Angular distribution of solar cosmic rays and scattering properties of interplanetary medium

Details Angular distribution of solar cosmic rays and scattering properties of interplanetary medium Angular distribution of solar cosmic rays and scattering properties of interplanetary medium

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005kfnt...21...83f&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 21, no. 2, p. 83-98

Physics

Scientific paper

The steady-state solution of kinetic equation, describing solar cosmic
ray propagation in the interplanetary space, is derived. The calculated
cosmic ray distribution function is applied to the determination of
parameters of energetic charged particles scattering in interplanetary
magnetic fields.

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