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Detailed Numerical Investigation of the Bohm Limit in Cosmic Ray Diffusion Theory

  • Authors: M. Hussein and A. Shalchi

Hussein & Shalchi 2014 The Astrophysical Journal 785 31.

  • Provider: AAS Journals

Caption: Figure 1.

Spectrum for slab, composite, and isotropic turbulence with respective values of q = 0.0, 2.0, and 3.0 over a spread of wave-numbers ranging from k min l 0 = 10 −3 to k max l 0 = 10 3 in dimensionless units. At kl 0 = 1, a transition from energy to inertial range takes place.

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