Soft X-ray variability over the present minimum of solar activity as observed by SphinX
Soft X-ray variability over the present minimum of solar activity as observed by SphinX
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DOI：
10.1134/s0038094611020055
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发表时间：
2011-04-01
影响因子：
0.9
通讯作者：
Kuzin, S.
中科院分区：
文献类型：
--
作者：
Gburek, S.;Siarkowski, M.;Kuzin, S.
太阳X射线光度计（SphinX）是一种用于观测太阳X射线的仪器，能量范围为0.85-15.00 keV。SphinX被纳入俄罗斯TESIS X和EUV望远镜复合体，搭载于2009年1月30日13：30 UT从俄罗斯北方普列谢茨克航天发射场发射的CORONAS-Photon卫星。自2009年2月以来，SphinX几乎一直在测量太阳X射线辐射。研究了SphinX的工作原理和仪器数据归档的内容。讨论了与SphinX校准、数据、储存库镜像位置、数据类型和元数据的传播有关的问题。使用SphinX在整个使命期间收集的数据研究了软X射线太阳通量的变化。
Solar Photometer in X-rays (SphinX) is an instrument designed to observe the Sun in X-rays in the energy range 0.85-15.00 keV. SphinX is incorporated within the Russian TESIS X and EUV telescope complex aboard the CORONAS-Photon satellite which was launched on January 30, 2009 at 13:30 UT from the Plesetsk Cosmodrome, northern Russia. Since February, 2009 SphinX has been measuring solar X-ray radiation nearly continuously. The principle of SphinX operation and the content of the instrument data archives is studied. Issues related to dissemination of SphinX calibration, data, repository mirrors locations, types of data and metadata are discussed. Variability of soft X-ray solar flux is studied using data collected by SphinX over entire mission duration.