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JOURNALS // Uspekhi Fizicheskikh Nauk // Archive

UFN, 1985 Volume 145, Number 3, Pages 403–440 (Mi ufn8276)

This article is cited in 14 papers

REVIEWS OF TOPICAL PROBLEMS

Short-period variations in cosmic-ray intensity

L. I. Dorman, I. Ya. Libin

Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences, Troitsk, Moskovskaya obl.

Abstract: The origin and propagation mechanisms of fluctuations in the cosmic rays observed by instruments on the ground, in the stratosphere, and in space are discussed. Recent experimental results on fluctuations at frequencies from 10$^{-3}$ to 10$^{-6}$ Hz are discussed. The primary cause of the statistically significant fluctuations in the cosmic rays is the scattering of charged particles of the cosmic rays by random inhomogeneities of the interplanetary magnetic field.

UDC: 524.1 + 537.591.5

PACS: 98.70.Sa, 96.50.sh, 96.50.Bh, 96.50.Ci, 96.60.Vg

DOI: 10.3367/UFNr.0145.198503b.0403


 English version:
Physics–Uspekhi, 1985, 28:3, 233–256


© Steklov Math. Inst. of RAS, 2026