Division on Solar-Terrestrial Sciences (ST)
The ST Division considers all aspects of solar and heliospheric physics, specifically the solar-terrestrial connection. It covers the physical processes occurring on the Sun, in the solar wind, as well as in Earth's magnetosphere and ionosphere. Solar activity (e.g. coronal mass ejections, solar flares, solar energetic particle events) and the response of the near-Earth space environment to these solar phenomena are studied on a wide-range of temporal and spatial scales. Data analysis and interpretation of space-borne and ground-based data, as well as theoretical studies and different modeling techniques are used to better our understanding of how our local star defines the neighborhood that we live in.
Current issue of the EGU newsletter
In just a couple of days, the meeting programme for the EGU 2017 General Assembly (23–28 April, Vienna) will be published online. If you have an abstract accepted to the meeting, you should receive your letter of schedule soon, too. Before then, make sure you enter the EGU Photo Competition (deadline 1 March) for a chance to win a free registration to next year's General Assembly.
For the first time, the EGU is offering a mentoring programme for novice conference attendees at its annual General Assembly to connect them with more experienced participants. The programme promises to be a rewarding experience for both mentees and mentors, so do consider signing up if you are either an early career scientist (ECS) or would like to mentor first timers!
For those interested in helping further the EGU outreach and ECS programmes, apply to be an ECS representative or be part of the EGU Outreach Committee. If you'd like to organise an EGU Galileo Conference, a meeting addressing a well-focused, cutting-edge topic at the frontier of geosciences research, this is your last chance to apply for funding from the EGU (deadline 28 February).
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