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The self-consistent transport of cosmic rays in a non-uniform magnetic field produced via the nonresonant streaming instability

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Reville,  Brian
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Kirk,  John G.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Citation

Reville, B., O'Sullivan, S., Duffy, P., & Kirk, J. G. (n.d.). The self-consistent transport of cosmic rays in a non-uniform magnetic field produced via the nonresonant streaming instability.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-7BB0-8
Abstract
The transport properties of relativistic protons in the precursor of a supernova remnant shock are investigated. The growth of magnetic waves via the nonresonant cosmic-ray current-driven instability is simulated using high resolution magnetohydrodynamic (MHD) simulations. The resulting diffusion of relativistic protons in the non-uniform field is investigated numerically, and the asymptotic diffusion coefficients are determined.