![Dynamics / Taylor–Couette flow / Magnetorotational instability / Turbulence / Hydrodynamic stability / Accretion disc / Reynolds number / Reynolds stress / Couette flow / Fluid dynamics / Physics / Fluid mechanics Dynamics / Taylor–Couette flow / Magnetorotational instability / Turbulence / Hydrodynamic stability / Accretion disc / Reynolds number / Reynolds stress / Couette flow / Fluid dynamics / Physics / Fluid mechanics](https://www.pdfsearch.io/img/a59121055bfee5ba46e646f6a6273031.jpg) Date: 2006-11-15 15:09:40Dynamics Taylor–Couette flow Magnetorotational instability Turbulence Hydrodynamic stability Accretion disc Reynolds number Reynolds stress Couette flow Fluid dynamics Physics Fluid mechanics | | Vol 444 | 16 November 2006 | doi:nature05323 LETTERS Hydrodynamic turbulence cannot transport angular momentum effectively in astrophysical disks Hantao Ji1, Michael Burin1{, Ethan Schartman1 & Jeremy Goodman1Add to Reading ListSource URL: mri.pppl.govDownload Document from Source Website File Size: 341,91 KBShare Document on Facebook
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