Working Groups
A majority of the time in this
workshop will be spent in working groups. Each working group is tasked to
address a broad question. These groups are organized by at least two people from
the solar and heliospheric community. Communication, event lists are provided by
the working group leaders
|
1.When, where and how are electrons accelerated and how do they
propagate into the heliosphere?
|
Dennis Haggerty, Sa"m Krucker | Working Group Description |
|
1.When, where and how are ions accelerated and how do they
propagate into the heliosphere?
|
Christina Cohen, Jim Miller | Working Group Description |
|
1.Do accelerated particles fit into the big picture?
The relationship between flare microphysics and global topological evolution. |
Loukas Vlahos, Dana Longcope, Nathan Schwadron | Working Group Description |
|
1.Flare
Structure, 3He and gamma rays.
|
Hugh Hudson, Mark Popecki Mark Wiedenbeck, Rick Leske, Gerry Share | |
|
1.What is the overall energy budget of a CME / flare event?
|
Gordon Emslie, Harald Kucharek | Working Group Description |