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The Efficiency of Second-order Fermi Acceleration by Weakly Compressible Magnetohydrodynamic Turbulence

  • Authors: Jacob W. Lynn, Eliot Quataert, Benjamin D. G. Chandran, and Ian J. Parrish

Lynn et al. 2013 The Astrophysical Journal 777 128.

  • Provider: AAS Journals

Caption: Figure 7.

Particle heating rate , normalized by the turbulent cascade rate , as a function of thermal velocity v th, for an initially Maxwellian distribution function. The heating rate is measured from t = 2.5–20 L/ c s in the fiducial simulation and is ∝ n test/ n, where n test/ n is the number density of test particles relative to the fluid density in the simulation. Modest pitch-angle scattering rates ν enforce isotropy and significantly enhance the turbulent heating of the plasma.

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