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Writing your own press release

Writing your own press release

Do you have an upcoming publication and would like to extend its reach through a press release? Maybe your university doesn’t have a media office able to help, you are short on time, and/or don’t know where to start. Don’t fret, this week Grace Shephard (Researcher at CEED, University of Oslo) shares some tips for writing your own press release and includes a handy template for download. She also spoke to experts from the EGU and AGU press offices on writing a pitch to the media.

A press release is a really easy way to maximise the reach and impact of your latest paper. However, you might think that press releases are only reserved for papers in “high impact” journals or are written by magical gnomes that live in everyone else’s science garden but your own. But I think every research output deserves to be, and can be, shared in a concise, digestible, and fun way. Plus, without an enthusiastic journal handling editor or university media office on hand, it is often up to you – the author or co-author – to write it. Need a few more reasons? Well, the taxpayer likely pays for some of your funding, and science should be accessible for everyone. You’ve spent a long (*cough* sometimes very long) time and expended a lot of effort preparing and publishing that manuscript so spending a little extra effort with outreach won’t hurt. And even if your paper is behind a paywall this is a great way to share the main results and context in a format that isn’t the scientific abstract.

And finally, your own friends and family are much more likely to click on it than that boring looking DOI hyperlink that may have crawled its way onto your social media page. And who knows, they may actually ask you about your research sometime…

This gnome is too busy working on someone else’s press release. Credit: Craig McLauchlan (Unsplash)

What should a press release include?

You’ve all read press releases or science news write-ups before (examples included at bottom) but here are some tips for writing your own. The template is located just below:

    • Catchy headline – We’re not in the business of click-bait, unless it is nerdy scientific click-bait! Think informative but catchy and concise.
    • Cover image – Possibly more important than the headline. Find a fun photo or schematic image that is enticing. You could adapt one from your paper (but please not that snore-fest of an xy plot – keep that in the paper), or why not check out the EGU Imaggeo photos, or other online photo repositories for inspiration? Remember copyright/attribution.
    • Ingress – Ok, so they’ve clicked on your link and then will next read the first ~3-4 sentences. The ingress should summarize the main finding(s), the journal it was published in, and key author info. You can think of this like a tasty hint for the main body of the press release.
    • Jargon – Keep the tricky lingo on the down-low. Remember, you are writing for a diverse audience and should avoid jargon – or when it is unavoidable, define it! This is relevant for both the ingress and the main text. For tips on avoiding jargon see here. Being able to identify jargon is also applicable when writing those Plain Language Summaries that are increasingly featuring alongside published articles. The EGU Communications Officer Olivia Trani also provides some wise advice “When writing blog posts for the general public, science writer Julie Ann Miller says it best: ‘Don’t underestimate your readers’ intelligence, but don’t overestimate their knowledge of a particular field.’ As you discuss certain regions, processes, ideas, and theories, make sure you clearly show why they are important and what implications are present”.
    • Main text – Keep it short-ish – it is much more likely to be read in its entirety at 3-4 short paragraphs, or somewhere between 500-800 words. Writing in the third person and an active voice is probably the easiest and feels less like one is ‘tooting one’s own horn’. Mention the key results, some background and context, how the results were obtained (e.g. methods – keep it in logical order). Finally, the press release could mention what is novel about this work and maybe even what the study doesn’t address and any avenues for future research. Include subheadings to break it up or frame it around questions. Nanci Bompey, Assistant Director for Public Information at AGU suggests: “For scientific studies, the news should tell the reader what the researchers found – their main discovery or conclusions. Don’t let the study itself be the news; the study’s results are the news.
    • Think “big picture” – Remember to place your results in the broader context – why should the reader care? Hot topics like earthquakes, volcanoes, climate, sea-level, or Mars, may seem to quickly attract the readers so your challenge is to be creative and find nerdy analogies and indirect consequences no matter what your topic!
    • Images and video – Include 2-3 images to explain processes and highlight the results. A video or animation will collect bonus points too (check out this amazing video about the Iceland Hotspot). Include a caption and remember attribution. Another tip is if you’re creating original image content, consider adding a little watermark or signature in the image. Also consider putting yourself in the picture too – readers often relate more if they see the human face(s) behind the research (see also ‘Scientists who Selfie Break Down Stereotypes’).
    • Proof read – Ask a colleague or friend, either within or outside of the geosciences, to proof read.
    • Contact author – Include again the reference and link to the article, and who to contact for more info.
*Download the press release template and check-list here as a PDF *
When should it appear online?
    • As soon as possible – It’s up to you, of course, but ideally as close to the online publication date of the article as possible. You might like to wait until the nice proof versions are online, however, that can take weeks to months and you may run out of steam by then. 
Where to post the press release?
  • University webpage – If you have a media/communications office at your institute or university do get in touch with them to ask about options. Your post will likely appear on a university webpage and they will likely have an account that will re-share the press release on the likes of Phys.org and other news websites.
  • Personal website – In the event that a university-hosted platform doesn’t exist you could upload the release to your own personal page or blog. You’ll probably like to re-post it there anyway.

A short clip from – Film about the Creation of Iceland – by Alisha Steinberger and associated with press release for Steinberger et al. (2018; Nat.Geosci).

Maybe you want pitch your press release (or a shorter/alternative version of it) at an even bigger platform – here are some more possibilities.

  • EGU blogs – There are more options here than you can poke a stick at. Along with the other EGU Division Blogs we here on the GD blog welcome content related to your latest paper – just look up an editor’s contact details! You can also approach the EGU Communications and Media team directly:
      • You can send in a pitch for the EGU GeoLog which can include reports from Earth science events, conferences and fieldwork, comments on the latest geoscientific developments and posts on recently published findings in peer-reviewed journals.  For example, I tried my hand at GeoLog with ‘Mapping Ancient Oceans’ and received some really useful feedback from the EGU team!
      • If you are publishing research in one of the EGU journals that you believe to be newsworthy, you can pitch your paper to media@egu.eu . They regularly issue press releases on science published in EGU journals – as EGU’s Media and Communications Manager Bárbara Ferreira notes, “however, that we would prefer to hear about it even before the paper has been accepted: preparing a press release can take some time so it’s useful to know well in advance what papers we should be looking at. Naturally, any press release would be conditional on paper acceptance and would only be published when the final, peer-reviewed paper is published in the journal.”
  • AGU’s Eos Eos is another ‘Earth and Space Science News’ platform to send your pitch for an article.
    Heather Goss, Editor-in-Chief of Eos, suggests that when writing a pitch to the media you “keep your pitch between 200 and 500 words. (You can link to your research, or include more detail at the end of the message.) Begin with a sentence or two that highlights the article’s focus: Do you have an exciting finding? Is it a new method? Did it raise an interesting new question? Explain both the focus and what it is right up front. Then break down your research into 2-3 key points that you want to get across to the journalist. This might be your research method, a challenge that you had to overcome for the result, or it might simply be breaking down your research finding into a few digestible pieces. If there is a fun detail that adds colour, here is the place to add it. Finally, explain in a sentence or two why the publication’s audience should care. It helps the journalist put your work in context, and shows that you understand the outlet you’re pitching to—this is a crucial step if you’re actually writing the piece that would be published, as with Eos.”
  • Other Science news outlets – you could approach freelance journalist, local radio or news station, or those behind the popular sites like ScienceAlert, The Conversation (more in-depth), IFLS, National Geographic, Science Magazine etc. However, they receive a lot of mail and only follow up on selected pitches so just see what happens! 
Some additional tips before we part:
  • You can also use a little glossary or side bar to explain unavoidable technical terms (for example, “subduction” and “plate tectonics”, are terms I find hard to avoid).
  • Writing in English would reach a wide audience but consider including a shorter summary or translation to other languages.
  • Add hyperlinks and references for more info.
  • Include some direct quotes – if you write in third person then it makes it a little less awkward to quote yourself. You could also add a quote from a co-author or someone not-related to the study.
  • Need more inspiration? – head over to your favourite science news website, EGU GeoLog, or check out EGU/AGU’s social media accounts and take a look on how others write-up science news and press releases.

A couple more examples of press releases or similar-style science news articles:

I hope you find some of the tips above of use, and good luck with writing!

 

Thanks very much to Olivia Trani and Bárbara Ferreira (EGU), and Heather Goss and Nanci Bompey (AGU) again for their press release, pitch and outreach tips!

 

 

The past is the key

The past is the key

Lorenzo Colli

“The present is the key to the past” is a oft-used phrase in the context of understanding our planet’s complex evolution. But this perspective can also be flipped, reflected, and reframed. In this Geodynamics 101 post, Lorenzo Colli, Research Assistant Professor at the University of Houston, USA, showcases some of the recent advances in modelling mantle convection.  

 

Mantle convection is the fundamental process that drives a large part of the geologic activity at the Earth’s surface. Indeed, mantle convection can be framed as a dynamical theory that complements and expands the kinematic theory of plate tectonics: on the one hand it aims to describe and quantify the forces that cause tectonic processes; on the other, it provides an explanation for features – such as hotspot volcanism, chains of seamounts, large igneous provinces and anomalous non-isostatic topography – that aren’t accounted for by plate tectonics.

Mantle convection is both very simple and very complicated. In its essence, it is simply thermal convection: hot (and lighter) material goes up, cold (and denser) material goes down. We can describe thermal convection using classical equations of fluid dynamics, which are based on well-founded physical principles: the continuity equation enforces conservation of mass; the Navier-Stokes equation deals with conservation of momentum; and the heat equation embodies conservation of energy. Moreover, given the extremely large viscosity of the Earth’s mantle and the low rates of deformation, inertia and turbulence are utterly negligible and the Navier-Stokes equation can be simplified accordingly. One incredible consequence is that the flow field only depends on an instantaneous force balance, not on its past states, and it is thus time reversible. And when I say incredible, I really mean it: it looks like a magic trick. Check it out yourself.

With four parameters I can fit an elephant, and with five I can make him wiggle his trunk

This is as simple as it gets, in the sense that from here onward every additional aspect of mantle convection results in a more complex system: 3D variations in rheology and composition; phase transitions, melting and, more generally, the thermodynamics of mantle minerals; the feedbacks between deep Earth dynamics and surface processes. Each of these additional aspects results in a system that is harder and costlier to solve numerically, so much so that numerical models need to compromise, including some but excluding others, or giving up dimensionality, domain size or the ability to advance in time. More importantly, most of these aspects are so-called subgrid-scale processes: they deal with the macroscopic effect of some microscopic process that cannot be modelled at the same scale as the macroscopic flow and is too costly to model at the appropriate scale. Consequently, it needs to be parametrized. To make matters worse, some of these microscopic processes are not understood sufficiently well to begin with: the parametrizations are not formally derived from first-principle physics but are long-range extrapolations of semi-empirical laws. The end result is that it is possible to generate more complex – thus, in this regard, more Earth-like – models of mantle convection at the cost of an increase in tunable parameters. But what parameters give a truly better model? How can we test it?

Figure 1: The mantle convection model on the left runs in ten minutes on your laptop. It is not the Earth. The one on the right takes two days on a supercomputer. It is fancier, but it is still not the real Earth.

Meteorologists face similar issues with their models of atmospheric circulation. For example, processes related to turbulence, clouds and rainfall need to be parametrized. Early weather forecast models were… less than ideal. But meteorologists can compare every day their model predictions with what actually occurs, thus objectively and quantitatively assessing what works and what doesn’t. As a result, during the last 40 years weather predictions have improved steadily (Bauer et al., 2015). Current models are better at using available information (what is technically called data assimilation; more on this later) and have parametrizations that better represent the physics of the underlying processes.

If time travel is possible, where are the geophysicists from the future?

We could do the same, in theory. We can initialize a mantle convection model with some best estimate for the present-day state of the Earth’s mantle and let it run forward into the future, with the explicit aim of forecasting its future evolution. But mantle convection evolves over millions of years instead of days, thus making future predictions impractical. Another option would be to initialize a mantle convection model in the distant past and run it forward, thus making predictions-in-the-past. But in this case we really don’t know the state of the mantle in the past. And as mantle convection is a chaotic process, even a small error in the initial condition quickly grows into a completely different model trajectory (Bello et al., 2014). One can mitigate this chaotic divergence by using data assimilation and imposing surface velocities as reconstructed by a kinematic model of past plate motions (Bunge et al., 1998), which indeed tends to bring the modelled evolution closer to the true one (Colli et al., 2015). But it would take hundreds of millions of years of error-free plate motions to eliminate the influence of the unknown initial condition.

As I mentioned before, the flow field is time reversible, so one can try to start from the present-day state and integrate the governing equations backward in time. But while the flow field is time reversible, the temperature field is not. Heat diffusion is physically irreversible and mathematically unstable when solved back in time. Plainly said, the temperature field blows up. Heat diffusion needs to be turned off [1], thus keeping only heat advection. This approach, aptly called backward advection (Steinberger and O’Connell, 1997), is limited to only a few tens of millions of years in the past (Conrad and Gurnis, 2003; Moucha and Forte, 2011): the errors induced by neglecting heat diffusion add up and the recovered “initial condition”, when integrated forward in time (or should I say, back to the future), doesn’t land back at the desired present-day state, following instead a divergent trajectory.

Per aspera ad astra

As all the simple approaches turn out to be either unfeasible or unsatisfactory, we need to turn our attention to more sophisticated ones. One option is to be more clever about data assimilation, for example using a Kalman filter (Bocher et al., 2016; 2018). This methodology allow for the combining of the physics of the system, as embodied by the numerical model, with observational data, while at the same time taking into account their relative uncertainties. A different approach is given by posing a formal inverse problem aimed at finding the “optimal” initial condition that evolves into the known (best-estimate) present-day state of the mantle. This inverse problem can be solved using the adjoint method (Bunge et al., 2003; Liu and Gurnis, 2008), a rather elegant mathematical technique that exploits the physics of the system to compute the sensitivity of the final condition to variations in the initial condition. Both methodologies are computationally very expensive. Like, many millions of CPU-hours expensive. But they allow for explicit predictions of the past history of mantle flow (Spasojevic & Gurnis, 2012; Colli et al., 2018), which can then be compared with evidence of past flow states as preserved by the geologic record, for example in the form of regional- and continental-scale unconformities (Friedrich et al., 2018) and planation surfaces (Guillocheau et al., 2018). The past history of the Earth thus holds the key to significantly advance our understanding of mantle dynamics by allowing us to test and improve our models of mantle convection.

Figure 2: A schematic illustration of a reconstruction of past mantle flow obtained via the adjoint method. Symbols represent model states at discrete times. They are connected by lines representing model evolution over time. The procedure starts from a first guess of the state of the mantle in the distant past (orange circle). When evolved in time (red triangles) it will not reproduce the present-day state of the real Earth (purple cross). The adjoint method tells you in which direction the initial condition needs to be shifted in order to move the modeled present-day state closer to the real Earth. By iteratively correcting the first guess an optimized evolution (green stars) can be obtained, which matches the present-day state of the Earth.

1.Or even to be reversed in sign, to make the time-reversed heat equation unconditionally stable.

Introducing the blog team!

Introducing the blog team!

It’s time for another proper introduction of the blog team! As you will probably know, things have been a bit silent on the blog front lately. This is because all the blog editors were very busy and also: it’s hard to upload 52 times a year. You come up with some great blog ideas! (if you do: e-mail us, please!). Luckily, we used the EGU General Assembly to find some fresh blood for the blog team. Together with the seasoned blog team members and a new blog strategy, we are buzzing to give you regular content once again. Expect the usual blog posts on Wednesday at 9:00 am and in the future, maybe expect a little extra on Fridays… But who are these great people providing you with your weekly dose of geodynamics news?

The Blog Team

Iris van Zelst
I am a PhD student in the Seismology and Wave Physics group at ETH Zürich, Switzerland. I am right at the seismology border of geodynamic research, as I am combining geodynamic modelling with dynamic rupture modelling to look at earthquakes in subduction zones on the entire timescale relevant to the process. I also occasionally look at some data, because you should always keep it real. I am in the final year of my PhD (oh help!), so my aim as Editor-in-Chief is to make sure everyone else is organised and uploading regularly, while I will be mostly pulling the strings behind the scenes and writing an occasional blog post. Such as this one! In my spare time, I love to read lots of books in all kinds of genres, go to the theatre, and play a little bit of theatre myself. I recently enrolled in an improv class and it is so much fun! All the world’s a stage. You can reach my via e-mail.

Luca Dal Zilio
I am a postdoctoral researcher in Mechanical Engineering and Geophysics at the California Institute of Technology (Caltech). My research is primarily aimed at understanding the relationship between crustal deformation and earthquakes in mountain belts, such as the Alps and Himalaya. By combining theoretical, computational, and observational approaches, I attempt to understand the interplay between geodynamic space–time scales of millions of years of slow and broadly distributed regional deformation with seismic space–time scales of rapid and localised earthquake processes. My passion lies in democratising science communication via innovative and accessible tools in order to spread scientific research and discovery. And yes, I like coffee. Espresso. You can reach me via e-mail.

Anne Glerum
I am a postdoctoral researcher at GFZ Potsdam, Germany. With numerical models, I investigate the link between local stress and strain observations and far-field forcing in the East African Rift System. Other modelling interests include magma-tectonic feedback and surface evolution during continental extension. Outside of research, I love to go on walks with my dog, to explore my new home Berlin and to read books on all possible topics. I’m excited to show you the variety of geodynamics and its overlap with other disciplines as an editor of the GD blog team. You can reach me via e-mail.

Anna Gülcher
I am a PhD student at the Geophysical Fluid Dynamics group at ETH Zürich, Switzerland. With the use of numerical modelling, I study the interior dynamics of the Earth and other planets. For my research, I am trying the put geophysical, geological, and geochemical observations in a geodynamically coherent framework (with an emphasis on trying). I found a passion for windsurfing early on while still living in my flat home country (the Netherlands). Yet, since moving to mountainous Switzerland, I have traded in my windsurfing equipment for hiking boots or snowboarding gear and try to spend my free time in the Alps to seek some adrenaline. I’ve very recently started to learn how to play the guitar, and am very proud to say that I can now play my very first complete song. I am excited to be part of the GD team as an Editor! You can reach me via e-mail.

Diogo Lourenço
I am a postdoctoral researcher at the Department of Earth and Planetary Sciences at the University of California Davis, USA. My research aims at understanding the evolution and interior dynamics of the Earth and other rocky planets, primarily through the use of numerical models. When I am not working on theoretical geodynamics, I like to keep things theoretical. I like reading and playing music. Sometimes I also exercise by walking around museums and looking at things. With my work as an editor in this blog, I hope to bring geodynamics to the reader in a friendly and exciting way. I also hope to help building a more involved and integrative geodynamics community. You can reach me via e-mail.

Tobias Meier
I am currently a PhD student at the Center for Space and Habitability (CSH) at the University of Bern. My research focuses on understanding the interior dynamics of rocky exoplanets, particularly planets that are partly molten. At the CSH, Earth and planetary scientists and astrophysicists work side-by-side to understand the formation and evolution of solar system bodies and exoplanets. As an editor of the GD blog I will nurture the link between geodynamics and terrestrial planet evolution and foster interactions between related disciplines.
As an undergraduate I worked in the field of cosmology, so it was necessary for me to downsize from thinking about the vast scales of the universe to zooming in on individual planets when I transitioned to my PhD work. At the time of writing, there has not been a confirmation of an inhabited exoplanet where we could possibly travel to. So, on our own wonderful planet, I enjoy hiking in the beautiful Swiss mountains and I also (almost) never say no to a game of table tennis. You can reach me (also for table tennis!) via e-mail.

Antoine Rozel
I am a senior researcher in ETH Zürich. After studying physics (nobody is perfect), I have been working on numerical simulations of mantle convection involving absurd rheologies for quite a while now, I am getting old. I am also interested in crust and craton production in all solar system planets. To make life even more beautiful, I have also finished the conservatory in classical piano and I organised some painting exhibitions in the last years (you can find my gallery here). I have also found recently that -when I do not play pinball or videogames- I can save time by doing both music and sport at the same time by playing Japanese drums (taiko)! You can reach me via e-mail.

Grace Shephard
I am a Researcher at the Centre for Earth Evolution and Dynamics (CEED) at the University of Oslo, Norway. My research links plate tectonics,​ palaeogeography, and deep mantle structure and dynamics. I spend much of my time hunting for evidence to constrain the opening and closure of ocean basins, particularly around the Arctic, Atlantic and the Pacific. I think GPlates is an excellent Tardis with which to time travel. Geodynamics offers a lot of interdisciplinary and creative avenues to explore – and why not follow up your idea with a blog post! You can reach me via e-mail or find a sporadic tweet at @ShepGracie.

The Sassy Scientist
I am currently employed at a first tier research institute where I am continuously working with the greatest minds to further our understanding of the solid Earth system. Whether it is mantle or lithosphere structure and dynamics, solid Earth rheology parameters, earthquake processes, integrating observations with model predictions or inversions: you have read a paper of mine. Even if you are working on a topic I haven’t mentioned here, I still know everything about it. Do you have any problems in your research career? I have already experienced them. Do you struggle with your work-life balance? Been there, done that. Nowadays, I have only one hobby: helping you out by answering the most poignant questions in geodynamics, research, and life. I am waiting for you right here. Get inspired.

GD Guide to EGU19

GD Guide to EGU19

With this year’s EGU General Assembly (GA; #EGU19) looming in less than a week, it’s time for all attendees to finish (or start) their own scientific contributions, create their own personal programs as well as plan other activities during the conference. In this blog Nico Schliffke (GD ECS Rep) would like to share some useful advice how to successfully navigate through the conference and highlight relevant activities, both scientific and social, for Geodynamics Early Career Scientists (ECS).

The huge variety of scientific contributions (~18,000 at EGU18) might seem intimidating to begin with and makes it impossible for any individual to keep track of everything. To be well prepared for the conference, allow for a bit of time to create your own personal programme by logging in with your account details and search for relevant sessions, keywords, authors, friends or any other fields of interest. If you have found anything interesting, add it to your personal programme by ticking the ‘star’. After completing your personal programme you can print your own timetable or open it in the EGU 2019 app.

Besides all the (specific) scientific content of the GA, EGU19 offers a wide spread of exciting workshops and short courses to boost your personal and career skills, as well great debates, union wide events and division social events. Below you will find a list of highlight events, special ECS targeted events, social events and other things to keep in mind and to make the best of EGU19:

For first time attendees:

How to navigate the EGU: tips and tricks (Mon, 08:30 – 10:15, Room -2.16) – This workshop is led by several EGU ECS representatives and will give an overview of procedures during EGU as well as useful tips and tricks how to successfully navigate the GA.

GD workshops and short courses:

Geodynamics 101A: Numerical methods (Thur, 14:00-15:45, Room -2.62) Building on last year’s short course, we are happy to announce two short courses this year as a part of the ’Solid Earth 101’ series together with Seismology 101 and Geology 101. The first course deals with the basic concepts of numerical modelling, including discretisation of governing equations, building models, benchmarking (among others).

Geodynamics 101B: Large-scale dynamical processes (Fri, 14:00-15:45, Room -2.62)  The second short course will discuss the applications of geodynamical modelling. It will cover a state-of-art overview of main large-scale dynamics on Earth (mantle convection, continental breakup, subduction dynamics, crustal deformation..) but also discuss constraints coming from seismology (tomography) or the geological record.

Geology 101: The (hi)story of rocks (Tue, 14:00 – 15:45, Room -2.62)The complementary workshop in the 101 series: Find more about structural and petrological processes on Earth. It’s definitely worth knowing, otherwise why should we be doing many of these Geodynamical models?

Seismology 101 (Wed, 14:00 – 15:45, Room -2.62)The second complementary workshop in the 101 series. Many geodynamical models are based on observations using seismological methods. Find out more about earthquakes, beachballs and what semiologists are actually measuring – this is essential for any numerical or analogue geodynamical model!

GD related award ceremonies and lectures:

Arne Richter Award for Outstanding ECS Lecture by Mathew Domeier (Tue, 12:00-12:30 Room -2.21) – The Arne Richter award is an union-wide award for young scientists. We are happy to see that Mathew as a Geodynamicist has won the medal this year! Come along and listen to his current research.

Augustus Love Medal Lecture by Anne Davaille (Thur, 14:45-15:45, Room D1) – Listen to the exciting work of the first female winner of the Augustus Love Medal (the GD division award), Anne Davaille! She is specialised on experimental and analytical fluid dynamics which has given Geodynamics many new insights.

 Arthur Holmes Medal Lecture by Jean Braun  (Tue, 12:45-13:45, Room E1) – This one of the most prestigious EGU award for solid Earth geosciences. Jean is a geodynamicist from Potsdam and works on integrating surface and lithospheric dynamics into numerical models.

 

 

GD division social activities:

ECS GD informal lunch  (Mon, 12:30-14:00) – Come and meet the ECS team behind these GD activities! Meet in front of the conference center (look for “GD” stickers), to head to the food court in Kagran (2 subway stops away from the conference center, opposite direction to city centre).

ECS GD dinner (Wed, 19:30-22:00) – Join us for a friendly dinner at a traditional Viennese ‘Heurigen’ with fellow ECS Geodynamicists at Gigerl – Rauhensteingasse 3, Wien 1. Bezirk!  If you would like to attend the ECS GD dinner on Wednesday, please fill out this form to keep track on the number of people: https://docs.google.com/forms/d/e/1FAIpQLScpi8gvDDMOOOjLbtq4BrElsoBtTv86Mud7qNQ5yl7qWP5cUA/viewform  Remember to bring some cash to pay for your own food and drinks!

GD/TS/SM drinks (Wed, after ECS GD dinner) – Don’t worry if you cannot make for the ECS GD dinner! After dinner we’ll have a 5 min walk to Bermuda Bräu – Rabensteig 6, 1010 Wien for some drinks together with ECS from Seismology (SM) and Tectonics/Structural (TS), so you can meet us there too!  

GD Division meeting (Fri, 12:45-13:45 Room D2) – Elections and reports from the division president, ECS representative and other planning in GD related matters. Lunch provided!

Meet the division president of Geodynamics (Paul Tackley) and the ECS representative (Nico Schliffke) (Wed, 11:45-12:30, EGU Booth) – Come and discuss with the president and ECS rep about any GD related issues, suggestions or remarks.

Geodynamicists eating lunch at Kagran – it’s tradition by now.

EGU wide social activities:

Networking and ECS Zone (all week – red area)This area is dedicated to early career scientist all week and provides space to chillout, get your well deserved coffee or find out more about ECS related announcements.

Opening reception (Sun, 18:30 – 21:00, Foyer F) – Don’t miss out on many new faces and friends, as well as free food and drinks and the opening (ice-breaker) reception! There will also be a ECS corner to meet fellow young scientists, especially if it’s your first EGU.

EGU Award Ceremony (Wed, 17:30 – 20:00, Room E1) – All EGU medallists will receive their award at this ceremony.

ECS Forum (Wed, 12:45 – 13:45, Room L2)An open discussion on any ECS topic

ECS Networking and Careers Reception (by invitation only) (Tue, 19:00-20:30, Room F2)

Conveners’ reception (by invitation only) (Fri 19:30 – 0:00, Foyer F) 

Credit: Kai Boggild (distributed via imaggeo.egu.eu)

Great debates

Science in policymaking: Who is responsible?  (Mon, 10:45 – 12:30, Room E1) – Actively take part in one of the presently most important and hot topic!

How can Early Career Scientists prioritise their mental wellbeing? (Tue, 19:00 – 20:30, Room E1) – Many ECS find it challenging to prioritise their mental wellbeing. Discuss with many other young scientist how to tackle this really important issue and maybe learn helpful tips how to improve your own wellbeing! 

Other useful skills to polish your career/CV:

Help! I’m presenting at a scientific conference (Mon, 14:00 –15:45, Room -2.62) – Your first conference talk might be daunting. Find out best practices and tips how to create a concise and clear conference talk.

How to share your research with citizens and why it’s so important (Mon, 14:00-15:45, Room -2.16) – Do you share your research with the public? Can you explain in simple matters? An important topic for researchers currently!

How to make the most of your PhD or postdoc experience for getting your next job in academia (Tue, 16:15 – 18:00, Room -2.85) – It’s never too early to plan your next career step.

How to convene and chair a session at the General Assembly (Tue, 08:30-10:15, Room -2.85) – Find out what it needs to convene a session of short course at EGU. You may be surprised, but you could to it next year if you liked,

How to peer-review? (Mon, 16:15 -18:00, Room -2.85) – After the end of a PhD (or sometimes even earlier!) you may be asked to peer-review journal contributions, but hardly anyone knows the process beforehand.

How to find funding and write a research grant (Tue, 10:45-12:30, Room -2.16) – One of the major tasks when you finish your PhDs. It might even be useful when writing applications for travel support etc.

Funding opportunities: ERC grants (Tue, 12:45-13:45, Room 0.14) – Find out more about these generous grants and how to successfully apply for them

How to apply for the Marie Sklodowska-Curie grants (Wed, 12:45-13:45, Room 0.14)

Balancing work and personal life as a scientist (Wed, 16:15 – 18:00, Room -2.85) – Find out how not to lose sight of your hobbies and personal life in a increasingly competitive academic environment. 

Other interesting events:

Academia is not the only route (Thu, 10:45-12:30, Room -2.16) – Are you finishing your degree and not overly excited by an academic future? Try this short course on exploring career alternatives both inside and outside academia

Games for Geoscience (Wed, 16:15-18:00 (Talks) in Room L8 and 14:00-15:45 (Posters), Hall X4) – Games are more fun than work! Learn more on how to use games for communication, outreach and much more. 

Unconscious bias (Wed, 12:45-13:45, Room -2.32) – Become aware of the obstacles that some of your colleagues face every day, and that might prevent them from doing the best science

Promoting and supporting equality of opportunities in geosciences (Thu, 14:00-18:00, Room E1) – Any of us should promote an open, equal opportunity working environment and this session promises some very interesting talk on common issues, solutions and initiatives.

What I’ve learned from teaching geosciences in prisons – (Thu, 14:00-15:45, Hall X4 – Poster) by GD ECS Phil Heron.

Rhyme Your Research (Tue, 14:00 – 15:45, Room -2.16) – Reveal the poet in you and explain your research in an interesting and unusual way!

This is just a small list of possible activities during EGU19, and I’m sure to have missed out many more. So keep your eyes and ears open for additional events and spread the word if you know anything of particular interest. Also make sure you follow the GD Blog, our social media (EGU GD Facebook page) and EGU Twitter, to keep updated with any more information during the week! The official hashtag is #EGU19. All the best for EGU and I am looking forward to meeting many of you there!