Image Details
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.
© 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.