Anisotropy of cosmic rays of energy 10 (15) eV to 10 (17) eV observed at Akeno

Details Anisotropy of cosmic rays of energy 10 (15) eV to 10 (17) eV observed at Akeno Anisotropy of cosmic rays of energy 10 (15) eV to 10 (17) eV observed at Akeno

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..242k&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 242-245 (SEE N85-34006 22-93)

Physics

Anisotropy, Cosmic Ray Showers, Harmonic Analysis, Muons, Amplitudes, Energy Spectra, Spectrum Analysis

Scientific paper

Anisotropy of cosmic rays is studied with extensive air showers (EAS) data by muon trigger. The present results support those obtained by electron trigger which suggest the significant anisotropy of second harmonics with phase around 100 deg in right ascension for showers of 10 to the 16th power - 10 to the 17th power eV, and predominant arrival direction of 230 deg in right ascension for muon-rich showers. It seems that the phase of the first harmonics in the energy range below 10 to the 11th power eV is about 300 deg in right ascension and the second harmonics near 6 x 10 to the 14th power eV is statistically significant with an amplitude of 0.39 + or - 0.13% in direction of 83 + or - 10 deg in right ascension.

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