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Temporal evolution of the chromospheric electron density in the flare of January 5, 1992

✍ Scribed by E. Rolli; A. Magun


Publisher
Springer
Year
1995
Tongue
English
Weight
660 KB
Volume
160
Category
Article
ISSN
0038-0938

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Chromospheric heating by electron and pr
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Using observations of both hard X-rays and y-rays in the large solar flare on June 7, 1980, we infer the amount of chromospheric heating due to bombardment both by non-thermal electrons and by protons, respectively. If a thick-target model for the X-ray bremsstrahlung is adopted, then proton heating