The formation of shocks and shock heating by radiatively damped longitudinal waves in solar magnetic flux tubes of different filling factors is studied. We consider three flux tubes of filling factors: 1%, 20%, and exponentially spreading which represent normal, enhanced network regions and the inte
Longitudinal flows in stellar magnetic flux tubes
β Scribed by M.H. Gokhale; K.M. Hiremath
- Publisher
- Elsevier Science
- Year
- 1986
- Tongue
- English
- Weight
- 185 KB
- Volume
- 6
- Category
- Article
- ISSN
- 0273-1177
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