Image Details

Choose export citation format:

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 3.

λ normalized to the bendover length l 0 vs. turbulence strength δ B/ B 0 for low energetic particles R = 0.1. The plot also shows λ / l 0 for the three different models (slab, composite, and isotropic), plotted as circles, squares, and stars, respectively. The dashed lines represent the standard Bohm limit with λ ~ R L , whereas the solid lines indicate the modified Bohm limit where λ ~ R LB 0B. Triangles represent the Shalchi (2005) simulations.

Other Images in This Article
Copyright and Terms & Conditions