Analysis of the small-scale cosmic ray fluctuations spectrum inferred from ground-based cosmic ray observation data
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En el presente trabajo se estudian teóricamente las relaciones existentes entre las características espectrales de la intensidad de los rayos cósmicos y el campo magnético interplanetario, usando para esto las características espectrales de la intensidad de la radiación cósmica inferidas de datos observados en superficie. Se determinan las características espectrales medias del campo magnético interplanetario y los resultados se comparan con las observaciones. Se describen, así mismo, los resultados del análisis de las fluctuaciones en la intensidad de los rayos cósmicos durante varios periodos y para varias estaciones.
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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.