... RADIOACTIVE LINE EMISSION FROM SOLARFLARES V. Tatischeff1 , B. Kozlovsky2, J ... INTRODUCTION Gamma-ray lines from solarflares were first observed in 1972 with the ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B38_Tatischeff01-14Feb07_12:46:42.pdf -- 67.8 Кб -- 14.02.2007 Похожие документы
... Studies of 7 strong SolarFlares (SF) give polarization levels between 2% and 50 ... to provide high resolution images and spectra from SolarFlares in X-rays and -rays ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/I33_Hajdas02-09May07_09:01:42.pdf -- 188.7 Кб -- 09.05.2007 Похожие документы
... by solar physical and geometric quantities, suggest that both flares studied here ... origin of high-energy emissions from solarflares, where a magnetic loop rising from ... loss of efficiency to the Ge detectors when detecting solarflare photons ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B37_Harris01-13Sep06_18:35:19.pdf -- 157.6 Кб -- 13.09.2006 Похожие документы
... Hajdas, RHESSI instrumental limits on measurements of linear photon polarization from GRBs, SGRs and SolarFlares [I] . ... Tatischeff, Delayed X- and gamma-ray line emission from Solarflare radioactivity [B] . ...
... нray lines, emitted by C and O nuclei at the energies of 4.438 MeV and 6.129 MeV, which have been detected in solarflares ... Before performing the analysis, the data are cleaned of solarflares and radiationнbelt passages. y y We performed a ...
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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
... 340, pre 0.08-0.11 Rev. 341, pre 0.22-0.24 No data due to a solarflare 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 solarflare. 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