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

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.

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 Creators:
Reville, Brian1, Author           
O'Sullivan, Stephen2, Author
Duffy, Peter2, Author
Kirk, John G.1, Author           
Affiliations:
1Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550              
2UCD school of physics, Dublin School of mathematical sciences, DCU, Dublin, ou_persistent22              

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 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.

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Language(s): eng - English
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 Publication Status: Not specified
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 Rev. Type: -
 Identifiers: eDoc: 333717
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Title: Seventh European Workshop on Collisionless Shocks
Place of Event: Paris, France
Start-/End Date: 2007-11-07 - 2007-11-09

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