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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 4.

Time evolution of the transverse magnetic fields B⊥ for the runs in Table 2. Their linear growth shows good agreement with the analytical prediction (gray solid lines). However, the saturated magnetic fields are different.

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