Impulsive heating of the upper chromosphere by a very powerful thermal flux is studied as the cause of hard X-rays during a solar flare. The electron temperature at the boundary between the corona and chromosphere is assumed to change in accordance with the hard X-ray intensity in an elementary flar
Hydrodynamic response of the solar chromosphere to an elementary flare burst
β Scribed by B. V. Somov; S. I. Syrovatskii; A. R. Spektor
- Publisher
- Springer
- Year
- 1981
- Tongue
- English
- Weight
- 470 KB
- Volume
- 73
- Category
- Article
- ISSN
- 0038-0938
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