Nonstationary modulation of galactic cosmic rays in a nonlinear model

Details Nonstationary modulation of galactic cosmic rays in a nonlinear model Nonstationary modulation of galactic cosmic rays in a nonlinear model

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..214b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 214-217 (SEE N85-34991 23-93)

Physics

Cosmic Rays, Diffusion Coefficient, Galactic Radiation, Solar Wind Velocity, Heliosphere, Hydrodynamics, Interplanetary Space, Pioneer 11 Space Probe, Propagation Velocity, Solar Flares, Solar Wind

Scientific paper

An automodel equation for the solar wind velocity is obtained in the
self-consistent model. The solution of the convection-diffusion equation
is obtained for the density of galactic cosmic rays at a definite
dependence of the diffusion coefficient and solar wind velocity on the
rigidity and distance.

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