Figure 9 from Detailed Numerical Investigation of the Bohm Limit in Cosmic Ray Diffusion Theory

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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 9.

Perpendicular mean free path, λ _⊥, normalized to l ₀ with respect to rigidity R for high turbulence scenarios of δ B/ B ₀ = 10, 50, and 100, plotted as circles, stars, and squares, respectively, for composite (solid lines) and isotropic (dashed lines) models.

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