The magnetorotational instability prefers three dimensions

The magnetorotational instability (MRI) occurs when a weak magnetic field destabilizes a rotating, electrically conducting fluid with inwardly increasing angular velocity. The MRI is essential to astrophysical disc theory where the shear is typically Keplerian. Internal shear layers in stars may als...

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Shranjeno v:
Bibliografske podrobnosti
izdano v:Proc Math Phys Eng Sci
Main Authors: Oishi, Jeffrey S., Vasil, Geoffrey M., Baxter, Morgan, Swan, Andrew, Burns, Keaton J., Lecoanet, Daniel, Brown, Benjamin P.
Format: Artigo
Jezik:Inglês
Izdano: The Royal Society Publishing 2020
Teme:
Research Article
Online dostop:https://ncbi.nlm.nih.gov/pmc/articles/PMC7016557/
https://ncbi.nlm.nih.gov/pubmed/32082064
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rspa.2019.0622
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