Physics
Scientific paper
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.
Bhat C. L.
Houston B. P.
Mayer John C.
Wolfendale Arnold W.
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