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¦
The configuration of the loop-like structure of the solar atmosphere
β Scribed by Cheng Jiu-heng
- Publisher
- Elsevier Science
- Year
- 1992
- Tongue
- English
- Weight
- 468 KB
- Volume
- 16
- Category
- Article
- ISSN
- 0275-1062
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