Figure 1 from The Efficiency of Second-order Fermi Acceleration by Weakly Compressible Magnetohydrodynamic Turbulence

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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 1.

1D angle-averaged kinetic energy power spectra in our turbulence simulations. Simulating many "outer-scale" eddies in the parallel direction limits the inertial range of our turbulence to less than a decade.

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