The extent to which the early phases of solar-flare development can be accounted for by a simple high-temperature chromospheric explosion model is investigated without involving a particular energy source. A model is developed in which it is shown that a point explosion in the lower chromosphere can
โฆ LIBER โฆ
Development dynamics of intense solar proton flares
โ Scribed by A. B. Struminsky; I. V. Zimovets
- Book ID
- 111437185
- Publisher
- Springer
- Year
- 2007
- Tongue
- English
- Weight
- 609 KB
- Volume
- 33
- Category
- Article
- ISSN
- 1063-7737
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