The stratorotational instability of Taylor-Couette flows with moderate Reynolds numbers

dc.bibliographicCitation.firstPage429
dc.bibliographicCitation.issue6
dc.bibliographicCitation.journalTitleGeophysical & astrophysical fluid dynamicseng
dc.bibliographicCitation.lastPage447
dc.bibliographicCitation.volume111
dc.contributor.authorRüdiger, G.
dc.contributor.authorSeelig, T.
dc.contributor.authorSchultz, M.
dc.contributor.authorGellert, M.
dc.contributor.authorEgbers, C.
dc.contributor.authorHarlander, U.
dc.date.accessioned2023-04-20T07:36:00Z
dc.date.available2023-04-20T07:36:00Z
dc.date.issued2017
dc.description.abstractIn view of new experimental data the instability against adiabatic nonaxisymmetric perturbations of a Taylor-Couette flow with an axial density stratification is considered in dependence of the Reynolds number (Re) of rotation and the Brunt-Väisälä number (Rn) of the stratification. The flows at and beyond the Rayleigh limit become unstable between a lower and an upper Reynolds number (for fixed Rn). The rotation can thus be too slow or too fast for the stratorotational instability. The upper Reynolds number above which the instability decays, has its maximum value for the potential flow (driven by cylinders rotating according to the Rayleigh limit) and decreases strongly for flatter rotation profiles finally leaving only isolated islands of instability in the (Rn/Re) map. The maximal possible rotation ratio μmax only slightly exceeds the shear value of the quasi-uniform flow with Uφ≃const. Along and between the lines of neutral stability the wave numbers of the instability patterns for all rotation laws beyond the Rayleigh limit are mainly determined by the Froude number Fr which is defined by the ratio between Re and Rn. The cells are highly prolate for Fr > 1 so that measurements for too high Reynolds numbers become difficult for axially bounded containers. The instability patterns migrate azimuthally slightly faster than the outer cylinder rotates.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/12045
dc.identifier.urihttp://dx.doi.org/10.34657/11078
dc.language.isoeng
dc.publisherLondon [u.a.] : Taylor and Francis
dc.relation.doihttps://doi.org/10.1080/03091929.2017.1382487
dc.relation.essn1029-0419
dc.relation.issn0309-1929
dc.rights.licenseCC BY-NC-ND 4.0 Unported
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0
dc.subject.ddc520
dc.subject.ddc550
dc.subject.otherAstrophysical fluid dynamicseng
dc.subject.otherstratified Taylor-Couette floweng
dc.subject.otherstratorotational instabilityeng
dc.titleThe stratorotational instability of Taylor-Couette flows with moderate Reynolds numberseng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccess
wgl.contributorAIP
wgl.subjectPhysikger
wgl.subjectGeowissenschaftenger
wgl.typeZeitschriftenartikelger
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