Diffusion-convection function of cosmic rays

Details Diffusion-convection function of cosmic rays Diffusion-convection function of cosmic rays

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983sssmp..26...88z&link_type=abstract

Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences, vol. 26, Jan. 1983, p. 88-101.

Astronomy and Astrophysics

Astronomy

Convection, Diffusion Theory, Particle Diffusion, Solar Cosmic Rays, Diffusion Coefficient, Heliosphere

Scientific paper

The diffusion-convection (D-C) function is an elementary composite function of the solution of the D-C equation for particles injected impulsively from a diffusive point source into a uniform, unbounded and spherically symmetrical medium. Attention is presently given to fundamental properties and several numerical results of the diffusion equation for the case of an impulsive, cosmic ray point source in a uniform, unbounded and spherically symmetrical moving medium.

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