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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 6.

λ /( Rl 0) vs. R for δ B/ B 0 = 10.0, 50.0, and 100.0 plotted as circles, stars, and squares, respectively, for the slab model validating the relation of λ /( Rl 0) ~ B 0B. Dashed lines from top to bottom correspond to the right hand side of the latter relation, that is B 0B = 0.1, 0.02, and 0.01.

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