A model based on a self-similar magnetohydrodynamic (MHD) solution is presented which accounts for the dynamic behavior of the birth of an active region due to the emergence of magnetic flux. The constraints of this model are deduced from observations. Specifically, this self-similar MHD solution ex
The self-similar, non-linear evolution of rotating magnetic flux ropes
β Scribed by C. J. Farrugia; V. A. Osherovich; L. F. Burlaga
- Publisher
- Copernicus Group
- Year
- 1995
- Tongue
- English
- Weight
- 65 KB
- Volume
- 13
- Category
- Article
- ISSN
- 0992-7689
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