Origin of energetic cosmic rays 1 – galactic diffusion in the energy range 1014 – 1017eV

  1. Lookup NU author(s)
  2. Professor Margaret Carol Bell CBE
Author(s)Bell MC, Wolfendale AW
Publication type Article
JournalJournal of Physics A: Mathematical, Nuclear and General
ISSN (print)0301-0015
ISSN (electronic)1751-8121
Full text for this publication is not currently held within this repository. Alternative links are provided below where available.
A brief survey is given of measurements leading to the determination of the energy spectrum of primary cosmic rays in the energy range 1014-1017 eV with particular reference to the change of exponent which occurs in the region of 3*1015 eV (the spectral 'kink') and an attempt is made to give a quantitative explanation in terms of galactic diffusion. Reasonable astronomical values for various parameters (cloud sizes, magnetic fields, etc) give some measure of success in accounting for the sharpness of the kink in the energy spectrum, the energy at which it occurs and the magnitude of the change of exponent. Problems arise with the predicted anisotropy however and the adopted model breaks down above about 1017 eV.
PublisherInstitute of Physics Publishing Ltd.
Actions    Link to this publication

Altmetrics provided by Altmetric