Chromospheric heating by electron and pr
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A. Gordon Emslie
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Article
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1983
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Springer
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English
โ 370 KB
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