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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 2.

Evolution of the total energy components compared for different runs. All values are normalized to the initial total energy. Line colors indicate the mean value of the hot magnetization: σhot = 0.7 (gray), σhot = 1.4 (red), σhot = 2.7 (green), and σhot = 5.5 (blue). Line types indicate the simulation domain size: L = 400ρ0 (dotted), L = 800ρ0 (dashed), and L = 1600ρ0 (solid).

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