We evaluate the possibility that the short-lived Balmer line emission at H9 A3835 A. of the 1972, August 2 (1839 UT) solar flare is due to heating of the chromosphere by bombarding electrons. We point out some of the problems of comparing the time behavior and spatial distribution of simultaneous ha
Laboratory-produced radiation related to the solar flare emission
β Scribed by R. C. Elton; T. N. Lie
- Book ID
- 104667717
- Publisher
- Springer Netherlands
- Year
- 1972
- Tongue
- English
- Weight
- 697 KB
- Volume
- 13
- Category
- Article
- ISSN
- 0038-6308
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