Scale size of the cosmic ray modulating region

Details Scale size of the cosmic ray modulating region Scale size of the cosmic ray modulating region

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...246.1010k&link_type=abstract

Astrophysical Journal, Part 1, vol. 246, June 15, 1981, p. 1010-1013. Financiadora de Estudos e Projetos

Astronomy and Astrophysics

Astrophysics

2

Cosmic Rays, Forbush Decreases, Galactic Radiation, Particle Intensity, Long Term Effects, Modulation, Neutron Counters, Size Determination

Scientific paper

An analysis of long-term changes in cosmic ray intensities, as recorded by neutron monitors at the Deep River (1965-1977) and Huancayo (1955-1965), indicates that the monthly mean values may be considerably distorted due to the Forbush decrease effects. It is found that while the mean values show a wide hysteresis loop, the maximum values are characterized by a narrower loop and thereby imply reduced dimensions of a modulating region for galactic cosmic ray intensity.

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