Please use this identifier to cite or link to this item:
|Scopus||Web of Science®||Altmetric|
|Title:||The angular deviation of ultra high energy cosmic rays in intergalactic magnetic fields|
|Citation:||Astroparticle Physics, 1998; 9(3):221-225|
|Publisher:||ELSEVIER SCIENCE BV|
|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.|
|Appears in Collections:||Physics publications|
Files in This Item:
There are no files associated with this item.
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.