Neutral surface of the interplanetary magnetic field and intensity of galactic cosmic rays

Details Neutral surface of the interplanetary magnetic field and intensity of galactic cosmic rays Neutral surface of the interplanetary magnetic field and intensity of galactic cosmic rays

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..717s&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, July-Aug. 1991, p. 717-719. In Russian.

Physics

Galactic Cosmic Rays, Heliosphere, Interplanetary Magnetic Fields, Neutron Flux Density, Solar Wind Velocity, Diurnal Variations, Magnetic Flux, Radiant Flux Density, Solar Terrestrial Interactions

Scientific paper

An analysis is made of the behavior of galactic-cosmic-ray (GCR) intensity for two revolutions of the sun in 1974 with respect to the position of the neutral surface of the IMF. The analysis is based on global neutron-monitor data. It is shown that the behavior of the GCR intensity can be explained on the basis of an asymmetric (with respect to the ecliptic plane) region of cosmic-ray modulation.

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