Cosmic ray anisotropy in interplanetary space

Details Cosmic ray anisotropy in interplanetary space Cosmic ray anisotropy in interplanetary space

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979izyer..43.2558d&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yerevan, Armenian SSR, June 1979.) Akademiia Nauk SSSR, Izvestiia, Seriia Fi

Physics

Anisotropy, Cosmic Rays, Interplanetary Magnetic Fields, Interplanetary Space, Distribution Functions, Kinetic Equations, Larmor Radius, Particle Flux Density, Spherical Harmonics, Transport Properties

Scientific paper

The kinetic equation describing cosmic ray propagation in interplanetary space is used to obtain a system of equations in the diffusion approximation. If the Larmor radius of particles in the regular field is much greater than the correlation radius of the random magnetic field, the second harmonic of the cosmic ray distribution function is included neither in the cosmic ray transport equation nor in the particle flux density expression. The expression for the second spherical harmonic in the case of a strong regular field and in the opposite limiting case is analyzed.

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