For much of May and June, XRT was experimenting with a new observing
program for flares that used a rapid
succession of long and short exposure pairs. Such pairs,
regularly used during XRT's
synoptic
observations, allow us to simultaneously see bright and
faint structures by replacing saturated pixels in the long exposure
with unsaturated data from the short exposure. You'll notice
the extended "diamond" shapes surrounding the flare cores, which are
due to an
artifact known as CCD
blooming,
whereby saturation in the long exposure spills out into
adjacent pixels. The linked movie shows all of the over 20 flare responses to use
this program, which includes some 17 C- and 5 M-flares, most of which
coming from Active Region
11476 between the 7th and 14th of May.
[Filters: Ti Poly]
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