WKB thresholds of standard, helical, and azimuthal magnetorotational instability

Oleg Kirillov, Frank Stefani

    Research output: Contribution to journalArticlepeer-review

    7 Citations (Scopus)

    Abstract

    We consider rotating flows of an electrically conducting, viscous and resistive fluid in an external magnetic field with arbitrary combinations of axial and azimuthal components. Within the short-wavelength approximation, the local stability of the flow is studied with respect to perturbations of arbitrary azimuthal wavenumbers. In the limit of vanishing magnetic Prandtl number (Pm) we find that the maximum critical Rossby number (Ro) for the occurrence of the magnetorotational instability (MRI) is universally governed by the Liu limit which is below the value for Keplerian rotation
    Original languageEnglish
    Pages (from-to)233-234
    JournalProceedings of the International Astronomical Union
    Volume8
    Issue numberS290
    DOIs
    Publication statusPublished - 21 Feb 2012

    Keywords

    • Magnetorotational instability
    • WKB approximation
    • accretion disks

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