AMENDED RESULTS FOR HARD X-RAY EMISSION BY NON-THERMAL THICK TARGET RECOMBINATION IN SOLAR FLARES
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/824/i=2/a=90/pdf
Reference18 articles.
1. On the stopping of fast particles and on the creation of positive electrons
2. The deduction of energy spectra of non-thermal electrons in flares from the observed dynamic spectra of hard X-ray bursts
3. Non-thermal recombination – a neglected source of flare hard X-rays and fast electron diagnostic
4. FLARE HARD X-RAY SOURCES DOMINATED BY NONTHERMAL RECOMBINATION
5. Non-thermal recombination – a neglected source of flare hard X-rays and fast electron diagnostics(Corrigendum)
Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Understanding the Duration of Solar and Stellar Flares at Various Wavelengths;The Astrophysical Journal;2023-11-01
2. The Direct Relation between the Duration of Magnetic Reconnection and the Evolution ofGOESLight Curves in Solar Flares;The Astrophysical Journal;2017-12-05
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