M. Yu. Zotov, G. V. Kulikov
Published 2009-02-10Version 1
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.
Comments: 4 pages, 3 figures; presented at the 30th Russian Cosmic Ray Conference, Saint-Petersburg, July 2-7, 2008
Journal: Bull. Russ. Acad. Sci.: Physics, 2009, v.73, pp.574-576
Three Regions of Excessive Flux 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
Observation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above $8 \times 10^{18}$ eV
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