Magnetorotational instability: recent developments
The magnetorotational instability is believed to play an important role in accretion disc physics in extracting angular momentum from the disc and allowing accretion to take place. For this reason the instability has been the subject of numerous numerical simulations and, increasingly, laboratory ex...
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Published in | Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences Vol. 368; no. 1916; pp. 1607 - 1633 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
England
The Royal Society Publishing
13.04.2010
The Royal Society |
Subjects | |
Online Access | Get full text |
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Summary: | The magnetorotational instability is believed to play an important role in accretion disc physics in extracting angular momentum from the disc and allowing accretion to take place. For this reason the instability has been the subject of numerous numerical simulations and, increasingly, laboratory experiments. In this review, recent developments in both areas are surveyed, and a new theoretical approach to understanding the nonlinear processes involved in the saturation of the instability is outlined. |
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Bibliography: | istex:8D9D5E64F989C87BB5C5BA4366E6D522EC83D41E href:rsta20090251.pdf ArticleID:rsta20090251 ark:/67375/V84-978RKBRZ-1 Theme Issue 'Turbulent mixing and beyond' compiled and edited by Snezhana I. Abarzhi and Katepalli R. Sreenivasan ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 1364-503X 1471-2962 |
DOI: | 10.1098/rsta.2009.0251 |