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• W3100344891 abstract "We report on the formation of small solar flares produced by patchy magnetic reconnection between interacting magnetic loops. A three-dimensional (3D) magnetohydrodynamic (MHD) numerical experiment was performed, where a uniform magnetic flux sheet was injected into a fully developed convective layer. The gradual emergence of the field into the solar atmosphere results in a network of magnetic loops, which interact dynamically forming current layers at their interfaces. The formation and ejection of plasmoids out of the current layers leads to patchy reconnection and the spontaneous formation of several small (size ? 1-2Mm) flares. We find that these flares are short-lived (30 s - 3 min) bursts of energy in the range O(10^25 - 10^27) ergs, which is basically the nanoflare-microflare range. Their persistent formation and co-operative action and evolution leads to recurrent emission of fast EUV/X-ray jets and considerable plasma heating in the active corona." @default.
• W3100344891 created "2020-11-23" @default.
• W3100344891 creator A5037450222 @default.
• W3100344891 creator A5056231060 @default.
• W3100344891 date "2014-05-20" @default.
• W3100344891 modified "2023-10-15" @default.
• W3100344891 title "CLUSTERS OF SMALL ERUPTIVE FLARES PRODUCED BY MAGNETIC RECONNECTION IN THE SUN" @default.
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• W3100344891 doi "https://doi.org/10.1088/2041-8205/788/1/l2" @default.
• W3100344891 hasPublicationYear "2014" @default.
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