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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Detalles Bibliográficos
Autores: 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.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:1988
País:México
Institución:UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO
Repositorio:Geofísica Internacional
Idioma:español
OAI Identifier:oai:revistagi.geofisica.unam.mx:article/1123
Acceso en línea:http://revistagi.geofisica.unam.mx/index.php/RGI/article/view/1123
Access Level:acceso abierto
Palabra clave:Rayos cósmicos
anisotropía
fluctuaciones
Cosmic rays
anisotropy
fluctuations
Descripción
Sumario: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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