ISCS WORKING GROUP 3 ON SOLAR EMISSIONS:
ORIGINS AND TRANSPORT THROUGH THE HELIOSPHERE
The main scientific objective of ISCS Working Group 3 is to study the
origins and transport of solar emissions through the heliosphere.
The emphasis of the group is
on observational and theoretical studies of dynamic activity in the mid to
outer corona and its influence on the solar wind.
WG3 has three subareas of study:
- Dynamic solar emissions in the increasing and maximum portion of solar cycle 23.
- Propagation in the interplanetary medium (coronal mass ejections,
interplanetary shocks, and energetic particles).
- Interaction of coronal mass ejections and solar wind streams
with Earth's magnetosphere.
Click on the following pages for information on Working Group 3:
For information on the activities of WG3 and how to participate, contact either
of the Coordinators:
George Simnett (UK)
E-mail: gms@star.sr.bham.ac.uk
Phone: 44-121-414-6469
David Webb (USA)
E-mail: webb@plh.af.mil
Phone: 1-781-377-3086
Last revised: September 13, 2001
