Cosmic-ray transport during anisotropic turbulence in the IMF

Details Cosmic-ray transport during anisotropic turbulence in the IMF Cosmic-ray transport during anisotropic turbulence in the IMF

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ge%26ae..21..412k&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 21, May-June 1981, p. 412-419. In Russian.

Computer Science

2

Boltzmann Transport Equation, Cosmic Rays, Interplanetary Magnetic Fields, Quantum Theory, Turbulence Effects, Anisotropic Media, Particle Diffusion, Particle Flux Density, Tensor Analysis

Scientific paper

The methods of quantum scattering theory are used to average the collisionless Boltzmann equation over a stochastic-field ensemble. The cosmic-ray transport equation and flux density are obtained for arbitrary anisotropic turbulence in the interplanetary magnetic field (IMF). An equation is derived which gives the relation between the cosmic-ray diffusion tensor and the correlation tensor of the stochastic component of the IMF. The cosmic-ray diffusion tensor is obtained for the case of axisymmetric turbulence.

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