A search for hard X-ray microflares near
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R. P. Lin; K. C. Hurley; D. M. Smith; R. M. Pelling
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Article
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1991
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Springer
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English
⚖ 435 KB
Near solar maximum, hard X-ray microflares with peak 20 keV fluxes of > 10-2 (cm 2 s keV)-1, more than ten times smaller than for typical flares and subflares, can occur at the rate of about once every five minutes. We report here on a search for hard X-ray microflares made on a long duration balloo