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

Main Article Content

O. V. Gulinsky
L. I. Dorman
N. S. Kaminer
T. Lanina
I. Ya. Libin
N. V. Mymrina
R. E. Prilutsky
K. F. Yudakhin
L. G. Chuvilgin
K. Kudela
M. Steglik
J. A. Otaola
J. Pérez Peraza

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.

Article Details

How to Cite
Gulinsky, O. V., Dorman, L. I., Kaminer, N. S., Lanina, T., Libin, I. Y., Mymrina, N. V., Prilutsky, R. E., Yudakhin, K. F., Chuvilgin, L. G., Kudela, K., Steglik, M., Otaola, J. A., & 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
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Article
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