The sidereal anisotropy of cosmic rays around 3 X 10 (15) eV observed at a middle north latitude

Details The sidereal anisotropy of cosmic rays around 3 X 10 (15) eV observed at a middle north latitude The sidereal anisotropy of cosmic rays around 3 X 10 (15) eV observed at a middle north latitude

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..250m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 250-253 (SEE N85-34006 22-93)

Mathematics

Anisotropy, Cosmic Ray Showers, Detectors, Muons, Sidereal Time, Background Radiation, Diurnal Variations, Vectors (Mathematics)

Scientific paper

The sidereal time variation of cosmic rays (median primary energy : 3 10 to the 15th power eV) is investigated with air shower observations at Akeno, Japan (900 m a.s.l.) which started in September 1981. Air showers are detected by a coincidence requirement on several muon detectors. The result obtained for three years is suggestive of a big semi-diurnal variation (0.37 % in amplitude). On the other hand, the diurnal variation is rather small than the semi-diurnal one. The feature of the sidereal anisotropy supposed from the present result looks quite different from that below 10 to the 14th power eV.

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