The excitation of spiral density waves through turbulent fluctuations in accretion discs - II. Numerical simulations with MRI-driven turbulence
Open Access
- 10 July 2009
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 397 (1) , 64-74
- https://doi.org/10.1111/j.1365-2966.2009.14800.x
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This publication has 15 references indexed in Scilit:
- MRI channel flows and their parasitesMonthly Notices of the Royal Astronomical Society, 2009
- MHD simulations of the magnetorotational instability in a shearing box with zero net fluxAstronomy & Astrophysics, 2007
- Properties and stability of freely propagating nonlinear density waves in accretion disksAstronomy & Astrophysics, 2007
- Hydromagnetic turbulence in computer simulationsComputer Physics Communications, 2002
- Planetary Torques as the Viscosity of Protoplanetary DisksThe Astrophysical Journal, 2001
- Linear Theory of Magnetized, Viscous, Self-gravitating Gas DisksThe Astrophysical Journal, 1996
- Dynamo-generated Turbulence and Large-Scale Magnetic Fields in a Keplerian Shear FlowThe Astrophysical Journal, 1995
- Local Three-dimensional Magnetohydrodynamic Simulations of Accretion DisksThe Astrophysical Journal, 1995
- The formation of the Cassini division in Saturn's ringsIcarus, 1978
- On sound generated aerodynamically I. General theoryProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1952