Cyclic variations of the barometric coefficient of the neutron component of cosmic rays

Details Cyclic variations of the barometric coefficient of the neutron component of cosmic rays Cyclic variations of the barometric coefficient of the neutron component of cosmic rays

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..343r&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, Mar.-Apr. 1991, p. 343-345. In Russian.

Computer Science

Cosmic Rays, Energy Spectra, Neutron Flux Density, Periodic Variations, Solar Cycles, Corpuscular Radiation, Interplanetary Magnetic Fields, Solar Activity

Scientific paper

An analysis of multiyear neutron-monitor data reveals an 11-year cyclicity of the barometric coefficient beta of the cosmic-ray neutron component. Beta reaches its maximum near the solar minimum, and its minimum near the solar maximum. This phenomenon is interpreted by assuming a connection between the observed effect and 11-year variations of the cosmic-ray energy spectrum.

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