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
Magnetic clouds and interplanetary particle transport: a numerical model
โ Scribed by May-Britt Kallenrode
- Book ID
- 104407429
- Publisher
- Elsevier Science
- Year
- 2002
- Tongue
- English
- Weight
- 148 KB
- Volume
- 64
- Category
- Article
- ISSN
- 1364-6826
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