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

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 t...

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Bibliographic Details
Authors: Gulinsky, O. V., Dorman, L. I., Kaminer, N. S., Lanina, T., Libin, I. Ya., Mymrina, N. V., Prilutsky, R. E., Yudakhin, K. F., Chuvilgin, L. G., Kudela, K., Steglik, M., Otaola, J. A., Pérez Peraza, J.
Format: article
Status:Published version
Publication Date:1988
Country:México
Institution:UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO
Repository:Geofísica Internacional
Language:Spanish
OAI Identifier:oai:revistagi.geofisica.unam.mx:article/1123
Online Access:http://revistagi.geofisica.unam.mx/index.php/RGI/article/view/1123
Access Level:Open access
Keyword:Rayos cósmicos
anisotropía
fluctuaciones
Cosmic rays
anisotropy
fluctuations
Description
Summary: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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