Physics – Plasma Physics
Scientific paper
Oct 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aps..dpprp1085j&link_type=abstract
American Physical Society, 43rd Annual Meeting of the APS Division of Plasma Physics October 29 - November 2, 2001 Long Beach, C
Physics
Plasma Physics
Scientific paper
Rapid angular momentum transport in accretion disks has been a longstanding astrophysical puzzle. The molecular viscosity of astrophysical gases and plasmas is completely inadequate to explain observationally inferred accretion rates. Recent theoretical work indicates that purely hydrodynamic instabilities are absent or ineffective, but that magnetorotational instabilities (MRI) are robust and support vigorous turbulence in electrically-conducting disks ranging from quasars and X-ray binaries to cataclysmic variables and perhaps even protoplanetary disks. Despite its popularity, however, MRI has never been demonstrated and studied in the laboratory. The possibility of studying MRI in a rotating liquid-metal disk (Couette flow) is explored by local(H. Ji, et al.), to appear in Mon. Not. Lett. Roy. Astron. Soc. (2001). and global(J. Goodman and H. Ji, submitted to J. Fluid Mech. (2001).) stability analysis and MHD simulations. Stability diagrams are drawn in dimensionless parameters, and also in terms of the angular velocities at the inner and outer cylinders. It is shown that MRI can be triggered in a moderately rapidly rotating table-top apparatus, using easy-to-handle metals such as gallium. Detailed analysis and apparatus designs as well as the results from prototype experiments using water to study Ekman circulation and nonlinear hydrodynamics instabilities are presented.
Goodman Jeremy
Ji Hantao
Kageyama Akira
Shoshan Eli
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