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

Gulinsky, O. V.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.; Dorman, L. I.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.; Kaminer, N. S.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.; Lanina, T.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.; Libin, I. Ya.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.; Mymrina, N. V.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.; Prilutsky, R. E.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.; Yudakhin, K. F.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.; Chuvilgin, L. G.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.; Kudela, K.; Institute of Geophysics of the Slovak Academy of Science, Kosice, CHECOSLOVAKIA.; Steglik, M.; Institute of Geophysics of the Slovak Academy of Science, Kosice, CHECOSLOVAKIA.; Otaola, J. A.; Instituto de Geofísica, UNAM, México, 04510, D.F., MEXICO.; Pérez Peraza, J.; Instituto Nacional de Astronomía, Óptica y Electrónica, Puebla, MEXICO.

Artículos de revistas

Registro en:

http://ojs.unam.mx/index.php/geofisica/article/view/39374

http://repositorioslatinoamericanos.uchile.cl/handle/2250/1203060

Autor

Gulinsky, O. V.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.

Dorman, L. I.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.

Kaminer, N. S.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.

Lanina, T.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.

Libin, I. Ya.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.

Mymrina, N. V.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.

Prilutsky, R. E.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.

Yudakhin, K. F.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.

Chuvilgin, L. G.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.

Kudela, K.; Institute of Geophysics of the Slovak Academy of Science, Kosice, CHECOSLOVAKIA.

Steglik, M.; Institute of Geophysics of the Slovak Academy of Science, Kosice, CHECOSLOVAKIA.

Otaola, J. A.; Instituto de Geofísica, UNAM, México, 04510, D.F., MEXICO.

Pérez Peraza, J.; Instituto Nacional de Astronomía, Óptica y Electrónica, Puebla, MEXICO.

Institución

Universidad Nacional Autónoma de México

Resumen

The work treats with the behavior of the cosmic ray fluctuation power spectrum in the frequency range below 10-4 Hz 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.

Se estudia el comportamiento del espectro de potencia de las fluctuaciones en la intensidad de los rayos cosméticos para frecuencias menores de 10-4 HZ, 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.

Materias

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