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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 4.

Left panel: accuracy of total helicity conservation ﹩{ \mathcal H }(t)/{ \mathcal H }(0)-1﹩ compared for several simulations. Line colors and types are the same as in Figure 2. Middle panel: time evolution of the helicity profile ﹩\partial { \mathcal H }/\partial {A}_{z}﹩ for Run s14L1600. Right panel: time evolution of the magnetic energy profile ﹩\partial ({B}^{2})/\partial {A}_{z}﹩ for Run s14L1600. For the middle and right panels, the color scale indicates simulation time normalized to the light-crossing timescale L/c.

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