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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 1.

Snapshot of the GRMHD model showing the quantity ﹩{{nB}}^{2}{{\rm{\Theta }}}^{2}﹩, which is proportional to the comoving synchrotron power per unit volume. The floor material has been excised from the funnel region. Both the synchrotron power and the synchrotron self-Compton component are strongly dominated by the inner ﹩\sim 5\,M﹩.

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