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Blazar Variability from Turbulence in Jets Launched by Magnetically Arrested Accretion Flows

  • Authors: Michael O' Riordan, Asaf Pe'er, and Jonathan C. McKinney

2017 The Astrophysical Journal 843 81.

  • Provider: AAS Journals

Caption: Figure 2.

Snapshot of the GRMHD model at ﹩t={\rm{15,700}}\,M﹩. The top panel shows the comoving electron number density and the bottom panel shows the comoving magnetic field strength. The white regions correspond to floor material that has been removed. Clearly, there are fluctuations in both n and B on scales smaller than rg.

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