Galactic cosmic ray anisotropy at approximately 6.1013 E

Details Galactic cosmic ray anisotropy at approximately 6.1013 E Galactic cosmic ray anisotropy at approximately 6.1013 E

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7622142g&link_type=abstract

Presented at the 14th Intern. Cosmic Ray Conf., West Germany, 15 Aug. 1975

Mathematics

Logic

Anisotropy, Cosmic Rays, Galactic Radiation, Hungary, Interstellar Magnetic Fields, Meteorological Parameters, Mountains, Regression Analysis, Sidereal Time

Scientific paper

Arrival times of 1.14 x ten to the eighth power extensive air showers registered on the peak Musala (geographical latitude 42 deg N) were analyzed for sidereal variation. The solar and antisidereal waves remain below noise level while the first and second sidereal daily waves prove to be significant adding up to an anisotropy of 0.1 per cent. Intensity maximum is obtained when directions near the galactic plane are scanned. Some consequences of the result obtained are discussed.

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