The cosmic radiation in the heliosphere at successive solar minima 3. Steady state drift solutions of the transport equation

Details The cosmic radiation in the heliosphere at successive solar minima 3. Steady state drift solutions of the transport equation The cosmic radiation in the heliosphere at successive solar minima 3. Steady state drift solutions of the transport equation

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996jgr...10121581r&link_type=abstract

Journal of Geophysical Research, Volume 101, Issue A10, p. 21581-21588

Physics

Plasma Physics

14

Interplanetary Physics: Cosmic Rays, Interplanetary Physics: Interplanetary Magnetic Fields, Space Plasma Physics: Charged Particle Motion And Acceleration, Space Plasma Physics: Transport Processes

Scientific paper

Cosmic ray intensities and density gradients, as observed by the Pioneer 10 and 11, Voyager 1 and 2, and IMP 8 spacecraft during the 1977 and 1987 solar minimum periods, are interpreted in terms of a two-dimensional version of the cosmic ray transport equation that includes drifts. This paper is a follow-up of an earlier no-drift version to elucidate the necessity and limitations of drift effects as demanded by actual observations.

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