Electron acceleration in solar flares: observations versus numerical simulations
Abstract
We use RHESSI hard X-ray observations to constrain acceleration of solar flare electrons, generally considered to be a primary recipient of the released energy.
- Publication:
-
Highlights of Astronomy
- Pub Date:
- August 2007
- DOI:
- 10.1017/S1743921307009908
- Bibcode:
- 2007HiA....14...87B