Parametric Survey of Nonaxisymmetric Accretion Disk Instabilities: Magnetorotational Instability to Super-Alfvénic Rotational Instability
Accretion disks are highly unstable to magnetic instabilities driven by shear flow, where classically, the axisymmetric, weak-field magnetorotational instability (MRI) has received much attention through local WKB approximations. In contrast, discrete nonaxisymmetric counterparts require a more invo...
Wedi'i Gadw mewn:
| Prif Awduron: | , , |
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| Fformat: | Artigo |
| Iaith: | Inglês |
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IOP Publishing
2024-01-01
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| Cyfres: | The Astrophysical Journal |
| Pynciau: | |
| Mynediad Ar-lein: | https://doi.org/10.3847/1538-4357/ad3d52 |
| Tagiau: |
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