The solar magnetic field and two-year cosmic-ray variations

Details The solar magnetic field and two-year cosmic-ray variations The solar magnetic field and two-year cosmic-ray variations

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ge%26ae..32..154o&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 32, no. 2, Mar.-Apr. 1992, p. 154-156. In Russian.

Computer Science

Interplanetary Magnetic Fields, Solar Cosmic Rays, Solar Magnetic Field, Solar Wind Velocity, Stratosphere, Interplanetary Space, Magnetic Flux, Periodic Variations

Scientific paper

The paper presents a study of two-year variations of mean monthly values of the magnetic field strength of the sun as a star, the solar wind velocity and the IMF strength, the cosmic-ray intensity in the stratosphere, and the neutron component for the 1965-1988 period. The two-year variation of the solar magnetic field, extended by the solar wind into interplanetary space, is shown to be the cause of the two-year cosmic-ray variation.

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