Tracer dye experiments in a Milky Way-mass galaxy simulation show that circumgalactic gas mixing is best predicted by velocity dispersion and shear tensors, with nearly linear diffusion scaling.
Turbulence and Diffusion, @doi 10.1007/978-3-540-68222-6
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Understanding gas mixing in the circumgalactic medium
Tracer dye experiments in a Milky Way-mass galaxy simulation show that circumgalactic gas mixing is best predicted by velocity dispersion and shear tensors, with nearly linear diffusion scaling.