Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993acaps..12..374z&link_type=abstract
Chinese Astronomy and Astrophysics (ISSN 0275-1062) Transl. of Acta Astrophysica Sinica, vol. 12, no. 4, 1992, p. 374-377., vol.
Astronomy and Astrophysics
Astrophysics
Solar Flares, Solar Radio Bursts, Solar X-Rays, Sunspots, Astronomical Observatories, Emission Spectra, Solar Magnetic Field
Scientific paper
A solar white-light flare (WLF) was observed at the Beijing Astronomical Observatory in AR6659 on June 6, 1991. The white light emission was accompanied by intense H-alpha, X-ray, and microwave emissions. We studied this event and estimated the total power emitted by the WLF knots in the wavelength band of the observation (between 3590 and 3610A) to be P = 4.96 x 10 exp 25 ergs. The energy of the WLF on 3600 A is estimated to be E(3600 A) = 7.54 x 10 exp 28 erg. The estimated energy of WLF in the whole optical wavelength range (3590 - 6391 A) is E = 1.21 x 10 exp 31 erg.
Shen Long-Xiang
Zhu Cui-Lian
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