The morphology and physical characteristics of the extended solar wind transsonic region, an intrinsically unique regime of the heliosphere, are described. It is here where the primary acceleration of the solar wind occurs and both subsonic and supersonic plasma flows co-exist and interact. This con
The investigation of the solar wind transsonic region at meter wavelengths
β Scribed by N. A. Lotova; Ya. V. Nagelys
- Publisher
- Springer
- Year
- 1988
- Tongue
- English
- Weight
- 381 KB
- Volume
- 117
- Category
- Article
- ISSN
- 0038-0938
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