Comparison of distribution of solar wind streams as a function of Bartels rotation days for two successive epochs indicates several significant differences, These are likely to be due to the differing nature of IMF and solar wind in the two solar cycles 20 and 21.
Preferred bartels days of high-speed plasma streams in the solar wind
β Scribed by B. A. Lindblad
- Publisher
- Springer
- Year
- 1981
- Tongue
- English
- Weight
- 406 KB
- Volume
- 74
- Category
- Article
- ISSN
- 0038-0938
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