Magnetorotational instability in a rotating liquid metal annulus

Hantao Ji, Jeremy Goodman, Akira Kageyama

Research output: Contribution to journalArticle

122 Scopus citations

Abstract

Although the magnetorotational instability (MRI) has been widely accepted as a powerful accretion mechanism in magnetized accretion discs, it has not been realized in the laboratory. The possibility of studying MRI in a rotating liquid metal annulus (Couette flow) is explored by local and global stability analysis. 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. Practical issues of this proposed experiment are discussed.

Original languageEnglish (US)
Pages (from-to)L1-L5
JournalMonthly Notices of the Royal Astronomical Society
Volume325
Issue number2
DOIs
StatePublished - Aug 1 2001

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Accretion, accretion discs
  • Galaxy: disc
  • Instabilities
  • MHD
  • Magnetic fields
  • Planetary systems: protoplanetary discs

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