European Geosciences Union

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Division on Solar-Terrestrial Sciences (ST)

President: Margit Haberreiter, st@egu.eu
Deputy President: Olga Malandraki, omaland@astro.noa.gr

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

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Last week (23–28 April), the EGU had the pleasure to host 14,500 participants at the EGU 2017 General Assembly in Vienna. This was a record-breaking meeting, with close to 17,500 oral, poster and PICO presentations, and over 1000 sessions and side events. For making the meeting a success, the EGU would like to thank all participants, as well as everyone involved in the organisation of the meeting: conveners, members of the EGU Programme Committee, Copernicus Meetings, conference assistants, and ACV and EGU office staff. A heartfelt thank-you goes to Gerrit de Rooij, the EGU Programme Committee Chair for the past three years, for his brilliant stewardship of the conference. Susanne Buiter, to whom we send a warm welcome, has now replaced Gerrit de Rooij as the chair of the Programme Committee.

As a participant, we especially welcome your suggestions and feedback, which will be instrumental to ensuring an even more successful General Assembly in 2018 (8–13 April, Vienna).

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