Fig. 7

Nominal, normalized AIA temperature response functions, with CDS enhancement factors (normalized to the largest value which occurs for Fe XIX) for four times during the M2.3 flare, including (1) the first peak of the first precursor at 17:45:56 UT (the top-most CDS curve in Fig. 6, but here not multiplied by 10), (2) the start of the impulsive increase of the Fe XIX emission at 18:08:24 UT, (3) the peak intensity of the cool, transition region emission lines at 18:10:32 UT, and (4) the peak intensity of the Fe XIX line observed by CDS at 18:15:18 UT (the maximum to which all of the CDS enhancements are normalized). The interval between exposures is 9.8 s.
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