Evidence for an energy dependence in the short pathlengths of the cosmic ray pathlength distribution

Details Evidence for an energy dependence in the short pathlengths of the cosmic ray pathlength distribution Evidence for an energy dependence in the short pathlengths of the cosmic ray pathlength distribution

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....2..210g&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 2 (A85-2

Computer Science

Cosmic Rays, Particle Energy, Radiation Distribution, Abundance, Particle Motion

Scientific paper

The energy dependence of the short pathlengths in the cosmic ray pathlength distribution is investigated in a galactic propagation plus solar modulation calculation. In order to reproduce, simultaneously, the compiled B/C and sub-Fe/Fe measurements, an energy dependent deficiency of short pathlengths is required which is largest at low energies and becomes negligible above a few GeV/nucleon. Such behavior could imply a significant contribution from matter in the vicinity of the cosmic ray source or the acceleration site.

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