We present here a model, based on observations, for the magnetic-field equilibrium of a cool coronal loop. The pressure structure, taken from the Harvard/Skylab EUV data, is used to modify the usual force-free-field form in quasi-cylindrical symmetry. The resulting field, which has the same directio
โฆ LIBER โฆ
The structure of coronal magnetic loops
โ Scribed by Riccardo Giachetti; Gerard Hoven; Claudio Chiuderi
- Publisher
- Springer
- Year
- 1977
- Tongue
- English
- Weight
- 846 KB
- Volume
- 55
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
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