The solution curves of the differential equations determining the behavior of the solar wind are calculated for the case where the heat flux has its maximum value ~ nkTv~h. All the supersonic solutions are asymptotically adiabatic, T~ r -4/3.
A note on the mass-loaded MHD flow of the solar wind towards a cometary nucleus
โ Scribed by K. R. Flammer; D. A. Mendis
- Publisher
- Springer Netherlands
- Year
- 1996
- Tongue
- English
- Weight
- 341 KB
- Volume
- 182
- Category
- Article
- ISSN
- 0004-640X
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