Regions of Excessive Flux of PeV Cosmic Rays
arXiv:0902.1637 · doi:10.3103/S1062873809050128
Abstract
An analysis of arrival directions of extensive air showers generated by cosmic rays in the PeV energy range and registered with the EAS MSU and EAS-1000 Prototype arrays reveals a considerable number of regions of excessive flux of cosmic rays. We present results of comparative analysis of regions found in the two data sets, estimate probabilities of their appearance, and discuss correlation of their locations with coordinates of possible astrophysical sources of PeV cosmic rays.
4 pages, 3 figures; presented at the 30th Russian Cosmic Ray Conference, Saint-Petersburg, July 2-7, 2008
References in corpus (5)
- The ATNF Pulsar Catalogue
- Discovery of Localized Regions of Excess 10-TeV Cosmic Rays
- The puzzling MILAGRO hot spots
- A search for outstanding sources of PeV cosmic rays: Cassiopeia A, the Crab Nebula, the Monogem Ring--But how about M33 and the Virgo cluster?
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Cited by in corpus (5)
- A Search for Small-Scale Anisotropy of PeV Cosmic Rays
- Region of Excessive Flux of PeV Cosmic Rays in the Direction Toward Pulsars PSR J1840+5640 and LAT PSR J1836+5925
- Three Regions of Excessive Flux of PeV Cosmic Rays
- Regions of an excessive flux of cosmic rays according to data of the FIAN and MSU arrays
- A search for small and medium scale anisotropy of cosmic rays above 1 PeV registered at the Tunka-133 array