Modulation of galactic cosmic rays in the case of a stepwise dependence of the diffusion coefficient on momentum

Details Modulation of galactic cosmic rays in the case of a stepwise dependence of the diffusion coefficient on momentum Modulation of galactic cosmic rays in the case of a stepwise dependence of the diffusion coefficient on momentum

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..900c&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, Nov.-Dec. 1987, p. 900-905. In Russian.

Physics

2

Diffusion Coefficient, Energy Spectra, Galactic Cosmic Rays, Solar Wind, Modulation, Particle Acceleration

Scientific paper

An exact solution to the stationary problem involving the modulation of cosmic rays with a monoenergetic spectrum specified at infinity by the spherically symmetric solar wind is obtained in the isotropic-diffusion approximation. It is assumed that the dependence of the diffusion coefficient on the momentum has a stepwise form. The particle acceleration by a standing shock wave at the boundary of the heliosphere is taken into account.

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