Analysis of the small-scale cosmic ray fluctuations spectrum inferred from ground-based cosmic ray observation data
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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.
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References
BENDAT, J. and A. PIERSOL, 1974. Measurements and analysis of random processes. Mir, Moscow.
BENDAT, J. and A. PIERSOL, 1983. Applications of the correlational and spectral analysis. Mir, Moscow.
BLOKH, Ya L., I. Ya LIBIN and K. F. YUDAKHIN, 1984. Cosmic ray fluctuations at the Earth during solar flares. Geomagn. i aeron., 24, 6, 875.
BODE, H. W., 1945. Network analysis and feedback amplifier design. Van Nostrand New York.
DORMAN, L. I. and I. Ya LIBIN. 1984. Cosmic scintillations and dynamic processes in space. Space Sci. Rev., 39. 91. DOI: https://doi.org/10.1007/BF00173671
DORMAN, L. I. and I. Ya. LIBIN, 1985. Short-period cosmic ray intensity variations. Uspeklzi Fiz. Nauk., 145, 3, 403. DOI: https://doi.org/10.3367/UFNr.0145.198503b.0403
DORMAN, L. I., I. Ya LIBIN and Ya. L. BLOKH, 1979. Scintillation method of studying cosmic ray variations. Nauka, Moscow, p. 107.
DORMAN, L. I., I. A. PIMENOV and V. V. SATSUK, 1978. Software to study the geophysical regularities using the example of cosmic rays. Nauka, Moscow, p. 152.
GULINSKY, O. V. and I. Ya LIBIN, 1979. Cosmic ray fluctuation events inferred from the data of the IZMIRAN Multidirectional Telescope. Preprint IZMIRAN, 30/258.
GULINSKY, O. V., I. Ya. LIBIN, F. A. STARKOV et al., 1983. Combined analysis of the data obtained by detecting the general muon and neutron components of cosmic ray intensity on May 7, 1978. Cosmic Rays, Radio i Svyaz, Moscow, p. 20.
JENKINS, G. M. and D. G. WATTS, 1972. Spectral analysis and its applications. Mir, Moscow.
KOZLOV, V. I., 1981 a. About the turbulence structure of the large-scale solar wind disturbances as inferred from cosmic ray fluctuation studies. Preprint, Moscow State University.
KOZLOV. V. I., 1981 b. Turbulent pulsations of magnetic field in shock waves. Geomagn. i. aeron. 21, 6, 1115.
KOZLOV, V. I., 1984. Early prediction of interplanetary shock waves by studying the dynamic properties of the characteristics of cosmic ray fluctuations. Preprint IKFIA. Siberian Branch, Acad. Sci. USSR, Yakutsk.
LIBIN, I. Ya., 1983 a. Spectral characteristics of cosmic ray fluctuations. Cosmic Rays, Radio i Svyaz, Moscow, p. 14.
LIBIN, I. Ya., 1983 b. Study of cosmic ray fluctuations during Forbush decreases. Cosmic Rays, Radio i Svyaz, Moscow, p. 21.
MAX. J., 1983. Methods and techniques for processing signals during physical measurements. Mir. Moscow.