Cosmic ray perpendicular gradient during 1962-1972

Details Cosmic ray perpendicular gradient during 1962-1972 Cosmic ray perpendicular gradient during 1962-1972

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976jgr....81.4627a&link_type=abstract

Journal of Geophysical Research, vol. 81, Sept. 1, 1976, p. 4627-4632.

Physics

7

Annual Variations, Cosmic Rays, Galactic Radiation, Solar Cycles, Autocorrelation, Gradients, Neutron Flux Density, Particle Intensity, Solar Activity Effects

Scientific paper

An analysis of the perpendicular gradient of galactic cosmic rays performed on the basis of an estimate of annual and semiannual variations in cosmic-ray intensity is reported. Daily cosmic-ray intensity data detected by the Deep River neutron monitors have been used for the period from 1962 to 1972. The perpendicular gradient can be separated into two components which are asymmetrical and symmetrical, respectively, with respect to the solar equatorial plane. The asymmetrical gradient component is quasi-steady over the whole period, while the symmetrical one reverses its direction once. In northern and southern regions of the solar modulating cavity, the perpendicular gradient displays different characteristics in both value and direction, which depend on the solar-cycle phase.

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