Physics
Scientific paper
Mar 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976izssr..40..607k&link_type=abstract
(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Samarkand, Uzbek SSR, Oct. 29-31, 1975.) Akademiia Nauk SSSR, Izvest
Physics
Cosmic Rays, Diurnal Variations, Magnetic Storms, Particle Flux Density, Anisotropy, Magnetic Effects, Particle Energy
Scientific paper
Preliminary results are presented for a study that was undertaken to determine the first and second E-W, N-S, S-E, and N-W diurnal harmonics of changes in cosmic-ray intensity. All the data were obtained during magnetic storms which occurred in the period from June 1971 to December 1973; the dependence of the diurnal variation in intensity differences on magnetic-storm class is analyzed. It is found that all particles with energies less than about 200 GeV enter a narrow belt along the equator and that higher-energy particles are primarily responsible for changes in the intensity differences. It is concluded that a strongly concentrated inhomogeneity during large storms can successively modulate the intensity in each direction.
No associations
LandOfFree
Directional anisotropy in cosmic-ray intensity does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Directional anisotropy in cosmic-ray intensity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Directional anisotropy in cosmic-ray intensity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1219295