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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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| Publicado no: | Proc Math Phys Eng Sci |
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| Main Authors: | , , , , , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
The Royal Society Publishing
2020
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| Assuntos: | |
| Acesso em linha: | 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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