Flares in Accretion Disks
Abstract
Present understanding of solar flares suggests that violent flare phenomena are common place in coronae of accretion disks. In particular near magnetized compact objects accretion can be modified by repeated magnetic energy storage and release. Further also in the absence of a central magnetosphere, such as around galactic and extragalactic black holes, magnetic flaring activity is possible in a corona on both sides of the disk.
- Publication:
-
Coronal Magnetic Energy Releases
- Pub Date:
- 1995
- DOI:
- 10.1007/3-540-59109-5_47
- Bibcode:
- 1995LNP...444..135K