Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000apj...538..192m&link_type=abstract
The Astrophysical Journal, Volume 538, Issue 1, pp. 192-202.
Astronomy and Astrophysics
Astronomy
39
Ism: Cosmic Rays, Diffusion, Magnetohydrodynamics: Mhd, Plasmas, Turbulence
Scientific paper
The perpendicular diffusion of charged test particles in a static representation of low-frequency, weakly turbulent magnetic fields superimposed on a steady background field is investigated with numerical simulations. The magnetic field variation is purely one-dimensional, consistent with an ensemble of field-aligned Alfvén waves in the limit of zero Alfvén speed. The diffusion coefficient κ⊥ obtained from the numerical simulations is compared with Bieber & Matthaeus's recent theory of spatial diffusion, specialized to one-dimensional field geometry, for a number of particle energies/rigidities. It is found that the recent theory provides a better fit to the numerical data for Ωτ>2, where Ω is the particle gyrofrequency and τ is a rigidity-dependent decorrelation time, than does the well-known quasi-linear theory, or field line random walk limit. However, while the Bieber & Matthaeus theory fails to fit the simulation data for Ωτ<1, the theory corresponding to the field line random walk limit exhibits only a 20% error here. Possible reasons for the discrepancy between the theory and simulations are discussed.
Bieber John W.
Mace Richard L.
Matthaeus William H.
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