期刊
PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES
卷 368, 期 1916, 页码 1607-1633出版社
ROYAL SOC
DOI: 10.1098/rsta.2009.0251
关键词
fluid dynamics; magnetorotational instability; accretion discs
资金
- NASA [NNG05GD37G]
- University of Colorado
- Direct For Mathematical & Physical Scien
- Division Of Physics [923838] Funding Source: National Science Foundation
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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