Variations in solar shortwave radiation in the solar activity cycle as measured by the CORONAS satellites

Details Variations in solar shortwave radiation in the solar activity cycle as measured by the CORONAS satellites Variations in solar shortwave radiation in the solar activity cycle as measured by the CORONAS satellites

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sosyr..42..359k&link_type=abstract

Solar System Research, Volume 42, Issue 4, pp.359-362

Computer Science

96.60.Ub

Scientific paper

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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