A basic procedure is presented for dealing with the resonance problems that appear in MHD of which resonant absorption of waves at the Alfv~n resonance point is the best known example in solar physics. The procedure avoids solving the full fourth-order differential equation of dissipative MHD by usi
Resonant interactions of modes in coronal magnetic flux tubes
β Scribed by V. M. Nakariakov; V. N. Oraevsky
- Publisher
- Springer
- Year
- 1995
- Tongue
- English
- Weight
- 685 KB
- Volume
- 160
- Category
- Article
- ISSN
- 0038-0938
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