Sumarry
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Group 5 will focus on
the constrains put forward by the analysis of the RHESSI data to the
models for particle acceleration. The second goal of this group is to
correlate the existing MHD models with the for Flares and CME with the
kinetic aspects of particle acceleration and propagation.
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Outline of topics to be
discussed
(to be updated soon)
- What are the requirements for the acceleration
mechanisms in the sun? This work will be accomplished in close
collaboration with the other Working Groups.
- A review/tutorial and discussion on the current
status of models for particle acceleration (Pros and Cons)
- Presentations on the current acceleration mechanisms.
- Are the current acceleration mechanisms compatible with
the energy release processes in flares?