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Impact of Cosmic-Ray Distribution on the Growth and Saturation of Bell Instability

  • Authors: Saikat Das, Siddhartha Gupta, Prateek Sharma

Saikat Das et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 12.

Evolution of transverse magnetic field B for the runs PLI:5-400:p−3, PLI:5-400(p−4), and PLI:5-400:p−5. Inset: saturated magnetic field ﹩{\left({B}_{\perp }/{B}_{0}\right)}_{\,\rm{sat}\,}﹩ vs. anisotropy parameter ξ for these runs (green pentagon for p−5, pink square for p−4, blue nabla for p−3). The gray dashed line represents Equation (15).

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