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Energy Partition in Two M-class Circular-ribbon Flares
Zhang, Q. M.; Cheng, J. X.; Feng, L.; Su, Y.; Lu, L.; Huang, Y.; Li, D.; Zhou, T. H.; Chen, J. L.
KeywordSun: flares Sun: magnetic fields Sun: UV radiation Sun: X-rays, gamma rays
AbstractIn this paper, we investigate the energy partition of two homologous M1.1 circular-ribbon flares (CRFs) in active region (AR) 12434. They were observed by SDO, GOES, and RHESSI on 2015 October 15 and 16, respectively. The peak thermal energy, nonthermal energy of flare-accelerated electrons, total radiative loss of hot plasma, and radiant energies in 1-8 angstrom and 1-70 angstrom of the flares are calculated. The two flares have similar energetics. The peak thermal energies are (1.94 +/- 0.13) x 10(30) erg. The nonthermal energies in flare-accelerated electrons are (3.9 +/- 0.7) x 10(30) erg. The radiative outputs of the flare loops in 1-70 angstrom, which are similar to 200 times greater than the outputs in 1-8 angstrom, account for similar to 62.5% of the peak thermal energies. The radiative losses of SXR-emitting plasma are one order of magnitude lower than the peak thermal energies. Therefore, the total heating requirements of flare loops including radiative loss are (2.1 +/- 0.1) x 10(30) erg, which could sufficiently be supplied by nonthermal electrons.
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Zhang, Q. M.,Cheng, J. X.,Feng, L.,et al. Energy Partition in Two M-class Circular-ribbon Flares[J]. ASTROPHYSICAL JOURNAL,2019,883(2):124.
APA Zhang, Q. M..,Cheng, J. X..,Feng, L..,Su, Y..,Lu, L..,...&Chen, J. L..(2019).Energy Partition in Two M-class Circular-ribbon Flares.ASTROPHYSICAL JOURNAL,883(2),124.
MLA Zhang, Q. M.,et al."Energy Partition in Two M-class Circular-ribbon Flares".ASTROPHYSICAL JOURNAL 883.2(2019):124.
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