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Spectroscopic Properties of Dynamical Chromospheric Processes in a Confined Solar Flare

✍ Scribed by H. Li; J. You; Q. Du


Publisher
Springer
Year
2006
Tongue
English
Weight
447 KB
Volume
235
Category
Article
ISSN
0038-0938

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Chromospheric heating by electron and pr
✍ A. Gordon Emslie πŸ“‚ Article πŸ“… 1983 πŸ› Springer 🌐 English βš– 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