The equilibrium positions of coronal currents are determined. It is shown that the fact that the photosphere has a very large inertia as compared to the corona, poses an important boundary condition at the surface. Electric currents flowing in a coronal active region show a tendency to concentrate a
The microwave structure of coronal condensations and its relation to proton flares
✍ Scribed by Haruo Tanaka; Shinzo Énomé
- Publisher
- Springer
- Year
- 1975
- Tongue
- English
- Weight
- 467 KB
- Volume
- 40
- Category
- Article
- ISSN
- 0038-0938
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