Diurnal sidereal variation of cosmic rays

Details Diurnal sidereal variation of cosmic rays Diurnal sidereal variation of cosmic rays

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ge%26ae..17..377g&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 17, May-June 1977, p. 377-380. In Russian.

Other

Cosmic Rays, Diurnal Variations, Muons, Particle Telescopes, Phase Shift, Solar Wind, Anisotropy, Sidereal Time, Solar Magnetic Field, Star Distribution

Scientific paper

Data obtained from the Yakutsk muon telescopes between 1958 and 1975 for registration levels between 0.7 and 20 m.w.e. show a semi-annual anisotropy cycle in sidereal time. The results are compared with data from other observatories. A phase shift which increases with increasing energy above 50 GeV is associated with the solar field reversal which started in 1968.

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