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Study of cosmic ray motion in cosmic space near the earthData are presented on experimental installations developed in the cosmic ray variations laboratory in Kazgu (Alma-Ata). Various experiments on modelling the interaction of plasma with the geomagnetic field as well as the plasma distribution in quiet and disturbed fields are described. The characteristics of the meson supertelescope using scintillators (effective area, 10 sq m) for vertical alignments designed to study microvariations of the cosmic rays and their interrelation with magnetospheric fluctuations and the study of solar wind parameters are given.
Document ID
19750008423
Acquisition Source
Legacy CDMS
Document Type
Book
Authors
Budilov, V. K.
(Kanner (Leo) Associates Redwood City, CA, United States)
Ivanov, V. I.
(Kanner (Leo) Associates Redwood City, CA, United States)
Kozak, L. V.
(Kanner (Leo) Associates Redwood City, CA, United States)
Mirkin, L. A.
(Kanner (Leo) Associates Redwood City, CA, United States)
Tsukerman, I. G.
(Kanner (Leo) Associates Redwood City, CA, United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1975
Publication Information
Publication: Cosmic Rays (NASA-TT-F-807)
Subject Category
Space Radiation
Accession Number
75N16495
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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