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KINETIC SIMULATIONS OF THE LOWEST-ORDER UNSTABLE MODE OF RELATIVISTIC MAGNETOSTATIC EQUILIBRIA

  • Authors: Krzysztof Nalewajko, Jonathan Zrake, Yajie Yuan, William E. East, and Roger D. Blandford

2016 The Astrophysical Journal 826 115.

  • Provider: AAS Journals

Caption: Figure 10.

Top panel: dependence of the number (blue squares) and energy (red circles) fractions contained in the high-energy tail of the electron distribution, averaged for ct/L ∈ [9:10], on the mean hot magnetization value. Bottom panel: dependence of the maximum Lorentz factor measured at the level of u2N(u) = 10−3 for normalized electron distributions, averaged for ct/L ∈ [9:10]. The point size indicates the simulation domain size L.

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