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

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

dc.creatorGulinsky, O. V.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
dc.creatorDorman, L. I.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
dc.creatorKaminer, N. S.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
dc.creatorLanina, T.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
dc.creatorLibin, I. Ya.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
dc.creatorMymrina, N. V.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
dc.creatorPrilutsky, R. E.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
dc.creatorYudakhin, K. F.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
dc.creatorChuvilgin, L. G.; Department of Cosmic Rays, IZMIRAN, Troitsk 142092, U.S.S.R.
dc.creatorKudela, K.; Institute of Geophysics of the Slovak Academy of Science, Kosice, CHECOSLOVAKIA.
dc.creatorSteglik, M.; Institute of Geophysics of the Slovak Academy of Science, Kosice, CHECOSLOVAKIA.
dc.creatorOtaola, J. A.; Instituto de Geofísica, UNAM, México, 04510, D.F., MEXICO.
dc.creatorPérez Peraza, J.; Instituto Nacional de Astronomía, Óptica y Electrónica, Puebla, MEXICO.
dc.date2012-08-06
dc.date.accessioned2018-03-16T15:51:40Z
dc.date.available2018-03-16T15:51:40Z
dc.identifierhttp://ojs.unam.mx/index.php/geofisica/article/view/39374
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1203060
dc.descriptionThe 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.en-US
dc.descriptionSe 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.es-ES
dc.formatapplication/pdf
dc.languagespa
dc.publisherInstituto de Geofísicaes-ES
dc.relationhttp://ojs.unam.mx/index.php/geofisica/article/view/39374/35809
dc.sourceGeofísica Internacional; Vol 27, No 2 (1988)es-ES
dc.source0016-7169
dc.titleLarge-scale cosmic ray fluctuations inferred from the ground-based neutron and ionizing component observations and their relevance to cosmic ray anisotropyes-ES
dc.titleLarge-scale cosmic ray fluctuations inferred from the ground-based neutron and ionizing component observations and their relevance to cosmic ray anisotropyen-US
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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