Anisotropy and corotation of galactic cosmic rays.

Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan.
Science (Impact Factor: 31.48). 11/2006; 314(5798):439-43. DOI: 10.1126/science.1131702
Source: PubMed

ABSTRACT The intensity of Galactic cosmic rays is nearly isotropic because of the influence of magnetic fields in the Milky Way. Here, we present two-dimensional high-precision anisotropy measurement for energies from a few to several hundred teraelectronvolts (TeV), using the large data sample of the Tibet Air Shower Arrays. Besides revealing finer details of the known anisotropies, a new component of Galactic cosmic ray anisotropy in sidereal time is uncovered around the Cygnus region direction. For cosmic-ray energies up to a few hundred TeV, all components of anisotropies fade away, showing a corotation of Galactic cosmic rays with the local Galactic magnetic environment. These results have broad implications for a comprehensive understanding of cosmic rays, supernovae, magnetic fields, and heliospheric and Galactic dynamic environments.


Available from: Huihai He, Jul 13, 2014
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