Eclipse photographs indicate that large regions of the inner solar corona are confined in various types of closed magnetic configurations and, as a result, do not participate in the general solar wind expansion. In this paper, the rotation of initially poloidal loop configurations of this type, as i
β¦ LIBER β¦
On the heating mechanism of magnetic flux loops in the solar atmosphere
β Scribed by M.T. Song; S.T. Wu
- Book ID
- 107936034
- Publisher
- Elsevier Science
- Year
- 1984
- Tongue
- English
- Weight
- 271 KB
- Volume
- 4
- Category
- Article
- ISSN
- 0273-1177
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