Theories of solar flares based on the storage of energy (usually as magnetic energy) in the solar atmosphere are shown to be incompatible with observational data. The sunspot energy deficit and the photospheric faculae both involve energy fluxes comparable with the flare requirement ( ~ 3 โข 1029 er
โฆ LIBER โฆ
A kinematic model of a solar flare
โ Scribed by Y. Nakagawa; S. T. Wu; S. M. Han
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 492 KB
- Volume
- 30
- Category
- Article
- ISSN
- 0038-0938
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