Saturation of the magnetorotational instability by stable magnetoacoustic modes

Edward Liverts, Yuri Shtemler, Michael Mond, Orkan M. Umurhan, Dmitry V. Bisikalo

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

The magnetorotational instability (MRI) of thin, vertically-isothermal Keplerian discs, under the influence of an axial magnetic field is investigated near the instability threshold. The nonlinear interaction of Alfven-Coriolis (MRI) modes with stable magnetoacoustic waves is considered. The transition of the Alfven-Coriolis modes to instability occurs when the linearized system has zero eigenvalue of multiplicity two. As a result the nonlinear ordinary differential equation that describes the evolution of the amplitude of the MRI mode near the threshold is of second order. Solutions of that amplitude equation reveal that the MRI is saturated to bursty periodical oscillations due to the transfer of energy to the stable magnetosonic modes.

Original languageEnglish
Title of host publicationSolar and Astrophysical Dynamos and Magnetic Activity
EditorsAlexander G. Kosovichev, Elisabete de Gouveia Dal Pino, Yihua Yan
Pages365-366
Number of pages2
EditionS294
DOIs
StatePublished - 1 Aug 2012

Publication series

NameProceedings of the International Astronomical Union
NumberS294
Volume8
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

Keywords

  • Accretion
  • instabilities
  • magnetohydrodynamics

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

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