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Measurement of the Energy Release Rate and the Reconnection Rate in Solar Flares

  • Authors: Hiroaki Isobe, Hiroyuki Takasaki, and Kazunari Shibata

Isobe, Takasaki, & Shibata 2005 The Astrophysical Journal 632 1184.

  • Provider: AAS Journals

Caption: Fig. 6.

Left: SXT image of the X2.3 flare on 2000 November 24. The image is negative. The solid lines indicate Lx (shorter line) and Ly (longer line) measured by eyes. Middle: Light curves of the Al 12 filter images (solid line) and Be filter images (dotted line). Right: Temporal variation of thermal energy Eth. The solid line indicates the least‐squares fitting of the impulsive phase, which yields ﹩dE_{\mathrm{th}\,}/ dt=1.6\times 10^{28}﹩ ergs s−1.

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