File:Lc 15April2002 hsi ql.jpg
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RHESSI light curves for the flare on 15 April 2002. The color-coded curves are for the five indicated energy ranges. Counts from the front segments of all detectors except for detectors #2 and #7 were summed and divided by the summed live times and the total effective sensitive area of 35.59 cm2 per detector to give the plotted values with a 4 s cadence to match the spacecraft spin period. The thin attenuators were in place above all detectors limiting the useful energy range to > 6 keV. The blue shaded areas show the first of the three time intervals between 00:00 and 00:05 UT used here and by Guo et al. (2012a, b, 2013) to determine the source dimensions.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 22:00, 17 September 2018 | | 932×720 (299 KB) | Bdennis (Talk | contribs) | (RHESSI light curves for the flare on 15 April 2002. The color-coded curves are for the five indicated energy ranges. Counts from the front segments of all detectors except for detectors #2 and #7 were summed and divided by the summed live times and the t) |
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