Computer simulation of the velocity diffusion of cosmic rays

Details Computer simulation of the velocity diffusion of cosmic rays Computer simulation of the velocity diffusion of cosmic rays

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977stin...7726059k&link_type=abstract

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Physics

Computerized Simulation, Cosmic Rays, Diffusion Coefficient, Monte Carlo Method, Velocity Distribution, Charged Particles, Field Theory (Physics), Magnetic Fields, Turbulence

Scientific paper

Monte Carlo simulation experiments were performed in order to study the velocity diffusion of charged particles in a static turbulent magnetic field. By following orbits of particles moving in a large ensemble of random magnetic field realizations with suitable chosen statistical properties, a pitch-angle diffusion coefficient is derived. Results are presented for a variety of particle rigidities and rms random field strengths and compared with the predictions of standard quasi-linear theory and the nonlinear partially averaged field theory.

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