The simulation of Forbush decreases with time-dependent cosmic-ray modulation models of varying complexity

Details The simulation of Forbush decreases with time-dependent cosmic-ray modulation models of varying complexity The simulation of Forbush decreases with time-dependent cosmic-ray modulation models of varying complexity

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...243..531l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 243, no. 2, March 1991, p. 531-545.

Astronomy and Astrophysics

Astrophysics

37

Astronomical Models, Cosmic Rays, Forbush Decreases, Heliosphere, Solar Activity, Time Dependence, Two Dimensional Models

Scientific paper

An axially-symmetric time-dependent numerical drift model with a wavy neutral sheet is developed. Forbush decreases were modeled under the assumption that they were caused by propagating regions of enhanced scattering and diminished drift. The magnitude and recovery times of the Forbush decreases in the intensity of 1 GeV protons in the equatorial plane were studied as a function of radial distance by varying the complexity of the models.

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