Cosmic ray modulation by a shock wave with allowance for adiabatic cooling and transverse diffusion - Self-similar solution

Details Cosmic ray modulation by a shock wave with allowance for adiabatic cooling and transverse diffusion - Self-similar solution Cosmic ray modulation by a shock wave with allowance for adiabatic cooling and transverse diffusion - Self-similar solution

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ge%26ae..20..990b&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 20, Nov.-Dec. 1980, p. 990-996. In Russian.

Physics

Cosmic Rays, Forbush Decreases, Interplanetary Space, Particle Diffusion, Shock Wave Propagation, Adiabatic Demagnetization Cooling, Boundary Conditions, Boundary Value Problems, Diffusion Coefficient, Numerical Differentiation

Scientific paper

A theoretical model is developed to study the modulation of cosmic rays by an interplanetary shock wave, taking into account adiabatic cooling and diffusion recovery after the passage of the wave. It is shown that a self-similar solution with boundary conditions on the moving boundary can describe not only the sharp decrease of cosmic ray intensity, but also the gradual recovery of intensity during a Forbush decrease.

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