Identification of a non-axisymmetric mode in laboratory experiments searching for standard magnetorotational instability

The standard magnetorotational instability (SMRI) is a promising mechanism for turbulence and rapid accretion in astrophysical disks. It is a magnetohydrodynamic (MHD) instability that destabilizes otherwise hydrodynamically stable disk flow. Due to its microscopic nature at astronomical distances a...

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Detalles Bibliográficos
Autores principales: Wang, Yin, Gilson, Erik P., Ebrahimi, Fatima, Goodman, Jeremy, Caspary, Kyle J., Winarto, Himawan W., Ji, Hantao
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2022
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9363437/
https://www.ncbi.nlm.nih.gov/pubmed/35945242
http://dx.doi.org/10.1038/s41467-022-32278-0

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9363437/
https://www.ncbi.nlm.nih.gov/pubmed/35945242
http://dx.doi.org/10.1038/s41467-022-32278-0

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