Physics
Scientific paper
Aug 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....3..861k&link_type=abstract
In: International Cosmic Ray Conference, 14th, Munich, West Germany, August 15-29, 1975, Conference Papers. Volume 3. (A76-26851
Physics
4
Charged Particles, Diffusion Coefficient, Digital Simulation, Interplanetary Magnetic Fields, Particle Diffusion, Turbulent Diffusion, Cosmic Rays, Magnetic Effects, Magnetic Rigidity, Pitch (Inclination), Power Series, Statistical Analysis
Scientific paper
Numerical simulation experiments have been 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 suitably-chosen statistical properties, a pitch-angle diffusion coefficient is derived. Results are presented for a variety of particle rigidities and r.m.s. random field strengths and a power spectrum typical of conditions found in interplanetary space.
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