Physics
Scientist
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Troitsk, USSR
AN SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok; Ural'skii Gosudarstvennyi Pedagogicheskii Institut, Uralsk, USSR
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok, USSR
Uralsk Pedagogical Inst.
AN SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok, USSR
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok, USSR; Ural'skii Gosudarstvennyi Pedagogicheskii Institut, Uralsk, Kazakh SSR
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok; Gosudarstvennyi Komitet SSSR po Gidrometeorologii i Kontroliu Prikladnoi Sredy, Institut Prikladnoi Geofiziki, Moscow, USSR
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Krasnaya Pakhra, USSR
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Leningrad, USSR
Joint Publications Research Service, Arlington, VA.
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok; Ural'skii Gosudarstvennyi Pedagogicheskii Institut, Uralsk, USSR
IZMIRAN, Troitsk, USSR
AN USSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok; Institut Prikladnoi Geofiziki, Moscow, USSR
Ural'skii Pedagogicheskii Institut, Uralsk, Kazakh SSR; IZMIRAN, Troitsk, USSR
An estimate of the shape and delay of the interplanetary shock wave on the basis of cosmic ray increase prior to the Forbush decrease on December 13, 1966
Anisotropy and time-dependent changes in the spectrum of cosmic-ray intensity variations during August, 1972
Barometric Effect of the Neutron Component of Cosmic Rays in the Presence of a Background
Characteristics of Cosmic-Ray Variations near the Solar Equatorial Plane
Characteristics of Forbush decreases in recurrent high-velocity streams of the solar wind
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