Computer Science
Scientist
Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Division, Russian Academy of Sciences
Institute of Cosmophysical Research and Aeronomy, Siberian Branch, Russian Academy of Sciences
Akademiia Nauk SSSR, Institut Kosmofizicheskikh Issledovanii i Aeronomii, Yakutsk; Akademiia Nauk SSSR, Institut Kosmicheskikh Issledovanii, Moscow, USSR
Rossiiskaia Akademiia Nauk, Institut Kosmofizicheskikh Issledovanii i Aeronomii, Yakutsk, Russia
Akademiia Nauk SSSR, Institut Kosmofizicheskikh Issledovanii i Aeronomii, Yakutsk, USSR
Yu. G. Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch of the Russian Academy of Sciences
Institute of Cosmophysical Investigations and Aeronomy of the Siberian Branch of the Russian Academy of Sciences
Institute of Cosmophysical Research and Aeronomy, Russia
Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy, SB RAS, 677980 Yakutsk, Russia
Akademiia Nauk SSSR, Institut Kosmofizicheskikh Issledovanii i Aeronomii, Iakutsk, USSR
AN SSSR, Institut Kosmofizicheskikh Issledovanii i Aeronomii, Yakutsk; AN SSSR, Poliarnyi Geofizicheskii Institut, Murmansk, USSR
Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch, Russian Academy of Sciences
AN SSSR, Institut Kosmofizicheskikh Issledovanii i Aeronomii, Yakutsk, USSR
Akademiia Nauk SSSR, Institut Kosmofizicheskikh Issledovanii i Aeronomii, Yakutsk; Moskovskii Gosudarstvennyi Universitet; Akademiia Nauk SSSR, Fizicheskii Institut, Moscow, USSR
Shafer Institute of Cosmophysical Research and Aeronomy, Yakut Research Center, Siberian Branch, Russian Academy of Sciences
Yu. G. Shafer Institute of Cosmophysical Research and Aeronomy SB of RAS Lenin Ave., 31, 677980 Yakutsk, Russian Federation
A new index of solar activity: An index of cosmic ray scintillation
A Possible Mechanism of Localization of Fission Fragments from a High-Altitude Thermonuclear Explosion
A Year Later: Solar, Heliospheric, and Magnetospheric Disturbances in November 2004
Analysis of fluctuations and currents of galactic cosmic rays during the passage of high-velocity recurrent streams of the solar wind
Anisotropy of cosmic rays with extremely high energies
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