Fig. 2.
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Observational results measured from MSS-1B/SXDU. Panel a: SXR spectrum integrated over one minute during the C2.8 flare in the range 1−10 Å. The magenta and cyan curves represent the Gaussian fitting results for the Fe and Ca lines, respectively. Panels b and c: Time series of the fitting peak and center for Fe (circular) and Ca (diamond) lines.
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