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

Contenido principal del artículo

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

Resumen

Se estudia el comportamiento del espectro de potencia de las fluctuaciones en la intensidad de los rayos cósmicos para frecuencias menores de 10-4Hz, determinado a partir de las observaciones en superficie de las componentes nucleónica y de ionización. Se hace un intento de describir el espectro de fluctuaciones, usando cambios en el valor de la anisotropía de rayos cósmicos y del espectro de inhomogeneidades del campo magnético interplanetario.

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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. Geofísica Internacional, 27(2), 167–190. https://doi.org/10.22201/igeof.00167169p.1988.27.2.781
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Biografía del autor/a

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



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