Division E Sun and Heliosphere


Yihua YAN

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

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

Last updated:
September 29, 2015


Sarah Gibson

p.o. box 3000
Boulder 80301-3000
United States

Phone: +1 303 497 1587
Fax: +1 303 497 1589
Email: sgibsonucaredu

Last updated:
September 29, 2015


Marc L DeRosa

Lockheed Martin Solar and Astrophysics Laboratory
3251 Hanover St. B/252
Palo Alto 94304
United States

Phone: +1 650-354-5238
Fax: +1 650-424-3994
Email: derosalmsalcom
Personal website: http://www.lmsal.com/~derosa
Organization website: http://www.lmsal.com

Last updated:
October 5, 2015


Lidia van Driel-Gesztelyi

University College
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:
September 22, 2015

Steering Committee


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 (1283)

Participating Commissions

Division E Commission E1 Solar Radiation and Structure
Division E Commission E2 Solar Activity
Division E Commission E3 Solar Impact throughout the Heliosphere

Division Working Groups

Division E WG Impact of Magnetic Activity on Solar and Stellar Environments

Inter-Division Working Groups

Inter-Division B-E WG Coordination of Synoptic Observations of the Sun
Inter-Division C-E WG Solar Eclipses

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