File:149f2.png: Difference between revisions

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(Time series of counts at 50-100 keV (gold) and at 2200-2250 keV (red), the latter a crude indication of the presence or absence of gamma-rays. In this case, despite the X classification of the flare, there were no detectable gamma rays and only a weak 50-)
 
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Time series of counts at 50-100 keV (gold) and at 2200-2250 keV (red), the latter a crude indication of the presence or absence of gamma-rays. In this case, despite the X classification of the flare, there were no detectable gamma rays and only a weak 50-100 keV hard X-ray signature.
Time series of counts at 100 keV (blue), 200 keV (gold) and at 2200-2250 keV (red), the latter a crude indication of the presence or absence of gamma-rays. In this case, despite the X classification of the flare, there were no detectable gamma rays and only a weak hard X-ray signature
with a relatively steep spectrum.

Revision as of 11:39, 12 April 2011

Time series of counts at 100 keV (blue), 200 keV (gold) and at 2200-2250 keV (red), the latter a crude indication of the presence or absence of gamma-rays. In this case, despite the X classification of the flare, there were no detectable gamma rays and only a weak hard X-ray signature with a relatively steep spectrum.

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