| タイトル | Temporal evolution of an energetic electron population in an inhomogeneous medium: Application to solar hard X-ray bursts |
| 本文（外部サイト） | http://hdl.handle.net/2060/19850026428 |
| 著者（英） | Trottet, G.; Mackinnon, A. L.; Vilmer, N. |
| 著者所属（英） | Observatoire de Paris-Meudon |
| 発行日 | 1985-08-01 |
| 言語 | eng |
| 内容記述 | Energetic electrons accelerated during solar flares can be studied through the hard X-ray emission they produce when interacting with the solar ambient atmosphere. In the case of the non thermal hard X-ray emission, the instanteous X-ray flux emitted at one point of the atmosphere is related to the instantaneous fast electron spectrum at that point. A hard X-ray source model then requires the understanding of the evolution in space and time of the fast particle distribution. The physical processes involved here are energy losses due to Coulomb collisions and pitch angle scattering due to both collisions and magnetic field gradients. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 85N34741
SH-1.2-6 |
| 権利 | No Copyright |
