Solar coronal non-thermal processes (Solar Maximum Mission)
Abstract
The Solar Maximum Mission was used to study solar coronal phenomena in hard X-radiation, since its instrument complement included the first solar hard X-ray telescope. Phenomena related to those discovered from OSO-5 and OSO-7 observations were emphasized.
- Publication:
-
California Univ., San Diego Report
- Pub Date:
- February 1983
- Bibcode:
- 1983ucsd.reptQ....H
- Keywords:
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- Photosphere;
- Solar Corona;
- X Ray Sources;
- Electron Transfer;
- Monte Carlo Method;
- Solar Maximum Mission;
- X Ray Telescopes;
- Solar Physics