Long-term modulation of galactic cosmic rays in high-energy region

Details Long-term modulation of galactic cosmic rays in high-energy region Long-term modulation of galactic cosmic rays in high-energy region

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5...94k&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 94-97 (SEE N85-34991 23-93)

Physics

Cosmic Rays, Galactic Radiation, Muons, Radiant Flux Density, Solar Activity, Solar Magnetic Field, Solar Wind Velocity, Energy Spectra, Geomagnetism, Ionization Chambers, Solar Cycles

Scientific paper

The results of continuous registration of the cosmic ray muon intensity on the ground and underground at 7, 20 and 60 m w.e. depths in Yakutsk for 1957 - 1983 are presented. In years of the solar activity maximum in cosmic ray density were found two minima or two-stepped decrease. The second intensity minimum appears to be not the result of the inversion of the general magnetic field of the sun but caused by the increase of the solar wind speed.

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