Variations in solar shortwave radiation in the solar activity cycle as measured by the <Emphasis Type="Italic">CORONAS</Emphasis> satellites |
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Authors: | T V Kazachevskaya A A Nusinov V V Katyushina D A Gonjyukh |
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Institution: | (1) Institute of Applied Geophysics, Rostokinskaya ul. 9, Moscow, 129128, Russia;(2) Central Design Office of Hydrometeorological Instrument Production, Koroleva ul. 6, Obninsk, Kaluzhskaya oblast, 249039, Russia |
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Abstract: | The CORONAS-I and CORONAS-F data on variations in the ionizing shortwave ultraviolet (UV) solar radiation (EUV radiation) at wavelengths of less than 130 nm and near the H Lyman-alpha line are presented. The CORONAS-I data refer to the period close to solar minimum (the index F 10.7 = 80?100), and the CORONAS-F measurements were held close to solar maximum (F10.7 = 140?280). The UV data are compared to those from the UARS and SOHO satellites and to the results obtained from the ionospheric measurements of ionosphere critical frequencies. |
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Keywords: | PACS Nos" target="_blank">PACS Nos 96 60 Ub |
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