Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/12423
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Type: Journal article
Title: The angular deviation of ultra high energy cosmic rays in intergalactic magnetic fields
Author: Clay, R.
Cook, S.
Dawson, B.
Smith, A.
Lampard, R.
Citation: Astroparticle Physics, 1998; 9(3):221-225
Publisher: ELSEVIER SCIENCE BV
Issue Date: 1998
ISSN: 0927-6505
Statement of
Responsibility: 
R. W. Clay, S. Cook, B. R. Dawson, A. G. K. Smith and R. Lampard
Abstract: The angular deviation associated with the propagation of ultra high energy cosmic ray protons through turbulent intergalactic magnetic fields is examined including the effect of interactions with the cosmic microwave background. It is found that the deviation of the particles is consistent with diffusion ideas but the magnitude of the deviation is appreciably less than suggested by simple models for a given mean field strength and observational energy.
Keywords: Intergalactic magnetic field
Scattering of cosmic rays
Description: Copyright © 1998 Published by Elsevier Science B.V.
DOI: 10.1016/S0927-6505(98)00023-1
Published version: http://dx.doi.org/10.1016/s0927-6505(98)00023-1
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Physics publications

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