A numerical method is developed for solving the force-free magnetic field equation, V โข B = aB, with spatially-varying c~. The boundary conditions required are the distribution of Bn (viz. normal component of the field on the photosphere) as well as the value of a in the region of positive (or negat
Magnetic stars with an external non-linear force-free field
โ Scribed by M. A. Raadu
- Publisher
- Springer Netherlands
- Year
- 1971
- Tongue
- English
- Weight
- 463 KB
- Volume
- 14
- Category
- Article
- ISSN
- 0004-640X
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