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
Uralsk Pedagogical Inst.
Akademiia Nauk 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
AN SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok, USSR
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Leningrad, USSR
Joint Publications Research Service, Arlington, VA.
IZMIRAN, Troitsk, USSR
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok; Ural'skii Gosudarstvennyi Pedagogicheskii Institut, Uralsk, 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
Characteristics of Forbush decreases in recurrent high-velocity streams of the solar wind
Characteristics of Forbush effects in recurrent high-velocity streams of the solar wind.
Correlation of interplanetary medium parameters in transition region of high-velocity solar wind streams
Cosmic ray anisotropy relevant to high-velocity solar wind fluxes
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