# Turbulence in Accretion Disks: Vorticity Generation and Angular Momentum Transport via the Global Baroclinic Instability

@article{Klahr2002TurbulenceIA, title={Turbulence in Accretion Disks: Vorticity Generation and Angular Momentum Transport via the Global Baroclinic Instability}, author={H. Klahr and Patrick Seitzer UCOLick Observatory and C. Physics and I. F. Astrophysik and U. Tuebingen and H Germany}, journal={The Astrophysical Journal}, year={2002}, volume={582}, pages={869-892} }

In this paper we present the global baroclinic instability as a source for vigorous turbulence leading to angular momentum transport in Keplerian accretion disks. We show by analytical considerations and three-dimensional radiation-hydrodynamic simulations that, in particular, protoplanetary disks have a negative radial entropy gradient, which makes them baroclinic. Two-dimensional numerical simulations show that a baroclinic flow is unstable and produces turbulence. These findings are tested… Expand

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