Modeling cosmic ray anisotropies near 10(18) eV

Details Modeling cosmic ray anisotropies near 10(18) eV Modeling cosmic ray anisotropies near 10(18) eV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..304s&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 304-307 (SEE N85-34006 22-93)

Mathematics

Anisotropy, Cosmic Ray Showers, Flux (Rate), Interstellar Magnetic Fields, Energy Spectra, Faraday Effect, Heavy Nuclei, Mathematical Models

Scientific paper

A galactic magnetic field reversal near the Sagittarius spiral arm may be responsible for the southern excess (or northern shortage) of cosmic rays near 10 to the 18th power eV. The north-south asymmetry produced by such a reversal would increase with energy in the same manner as the observed asymmetry. The existence of a reversal has been inferred from analyses of Faraday rotation measures.

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