Computer Science
Scientist
Gor'kovskii Gosudarstvennyi Universitet, Gorki, USSR
Akademiia Nauk SSSR, Sibirskii Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Irkutsk, USSR
Institute of Solar-Terrestrial Physics, Russian Academy of Sciences, P.O. Box 4026, 664033 Irkutsk, Russian Federation
AN SSSR, Sibirskii Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Irkutsk, USSR
AN SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Irkutsk, USSR
Academy of Sciences, Irkutsk, Russia
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma Ionosfery i Rasprostraneniia Radiovoln, Irkutsk, USSR
RAS
Institute of Solar-Terrestrial Physics, Russian Academy of Science, Irkutsk, Russian Federation
Institute of Solar Terrestrial Physics, Russia Acdemy of Sciences, Lermontov St. 126, Irkutsk, 664033 Russian Federation of Solar-Terrestrial Physics, Irkutsk, Russia
Institute of Solar-Terrestrial Physics, Russian Academy of Sciences, Irkutsk, Russia
Department of Chemistry, University of Maryland, College Park, Maryland, 20742-2021
Institute of Solar-Terrestrial Physics, Russian Academy of Sciences, Siberian Branch
Accelerated motions of the magnetopause as a trigger of the Kelvin-Helmholtz instability
Active phase of a substorm as a chain of two types of reconnection: In the closed plasma sheet and in the open tail lobes
Events of August 2, 2002: Features of substorm field-aligned currents
Geomagnetic signatures of current wedge produced by fast flows in a plasma sheet
Hydromagnetic pulsations in the magnetosphere and the Kelvin-Helmholtz instability
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