The mean free path of low rigidity cosmic rays

Details The mean free path of low rigidity cosmic rays The mean free path of low rigidity cosmic rays

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979stin...7928114g&link_type=abstract

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Computer Science

Cosmic Rays, Interplanetary Magnetic Fields, Magnetic Rigidity, Mean Free Path, Galactic Radiation, Magnetohydrodynamic Waves, Solar Radiation, Turbulent Diffusion

Scientific paper

A simple heuristic argument is presented which suggests that the large rigidity independent mean free paths observed for low rigidity solar and galactic cosmic rays can be understood in terms of weak turbulence diffusion theory if one assumes that the interplanetary magnetic turbulence consists of a combination of Alfven waves propagating with constant field magnitude and a small (approximately 5-10%) admixture of compressive fluctuations.

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