| Sumarry |
| 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 for Flares and CMEs with the kinetic aspects of particle acceleration and propagation. |
| 0:900-10:30 | Plenary
Session |
|
| 10:30-11:00 |
Coffee |
|
| 11:00-13:00 |
Discussion
on the goals of the group (L. Vlahos) What can we tell the theorists? (G. Emslie) On the Relation of the Coronal Source and the Footpoints (A. Benz) 2D electron spectroscopy on solar flares (E. Kontar) |
|
| 13:00-14:30 |
Lunch |
|
| 14:30-18:00 |
|
| 9:00-10:30 |
|
| 10:30-11:00 |
Coffee |
| 11:00-13:00 |
Electron
acceleration at the reconnection outflow shock by Mann, Warmuth, and Aurass Electron acceleration at DC electric fields in the corona by Oenel and Mann |
| 13:00-14:30 |
Lunch |
| 14:30-16:00 |
The
effect of tangential and guiding fields on particle acceleration in a
3D reconnecting current sheet (by Valentina
Zharkova) |
| 16:00-16:30 | Coffee |
| 16:30-18:00 |
Common session with WG 4 and 3: (i) tight correlation between spectral hardness and total flux(ii) the 'challenge' of the high electron fluxes implied by HXR intensities and the small footpoint sizes; implications for beam physics, return currents, electron number flux and resupply etc. |
| 9:00-10:300 |
Discussion special aspects on Magnetic topology, reconnection and acceleration and the predictions from theory (by Pascal Demoulin) |
| 10:30-11:00 |
Coffee |
| 11:00-13:00 |
Common session with WG-2: Constrains on theories of particle acceleration from Ion acceleration and Interaction |
| 12:30-14:00 |
Lunch |
| 14:30-16:00 |
Common
session with WG-1: observational and theoretical constraints on
particle acceleration mechanisms |
| 16:00-16:30 |
Coffee |
| Plenary session
Saturday April 8 |
Summary
(by L. Vlahos) |