Studies of coronal mass ejections and associated radio bursts with the cooperative observations of ground-based and spaceborne instruments
Abstract
The great achievement in solar-terrestrial physics, which the key solar phenomena responsible for interplanetary shocks, non-recurrent geomagnetic storms and large SEPs are caused by the coronal mass ejections (CMEs) instead of flares, is reviewed. The radio signatures of coronal mass ejections are described. The physical processes for the generation of radio bursts and energetic proton streams during the typical event 1991-06-15 CME are discussed in detail, and recent progress in studying the CMEs and associated radio bursts with cooperative observations of ground-based and spaceborne radiospectrograph is presented. Finally, some suggestions for future research works are proposed.
- Publication:
-
Progress in Astronomy
- Pub Date:
- September 2002
- Bibcode:
- 2002PABei..20..211L
- Keywords:
-
- Sun;
- CMEs;
- Radio Bursts;
- Shock Waves;
- Magnetic Reconnection;
- SEPs