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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 3.

Similar to Figure 2, except that the CRs initially have cone distributions. Left panels: The spatial profiles of the magnetic field components at ﹩t\approx 7{\gamma }_{\,\rm{fast}\,}^{-1}﹩. The x-axes are normalized to λfast = 2π/kfast ≈ 50di. In the shaded zoomed-in part, the dominant wavelengths ∼λfast are prominent. Right panels: Time evolution of helicities Δϕ(k).

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