Differential rotation in precession driven flow

Details Differential rotation in precession driven flow Differential rotation in precession driven flow

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..733..154t&link_type=abstract

MHD COUETTE FLOWS: Experiments and Models. AIP Conference Proceedings, Volume 733, pp. 154-164 (2004).

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Vortex Dynamics, Rotating Fluids, Flow Instabilities

Scientific paper

Magnetorotational instability (MRI) occurs for suitable dependencies of the angular velocity of a fluid with distance from a rotation axis. In the case of precession driven flow, this dependence is not well known. Precession driven flow does become unstable in experiments and numerical simulations. There is one well understood mechanism based on triad resonances by which these flows can become unstable. However, in the geophysical application and other contexts not directly accessible to simulation, other mechanisms such as MRI may become predominant.

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