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dc.contributor.authorLi, Ligangen_GB
dc.contributor.authorLiao, X.en_GB
dc.contributor.authorChan, K.H.en_GB
dc.contributor.authorZhang, Kekeen_GB
dc.date.accessioned2013-03-04T15:21:16Zen_GB
dc.date.accessioned2013-03-20T12:32:49Z
dc.date.issued2008-11-11en_GB
dc.description.abstractLinear and nonlinear convection in a rotating annular cylinder, under experimental boundary conditions, heated from below and rotating about a vertical axis are investigated. In addition to the usual physical parameters such as the Rayleigh and Taylor number, an important geometric parameter, the ratio of the inner to outer radius, enters into the problem. For intermediate ratios, linear stability analysis reveals that there exist two countertraveling convective waves which are nonlinearly significant: a retrograde wave located near the outer sidewall and a prograde wave adjacent to the inner sidewall. Several interesting phenomena of nonlinear convection are found: (i) tempospatially modulated countertraveling waves caused by an instability of the Eckhaus-Benjamin-Feir type, (ii) destructive countertraveling waves in which the existence or disappearance of the prograde wave is determined by its relative phase to the retrograde wave, and (iii) a saddle-node-type bifurcation in which the prograde wave takes an infinite amount of time to pass over the retrograde wave.en_GB
dc.identifier.citationVol. 78 (5), article 056303en_GB
dc.identifier.doi10.1103/PhysRevE.78.056303en_GB
dc.identifier.urihttp://hdl.handle.net/10036/4403en_GB
dc.language.isoenen_GB
dc.publisherAmerican Physical Societyen_GB
dc.titleLinear and nonlinear instabilities in rotating cylindrical Rayleigh-Bénard convectionen_GB
dc.typeArticleen_GB
dc.date.available2013-03-04T15:21:16Zen_GB
dc.date.available2013-03-20T12:32:49Z
dc.identifier.issn1539-3755en_GB
exeter.place-of-publicationUnited Statesen_GB
dc.descriptionCopyright © 2008 The American Physical Societyen_GB
dc.identifier.eissn1550-2376en_GB
dc.identifier.journalPhysical Review E - Statistical, Nonlinear and Soft matter Physicsen_GB


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