Polarity-dependent heliolatitudinal gradient of Galactic cosmic rays

Details Polarity-dependent heliolatitudinal gradient of Galactic cosmic rays Polarity-dependent heliolatitudinal gradient of Galactic cosmic rays

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...299..505k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 299, Dec. 1, 1985, p. 505-509.

Astronomy and Astrophysics

Astrophysics

Galactic Cosmic Rays, Milky Way Galaxy, Polarization Characteristics, Radiation Measurement, Astronomical Models, Interplanetary Medium, Particle Telescopes, Solar Activity

Scientific paper

An attempt is made to reveal the polarity-dependent heliolatitudinal gradient of galactic cosmic rays predicted by drift models. The 7°.5 excursion of Earth from the helioequator results in opposite yearly intensity waves in the inward and outward interplanetary magnetic sectors. Data from the Nagoya ground level vertical cosmic-ray telescope are analysed for the period of 1974 - 1982. Evidence is presented in favor of a gradient rising away from the neutral sheet in the epoch of 1974 - 1979. The results obtained for 1980 - 1982 remain inconclusive.

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