Enhanced Diffusion in Strongly Magnetized Astrophysical Plasmas

Details Enhanced Diffusion in Strongly Magnetized Astrophysical Plasmas Enhanced Diffusion in Strongly Magnetized Astrophysical Plasmas

Aug 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973ap%26ss..23..339l&link_type=abstract

Astrophysics and Space Science, Volume 23, Issue 2, pp.339-346

Astronomy and Astrophysics

Astrophysics

13

Scientific paper

We demonstrate that the diffusion coefficient for low energy particles, tied to a magnetic field which random walks, may be considerably larger than previously estimated in a strongly magnetized system — like the solar wind or the Galaxy. This is of interest with respect to propagation and lifetime considerations of low energy cosmic rays in the solar wind and the Galaxy.

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