An instability associated with the magnetosonic wave driven unstable due to coupling with electron and ion drift modes has been considered as a potential source for driving the hydromagnetic turbulence observed in Giacobini-Zinner (G-Z) Cometary plasma. The instability has good growth rate for propa
β¦ LIBER β¦
Hydromagnetic turbulence in computer simulations
β Scribed by A. Brandenburg; W. Dobler
- Book ID
- 108314043
- Publisher
- Elsevier Science
- Year
- 2002
- Tongue
- English
- Weight
- 130 KB
- Volume
- 147
- Category
- Article
- ISSN
- 0010-4655
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