Second harmonic of the cosmic-ray distribution function for the case of a strong magnetic field

Details Second harmonic of the cosmic-ray distribution function for the case of a strong magnetic field Second harmonic of the cosmic-ray distribution function for the case of a strong magnetic field

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22..192k&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 22, Mar.-Apr. 1982, p. 192-196. In Russian.

Physics

Cosmic Rays, Interplanetary Magnetic Fields, Particle Flux Density, Charged Particles, Distribution Functions, Kinetic Equations, Nonuniform Magnetic Fields, Particle Interactions, Plasma Drift, Spherical Harmonics, Transport Properties

Scientific paper

A drift kinetic equation is derived with allowance for multiple scattering of particles by random irregularities of the interplanetary magnetic field. A transport equation is obtained as well as first and second spherical harmonics of the particle distribution function for the case of a strong magnetic field. The density, current, and second harmonic of the particles are related to the density, current, and second harmonic of Larmor disks.

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