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About Factors of Solar Radiation Affecting the Ionosphere

Published online by Cambridge University Press:  24 July 2018

Aleksander V. Rakhlin
Affiliation:
Radiophysical Research Institute, National Lobachevsky State University, 25/12A Bol’shaya Pecherskaya str., 603950, Nizhny Novgorod, Russian Federation email: rakhlin.alex@nirfi.unn.ru
Olga A. Sheiner
Affiliation:
Radiophysical Research Institute, National Lobachevsky State University, 25/12A Bol’shaya Pecherskaya str., 603950, Nizhny Novgorod, Russian Federation email: rakhlin.alex@nirfi.unn.ru
Feodor I. Vybornov
Affiliation:
Radiophysical Research Institute, National Lobachevsky State University, 25/12A Bol’shaya Pecherskaya str., 603950, Nizhny Novgorod, Russian Federation email: rakhlin.alex@nirfi.unn.ru
Aleksander V. Pershin
Affiliation:
Radiophysical Research Institute, National Lobachevsky State University, 25/12A Bol’shaya Pecherskaya str., 603950, Nizhny Novgorod, Russian Federation email: rakhlin.alex@nirfi.unn.ru
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Abstract

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In this report we present an attempt to find a characteristic set of the space weather parameters allowed to identify the dominant physical connections. This study is based on the data of vertical and oblique sounding of the ionosphere in 2015-2016.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Sheiner, O. A., Fridman, V. M., Krupenya, N. D., Mityakova, E. E. & Rakhlin, A. V. 2002, in: Huguette Sawaya-Lacoste (ed.), Second Solar Cycle and Space Weather, Proc. Euroconference ESA SP-477 (Vico Equense: ESA), p. 479Google Scholar
Uryadov, V. P., Vybornov, F. I., Kolchev, A. A., Shumaev, V. V., Chernov, A. G. & Egoshin, A. I., 2016, Radiophysics & Quantum Electronics, 59, 431Google Scholar