Computer Science – Sound
Scientific paper
Sep 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983izssr..47.1822e&link_type=abstract
(Seminar po Solnechnoi Aktivnosti i Solnechnym Kosmicheskim Lucham, Leningrad, USSR, Nov. 1982) Akademiia Nauk SSSR, Izvestiia,
Computer Science
Sound
Cosmic Rays, Magnetic Field Inversions, Particle Flux Density, Solar Magnetic Field, Atmospheric Sounding, Periodic Variations, Solar Activity Effects, Solar Cycles, Solar Terrestrial Interactions, Stratosphere
Scientific paper
Experimental data on cosmic-ray intensity were acquired at various atmospheric heights above Alma-Ata during 1962-1982. A 22-year wave was found in the relative change of the temporal course of cosmic-ray intensity at heights not below 320 g/sq cm, and the energy spectrum of the variations of this wave was found to have a positive index. From the standpoint of modulation effects, the presence of drift motions is shown to lead to a change (compared to the traditional modulated spectrum) of the modulated spectrum of cosmic rays in a definite energy range, this change depending on the sign of the solar magnetic field. This effect is most distinct in two successive minima of solar activity (e.g., 1965 and 1975).
Erkhov V. I.
Kolomeets E. V.
Likhoded V. A.
Stekolnikov N. V.
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