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Vortices in Thin, Compressible, Unmagnetized Disks
2005
Astrophysical Journal
We consider the formation and evolution of vortices in a hydrodynamic shearing-sheet model. The evolution is done numerically using a version of the ZEUS code. Consistent with earlier results, an injected vorticity field evolves into a set of long-lived vortices, each of which has a radial extent comparable to the local scale height. But we also find that the resulting velocity field has a positive shear stress, . This effect appears only at high resolution. The transport, which decays with
doi:10.1086/497358
fatcat:wcgilh7zyvafrp2jqcc3swya6u