAAAAAQAAAAAIAAAAAAUKAAAAAQAAAAAIAAAAAABeCQAAAbIAAAABBhIAAAAkBAAAAAAlBAAAAAAmBAAAAAAJBgwAAAAoBAAAAAApBLQAAAAaBgAAAAAbBnwAAAAAGgAAAAADAAAABQQAAAAABgQEAAAAAwH/BwT/////ARoAAAAAAwAAAAUEAAAAAAYEBAAAAAMB/wcE/////wIaAAAAAAMAAAAFBAAAAAAGBAQAAAADAf8HBP////8DGgAAAAADAAAABQQAAAAABgQEAAAAAwH/BwT/////AqIIAAAF9AAAAAFrAAAABAYSAAAATwBwAGUAbgAgAFMAYQBuAHMABQYSAAAATwBwAGUAbgAgAFMAYQBuAHMABwYSAAAATwBwAGUAbgAgAFMAYQBuAHMABgYSAAAATwBwAGUAbgAgAFMAYQBuAHMACAQUAAAACQMzMzMIfwAAAAB6AAAATABlAHQAIAB1AHMAIABrAG4AbwB3ACAAdwBoAGEAdAAgAHkAbwB1ACAAdABoAG8AdQBnAGgAdAAgAG8AZgAgAHQAaABpAHMAIAB5AGUAYQByABkgcwAgAEcAZQBuAGUAcgBhAGwAIABBAHMAcwBlAG0AYgBsAHkAoAAK+AIAAAFMAAAAaAB0AHQAcABzADoALwAvAHMAdQByAHYAZQB5AC4AegBvAGgAbwBwAHUAYgBsAGkAYwAuAGUAdQAvAHoAcwAvAFIATQB4AFkAUgBoAANMAAAAaAB0AHQAcABzADoALwAvAHMAdQByAHYAZQB5AC4AegBvAGgAbwBwAHUAYgBsAGkAYwAuAGUAdQAvAHoAcwAvAFIATQB4AFkAUgBoAAQBAAAAAQBLAgAADScBAAACBAAAAAYAAAAAJgAAAEkAbABpAGEAcwAgAFAAZQBjAGgAbABpAHYAYQBuAGkAZABpAHMAASgAAAAyADAAMgA2AC0AMAA1AC0AMwAxAFQAMQA1ADoAMwA2ADoAMQAzAFoAAyYAAABvAGMAbQAzAG4AZQA3AGIAbAB5ADIAZABfADIANAA2ADkAMQA5AASWAAAABZEAAAABegAAAAIBCwQGEgAAAE8AcABlAG4AIABTAGEAbgBzAAUGEgAAAE8AcABlAG4AIABTAGEAbgBzAAcGEgAAAE8AcABlAG4AIABTAGEAbgBzAAYGEgAAAE8AcABlAG4AIABTAGEAbgBzAAgEFAAAAAkDAHK8DQYGAAAAOAA4ADAACA0AAAAACAAAAEgARQBSAEUADBoBAAACBAAAAAcAAAAAJgAAAEkAbABpAGEAcwAgAFAAZQBjAGgAbABpAHYAYQBuAGkAZABpAHMAASgAAAAyADAAMgA2AC0AMAA1AC0AMwAxAFQAMQA1ADoAMwA2ADoAMQA2AFoAAyYAAABvAGMAbQAzAG4AZQA3AGIAbAB5ADIAZABfADIANAA2ADkAMQA5AASJAAAABYQAAAABegAAAAIBCwQGEgAAAE8AcABlAG4AIABTAGEAbgBzAAUGEgAAAE8AcABlAG4AIABTAGEAbgBzAAcGEgAAAE8AcABlAG4AIABTAGEAbgBzAAYGEgAAAE8AcABlAG4AIABTAGEAbgBzAAgEFAAAAAkDAHK8DQYGAAAAOAA4ADAACAAAAAAFhgEAAAFrAAAABAYSAAAATwBwAGUAbgAgAFMAYQBuAHMABQYSAAAATwBwAGUAbgAgAFMAYQBuAHMABwYSAAAATwBwAGUAbgAgAFMAYQBuAHMABgYSAAAATwBwAGUAbgAgAFMAYQBuAHMACAQUAAAACQMzMzMIEQEAAAAMAQAALgAgAFQAaABlACAARQBHAFUAIABHAGUAbgBlAHIAYQBsACAAQQBzAHMAZQBtAGIAbAB5ACAAMgAwADIANgAgAHcAaQBsAGwAIAB0AGEAawBlACAAcABsAGEAYwBlACAAZgByAG8AbQAgADQAIAATICAAOQB0AGgAIABBAHAAcgBpAGwAIAAyADAAMgA3AC4AIABLAGUAZQBwACAAYQBuACAAZQB5AGUAIABvAHUAdAAgAGYAbwByACAAawBlAHkAIABkAGEAdABlAHMAIABhAG4AbgBvAHUAbgBjAGUAZAAgAG8AdgBlAHIAIABzAHUAbQBtAGUAcgAgAGEAbgBkACAAdwBlACAAYwBhAA0YAQAAAgQAAAAIAAAAACYAAABJAGwAaQBhAHMAIABQAGUAYwBoAGwAaQB2AGEAbgBpAGQAaQBzAAEoAAAAMgAwADIANgAtADAANQAtADMAMQBUADEANQA6ADMANQA6ADUAOQBaAAMmAAAAbwBjAG0AMwBuAGUANwBiAGwAeQAyAGQAXwAyADQANgA5ADEAOQAEhwAAAAWCAAAAAWsAAAAEBhIAAABPAHAAZQBuACAAUwBhAG4AcwAFBhIAAABPAHAAZQBuACAAUwBhAG4AcwAHBhIAAABPAHAAZQBuACAAUwBhAG4AcwAGBhIAAABPAHAAZQBuACAAUwBhAG4AcwAIBBQAAAAJAzMzMwgNAAAAAAgAAABuAG4AbwB0AAwWAQAAAgQAAAAJAAAAACYAAABJAGwAaQBhAHMAIABQAGUAYwBoAGwAaQB2AGEAbgBpAGQAaQBzAAEoAAAAMgAwADIANgAtADAANQAtADMAMQBUADEANQA6ADMANgA6ADAAMABaAAMmAAAAbwBjAG0AMwBuAGUANwBiAGwAeQAyAGQAXwAyADQANgA5ADEAOQAEhQAAAAWAAAAAAWsAAAAEBhIAAABPAHAAZQBuACAAUwBhAG4AcwAFBhIAAABPAHAAZQBuACAAUwBhAG4AcwAHBhIAAABPAHAAZQBuACAAUwBhAG4AcwAGBhIAAABPAHAAZQBuACAAUwBhAG4AcwAIBBQAAAAJAzMzMwgLAAAADwYAAABuABkgdAAFxgAAAAFrAAAABAYSAAAATwBwAGUAbgAgAFMAYQBuAHMABQYSAAAATwBwAGUAbgAgAFMAYQBuAHMABwYSAAAATwBwAGUAbgAgAFMAYQBuAHMABgYSAAAATwBwAGUAbgAgAFMAYQBuAHMACAQUAAAACQMzMzMIUQAAAABMAAAAIAB3AGEAaQB0ACAAdABvACAAcwBlAGUAIAB5AG8AdQAgAGEAbABsACAAYQBnAGEAaQBuACAAbgBlAHgAdAAgAHkAZQBhAHIAIQAhAAUKAAAAAQAAAAAIAAAAAAUKAAAAAQAAAAAIAAAAAAoAAAAAAAAAABEAAAAANAMAAAAtAAAAAQYAAAAACQYbAAAAJwQUAQAACwEBHAEAKAQAAAAAHQEAKQTIAAAAGwYAAAAAAUsAAAAoAQcpAQcqAQcrAQUTAQEIBBYAAAAWBBYAAAAZBgoAAABlAG4ALQBHAEIAGgYKAAAAYQByAC0AUwBBABsGCgAAAGUAbgAtAFUAUwACrQIAAAA0AgAAAQYAAAA4ADMAOQACEgAAAEgAZQBhAGQAaQBuAGcAIAA1AAkBAAAAAwMGAAAAOAA5ADQABAYAAAA4ADkANAASBgAAADgANAA5AAoBAAAAAQsEAAAACQAAAA4BAAAAAQXGAAAAAAEAAQEAAgELAwEABAYKAAAAQQByAGkAYQBsAAUGCgAAAEEAcgBpAGEAbAAHBgoAAABBAHIAaQBhAGwABgYKAAAAQQByAGkAYQBsAAgEFgAAAAkDD0dhCgEADAEAJgQAAAAADwEAEAEAEQEAJwQAAAAAFAEAFQEAFgQWAAAAFwEAGAEAGQYKAAAAZQBuAC0ARwBCABoGCgAAAGEAcgAtAFMAQQAbBgoAAABlAG4ALQBVAFMAHAYGAAAAAQEAAwG/HgEALgEABgYBAAAAAQABBhIAAAAkBAAAAAAlBAAAAAAmBAAAAAAFAQEGAQEHAQEIAQAJBhsAAAAnBBQBAAALAQEcAQAoBFAAAAAdAQApBCgAAAAOBggAAAAAAQEBA////xkBARsGmwAAAAAaAAAAAAMAAAAFBAAAAAAGBAQAAAADAf8HBP////8BGgAAAAADAAAABQQAAAAABgQEAAAAAwH/BwT/////AhoAAAAAAwAAAAUEAAAAAAYEBAAAAAMB/wcE/////wMaAAAAAAMAAAAFBAAAAAAGBAQAAAADAf8HBP////8LGgAAAAADAAAABQQAAAAABgQEAAAAAwH/BwT/////IgQEAAAALAEALwEAAG8AAAABBgAAADgAOAAwAAISAAAASAB5AHAAZQByAGwAaQBuAGsACQEAAAABAwYAAAA4ADQANAALBAAAAGMAAAAOAQAAAAEFEQAAAAIBDAkDBWPBHAYDAAAAAQELBhIAAAABBgAAAAAJBgAAAAAbBgAAAAA=">At Monday lunchtime, the ECS team of the HS division, along with the <a title="https://iahs.info/" href="https://iahs.info/">International Association of Hydrological Sciences</a> (IAHS) and <a title="https://younghs.com/" href="https://younghs.com/">Young Hydrological Society</a> ran the increasingly-popular annual HydromMeet social gathering. With amazing weather, we were able to mingle and network in the sunshine and it was great to see so many new connections being made.</p>

<h5>Save the dates for the EGU General Assembly 2027!</h5>
Let us know what you thought of this year’s General Assembly <a title="https://survey.zohopublic.eu/zs/RMxYRh" href="https://survey.zohopublic.eu/zs/RMxYRh">HERE</a>. The EGU General Assembly 2026 will take place from 4 – 9th April 2027. Keep an eye out for key dates announced over summer and we cannot wait to see you all again next year!

&nbsp;]]></content:encoded>
																<wfw:commentRss>https://blogs.egu.eu/divisions/hs/2026/06/05/egu-general-assembly-2026-a-hydrological-wrap-up/feed/</wfw:commentRss>
					<slash:comments>0</slash:comments>
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							<item>
					<title><![CDATA[Melting Glaciers Move Lithospheric Plates and Fluctuate Mid-ocean Ridges’ Spreading]]></title>
					<link>https://blogs.egu.eu/divisions/gd/2026/06/03/melting-glaciers-move-lithospheric-plates-and-fluctuate-mid-ocean-ridges-spreading/</link>
					<comments>https://blogs.egu.eu/divisions/gd/2026/06/03/melting-glaciers-move-lithospheric-plates-and-fluctuate-mid-ocean-ridges-spreading/#comments</comments>
					<pubDate>Wed, 03 Jun 2026 08:00:05 +0000</pubDate>
					<dc:creator><![CDATA[Editorial team 1]]></dc:creator>
							<category><![CDATA[News & Views]]></category>
		<category><![CDATA[Uncategorised]]></category>
		<category><![CDATA[GIA]]></category>
		<category><![CDATA[Glacial Isostatic Adjustment]]></category>
		<category><![CDATA[Mantle Viscosity]]></category>
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											<description><![CDATA[The rise and fall of massive ice sheets have shaped Earth’s surface for millions of years, but their influence may extend far deeper than previously recognized. This week in News &amp; Views, Tao Yuan, a PhD student at the University of Colorado Boulder, explores how glacial cycles can alter lithospheric plate motions and even modulate the spreading of mid-ocean ridges. The ongoing melting of glaciers, including the Greenland and Antarctic ice sheets, is expected to raise global sea levels by meters over the next century, posing a critical threat to humanity. Although the current rapid melting of glaciers is largely a result of human activities, Earth has experienced fiercer advances and retreats of glaciers and ice sheets during glacial cycles over the last few million years. The waxing and waning of large ice sheets have a wide influence on Earth&#8217;s surface processes, perhaps more than we thought. For example, have you ever thought that melting glaciers can affect lithospheric plate motions and the spreading of mid-ocean ridges? How do ice sheets deform Earth during glacial cycles? Before getting to the effects of melting glaciers on plate motion and mid-ocean ridge spreading, let’s first understand how Earth is deformed by glacial loadings during glacial cycles. Quaternary glacial cycles are the repeated advances and retreats of ice sheets primarily driven by cyclic variations in Earth’s orbit and tilt (Milankovitch cycles). The last glacial cycle, starting from ~120 thousand years ago, reached its maximum at about 26 thousand years ago (the last glacial maximum), when much of North America and Fennoscandia was covered by ice sheets of over 3 km thick ice (Fig. 1). Since those continental ice sheets stayed for tens of thousands of years and the mantle deforms like a viscous fluid over long-term timescales, the surface of Earth was depressed by hundreds of meters under the weight of those ice sheets. When ice sheets melt away, Earth’s surface rebounds (Fig. 2). This process is called Glacial Isostatic Adjustment (GIA). Understanding the GIA process is important for various reasons. First, GIA, driven by the last deglaciation, is still deforming the Earth (Fig. 2). The land is rebounding in the former deglaciation center and subsiding in the peripheral regions, causing sea level changes. It also drives gravity changes as seen by GRACE satellites and needs to be removed from observed gravity signals in order to estimate surface mass changes. Currently, GIA is a big source of uncertainty in estimating the recent ice loss in Antarctica (Willen et al., 2025). Secondly, GIA can be used to infer both the history of ice sheets (i.e., how ice sheets evolved in glacial cycles) and mantle rheology (i.e., viscosity), thus having implications on both long-term climatic and mantle dynamic processes. In fact, GIA provides the first robust inference of mantle viscosity (Haskell, 1935), providing important support for the idea of mantle convection during the establishment of plate tectonics theory. So, how do we study GIA? The GIA process is recorded in various kinds of observations, including paleo-sea-level changes, current land rebound (Fig. 2), and time-varying gravity, etc. Those observations can be used to constrain GIA models, including both ice-sheet history and mantle rheology. There have been widely used GIA models, although most of them are based on simplified models, including an Earth rheology structure with only radial variations (Peltier et al., 2015). We are continuing to improve GIA models by using stronger data constraints and more realistic model parameterizations, and by exploring model uncertainty (Yuan et al. 2026). GIA on lithospheric plate motions and mid-ocean ridge spreading: The aforementioned GIA studies are primarily based on GIA-induced vertical motions (sea level, gravity, etc.). How about horizontal motion? GIA’s effects on horizontal motion are not negligible. When ice sheets grow, the surface bends to subside, the mantle moves away from the ice sheet centers – both processes cause horizontal motions on the surface (Fig. 2). GIA is still causing crustal horizontal motions in both Canada and Northern Europe as observed by GPS (Milne et al., 2001). So, how significant is the GIA-induced horizontal motion during glacial cycles? Could it be strong enough to compete with the long-term plate motion driven by mantle convection? If you compare the GIA-induced crustal horizontal motion recorded by GPS in Canada (Kreemer et al., 2018) to the current plate motion rate, you might say no – the latter is at least one order larger than the former. However, this comparison is only for the present day, and it is almost certain that the GIA-induced horizontal motion during the last glacial cycle was much more significant than it is now, given periods with much more rapid ice growth and melt. Could the glaciation/deglaciation affect the long-term tectonic plate motion? If so, plate motions in glacial cycles (tens of thousands of years timescale) would not be as stable as many thought. This question has not been explored previously and could have broad implications on tectonic processes during glacial cycles, including plate motion, mid-ocean ridge spreading, and mantle degassing rate. Unlike vertical motions recorded by paleo-sea level indicators, it is difficult to find direct observational evidence of GIA-induced horizontal motion throughout glacial cycles. So, to answer that question, we rely on numerical modeling. GIA modeling depends on input models of ice history and Earth’s rheology. Luckily, we have a basic understanding of ice history from sea-level and geomorphological records (Peltier et al., 2015) and some understanding of Earth’s rheology. Lithospheric plates have strong (i.e., less deformable) plate interiors and weak (i.e., less viscous, more deformable) plate boundaries, and mantle viscosity is on the order of 1021 Pa s (with a possibly less viscous asthenosphere beneath the lithosphere). By choosing model inputs as realistic as possible, we perform numerical calculations to simulate GIA-induced horizontal motion during the last glacial cycle. Our GIA models show strong influences of glacial forcing (loading and unloading) on lithospheric motion (i.e., motion on Earth’s surface). GIA causes plate-scale rotations in the North American plate, with a counterclockwise pattern during glaciation (Fig. 3a) and a clockwise pattern during deglaciation. The magnitude of the plate-scale rotation induced by GIA could reach ~25% of the current geologic plate motion rate for the North American plate. Note that the North American plate is where GIA has the greatest impact, since it hosted the largest ice sheet during the last glacial cycle. With the existence of weak plate margins (e.g., at mid-ocean ridges) that decouple strong lithospheric plates, GIA causes differential horizontal motion across mid-ocean ridges (Fig 3), affecting the spreading rate of mid-ocean ridges, especially for the North Atlantic mid-ocean ridge near the former Laurentide ice sheet. Similar effects of GIA on mid-ocean ridge spreading are also observed in our models around Antarctica (Fig. 3b). One particularly interesting area is the Iceland mid-ocean ridge, which is so close to the Greenland ice sheet. Models show that deglaciation in Greenland caused up to 40% fluctuations in the spreading rate of the Iceland Ridge between 12,000 and 6,000 years ago, which may explain Holocene volcanism in Iceland (Yuan and Zhong, 2025). The Greenland ice sheet is currently experiencing rapid melting. Could it soon affect Iceland Ridge&#8217;s spreading rate and magma production rate? It is an important question to investigate. These results, shown in Fig. 3 and in our paper (Yuan and Zhong, 2025), reveal an interesting dynamic interplay between glacial cycles, lithospheric motion, ridge spreading, and climate during ice ages. It is well known that tectonic processes strongly affect climate; for example, they may be responsible for the global cooling in the Cenozoic (Raymo and Ruddiman, 1992). However, it is less well known that climatic forcing can also leave a fingerprint on tectonic processes, including large-scale plate tectonics. In addition to what we showed in Fig. 3, it has also been discussed whether global sea-level fluctuations during glacial cycles could trigger observable crustal topography and/or thickness variations in the seafloor (Crowley et al., 2015; Olive et al., 2015). We hope our findings from numerical modeling can inspire greater interest in this topic and more efforts to detect subtle signals in observations to better quantify the impacts of climatic forcing on tectonics. References: Yuan, Tao, and Shijie Zhong. 2025. “Effects of Glacial Forcing on Lithospheric Motion and Ridge Spreading.” Nature, April 23, 1–7. https://doi.org/10.1038/s41586-025-08846-x. Yuan, Tao, Shijie Zhong, Glenn Milne, and Donna dePolo. 2026. “Reconciling Inferences of Mantle Viscosity and Late Quaternary Ice - the Importance of an Asthenosphere and 3-D Viscosity.” ESS Open Archive 2026 (0417). https://doi.org/10.22541/essoar.15001943/v2. Crowley, John W., Richard F. Katz, Peter Huybers, Charles H. Langmuir, and Sung-Hyun Park. 2015. “Glacial Cycles Drive Variations in the Production of Oceanic Crust.” Science 347 (6227): 1237–40. https://doi.org/10.1126/science.1261508. Haskell, N. A. 1935. “The Motion of a Viscous Fluid Under a Surface Load.” Physics 6 (8): 265–69. https://doi.org/10.1063/1.1745329. Kreemer, Corné, William C. Hammond, and Geoffrey Blewitt. 2018. “A Robust Estimation of the 3‐D Intraplate Deformation of the North American Plate From GPS.” Journal of Geophysical Research: Solid Earth 123 (5): 4388–412. https://doi.org/10.1029/2017JB015257. Milne, G. A., J. L. Davis, Jerry X. Mitrovica, et al. 2001. “Space-Geodetic Constraints on Glacial Isostatic Adjustment in Fennoscandia.” Science 291 (5512): 2381–85. https://doi.org/10.1126/science.1057022. Olive, J. A., M. D. Behn, G. Ito, W. R. Buck, J. Escartín, and S. Howell. 2015. “Sensitivity of Seafloor Bathymetry to Climate-Driven Fluctuations in Mid-Ocean Ridge Magma Supply.” Science 350 (6258): 310–13. https://doi.org/10.1126/science.aad0715. Peltier, W. R., D. F. Argus, and R. Drummond. 2015. “Space Geodesy Constrains Ice Age Terminal Deglaciation: The Global ICE-6G_C (VM5a) Model: Global Glacial Isostatic Adjustment.” Journal of Geophysical Research: Solid Earth 120 (1): 450–87. https://doi.org/10.1002/2014JB011176. Raymo, M. E., and W. F. Ruddiman. 1992. “Tectonic Forcing of Late Cenozoic Climate.” Nature 359 (6391): 117–22. https://doi.org/10.1038/359117a0. Willen, Matthias O., Bert Wouters, Taco Broerse, Eric Buchta, and Veit Helm. 2025. “Satellite Data Reveal Details of Glacial Isostatic Adjustment in the Amundsen Sea Embayment, West Antarctica.” The Cryosphere 19 (6): 2213–27. https://doi.org/10.5194/tc-19-2213-2025. UNAVCO, 2026, GPS Spotlight: Station CHUR: https://spotlight.unavco.org/station-pages/chur/chur.html (accessed May 2026).]]></description>
													<content:encoded><![CDATA[<strong>The rise and fall of massive ice sheets have shaped Earth’s surface for millions of years, but their influence may extend far deeper than previously recognized. This week in News &amp; Views, <a href="https://scholar.google.com/citations?user=UBjRYmwAAAAJ&amp;hl=en">Tao Yuan</a>, a PhD student at the University of Colorado Boulder, explores how glacial cycles can alter lithospheric plate motions and even modulate the spreading of mid-ocean ridges.</strong>

[caption id="attachment_42890" align="alignleft" width="300"]<img class="wp-image-42890 size-medium" src="https://blogs.egu.eu/divisions/gd/files/2026/06/photo_selfie_zoomin-300x270.jpg" alt="" width="300" height="270" /> Tao Yuan, from the Department of Physics, CU Boulder[/caption]

The ongoing melting of glaciers, including the Greenland and Antarctic ice sheets, is expected to raise global sea levels by meters over the next century, posing a critical threat to humanity. Although the current rapid melting of glaciers is largely a result of human activities, Earth has experienced fiercer advances and retreats of glaciers and ice sheets during glacial cycles over the last few million years. The waxing and waning of large ice sheets have a wide influence on Earth's surface processes, perhaps more than we thought. For example, have you ever thought that melting glaciers can affect lithospheric plate motions and the spreading of mid-ocean ridges?

<strong>How do ice sheets deform Earth during glacial cycles?</strong>

Before getting to the effects of melting glaciers on plate motion and mid-ocean ridge spreading, let’s first understand how Earth is deformed by glacial loadings during glacial cycles. Quaternary glacial cycles are the repeated advances and retreats of ice sheets primarily driven by cyclic variations in Earth’s orbit and tilt (Milankovitch cycles). The last glacial cycle, starting from ~120 thousand years ago, reached its maximum at about 26 thousand years ago (the last glacial maximum), when much of North America and Fennoscandia was covered by ice sheets of over 3 km thick ice (Fig. 1). Since those continental ice sheets stayed for tens of thousands of years and the mantle deforms like a viscous fluid over long-term timescales, the surface of Earth was depressed by hundreds of meters under the weight of those ice sheets. When ice sheets melt away, Earth’s surface rebounds (Fig. 2). This process is called Glacial Isostatic Adjustment (GIA).

[caption id="attachment_42903" align="alignright" width="1398"]<a href="https://blogs.egu.eu/divisions/gd/?attachment_id=42903" rel="attachment wp-att-42903"><img class="wp-image-42903 size-full" src="https://blogs.egu.eu/divisions/gd/files/2026/06/Screenshot-2026-06-02-at-5.46.36-PM.png" alt="" width="1398" height="758" /></a> Fig 1. Extent of continental ice sheets at the last glacial maximum (left) and at the present day (right). White represents ice sheets. From When Were the Ices Ages and Why Are They Called That? - Mammoth Discovery.[/caption]

Understanding the GIA process is important for various reasons. First, GIA, driven by the last deglaciation, is still deforming the Earth (Fig. 2). The land is rebounding in the former deglaciation center and subsiding in the peripheral regions, causing sea level changes. It also drives gravity changes as seen by GRACE satellites and needs to be removed from observed gravity signals in order to estimate surface mass changes. Currently, GIA is a big source of uncertainty in estimating the recent ice loss in Antarctica (Willen et al., 2025). Secondly, GIA can be used to infer both the history of ice sheets (i.e., how ice sheets evolved in glacial cycles) and mantle rheology (i.e., viscosity), thus having implications on both long-term climatic and mantle dynamic processes. In fact, GIA provides the first robust inference of mantle viscosity (Haskell, 1935), providing important support for the idea of mantle convection during the establishment of plate tectonics theory.

[caption id="attachment_42907" align="alignleft" width="271"]<a href="https://blogs.egu.eu/divisions/gd/?attachment_id=42907" rel="attachment wp-att-42907"><img class="wp-image-42907 size-medium" src="https://blogs.egu.eu/divisions/gd/files/2026/06/fig2_GIA_image-271x300.jpg" alt="" width="271" height="300" /></a> Fig 2. Illustration of glacial isostatic adjustment. The top panel depicts the glaciation stage in which ice loads cause depression. The lower panel shows the glaciation stage when the crust rebounds after ice melts (Source: UNAVCO 2026).[/caption]

So, how do we study GIA? The GIA process is recorded in various kinds of observations, including paleo-sea-level changes, current land rebound (Fig. 2), and time-varying gravity, etc. Those observations can be used to constrain GIA models, including both ice-sheet history and mantle rheology. There have been widely used GIA models, although most of them are based on simplified models, including an Earth rheology structure with only radial variations (Peltier et al., 2015). We are continuing to improve GIA models by using stronger data constraints and more realistic model parameterizations, and by exploring model uncertainty (Yuan et al. 2026).

<strong>GIA on lithospheric plate motions and mid-ocean ridge spreading:</strong>

The aforementioned GIA studies are primarily based on GIA-induced vertical motions (sea level, gravity, etc.). How about horizontal motion? GIA’s effects on horizontal motion are not negligible. When ice sheets grow, the surface bends to subside, the mantle moves away from the ice sheet centers – both processes cause horizontal motions on the surface (Fig. 2). GIA is still causing crustal horizontal motions in both Canada and Northern Europe as observed by GPS (Milne et al., 2001).

So, <strong>how significant is the GIA-induced horizontal motion during glacial cycles? Could it be strong enough to compete with the long-term plate motion driven by mantle convection?</strong> If you compare the GIA-induced crustal horizontal motion recorded by GPS in Canada (Kreemer et al., 2018) to the current plate motion rate, you might say no – the latter is at least one order larger than the former. However, this comparison is only for the present day, and it is almost certain that the GIA-induced horizontal motion during the last glacial cycle was much more significant than it is now, given periods with much more rapid ice growth and melt. <strong>Could the glaciation/deglaciation affect the long-term tectonic plate motion? </strong>If so, plate motions in glacial cycles (tens of thousands of years timescale) would not be as stable as many thought. This question has not been explored previously and could have broad implications on tectonic processes during glacial cycles, including plate motion, mid-ocean ridge spreading, and mantle degassing rate.

Unlike vertical motions recorded by paleo-sea level indicators, it is difficult to find direct observational evidence of GIA-induced horizontal motion throughout glacial cycles. So, to answer that question, we rely on numerical modeling. GIA modeling depends on input models of ice history and Earth’s rheology. Luckily, we have a basic understanding of ice history from sea-level and geomorphological records (Peltier et al., 2015) and some understanding of Earth’s rheology. Lithospheric plates have strong (i.e., less deformable) plate interiors and weak (i.e., less viscous, more deformable) plate boundaries, and mantle viscosity is on the order of 10<sup>21</sup> Pa s (with a possibly less viscous asthenosphere beneath the lithosphere). By choosing model inputs as realistic as possible, we perform numerical calculations to simulate GIA-induced horizontal motion during the last glacial cycle.

Our GIA models show strong influences of glacial forcing (loading and unloading) on lithospheric motion (i.e., motion on Earth’s surface). GIA causes plate-scale rotations in the North American plate, with a counterclockwise pattern during glaciation (Fig. 3a) and a clockwise pattern during deglaciation. The magnitude of the plate-scale rotation induced by GIA could reach ~25% of the current geologic plate motion rate for the North American plate. Note that the North American plate is where GIA has the greatest impact, since it hosted the largest ice sheet during the last glacial cycle.

With the existence of weak plate margins (e.g., at mid-ocean ridges) that decouple strong lithospheric plates, GIA causes differential horizontal motion across mid-ocean ridges (Fig 3), affecting the spreading rate of mid-ocean ridges, especially for the North Atlantic mid-ocean ridge near the former Laurentide ice sheet. Similar effects of GIA on mid-ocean ridge spreading are also observed in our models around Antarctica (Fig. 3b). One particularly interesting area is the Iceland mid-ocean ridge, which is so close to the Greenland ice sheet. Models show that deglaciation in Greenland caused up to 40% fluctuations in the spreading rate of the Iceland Ridge between 12,000 and 6,000 years ago, which may explain Holocene volcanism in Iceland (Yuan and Zhong, 2025). The Greenland ice sheet is currently experiencing rapid melting. Could it soon affect Iceland Ridge's spreading rate and magma production rate? It is an important question to investigate.

[caption id="attachment_42908" align="alignleft" width="1600"]<a href="https://blogs.egu.eu/divisions/gd/?attachment_id=42908" rel="attachment wp-att-42908"><img class="wp-image-42908 size-full" src="https://blogs.egu.eu/divisions/gd/files/2026/06/fig3_Combined-main_fig13.png" alt="" width="1600" height="615" /></a> Fig 3. GIA-induced surface horizontal motions in North America (a) and Antarctica (b). Color represents horizontal divergence, and vectors represent horizontal velocity. a) is during the glaciation stage at 110 thousand years ago, and b) is at the deglaciation stage at eight thousand years ago. The brown-colored linear features represent the enhanced horizontal divergence rate at mid-ocean ridges. Modified from Yuan and Zhong (2025).[/caption]

These results, shown in Fig. 3 and in our paper (Yuan and Zhong, 2025), reveal an interesting dynamic interplay between glacial cycles, lithospheric motion, ridge spreading, and climate during ice ages. It is well known that tectonic processes strongly affect climate; for example, they may be responsible for the global cooling in the Cenozoic (Raymo and Ruddiman, 1992). However, it is less well known that climatic forcing can also leave a fingerprint on tectonic processes, including large-scale plate tectonics. In addition to what we showed in Fig. 3, it has also been discussed whether global sea-level fluctuations during glacial cycles could trigger observable crustal topography and/or thickness variations in the seafloor (Crowley et al., 2015; Olive et al., 2015). We hope our findings from numerical modeling can inspire greater interest in this topic and more efforts to detect subtle signals in observations to better quantify the impacts of climatic forcing on tectonics.
<pre>References:

Yuan, Tao, and Shijie Zhong. 2025. “Effects of Glacial Forcing on Lithospheric Motion and Ridge Spreading.” <em>Nature</em>, April 23, 1–7. https://doi.org/10.1038/s41586-025-08846-x.

Yuan, Tao, Shijie Zhong, Glenn Milne, and Donna dePolo. 2026. “Reconciling Inferences of Mantle Viscosity and Late Quaternary Ice - the Importance of an Asthenosphere and 3-D Viscosity.” <em>ESS Open Archive</em> 2026 (0417). https://doi.org/10.22541/essoar.15001943/v2.

Crowley, John W., Richard F. Katz, Peter Huybers, Charles H. Langmuir, and Sung-Hyun Park. 2015. “Glacial Cycles Drive Variations in the Production of Oceanic Crust.” <em>Science</em> 347 (6227): 1237–40. https://doi.org/10.1126/science.1261508.

Haskell, N. A. 1935. “The Motion of a Viscous Fluid Under a Surface Load.” <em>Physics</em> 6 (8): 265–69. https://doi.org/10.1063/1.1745329.

Kreemer, Corné, William C. Hammond, and Geoffrey Blewitt. 2018. “A Robust Estimation of the 3‐D Intraplate Deformation of the North American Plate From GPS.” <em>Journal of Geophysical Research: Solid Earth</em> 123 (5): 4388–412. https://doi.org/10.1029/2017JB015257.

Milne, G. A., J. L. Davis, Jerry X. Mitrovica, et al. 2001. “Space-Geodetic Constraints on Glacial Isostatic Adjustment in Fennoscandia.” <em>Science</em> 291 (5512): 2381–85. https://doi.org/10.1126/science.1057022.

Olive, J. A., M. D. Behn, G. Ito, W. R. Buck, J. Escartín, and S. Howell. 2015. “Sensitivity of Seafloor Bathymetry to Climate-Driven Fluctuations in Mid-Ocean Ridge Magma Supply.” <em>Science</em> 350 (6258): 310–13. https://doi.org/10.1126/science.aad0715.

Peltier, W. R., D. F. Argus, and R. Drummond. 2015. “Space Geodesy Constrains Ice Age Terminal Deglaciation: The Global ICE-6G_C (VM5a) Model: Global Glacial Isostatic Adjustment.” <em>Journal of Geophysical Research: Solid Earth</em> 120 (1): 450–87. https://doi.org/10.1002/2014JB011176.

Raymo, M. E., and W. F. Ruddiman. 1992. “Tectonic Forcing of Late Cenozoic Climate.” <em>Nature</em> 359 (6391): 117–22. https://doi.org/10.1038/359117a0.

Willen, Matthias O., Bert Wouters, Taco Broerse, Eric Buchta, and Veit Helm. 2025. “Satellite Data Reveal Details of Glacial Isostatic Adjustment in the Amundsen Sea Embayment, West Antarctica.” <em>The Cryosphere</em> 19 (6): 2213–27. https://doi.org/10.5194/tc-19-2213-2025.

UNAVCO, 2026, GPS Spotlight: Station CHUR: <a href="https://spotlight.unavco.org/station-pages/chur/chur.html">https://spotlight.unavco.org/station-pages/chur/chur.html</a> (accessed May 2026).</pre>]]></content:encoded>
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					<title><![CDATA[Join the EGU Ocean Sciences blog team 🌊]]></title>
					<link>https://blogs.egu.eu/divisions/os/2026/06/02/join-egu-os-division/</link>
					<comments>https://blogs.egu.eu/divisions/os/2026/06/02/join-egu-os-division/#comments</comments>
					<pubDate>Tue, 02 Jun 2026 15:20:23 +0000</pubDate>
					<dc:creator><![CDATA[Jacqueline Behncke]]></dc:creator>
							<category><![CDATA[News]]></category>
		<category><![CDATA[OS Announcements]]></category>
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											<description><![CDATA[The EGU Ocean Sciences division blog is looking for new volunteer editors. So far, the team consists of two early career scientists, Jacqueline and Maurie — both working in ocean biogeochemistry — and we would love to grow. As an editor, you will keep an eye out for interesting new articles and datasets to write about, write short blog posts about ocean related news, and approach other scientists to contribute (e.g. at conferences or on LinkedIn). You can also run your own ocean science series if you feel like it. We are always looking for creative ideas and new formats. There are no fixed commitments: contribute as much or as little as you like. We are especially keen to hear from early career scientists working outside of biogeochemistry, though anyone with a passion for ocean sciences is warmly welcome! It is a great opportunity for those who enjoy writing, want to grow their network, or are looking for something meaningful to add to their CV. If that sounds like you, get in touch through our emails: jbehncke@geomar.de maurie.keppens@vliz.be]]></description>
													<content:encoded><![CDATA[<p class="font-claude-response-body break-words whitespace-normal leading-[1.7]">The EGU Ocean Sciences division blog is looking for new volunteer editors. So far, the team consists of two early career scientists, Jacqueline and Maurie — both working in ocean biogeochemistry — and we would love to grow. As an editor, you will keep an eye out for interesting new articles and datasets to write about, write short blog posts about ocean related news, and approach other scientists to contribute (e.g. at conferences or on LinkedIn). You can also run your own ocean science series if you feel like it. We are always looking for creative ideas and new formats. There are no fixed commitments: contribute as much or as little as you like. We are especially keen to hear from early career scientists working outside of biogeochemistry, though anyone with a passion for ocean sciences is warmly welcome! It is a great opportunity for those who enjoy writing, want to grow their network, or are looking for something meaningful to add to their CV. 

If that sounds like you, get in touch through our emails: 
<a href="mailto:jbehncke@geomar.de">jbehncke@geomar.de</a> 
<a href="mailto:maurie.keppens@vliz.be">maurie.keppens@vliz.be</a>]]></content:encoded>
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					<title><![CDATA[Reclaiming scientific publishing: Our duty to make science freely accessible to all]]></title>
					<link>https://blogs.egu.eu/divisions/hs/2026/06/02/reclaiming-scientific-publishing-our-duty-to-make-science-freely-accessible-to-all/</link>
					<comments>https://blogs.egu.eu/divisions/hs/2026/06/02/reclaiming-scientific-publishing-our-duty-to-make-science-freely-accessible-to-all/#comments</comments>
					<pubDate>Tue, 02 Jun 2026 14:23:22 +0000</pubDate>
					<dc:creator><![CDATA[Bettina Schaefli]]></dc:creator>
							<category><![CDATA[Opinion]]></category>
		<category><![CDATA[Science, Policy & Society]]></category>
		<category><![CDATA[diamond]]></category>
		<category><![CDATA[open access]]></category>
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											<description><![CDATA[Editor’s note: While this article explores the benefits of Diamond Open Access and critiques commercial, for-profit publishing structures, it is important to note that the European Geosciences Union (EGU) operates on a community-led, transparent, and not-for-profit Open Access model. EGU journals use Article Processing Charges (APCs) strictly to cover publishing costs and support the scientific community, alongside a strong waiver program to ensure financial accessibility for authors. When we (Camille Thomas and Romain Vaucher speaking) entered academia as graduate students in France and Switzerland, we were enthusiastic about the vast amount of research available with a simple click on our university computers. However, we also quickly felt disheartened by the significant amount of research work we couldn’t access when wrapping up our theses from home. Luckily, pirates existed. Empowered by Aaron Swartz’s Guerilla Open Access Manifesto, Alexandra Elbakyan created Sci-Hub in 2011, the greatest leak of scientific knowledge of the century. We felt right in the middle of an Open Access (OA) revolution that would finally make all scientific articles, old and new, accessible to everyone. Fifteen years later, our hopes as idealistic early-career researchers have been crushed by the oligopolistic model of scientific publishing and the subtle pressures of the “publish or perish” culture that reigns over our career development. In the meantime, publishers like Frontiers, MDPI and Springer Nature, to name a few, have exponentially expanded their number of titles. They have become increasingly exploitative of scholarly manpower, moving far away from the genuine accessibility they allegedly promised under the guise of this OA transformation. Open Access is to be praised, but the way it has been implemented through the mainstream Gold and Green OA models now primarily serves the status quo of large for-profit publishers. These entities hijack public money and voluntary editorial labour for their own profit and that of their shareholders (Butler et al., 2023; Shu and Larivière, 2024). In a nutshell, to offer reader accessibility, the Gold OA model requires authors to pay an Article Processing Charge (APC; around 2,000 $/€, rarely less, and often much more) covered by individual research funds, funding agencies or university library deals. The Green OA model allows authors to upload their accepted, non-formatted manuscripts to repositories after an embargo period. While both models allow compliance with funding agency mandates, true equity and accessibility are ultimately left behind. In an article we recently published (Vaucher and Thomas, 2026), we describe the mechanisms through which we, as researchers, inadvertently contribute to keeping research exclusive while driving the publishing model down an unsustainable path. Just like our broader economy, our publishing model and the ways science is evaluated fuelled a predatory system that demands more papers, funding and prestige at an ever-faster rate (Walter and Mullins, 2019), likely at the expense of quality, diversity and ethics (Frank et al., 2023; Heen and Vogt, 2024). These concerns aren’t entirely new. What is new, however, is the growing realisation among societies, universities and funding bodies that we must move away from this system. Initiatives like the European Diamond Capacity Hub, ALMASI and craft-OA are actively paving a way forward that we, as scientists, have yet to fully embrace. In the geosciences, a collective and concerted effort is currently being made by researchers to provide fairer, more sustainable alternatives through community-driven Diamond OA journals (which feature no APCs and completely free access to published articles). Volcanica (Farquharson and Wadsworth, 2018), Sedimentologika (Thomas et al., 2023), Tektonika (Fernández-Blanco et al., 2023), Seismica (Rowe et al., 2022), Geomorphica (Lefebvre et al., 2025), Open Paleontology (Drage et al., 2024), Advances in Geochemistry and Cosmochemistry (Pourret et al., 2025), Geodynamica, jSEDI and Planetary Research are all recently created, scholarly-run journals funded by university library investments to promote better ways of publishing. Their articles are peer-reviewed, free for readers to access, and free for authors to publish. They rely entirely on the voluntary involvement of scientists running open-source editorial platforms (such as Open Journal Systems), transparent workflows, copyediting, production and final dissemination. Diamond OA journals offer an alternative path for all of us to transform our broken publishing system and reclaim ownership of our own science. These efforts go hand in hand with greater involvement in our academic societies and non-profit publishing initiatives. Ultimately, real transformation can only happen if all of us as researchers realise how inherently unfair and exclusive the current system is to labs and institutions that cannot afford steep Gold OA APCs or paywalled journal subscriptions. It also means we must collectively stop evaluating science based on journal prestige and the flawed metrics they own (Posada and Chen, 2018; Sabel and Larhammar, 2025; Simons, 2008). Only by breaking these habits can we truly make knowledge accessible to all. Note by the editor, B. Schaefli: this is a blog post that is re-published from the Geolog &nbsp; References Butler, L.-A., Matthias, L., Simard, M.-A., Mongeon, P., and Haustein, S.: The oligopoly’s shift to open access: How the big five academic publishers profit from article processing charges, Quantitative Science Studies, 4, 778–799, https://doi.org/10.1162/qss_a_00272, 2023. Drage, H. B., Keating, J. N., Nielsen, M. L., Saleh, F., and Hearing, T. W. W.: Open Palaeontology: a new model of diamond open access journal for palaeontology, Open Palaeontology, 1, 1–6, https://doi.org/10.26034/la.opal.2024.6223, 2024. Farquharson, J. I. and Wadsworth, F. B.: Introducing Volcanica: The first diamond open-access journal for volcanology, Volcanica, 1, I–IX, https://doi.org/10.30909/vol.01.01.i-ix, 2018. Fernández-Blanco, D., Lacassin, R., Gouiza, M., Perez-Diaz, L., Magee, C., McCarthy, D., Doré, T., Péron-Pinvidic, G., Kavanagh, J., Bond, C., and Schmitt, R.: Tektonika: The Community-Led Diamond Open-Access Journal for Tectonics and Structural Geology, τeκτoniκa, 1, I–XIII, https://doi.org/10.55575/tektonika2023.1.1.56, 2023. Frank, J., Foster, R., and Pagliari, C.: Open access publishing – noble intention, flawed reality, Social Science &amp; Medicine, 317, 115592, https://doi.org/10.1016/j.socscimed.2022.115592, 2023. Heen, E. and Vogt, H.: Scientific rot: Unsustainable publishing practices threatens trust in medicine, Journal of Evaluation in Clinical Practice, 30, 941–944, https://doi.org/10.1111/jep.13989, 2024. Lefebvre, A., Bosch, R., Burrows, K., Giaime, M., Goodwin, G., Lai, L. S.-H., Stammler, M., and Fernández, R.: Geomorphica: The most accessible journal for the geomorphology community, Geomorphica, 1, https://doi.org/10.59236/geomorphica.v1i1.54, 2025. Posada, A. and Chen, G.: Inequality in Knowledge Production: The Integration of Academic Infrastructure by Big Publishers, in: ELPUB 2018, https://doi.org/10.4000/proceedings.elpub.2018.30, 2018. Pourret, O., Millet, M.-A., Marin-Carbonne, J., Mallik, A., Tierney, J. E., Darling, J. R., Kiseeva, E. S., Torres, M. A., Fonseca, R. O. C., Tartèse, R., Namur, O., Klöcking, M., Matthews, S. W., Dahrén, B., Ickert, R. B., and Board,  the inaugural A. in G. and C. editorial: Equitable Access, Open Science, and the Future of Publishing in Geochemistry and Cosmochemistry, Advances in Geochemistry and Cosmochemistry, 1, https://doi.org/10.33063/agc.v1i1.770, 2025. Rowe, C., Agius, M., Convers, J., Funning, G., Galasso, C., Hicks, S., Huynh, T., Lange, J., Lecocq, T., Mark, H., Okuwaki, R., Ragon, T., Rychert, C., Teplitzky, S., and Van den Ende, M.: The launch of Seismica: a seismic shift in publishing, Seismica, 1, https://doi.org/10.26443/seismica.v1i1.255, 2022. Sabel, B. and Larhammar, D.: Reformation of science publishing: the Stockholm Declaration, R Soc Open Sci., 12, 251805, https://doi.org/10.1098/rsos.251805, 2025. Shu, F. and Larivière, V.: The oligopoly of open access publishing, Scientometrics, 129, 519–536, https://doi.org/10.1007/s11192-023-04876-2, 2024. Simons, K.: The Misused Impact Factor, Science, 322, 165–165, https://doi.org/10.1126/science.1165316, 2008. Thomas, C., Privat, A., Vaucher, R., Spychala, Y., Zuchuat, V., Marchegiano, M., Poyatos-Moré, M., Kane, I., and Chiarella, D.: Sedimentologika: a community-driven diamond open access journal in sedimentology, Sedimentologika, 2023. Vaucher, R. and Thomas, C.: Diamond is the new Green—Why Green Open Access is not a sustainable long-term model for scientific publishing, Sedimentologika, 4, https://doi.org/10.57035/journals/sdk.2026.e41.2397, 2026. Walter, P. and Mullins, D.: From symbiont to parasite: the evolution of for-profit science publishing, Molecular Biology of the Cell, https://doi.org/https://doi.org/10.1091/mbc.E19-03-0147, 2019.]]></description>
													<content:encoded><![CDATA[<pre class="moz-quote-pre"><em>Editor’s note</em>: While this article explores the benefits of Diamond Open Access and critiques commercial, for-profit publishing structures, it is important to note that the European Geosciences Union (EGU) operates on a community-led, transparent, and not-for-profit Open Access model. EGU journals use Article Processing Charges (APCs) strictly to cover publishing costs and support the scientific community, alongside a strong waiver program to ensure financial accessibility for authors.</pre>
When we (Camille Thomas and Romain Vaucher speaking) entered academia as graduate students in France and Switzerland, we were enthusiastic about the vast amount of research available with a simple click on our university computers. However, we also quickly felt disheartened by the significant amount of research work we couldn’t access when wrapping up our theses from home. Luckily, pirates existed. Empowered by Aaron Swartz’s <a href="https://ia800101.us.archive.org/1/items/GuerillaOpenAccessManifesto/Goamjuly2008.pdf">Guerilla Open Access Manifesto</a>, Alexandra Elbakyan created Sci-Hub in 2011, the greatest leak of scientific knowledge of the century. We felt right in the middle of an Open Access (OA) revolution that would finally make all scientific articles, old and new, accessible to everyone.

Fifteen years later, our hopes as idealistic early-career researchers have been crushed by the oligopolistic model of scientific publishing and the subtle pressures of the “publish or perish” culture that reigns over our career development. In the meantime, publishers like Frontiers, MDPI and Springer Nature, to name a few, have exponentially expanded their number of titles. They have become increasingly exploitative of scholarly manpower, moving far away from the genuine accessibility they allegedly promised under the guise of this OA transformation.

Open Access is to be praised, but the way it has been implemented through the mainstream <a href="https://www.springernature.com/gp/open-science/about/green-or-gold-routes-to-oa">Gold and Green OA models</a> now primarily serves the status quo of large for-profit publishers. These entities hijack public money and voluntary editorial labour for their own profit and that of their shareholders (Butler et al., 2023; Shu and Larivière, 2024). In a nutshell, to offer reader accessibility, the Gold OA model requires authors to pay an Article Processing Charge (APC; around 2,000 $/€, rarely less, and often much more) covered by individual research funds, funding agencies or university library deals. The Green OA model allows authors to upload their accepted, non-formatted manuscripts to repositories after an embargo period. While both models allow compliance with funding agency mandates, true equity and accessibility are ultimately left behind.

<a href="https://doi.org/10.57035/journals/sdk.2026.e41.2397">In an article we recently published (Vaucher and Thomas, 2026),</a> we describe the mechanisms through which we, as researchers, inadvertently contribute to keeping research exclusive while driving the publishing model down an unsustainable path. Just like our broader economy, our publishing model and the ways science is evaluated fuelled a predatory system that demands more papers, funding and prestige at an ever-faster rate (Walter and Mullins, 2019), likely at the expense of quality, diversity and ethics (Frank et al., 2023; Heen and Vogt, 2024). These concerns aren’t entirely new. What is new, however, is the growing realisation among societies, universities and funding bodies that we must move away from this system. Initiatives like the European Diamond Capacity Hub, ALMASI and craft-OA are actively paving a way forward that we, as scientists, have yet to fully embrace.

In the geosciences, a collective and concerted effort is currently being made by researchers to provide fairer, more sustainable alternatives through community-driven Diamond OA journals (which feature no APCs and completely free access to published articles). Volcanica (Farquharson and Wadsworth, 2018), Sedimentologika (Thomas et al., 2023), Tektonika (Fernández-Blanco et al., 2023), Seismica (Rowe et al., 2022), Geomorphica (Lefebvre et al., 2025), Open Paleontology (Drage et al., 2024), Advances in Geochemistry and Cosmochemistry (Pourret et al., 2025), Geodynamica, jSEDI and Planetary Research are all recently created, scholarly-run journals funded by university library investments to promote better ways of publishing.

Their articles are peer-reviewed, free for readers to access, and free for authors to publish. They rely entirely on the voluntary involvement of scientists running open-source editorial platforms (such as Open Journal Systems), transparent workflows, copyediting, production and final dissemination. Diamond OA journals offer an alternative path for all of us to transform our broken publishing system and reclaim ownership of our own science. These efforts go hand in hand with greater involvement in our academic societies and non-profit publishing initiatives.

Ultimately, real transformation can only happen if all of us as researchers realise how inherently unfair and exclusive the current system is to labs and institutions that cannot afford steep Gold OA APCs or paywalled journal subscriptions. It also means we must collectively stop evaluating science based on journal prestige and the flawed metrics they own (Posada and Chen, 2018; Sabel and Larhammar, 2025; Simons, 2008). Only by breaking these habits can we truly make knowledge accessible to all.
<p style="text-align: right"><em>Note by the editor, B. Schaefli: this is a blog post that is re-published from the <a href="https://blogs.egu.eu/geolog/2026/06/01/reclaiming-scientific-publishing-our-duty-to-make-science-freely-accessible-to-all/">Geolog</a></em></p>
&nbsp;

<strong>References</strong>

Butler, L.-A., Matthias, L., Simard, M.-A., Mongeon, P., and Haustein, S.: The oligopoly’s shift to open access: How the big five academic publishers profit from article processing charges, Quantitative Science Studies, 4, 778–799, https://doi.org/10.1162/qss_a_00272, 2023.

Drage, H. B., Keating, J. N., Nielsen, M. L., Saleh, F., and Hearing, T. W. W.: Open Palaeontology: a new model of diamond open access journal for palaeontology, Open Palaeontology, 1, 1–6, https://doi.org/10.26034/la.opal.2024.6223, 2024.

Farquharson, J. I. and Wadsworth, F. B.: Introducing Volcanica: The first diamond open-access journal for volcanology, Volcanica, 1, I–IX, https://doi.org/10.30909/vol.01.01.i-ix, 2018.

Fernández-Blanco, D., Lacassin, R., Gouiza, M., Perez-Diaz, L., Magee, C., McCarthy, D., Doré, T., Péron-Pinvidic, G., Kavanagh, J., Bond, C., and Schmitt, R.: Tektonika: The Community-Led Diamond Open-Access Journal for Tectonics and Structural Geology, τeκτoniκa, 1, I–XIII, https://doi.org/10.55575/tektonika2023.1.1.56, 2023.

Frank, J., Foster, R., and Pagliari, C.: Open access publishing – noble intention, flawed reality, Social Science &amp; Medicine, 317, 115592, https://doi.org/10.1016/j.socscimed.2022.115592, 2023.

Heen, E. and Vogt, H.: Scientific rot: Unsustainable publishing practices threatens trust in medicine, Journal of Evaluation in Clinical Practice, 30, 941–944, https://doi.org/10.1111/jep.13989, 2024.

Lefebvre, A., Bosch, R., Burrows, K., Giaime, M., Goodwin, G., Lai, L. S.-H., Stammler, M., and Fernández, R.: Geomorphica: The most accessible journal for the geomorphology community, Geomorphica, 1, https://doi.org/10.59236/geomorphica.v1i1.54, 2025.

Posada, A. and Chen, G.: Inequality in Knowledge Production: The Integration of Academic Infrastructure by Big Publishers, in: ELPUB 2018, https://doi.org/10.4000/proceedings.elpub.2018.30, 2018.

Pourret, O., Millet, M.-A., Marin-Carbonne, J., Mallik, A., Tierney, J. E., Darling, J. R., Kiseeva, E. S., Torres, M. A., Fonseca, R. O. C., Tartèse, R., Namur, O., Klöcking, M., Matthews, S. W., Dahrén, B., Ickert, R. B., and Board,  the inaugural A. in G. and C. editorial: Equitable Access, Open Science, and the Future of Publishing in Geochemistry and Cosmochemistry, Advances in Geochemistry and Cosmochemistry, 1, https://doi.org/10.33063/agc.v1i1.770, 2025.

Rowe, C., Agius, M., Convers, J., Funning, G., Galasso, C., Hicks, S., Huynh, T., Lange, J., Lecocq, T., Mark, H., Okuwaki, R., Ragon, T., Rychert, C., Teplitzky, S., and Van den Ende, M.: The launch of Seismica: a seismic shift in publishing, Seismica, 1, https://doi.org/10.26443/seismica.v1i1.255, 2022.

Sabel, B. and Larhammar, D.: Reformation of science publishing: the Stockholm Declaration, R Soc Open Sci., 12, 251805, https://doi.org/10.1098/rsos.251805, 2025.

Shu, F. and Larivière, V.: The oligopoly of open access publishing, Scientometrics, 129, 519–536, https://doi.org/10.1007/s11192-023-04876-2, 2024.

Simons, K.: The Misused Impact Factor, Science, 322, 165–165, https://doi.org/10.1126/science.1165316, 2008.

Thomas, C., Privat, A., Vaucher, R., Spychala, Y., Zuchuat, V., Marchegiano, M., Poyatos-Moré, M., Kane, I., and Chiarella, D.: Sedimentologika: a community-driven diamond open access journal in sedimentology, Sedimentologika, 2023.

Vaucher, R. and Thomas, C.: Diamond is the new Green—Why Green Open Access is not a sustainable long-term model for scientific publishing, Sedimentologika, 4, https://doi.org/10.57035/journals/sdk.2026.e41.2397, 2026.

Walter, P. and Mullins, D.: From symbiont to parasite: the evolution of for-profit science publishing, Molecular Biology of the Cell, https://doi.org/https://doi.org/10.1091/mbc.E19-03-0147, 2019.]]></content:encoded>
																<wfw:commentRss>https://blogs.egu.eu/divisions/hs/2026/06/02/reclaiming-scientific-publishing-our-duty-to-make-science-freely-accessible-to-all/feed/</wfw:commentRss>
					<slash:comments>2</slash:comments>
									</item>
							<item>
					<title><![CDATA[Join the team! The TS division is looking for new volunteers]]></title>
					<link>https://blogs.egu.eu/divisions/ts/2026/06/02/join-the-team/</link>
					<comments>https://blogs.egu.eu/divisions/ts/2026/06/02/join-the-team/#comments</comments>
					<pubDate>Tue, 02 Jun 2026 12:15:54 +0000</pubDate>
					<dc:creator><![CDATA[Pauline Gayrin]]></dc:creator>
							<category><![CDATA[Editorial]]></category>
		<category><![CDATA[call for volunteers]]></category>
		<category><![CDATA[Tectonics and Structural Geology]]></category>
					<guid isPermaLink="false"></guid>
											<description><![CDATA[Hello there! Welcome to the TS-Blog! I&#8217;m Pauline, editor in chief. If you&#8217;re reading this, you&#8217;re probably already intrigued by our announcement and might wonder: What is it like being a blog editor? Or simply: What if the next editor of a post was&#8230; ME?  Well, let me tell you more about being an editor. Because our editor team is looking for new members to bring in their perspective and give visibility to people, topics, concerns. Yes, we are the Tectonics and Structural geology division blog, but that does not mean every post has to be about tectonics or structural geology specifically. Indeed, the freedom of topic of our team makes our success and the diversity of the TS division ensures a public for every message. Editors can publish about a lot of topics. Let me give you a (non exhaustive) list of ideas: geologic teaching, field trips, challenges in resources management, EGU medallist, new tools, a groundbreaking theory, lessons learned from failure, a global boundary stratotype, parenting as geologist travelling the world, publishing an article for the first time, a paper one should not miss, time management, creativity at making figures, a surprising geological feature etc. etc. your imagination is the limit. What does an editor do? As an editor you are in charge of publishing posts regularly. That does not mean you have to write every post yourself – you can of course – but you can also commission guest authors, which is also a good occasion to enrich your network. The medallist whose presentation you found inspiring at the General Assembly but could talk to in person? How about an interview with them? The author of the paper whose points you found really surprising? Why not give them the chance to make their points to the blog audience? You surely has someone in mind, to who you dream to ask questions&#8230; I feel you thinking. Yes, the blog is an opportunity to make it happen. And no worries if you&#8217;re a beginner in science communication, the team is supportive and will help you learn the new skills you need. Don’t feel like words are your thing? We are also looking for illustrators to embellish the featured image of the blog and share on social media, as we are proud to have a strict no AI policy to respect the work of the artists around. How much time shall I allow? How much time do you have? Your time commitment is chosen by you. We are aiming for regular posts, but the frequency depends on what you can provide. Even if you only have one idea and time for a single post – let us know! We are more than happy to feature you as a guest author. We can&#8217;t wait to read you soon here! How to volunteer? Easy! Just write to me: paulinegayrin@protonmail.com If you are still unsure – same – I am happy to provide you with more infos and answer all the questions you might still have. Me and the team are looking forward to hearing from you.]]></description>
													<content:encoded><![CDATA[<h4>Hello there! Welcome to the TS-Blog!</h4>
I'm Pauline, editor in chief.
If you're reading this, you're probably already intrigued by our announcement and might wonder: What is it like being a blog editor? Or simply:
<h4><em>What if the next editor of a post was... ME? </em></h4>
Well, let me tell you more about being an editor. Because our editor team is looking for new members to bring in their perspective and give visibility to people, topics, concerns.

Yes, we are the Tectonics and Structural geology division blog, but that does not mean every post has to be about tectonics or structural geology specifically. Indeed, the freedom of topic of our team makes our success and the diversity of the TS division ensures a public for every message. Editors can publish about a lot of topics. Let me give you a (non exhaustive) list of ideas: geologic teaching, field trips, challenges in resources management, EGU medallist, new tools, a groundbreaking theory, lessons learned from failure, a global boundary stratotype, parenting as geologist travelling the world, publishing an article for the first time, a paper one should not miss, time management, creativity at making figures, a surprising geological feature etc. etc. your imagination is the limit.
<h4><em>What does an editor do?</em></h4>
As an editor you are in charge of publishing posts regularly. That does not mean you have to write every post yourself – you can of course – but you can also commission guest authors, which is also a good occasion to enrich your network. The medallist whose presentation you found inspiring at the General Assembly but could talk to in person? How about an interview with them? The author of the paper whose points you found really surprising? Why not give them the chance to make their points to the blog audience? You surely has someone in mind, to who you dream to ask questions... I feel you thinking. Yes, the blog is an opportunity to make it happen.
And no worries if you're a beginner in science communication, the team is supportive and will help you learn the new skills you need.
<h4><em>Don’t feel like words are your thing?</em></h4>
We are also looking for illustrators to embellish the featured image of the blog and share on social media, as we are proud to have a strict no AI policy to respect the work of the artists around.
<h4><em>How much time shall I allow?</em></h4>
How much time do you have? Your time commitment is chosen by you. We are aiming for regular posts, but the frequency depends on what you can provide. Even if you only have one idea and time for a single post – let us know! We are more than happy to feature you as a guest author.

We can't wait to read you soon here!
<h4><em>How to volunteer?</em></h4>
Easy! Just write to me: <a href="mailto:paulinegayrin@protonmail.com">paulinegayrin@protonmail.com</a>

If you are still unsure – same – I am happy to provide you with more infos and answer all the questions you might still have. Me and the team are looking forward to hearing from you.]]></content:encoded>
																<wfw:commentRss>https://blogs.egu.eu/divisions/ts/2026/06/02/join-the-team/feed/</wfw:commentRss>
					<slash:comments>0</slash:comments>
									</item>
							<item>
					<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>
					<guid isPermaLink="false"></guid>
											<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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					<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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					<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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					<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 />

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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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					<slash:comments>0</slash:comments>
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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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					<slash:comments>0</slash:comments>
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							<item>
					<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>
					<guid isPermaLink="false"></guid>
											<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>
		<category><![CDATA[coding]]></category>
		<category><![CDATA[DEM]]></category>
		<category><![CDATA[matlab]]></category>
		<category><![CDATA[open-source]]></category>
		<category><![CDATA[python]]></category>
		<category><![CDATA[terrain analysis]]></category>
		<category><![CDATA[topographic analysis]]></category>
		<category><![CDATA[Topotoolbox]]></category>
		<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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									</item>
					</channel>
	</rss>
