Long term variability of the cosmic ray intensity

Details Long term variability of the cosmic ray intensity Long term variability of the cosmic ray intensity

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..345b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 345-348 (SEE N85-33902 22-93)

Physics

Acceleration (Physics), Anisotropy, Computerized Simulation, Cosmic Rays, Monte Carlo Method, Radiant Flux Density, Electrons, Interstellar Matter, Magnetic Fields, Particle Acceleration, Poisson Density Functions, Protons, Supernova Remnants

Scientific paper

In a previous paper Bhat, et al., assess the evidence for the continuing acceleration of cosmic rays in the Loop I supernova remnant. The enhanced gamma-ray emission is found consistent with the Blandford and Cowie model for particle acceleration at the remnant shock wave. The contributions of other supernovae remnants to the galactic cosmic ray energy density are now considered, paying anisotropy of cosmic rays accelerated by local supernovae ( 100 pc). The results are compared with geophysical data on the fluctuations in the cosmic ray intensity over the previous one billion years.

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