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Diffusion of High Energy Cosmic Rays from the Virgo Cluster

Published online by Cambridge University Press:  14 August 2015

M. Giler ,
J. Wdowczyk  and
A. W. Wolfendale
M. Giler
Affiliation:
University of Lodz, Poland
J. Wdowczyk
Affiliation:
Institute of Nuclear Research Lodz, Poland
A. W. Wolfendale
Affiliation:
University of Durham, U.K.

Extract

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The origin of the highest energy cosmic rays is unclear but the observation that many are seen to arrive from high Galactic latitudes supports the idea of Extragalactic sources. The characteristic features to be explained by any origin model are: the flattening of the energy spectrum above 1019eV and the apparent presence of a directional anisotropy which increases systematically with energy.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 94: Origin of Cosmic Rays , 1981 , pp. 69 - 70
Copyright
Copyright © Reidel 1981 

References

Krasilnikov, D.D., 1979, Proc. 16th Int. Cosmic Ray. Conf. (Kyoto) 8, 26 Google Scholar
Lloyd-Evans, J., Pollock, A.M.T., and Watson, A.A., 1979, Proc. 16th Int. Cosmic Ray Conf. (Kyoto) 13, 130.Google Scholar
Wdowczyk, J., and Wolfendale, A.W., 1979, Nature, 281, 5730, 356.Google Scholar