It was shown by Zheleznyakov and Zlotnik (1980a, b) that in complex configurations of solar magnetic fields (in hot loops above the active centres, in neutral current sheets in the preflare phase, in hot X-ray kernels in the initial flare phase) a system of cyclotron lines in the spectrum of microwa
Solar flare activity and the structure of the coronal neutral line
β Scribed by G. A. Stewart; S. Bravo
- Publisher
- Springer
- Year
- 1995
- Tongue
- English
- Weight
- 851 KB
- Volume
- 160
- Category
- Article
- ISSN
- 0038-0938
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