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The slide of my 3min presentation entitled "Rocky Tidal Pools -  Carbonate chemistry, diurnal variability and calcifying organisms in future CO2 conditions". It shows coastal variability (lack of observation and understanding - seldom integrated in predictive climate models), what tidal pools are and what tidal pool variability is in pH, with and without artificially added CO2. And how this relate to the net calcification rate in the community.

The slide of my 3min presentation entitled "Rocky Tidal Pools - Carbonate chemistry, diurnal variability and calcifying organisms in future CO2 conditions". It shows coastal variability (lack of observation and understanding - seldom integrated in predictive climate models), what tidal pools are and what tidal pool variability is in pH, with and without artificially added CO2. And how this relate to the net calcification rate in the community.

Should I have submitted my #vEGU21 presentation to @EGU_BioGeo instead of @EGU_Ocean session 🤨?

Maybe. Or not.

Anyway. I talked for 2 minutes about #biogeochemistry of #tidalpools. My display material : meetingorganizer.copernicus.org/EGU21/EGU21-...

Feel free to start a discussion here !

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Before #EGU22 is over, @annette_eicker handed over the @EGU_Geodesy division vOSPP award from #vEGU21 to Sebastian Strasser from @tugraz

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Attending #vEGU21 was awesome, but I'm never doing a nighttime conference again! After 15hrs of sleeping and an afternoon outside, I have finally stopped feeling like a zombie!

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Thanks to all who attended our #vEGU21 @EGU_Atmos session on "Chemistry, Aerosols and Radiative Forcing in CMIP6-era models" even though it was almost the last session of the last afternoon. Really enjoyed hearing about ongoing analysis. See more at...

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Session G4.3 "Acquisition and processing of gravity and magnetic field data and their integrative interpretation" (meetingorganizer.copernicus.org/EGU21/session/39917 15:30 - 17:00) brings together Earth's gravity and magnetic field. See you there! #vEGU21 #vEGU21_G

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Session G4.2 "Satellite Gravimetry: Data Analysis, Results and Future Mission Concepts" will start soon (meetingorganizer.copernicus.org/EGU21/session/39905 11:45 - 15:00). See you there! #vEGU21_G #vEGU21

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In session GMPV9.5 we take a close look at volcanic processes, tectonics and deformation (meetingorganizer.copernicus.org/EGU21/session/39473 Starting at 11:45! #vEGU21_G #vEGU21 #vEGU21_GMPV #vEGU21_G #vEGU21_NH #vEGU21_TS

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Take a look below Earth's surface in session G4.4 "New tools for terrain gravimetry" (meetingorganizer.copernicus.org/EGU21/session/39918 11:00 - 11:45) #vEGU21_G #vEGU21

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Find out about modern concepts for gravimetric earth observation in session G4.1 (meetingorganizer.copernicus.org/EGU21/session/39904 9:00 - 10:30)! #vEGU21_G #vEGU21

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CO Meeting Organizer EGU21 The surface of Mars is riddled with dunes that form by accumulating sand particles that are carried by the wind. Since dune geometry and orientation adjust in response to prevailing wind conditions, the morphometrics of dunes can reveal information about the winds that formed them. Previous studies inferred the prevailing local wind direction from the orientation of dunes by manually analyzing spacecraft imagery. However, building a global map remained challenging, as manual detection of individual dunes over the entire Martian surface is impractical. Here, we employ Mask R-CNN, a state-of-the-art instance segmentation neural network, to detect and analyze isolated barchan dunes on a global scale.We prepared a training dataset by extracting Mars Context Camera (CTX) scenes of dune fields from a global CTX mosaic, as identified in the global dune-fields catalog. Images were cropped and standardized to a resolution of 832x832 pixels, and labeled using Labelbox’s online instance segmentation platform. Image augmentation and weight decay were employed to prevent overfitting during training. By inspecting 100 sample images from the validation database, we find that the network correctly identified ~86% of the isolated dunes, falsely identifying one feature as a barchan dune in a single image.

Wanna learn more about how to map surface winds on Mars from dunes using machine learning? Make sure to check out @Liorruba’s #vEGU21 invited presentation @ 9:05 am CEST/12:05 am PDT!
Abstract:@EuroGeosciences @StanfordEarth

meetingorganizer.copernicus.org/EGU21/EGU21-12…

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All about the December 2020 earthquake sequence in Petrinja, Croatia, is discussed in session TS4.0 (meetingorganizer.copernicus.org/EGU21/session/41372 15:30-17:00). See you there! #vEGU21_G #vEGU21_TS #vEGU21_GM #vEGU21_NH #vEGU21_SM #vEGU21

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Ready to hear more about the relationship between ice sheets and the solid Earth? Then join us in session CR3.9 (meetingorganizer.copernicus.org/EGU21/session/39063 at 15:30. #vEGU21_G #vEGU21_CR #vEGU21_CL #vEGU21_GD #vEGU21_GM #vEGU21

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#vEGU21

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All aspects of Geodesy covered in one session? It's about time for the "Open Session in Geodesy" (G6.1, meetingorganizer.copernicus.org/EGU21/session/39897 Starting at 13:30. #vEGU21_G #vEGU21

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Interested in tides? Then join us in session OS4.1 "Tides in the past, present and future" (meetingorganizer.copernicus.org/EGU21/session/39711 at 11:45. #vEGU21_G #vEGU21_OS #vEGU21_HS #vEGU21_NH #vEGU21

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Recent advances in Geoid modelling techniques and results. Join us in session G1.5 "Local/Regional Geoid Determination: Methods and Models" (meetingorganizer.copernicus.org/EGU21/session/39915 11:45 - 12:30). #vEGU21_G #vEGU21

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Join us in session G1.4 where we look at data science and machine learning in #geodesy (meetingorganizer.copernicus.org/EGU21/session/39912 11:00–11:45) #vEGU21 #vEGU21_G

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How can #geodesy aid climate sciences? Join the #vEGU21 session G3.1: "Geodesy for Climate Research" co-organized by @EGU_Climate (meetingorganizer.copernicus.org/EGU21/session/39899 9:00 - 10:30). @IAG_climate #vEGU21_G

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The upside of a nighttime conference due to time zones is that I have the full day to do other things. The downside is that my brain is so tired but so caffeinated that I can’t work and can’t nap for the entire day. So all I can do is be on Twitter. #vEGU21

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What are drivers of coastal subsidence? Learn more in session GM6.5 "Coastal subsidence: Natural and anthropogenic drivers" (meetingorganizer.copernicus.org/EGU21/session/40295 starting at 14:15. #vEGU21_G #vEGU21_GM #vEGU21_NH #vEGU21

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@ania_klos. #vEGU21_G #vEGU21

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Do you want to meet the Geodesy Division Team? Then tomorrow between 14:30 and 15:30 (CEST) is your chance during our Pop-up networking event. Grab a coffee or tea and see you there. #vEGU21 #vEGU_G

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What's the math behind geodetic data sets? Find out in session G1.2 "Mathematical methods for the analysis of potential field data and geodetic time series" (meetingorganizer.copernicus.org/EGU21/session/39913 13:30 - 14:15) #vEGU21_G #vEGU21

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Why assessments of renewable energy potentials should be carefully used in welfare analysis frameworks is dicussed by @SebWehrle et al. Discuss with the authors
@EuroGeosciences
#vEGU21 on Friday. https://bit.ly/3eDW2ts

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#vEGU21_G #vEGU21

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Today our FREE #vEGU21 webinar:@icdpDrilling @ECORD_IODP 11:45-12:30 CEST. How to get involved in IODP and ICDP? https://bit.ly/3u04jOJ #scientificdrilling

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How can Geodesy help Seismology in identifying earthquake parameters? Check
out session G3.6 "Seismo-geodesy" co-organized by SM4 (meetingorganizer.copernicus.org/EGU21/session/39916 from 9:00 to 11:45 am. #vEGU21_G #vEGU21_SM #vEGU21

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Are there sufficient incentives to winterize Texan power system infrastructure? On average yes, but the low frequency of events makes investments risky say Katharina Gruber et al. Discuss with the authors
@EuroGeosciences #vEGU21 on Friday. https://bit.ly/3eDW2ts

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How can we improve the determination of satellite orbits? Learn more about recent advances in session G2.4 "Precise Orbit Determination for Geodesy and Earth Science" (meetingorganizer.copernicus.org/EGU21/session/39906 starting soon at 15:30. #vEGU21_G #vEGU21

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Two studies presented at #vEGU21 take a look at solar #campfires as seen by @ESASolarOrbiter’s @EuiTelescope. The tiny #flares are more frequent than larger ones and are caused by reconnection of magnetic field lines below: https://tinyurl.com/7xtnr33j @EuroGeosciences @AandA_journal

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