An impulsive solar X-ray burst in the energy range 90–400 keV |
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| Authors: | Y Fukada S Hayakawa I Kasahara F Makino I Suzuki Y Tanaka B V Sreekantan |
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| Institution: | (1) Dept. of Physics, Nagoya University, Nagoya, Japan;(2) Present address: Institute of Space and Aeronautical Science, University of Tokyo, Tokyo, Japan;(3) Tata Institute of Fundamental Research, Bombay, India |
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| Abstract: | A hard solar X-ray burst in the energy range 90–400 keV was observed at about 0528:30 UT on 13 April 1974. This event is peculiar in the sense that the X-ray flux is considerably high whereas the corresponding radio and optical flares are of moderate sizes, that the duration of the X-ray burst is very short, and that the X-ray peak is delayed by about 2.5 min relative to the first radio peak. |
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