We consider proposed mechanisms for the formation of coronal holes, and identify as crucial the issue whether the holes are permeated by rigidly rotating fields. It is suggested that the interaction between such a field and the differentially rotating, diffusive solar envelope will produce a fore af
The importance of photospheric magnetic field complexity for coronal energy storage
โ Scribed by W. Tend
- Publisher
- Springer
- Year
- 1980
- Tongue
- English
- Weight
- 497 KB
- Volume
- 66
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
Possibilities for the storage of energy in coronal electric currents in different magnetic background field configurations are investigated in the framework of the solar flare energy build-up model of Van Tend and Kuperus (1978), The results are compared to characteristics of filaments and X-ray loops. Empirical flare predictors are interpreted theoretically.
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