Coronal Propagation of Solar Flare Particles Observed by Geostationary Satellite
Abstract
Propagation of solar flare particles in corona was studied using the satellite data at the geostationary orbit. by selecting very fast rise time events only, the interplanetary propagation were assumed to be scatter free arrival. The results show that the propagation in corona does not depend on particle energy in 4 to 500 MeV protons, and the time delays from optical flare do not depend on the distance between the flare site and the base of the interplanetary magnetic field which connects to the Earth.
- Publication:
-
19th International Cosmic Ray Conference (ICRC19), Volume 4
- Pub Date:
- August 1985
- Bibcode:
- 1985ICRC....4..301K
- Keywords:
-
- Particle Diffusion;
- Solar Corona;
- Solar Cosmic Rays;
- Solar Flares;
- Interplanetary Magnetic Fields;
- Interplanetary Medium;
- Interplanetary Space;
- Models;
- Scattering;
- Solar Physics