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A substorm-associated enhancement in the XUV radiation measuring channel observed by ESP/EVE/SDO
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作者 Yan Yan hua-ningwang +1 位作者 Chao Shen Zhan-Le Du 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2016年第6期21-28,共8页
Comparing the ESP/EVE/SDO flux data of 2011 Feb 6, with the counterparts of XRS/GOES and SEM/SOHO, we find that there is an enhancement that is not apparent in the two latter datasets. The enhancement, possibly regard... Comparing the ESP/EVE/SDO flux data of 2011 Feb 6, with the counterparts of XRS/GOES and SEM/SOHO, we find that there is an enhancement that is not apparent in the two latter datasets. The enhancement, possibly regarded as a flare at first glimpse, nevertheless, does not involve an energy-release from the Sun. Based on the enhancement, we combine data from SXI/GOES 15 into a synthesized analysis, and concluded that it arises from a particle-associated enhancement in the channel that measures XUV radiation. Paradoxically, it seems to be somewhat of a particle-avalanching process. Prior to the event, a moderate geomagnetic storm took place. Subsequently, while the event is proceeding, a geomagnetic substorm is simultaneously observed. Therefore, the particles, though unidentified, are probably energetic electrons induced by substorm injection. 展开更多
关键词 Sun: X-rays gamma rays -- Sun: flares -- Sun: solar-terrestrial relations
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