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Monday evening’s Great Debate was definitely the place to be. Whether you were a PhD student, a professor, a research associate, a lecturer or, like me, a Postdoctoral researcher, this debate was here to raise awareness of the lack of permanent positions and the impact this has on a researcher’s career (and life!). As you may all know, getting a permanent position can sometimes feel like an ...[Read More]
It’s Thursday! Many European countries would actually have a holiday today with a long morning in bed or a nice stroll around nature, but what is there that’s better than spending this day at the EGU conference center?! To help you make the best out of this holiday, we’ll give you some highlights of the day to navigate around! We suggest you to start your day early, there are some great sessions o ...[Read More]
This Wednesday we are at exactly half time through the congress! Here are some tips for today as one looks forward to a wonderful day of learning and sharing. We start between 8.30 and 11.45 CEST immersing ourselves in the world of metamorphic minerals (session GMPV 7.2– Room D2 https://meetingorganizer.copernicus.org/EGU22/session/41922#Presentations) and geodynamic processes (session GD 6. ...[Read More]
This year for EGU22 we are very excited to be welcoming five fabulous people into our EGU Communications Team for the next month to help with social media, blogging and the press conferences. These interns and volunteers are going to be assisting EGU Media and Communications Officer Gillian D’Souza and Head of Communications Hazel Gibson, in the run up to, and during the General Assembly, so ...[Read More]
The Sun is an active radio emitter, it produces radio emissions in a wide frequency range from kHz to THz. The solar atmosphere has a complex distribution of magnetic field, plasma density, and temperature. These different properties of the solar atmosphere will result in different radio emission features at different frequencies. In principle, the plasma density decreases with the heliocentric di ...[Read More]
Tuesday, 24-05 GMPV folk, what did you think of the opening day of EGU GA 22? Exciting talks? Did you stopped by any of the ECS events or short-courses? After a kicking start yesterday evening, today session 9.4 continues in room D2 with plenty more on volcanic processes. There are several highlight talks that you should not dare to miss in the morning, and many more incredible talks. See which be ...[Read More]
The EGU community has always organised their own events, whether these are planned weeks to months in advance or spontaneously during the General Assembly. Since the advent of the EGU Pop-up Scheduler it’s now even easier to organise and plan your own event at the assembly. Many of the events are Division-specific, from picnics and dinners to networking sessions, so be sure to look and see w ...[Read More]
In the early 1970s, when Coronal mass ejections (CMEs), massive eruptions of magnetized solar plasma into interplanetary space, were first discovered, they were assumed to be always associated with the energetic solar phenomenon like solar flares, prominences, etc. With improved coronagraphic and multi-wavelength observational instruments, a class of CMEs emerging from the streamers was found and ...[Read More]
And, finally, here we go again, at EGU22!! After a long year, in person or virtually, we are sure will all attend amazing sessions. So here there is a quick guide for the first day of GMPV at EGU22, so you will not get lost! Let’s start in the morning with the geochemical and mineralogical study of the Oceanic Anoxic Event 2 in “Mass extinctions and major environmental changes througho ...[Read More]
This year at EGU22 we have a whole range of brilliant science-art activities, events and sessions taking place over the two weeks to entertain, educate and inspire you! From the special session on the Art-Science interface, EOS 1.2, the #ActualLivingScientist gallery, to show the diversity of people and research that makes up our community, to the vote for the EGU22 Photo Competition winners, and ...[Read More]
