Analysis of the small-scale cosmic ray fluctuations spectrum inferred from ground-based cosmic ray observation data

O. V. Gulinsky; L. I. Dorman; I. Ya. Libin; R. E. Prilutsky; K. F. Yudakhin; J. A. Otaola; V. Yu. Belashov; M. Steglik; J. Pérez-Peraza

doi:10.22201/igeof.00167169p.1988.27.1.1109

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Published: Jan 1, 1988

DOI: https://doi.org/10.22201/igeof.00167169p.1988.27.1.1109

Keywords:

Earth sciences geophysics cosmic rays magnetic field fluctuations spectral analysis

O. V. Gulinsky

Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Academy of Sciences of the USSR; Troitsk, Moscow Region 142092, USSR

L. I. Dorman

Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Academy of Sciences of the USSR; Troitsk, Moscow Region 142092, USSR

I. Ya. Libin

Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Academy of Sciences of the USSR; Troitsk, Moscow Region 142092, USSR

R. E. Prilutsky

Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Academy of Sciences of the USSR; Troitsk, Moscow Region 142092, USSR

K. F. Yudakhin

Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Academy of Sciences of the USSR; Troitsk, Moscow Region 142092, USSR

J. A. Otaola

Universidad Nacional Autónoma de México, Instituto de Geofísica, Ciudad Universitaria, Delegación Coyoacán, 04510, Mexico City, México

V. Yu. Belashov

Complex North-East Scientific Research Institute, Petropavlovsk-Kamchatsky, USSR

M. Steglik

Institute of Experimental Physics, Slovak Akademy of Sciences, Kosice, CZECHOSLOVAKIA

J. Pérez-Peraza

Instituto Nacionaide Astroflsica, Optica y Electr6nica, Tonantzintla, Puebla, MEXICO

Abstract

The relationships between the spectral characteristics of cosmic ray intensity and interplanetary magnetic field are studied theoretically using the spectral cosmic ray intensity characteristics inferred from ground-based observation data. The mean spectral characteristics of interplanetary magnetic field are calculated. The results of the calculations are compared with observational results. The results of analyzing the cosmic ray fluctuations during various periods and at various stations are described.

How to Cite

Gulinsky, O. V., Dorman, L. I., Libin, I. Y., Prilutsky, R. E., Yudakhin, K. F., Otaola, J. A., Belashov, V. Y., Steglik, M., & Pérez-Peraza, J. (1988). Analysis of the small-scale cosmic ray fluctuations spectrum inferred from ground-based cosmic ray observation data. Geofisica Internacional, 27(1), 3–36. https://doi.org/10.22201/igeof.00167169p.1988.27.1.1109

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Vol. 27 No. 1 (1988): January 1, 1988

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