| Sumarry |
| Group 5 will focus on the outline of 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 for Flares and CMEs with the kinetic aspects of particle acceleration and propagation. |
| 08:30-10:00 | Plenary
Session |
|
| 10:00-10:45 |
Coffee |
|
| 10:40-12:30 |
(a)
Discussion on the goals of the group (b) A short review on were we
stand on theories of particle acceleration (A.
Benz (tutorial)) A. Benz: Observational constrains for stochastic acceleration |
|
| 12:30-14:00 |
Lunch |
|
| 14:00-15:30 |
|
|
| 15:30-16:00 |
Coffee |
|
| 16:00-17:30 |
G.
Emslie:
Constrains on particle acceleration from the energy budget
of a flare M.
Onofri :
Particle acceleration in a turbulent electric field produced by 3D
reconnection |
|
| 19:00 |
Reception |
|
| 8:30-10:15 |
K. Azner: Acceleration in Force free corona with anomalous resistivity M. Aschwanden: Propagation and trapping of particles in RHESSI flares C. Dauphin-N. Vilmer: Simulations on Particle acceleration |
| 10:15-10:45 |
Coffee |
| 10:45-12:30 |
Common session with WG III: Constrains on theories of particle acceleration from the common analysis of Radio and Hard X-rays |
| 12:30-14:00 |
Lunch |
| 14:00-15:30 |
Special Topic Group Meeting |
| 15::30-16:00 |
Coffee |
| 16:00-17:30 |
Trip to IRSOL Solar
Telescop |