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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. 7.

Left and middle: TRACE 1600 Å images of the X2.3 flare at ﹩t_{1}=15\thinspace{:}\thinspace 07\thinspace{:}\thinspace 34﹩ and ﹩t_{2}=15\thinspace{:}\thinspace 14\thinspace{:}\thinspace 21﹩. The dashed lines indicate the outer edge of the flare ribbons at each time. Right: MDI magnetogram of the same field of view. The dashed lines indicate the locations of the outer edges of the ribbons both at ﹩t=t_{1}﹩ and t2. The solid lines in the left panel indicate the length of the ribbon Lribbon for the east (left) and west (right) ribbons.

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