Galactic cosmic rays during periods of solar-magnetic-field inversion

Details Galactic cosmic rays during periods of solar-magnetic-field inversion Galactic cosmic rays during periods of solar-magnetic-field inversion

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2100k&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Physics

Galactic Cosmic Rays, Magnetic Field Inversions, Solar Magnetic Field, Heliosphere, Radiant Flux Density, Stratosphere Radiation, Time Dependence

Scientific paper

Intensity anomalies of galactic cosmic rays associated with solar-magnetic-field inversion are examined on the basis of data of stratospheric measurements (Murmansk) and neutron monitors for 1957-1983. These inversion anomalies are interpreted as the superposition of two types of phenomena causally connected with the inversions: The first phenomenon consists in a decrease and subsequent increase in the strength of the regular IMF in the heliosphere during inversion periods; while the second phenomenon consists in increases or decreases of the intensity of galactic-cosmic-ray nuclei depending on whether dMz/dt is negative or positive.

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