Heat transport in the solar wind
โ Scribed by E. V. Mishin
- Publisher
- Springer Netherlands
- Year
- 1974
- Tongue
- English
- Weight
- 767 KB
- Volume
- 27
- Category
- Article
- ISSN
- 0004-640X
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๐ SIMILAR VOLUMES
Proton heating at stream interaction regions in the solar wind is investigated based on the solar wind data obtained by Suisei spacecraft between 0.68 and 1.01 AU from the Sun. The deflection angle of the solar wind flow in the ecliptic plane is used to identify the interaction region. In the solar
The non-linear saturation of whistler mode instability in the solar wind is considered here. The resulting heating and acceleration are calculated. It is shown that this instability heats predominantly the a-particles and the ratio of heating rates of a-particles to ions have been calculated. This i