A model of the large-scale magnetic field structure above the photosphere uses a Green's function solution to Maxwell's equations. Sources for the magnetic field are related to the observed photospheric field and to the field computed at a 'source' surface about 0.6 R G above the photosphere. The la
โฆ LIBER โฆ
A coronal magnetic field model with horizontal volume and sheet currents
โ Scribed by Xuepu Zhao; J. Todd Hoeksema
- Publisher
- Springer
- Year
- 1994
- Tongue
- English
- Weight
- 805 KB
- Volume
- 151
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
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