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Transition to chaos and modal structure of magnetized Taylor–Couette flow
Taylor–Couette flow (TCF) is often used as a simplified model for complex rotating flows in the interior of stars and accretion discs. The flow dynamics in these objects is influenced by magnetic fields. For example, quasi-Keplerian flows in Taylor–Couette geometry become unstable to a travelling or...
| Autores principales: | , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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The Royal Society
2023
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9884522/ https://www.ncbi.nlm.nih.gov/pubmed/36709782 http://dx.doi.org/10.1098/rsta.2022.0120 |