Known potential field solutions can be used to model the structure of magnetic fields in the solar photosphere. Several two-dimensional and axisymmetric solutions are compared. In the most satisfactory model the vertical component of the field is prescribed on a horizontal plane so as to be uniform
Magnetic field lines for a flux tube
โ Scribed by C. D. C. Steele; Rekha Jain
- Publisher
- Springer
- Year
- 1993
- Tongue
- English
- Weight
- 350 KB
- Volume
- 145
- Category
- Article
- ISSN
- 0038-0938
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