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INEFFICIENT DRIVING OF BULK TURBULENCE BY ACTIVE GALACTIC NUCLEI IN A HYDRODYNAMIC MODEL OF THE INTRACLUSTER MEDIUM

  • Authors: Christopher S. Reynolds, Steven A. Balbus, and Alexander A. Schekochihin

2015 The Astrophysical Journal 815 41.

  • Provider: AAS Journals

Caption: Figure 8.

Spacetime plots of “core samples” (﹩x=y=0,z\in [0,8h]﹩) of the tracer-﹩{\mu }_{2}﹩ for the ﹩{z}_{0}=2h﹩ (left) and ﹩{z}_{0}=h﹩ (right) “trapped” cases, employing a logarithmic color table spanning the range of ﹩{\mu }_{2}={10}^{-4}﹩ (light yellow) to ﹩{\mu }_{2}=1﹩ (black). Time is measured in units of ﹩h/{c}_{{\rm{iso,0}}}.﹩

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