| Literature DB >> 25062191 |
Martin Seilmayer1, Vladimir Galindo1, Gunter Gerbeth1, Thomas Gundrum1, Frank Stefani1, Marcus Gellert2, Günther Rüdiger2, Manfred Schultz2, Rainer Hollerbach3.
Abstract
The azimuthal version of the magnetorotational instability (MRI) is a nonaxisymmetric instability of a hydrodynamically stable differentially rotating flow under the influence of a purely or predominantly azimuthal magnetic field. It may be of considerable importance for destabilizing accretion disks, and plays a central role in the concept of the MRI dynamo. We report the results of a liquid metal Taylor-Couette experiment that shows the occurrence of an azimuthal MRI in the expected range of Hartmann numbers.Entities:
Year: 2014 PMID: 25062191 DOI: 10.1103/PhysRevLett.113.024505
Source DB: PubMed Journal: Phys Rev Lett ISSN: 0031-9007 Impact factor: 9.161