Large-scale cosmic ray fluctuations inferred from the ground-based neutron and ionizing component observations and their relevance to cosmic ray anisotropy

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Published: Apr 1, 1988
DOI: https://doi.org/10.22201/igeof.00167169p.1988.27.2.781
Keywords:
Cosmic rays, anisotropy, fluctuations

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O. V. Gulinsky
Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
L. I. Dorman
Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
N. S. Kaminer
Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
T. Lanina
Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
I. Ya. Libin
Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
N. V. Mymrina
Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
R. E. Prilutsky
Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
K. F. Yudakhin
Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
L. G. Chuvilgin
Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
K. Kudela
Institute of Geophysics of the Slovak Academy of Science, Kosice, CHECOSLOVAKIA
M. Steglik
Institute of Geophysics of the Slovak Academy of Science, Kosice, CHECOSLOVAKIA
J. A. Otaola
Universidad Nacional Autónoma de México, Instituto de Geofísica, Ciudad Universitaria, Delegación Coyoacán, 04510, Mexico City, México
J. Pérez Peraza
Instituto Nacional de Astronomía, Óptica y Electrónica, Puebla, MEXICO

Abstract

The work treats with the behaviour of the cosmic ray fluctuation power spectrum in the frequency range below 10-4Hz inferred from ground-based observations of the neutron and ionizing components. An attempt is made to describe the observed rearrangement of the fluctuation spectrum using changes in the value of the cosmic ray anisotropy and the rearrangement of the IMF inhomogeneity spectrum.

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How to Cite
Gulinsky, O. V., Dorman, L. I., Kaminer, N. S., Lanina, T., Libin, I. Y., Mymrina, N. V., … Pérez Peraza, J. (1988). Large-scale cosmic ray fluctuations inferred from the ground-based neutron and ionizing component observations and their relevance to cosmic ray anisotropy. Geofisica Internacional, 27(2), 167–190. https://doi.org/10.22201/igeof.00167169p.1988.27.2.781
Issue
Vol. 27 No. 2 (1988): April 1, 1988
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Article
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This work is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License.

Author Biographies

T. Lanina, Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.



K. Kudela, Institute of Geophysics of the Slovak Academy of Science, Kosice, CHECOSLOVAKIA



J. Pérez Peraza, Instituto Nacional de Astronomía, Óptica y Electrónica, Puebla, MEXICO



References

ANDERSEN, T., 1976. Statistical analysis of time series. Mir, Moscow.

BELOV, A. V. et al., 1973. Forbush-decreases in cosmic rays variations. Geomagn. i Aeron., 13, 339-342.

BEZRODNYKH, I. P. and V. A. KUZMIN, 1982. About the cosmic ray fluctuations near a sectorial boundary. In: Problems of scientific and technological research of the Yakutsk Division of the Siberian Branch of the Academy of Sciences of the USSR, Yakutsk, 17-19.

BEZRODNYKH, I. P., V. A. KUZMIN, V. I. KOZLOV, E. I. MOROZOVA and Yu. G. SHAFER, 1982. Dynamics of the frequency spectrum of the cosmic ray and IMF fluctuations. Geomagn. i. Aeron., 22, 6, 1016-1018.

BLOKH, Ya. L., I. Ya. LIBIN and K. F. YUDAKHIN, 1984. Cosmic ray fluctuations on the Earth during solar flares. Geomagn. i. Aeron., 24, 6, 875-878.

DORMAN, L. I. and I. Ya. LIBIN, 1985. Short-period cosmic ray intensity variations. Uspekhi Fiz. Nauk, 145, 3, 403-440. DOI: https://doi.org/10.3367/UFNr.0145.198503b.0403

DORMAN, L. I., I. Ya. LIBIN and K. F. YUDAKHIN, 1986. The role of anisotropy in the formation of statistically significant cosmic ray fluctuations. Geomagn. i. Aeron., 26, 1, 86-89.

DORMAN, L. I., N. S. KAMINER, A. E. KUZMICHEVA, I. Ya. LIBIN and N. V. MYMRINA, 1985. Cosmic ray variations relevant to the evolution of the parameters of a recurrent high-velocity solar wind flux. Geomagn. i Aeron., 25, 6, 1000-1002.

DORMAN, L. 1., K. KUDELA, S. F. NOSOV, M. STEGLIK and M. E. KATZ, 1983. Cosmic ray intensity fluctuations in the 10-6 - 10-4 Hz frequency band. Izv. Akad. Nauk SSSR, ser. phys., 47, 9, 1858-1860.

FILLISETTI, O., G. LOVERA and V. MUSSINO, 1982. Lett. Nuovo Cimento, 35, 10, 327-330. DOI: https://doi.org/10.1007/BF02754699

GULINSKY, O. V., L. I. DORMAN, I. Ya. LIBIN, R. E. PRILUTSKY and K. F. YUDAKHIN, 1985. Study of cosmic ray scintillations from 5-minute data of the scintillator telescope "IZMIRAN" and world-wide network stations. Proc. XIXth ICRC, La Jolla, U.S. A., 5, 281-284.

KEY, S. M. and S. L. MARPLE, 1981. Spectrum analysis - A modern perspective. TIIER, 69, 11, 5-48. DOI: https://doi.org/10.1109/PROC.1981.12184

KOZLOV, V. I., 1981 a. About the turbulence structure of the large-scale solar wind. Preprint, Moscow State University.

KOZLOV, V. L, 1981 b. Turbulent pulsations of magnetic field in shock waves. Geomagn. i Aeron., 21, 6, 1115-1117.

OWENS, A. J., 1974. Cosmic Ray Scintillations. J. Geophys. Res., 75, 2, 895-903. DOI: https://doi.org/10.1029/JA079i007p00895

SARI, J. V. and N. F. NESS, 1970. Acta Phys. Acad. Sci. Hungary, 29, 2, 373-378. DOI: https://doi.org/10.1007/BF03156945

SHAKHOV, B. A. and L. I. DORMAN, 1974. Anisotropy of cosmic ray variations. Izv. Acad. Nauk SSSR, ser. phys., 38, 9, 1885-1889.

TOLBA, M. F., M. A. POMERANTZ, S. P. DUGGAL and A. J. OWENS, 1981. Proc. XVIIth ICRC, Paris, France 4, 2, 52-55.

ZAVYALOV, Yu. S., B. I. KVASOV and V. L. MIROSHNICKENKO, 1980. Methods of spline-functions. Nauka, Moscow.