On the momentum and energy deposited by hydromagnetic waves in the solar wind
Journal Article
·
· J. Geophys. Res.; (United States)
The ratio of thernal energy to momentum (Q/D) deposited in the solar wind by hydromagnetic waves is determined primarily by the wind and Alfven speeds and by the rate of wave dissipation. When dissipation of Alfven waves dominates, then Q/D=2(V+A). This restricts models for the possible acceleration of the solar wind by hydromagnetic waves. It also affects the manner in which resonant cosmic rays can interact with the solar wind and the interstellar medium.
- Research Organization:
- Astronomy Program, University of Maryland, College Park, Maryland 20742
- OSTI ID:
- 7316899
- Journal Information:
- J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 82:4; ISSN JGREA
- Country of Publication:
- United States
- Language:
- English
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