The collisional equations for the solar wind assuming steady, spherically symmetric flow and including thermal conduction and an anisotropic proton temperature are analysed in the absence of a heat source function. The equations are cast in a form that involves one dimensionless parameter, effective
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Solar wind theory
β Scribed by S. Cuperman
- Publisher
- Springer Netherlands
- Year
- 1983
- Tongue
- English
- Weight
- 577 KB
- Volume
- 34
- Category
- Article
- ISSN
- 0038-6308
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