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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. 4.

Left: Synthesized light curves. The solid and dashed lines are the light curves of the thick Al and Be filters, respectively. They must be multiplied by ﹩3.2\times 10^{16}﹩ to obtain the value in DN s−1 pixel−1 for the full resolution image. Right: Temporal variation of eth, the thermal energy per unit area derived by the SXT filter ratio method. The solid line is the least‐squares fitting of the impulsive phase.

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