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• W1984573520 abstract "We investigate an active region that produced three C-class flares and one M-class flare within 2.5 hr. The morphology and location of the C-flares indicate that these events constitute a set of homologous flares. Radio observations indicate the occurrence of a downward-moving plasmoid during the impulsive phase of the M flare. We use TRACE 1700 A filtergrams and SOHO Michelson Doppler Imager magnetograms to examine the character of the UV brightenings; i.e., we search for re-brightenings of former flare areas both across the series of events and within one and the same event. We find that essentially the same footpoints re-brighten in each C flare. Based on the progression of both the derived magnetic flux change rate and the observed Radio Solar Telescope Network microwave emission, we speculate about a further re-brightening during the decay phase of the M flare as a further member of the series of homologous flares. We conclude that the postflare field is driven to repeated eruption by continuous, shear-increasing, horizontal, photospheric flows, as one end of the involved magnetic arcade is anchored in the penumbra of a large sunspot. The observed motion pattern of the UV kernels indicates that the arcade evolves during the series of events from a both highly sheared and heavily entangled state to a still sheared but more organized state." @default.
• W1984573520 created "2016-06-24" @default.
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• W1984573520 date "2010-08-03" @default.
• W1984573520 modified "2023-09-23" @default.
• W1984573520 title "OBSERVATIONS OF CHROMOSPHERIC FLARE RE-BRIGHTENINGS" @default.
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• W1984573520 doi "https://doi.org/10.1088/0004-637x/719/2/1750" @default.
• W1984573520 hasPublicationYear "2010" @default.
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