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Identification of two X-ray miniflares with Hα-subflares
Authors:A Schadee  V Gaizauskas
Institution:1. Laboratory for Space Research, Beneluxlaan 21, 3527 HS Utrecht, The Netherlands;7. Herzberg Institute of Astrophysics, National Research Council of Canada, Ottawa, Canada K1A 0R6
Abstract:Active regions show many short-lived emissions in the 3.5 – 5.5 keV range that are 100 to 1000 times weaker than “normal” X-ray flares. The hypothesis that they may well be miniflares is supported by the simultaneous occurrence of 2 Hα-subflares at the site of weak X-ray sources.
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