Division E Sun and Heliosphere

President

Lidia van Driel-Gesztelyi

MSSL
University College
London
United Kingdom

Phone: +44 1483 204906
Fax: +44 1483 278312
Email 1: LidiavanDrielobspmfr
Email 2: lvdgmssluclacuk
Personal website: http://www.mssl.ucl.ac.uk:/~lvdg/
Organization website: http://www.ucl.ac.uk/mssl

Last updated:
December 9, 2012

Vice-President

Yihua YAN

National Astronomical Observatories
20A Datun Rd
Chaoyang District
Beijing 100012
China PR

Phone: +86 10 6485 1674
Fax: +86 10 6486 3314
Email: yyhnaocascn
Organization website: http://www.bao.ac.cn/english/home.asp

Last updated:
February 26, 2013

Steering Committee

Secretary

Gianna Cauzzi

INAF
Osservatorio Astrofisico di Arcetri
Largo E Fermi 5
50125 Firenze
Italy

Phone: +39 055 275 2260
Fax: +39 055 220 039
Email 1: gcauzziarcetriastroit
Email 2: gcauzzigmailcom
Organization website: http://www.arcetri.astro.it/

Last updated:
October 4, 2013


Description

Division E provides a forum for astronomers (observers, theoreticians, modelers and instrumentalists) studying a wide range of phenomena related to the structure, radiation and activity of the Sun, the dynamic magnetized solar wind that shapes the heliosphere, and their combined impact on the multitude of bodies within the solar system, including the Earth. The branches of astrophysics within the realm of Division E start from the uniquely detailed study of a dynamic stellar interior enabled by helioseismology, and the unrivaled access to a functioning astrophysical dynamo. Studies of the solar interior, long-term irradiance changes and the dynamic atmospheric structure are directly coupled to the cyclic generation/amplification of magnetic fields and the solar cycle, which are intrinsically related to activity, i.e. transient, phenomena. Studies of transient aspects of the Sun include those of flares, eruptions, coronal mass ejections, particle acceleration, all occurring within the context of a more gradually evolving background atmosphere, which together shape the entirety of the heliosphere. Within the context of the heliosphere, Division E focuses on understanding the solar wind, the interplanetary magnetic field, and their transients, shocks and energetic particles, as well as the space weather phenomena that all of these processes drive around the bodies throughout the heliosphere, including, of course, Earth. The long-standing Division Task Group on Eclipses reaches out to professionals, amateurs and the public in general by providing information on, and facilitating involvement in eclipse research.


Division Members (1166)


Participating Commissions

Division E Commission 10 Solar Activity
Division E Commission 12 Solar Radiation & Structure
Division E Commission 49 Interplanetary Plasma & Heliosphere

Division Working Groups

Division E WG International Collaboration on Space Weather
Division E WG International Data Access
Division E WG Solar Eclipses

Inter-Division Working Groups

Inter-Division E-F WG Impact of Magnetic Activity on Solar and Stellar Environments
Inter-Division E-G WG Solar-Type Stars

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