... 340, pre 0.08-0.11 Rev. 341, pre 0.22-0.24 No data due to a solar flare 14-20 keV ISGRI cts/s 20-35 keV 35-60 keV 5 0 60 40 20 ... All JEM-X data from revolution 341 are rejected because of a strong solar flare. 3. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G42_Klochkov01-05Feb07_15:40:11.pdf -- 173.0 Кб -- 05.02.2007 Похожие документы
... DIAGNOSTIC OF FLARING ACTIVITY WITH INTEGRAL The reduction of the mosaic image of the source generated for March 2003-November ... Our analysis showed the source to be detected by IBIS telescope up to energies 100 keV and to exhibit flaring activity. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G51_Seifina01-12Dec06_03:14:40.pdf -- 496.4 Кб -- 12.12.2006 Похожие документы
... This may indicate a continous cooling following an optical flare. ... energy-dependent time delays occur during the cooling off of a flare, e.g. higher-energy photons are emitted earlier than lower ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/D35_Collmar01-27Feb07_19:21:51.pdf -- 260.7 Кб -- 27.02.2007 Похожие документы
... нray lines, emitted by C and O nuclei at the energies of 4.438 MeV and 6.129 MeV, which have been detected in solar flares ... performing the analysis, the data are cleaned of solar flares and radiationнbelt passages. y y We performed a lightнbucket ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B32_Cordier01-26Feb07_18:49:16.pdf -- 246.3 Кб -- 26.02.2007 Похожие документы
... flares" have been observed (in sources like GRS 1915+105) at a few erg/s, such major flares would last a few days and recur several times a year; in addition, even more power can be found to be produced in microflare episodes that take place between the ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/A07_Guessoum01-27Mar07_20:34:54.pdf -- 162.4 Кб -- 27.03.2007 Похожие документы