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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 2.

Magnitude of ﹩{\omega }_{z},\;﹩ the z-component of vorticity, in the y = 0 plane at times ﹩t=6,84,160,180,220,\;﹩ and ﹩400h/{c}_{{\rm{iso,0}}}﹩ (from left to right). The color table is set so that green is ﹩{\omega }_{z}=0,\;﹩ and red/blue saturate at ﹩{\omega }_{z}=\pm 0.2.﹩

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