File Download
  Links for fulltext
     (May Require Subscription)
Supplementary

Article: On nonlinear multiarmed spiral waves in slowly rotating systems

TitleOn nonlinear multiarmed spiral waves in slowly rotating systems
Authors
Li, LLiao, XChan, KHZhang, K
KeywordsPhysics
Issue Date2010
PublisherAmerican Institute of Physics. The Journal's web site is located at http://ojps.aip.org/phf
Citation
Physics of Fluids, 2010, v. 22 n. 1, article no. 011701 How to Cite?
DOI: http://dx.doi.org/10.1063/1.3276277
AbstractStable nonlinear equilibria of convection in the form of quasistationary, multiarmed spiral waves, up to a maximum of six spiral arms, are found in a slowly rotating fluid confined within a thin spherical shell governed by the three-dimensional Navier–Stokes equation, driven by a radial unstable temperature gradient and affected by a weak Coriolis force. It is shown that three essential ingredients are generally required for the formation of the multiarmed spirals: the influence of slow rotation, large-aspect-ratio geometry and the effect of weak nonlinearity.
Persistent Identifierhttp://hdl.handle.net/10722/65461
ISSN
1070-6631
2021 Impact Factor: 4.980
2020 SCImago Journal Rankings: 1.188
ISI Accession Number ID
WOS:000274180800001
Funding AgencyGrant Number
NSFC110310773022/10633030
CAS2006 AA01A125
Hong Kong RGC700308
UK NERC
STFC
SSC
Funding Information:

L. L. and X. L. are supported by NSFC (Contract No. 110310773022/10633030), CAS grants, and 863-project (Grant No. 2006 AA01A125). K. H. C. is supported by Hong Kong RGC (Grant No. 700308) and K.Z. is supported by UK NERC and STFC grants. The numerical computation was supported by SSC.

 

DC FieldValueLanguage
dc.contributor.authorLi, L-
dc.contributor.authorLiao, X-
dc.contributor.authorChan, KH-
dc.contributor.authorZhang, K-
dc.date.accessioned2010-08-09T07:51:28Z-
dc.date.available2010-08-09T07:51:28Z-
dc.date.issued2010-
dc.identifier.citationPhysics of Fluids, 2010, v. 22 n. 1, article no. 011701-
dc.identifier.issn1070-6631-
dc.identifier.urihttp://hdl.handle.net/10722/65461-
dc.description.abstractStable nonlinear equilibria of convection in the form of quasistationary, multiarmed spiral waves, up to a maximum of six spiral arms, are found in a slowly rotating fluid confined within a thin spherical shell governed by the three-dimensional Navier–Stokes equation, driven by a radial unstable temperature gradient and affected by a weak Coriolis force. It is shown that three essential ingredients are generally required for the formation of the multiarmed spirals: the influence of slow rotation, large-aspect-ratio geometry and the effect of weak nonlinearity.-
dc.languageeng-
dc.publisherAmerican Institute of Physics. The Journal's web site is located at http://ojps.aip.org/phf-
dc.relation.ispartofPhysics of Fluids-
dc.rightsCopyright 2010 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. The following article appeared in Physics of Fluids, 2010, v. 22 n. 1, article no. 011701 and may be found at https://doi.org/10.1063/1.3276277-
dc.subjectPhysics-
dc.titleOn nonlinear multiarmed spiral waves in slowly rotating systemsen_HK
dc.typeArticleen_HK
dc.identifier.openurlhttp://library.hku.hk:4550/resserv?sid=HKU:IR&issn=1070-6631&volume=22&issue=1&spage=011701&epage=&date=2010&atitle=On+nonlinear+multiarmed+spiral+waves+in+slowly+rotating+systems-
dc.identifier.emailChan, KH: mkhchan@hku.hk-
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1063/1.3276277-
dc.identifier.scopuseid_2-s2.0-77950982231-
dc.identifier.hkuros170911-
dc.identifier.volume22-
dc.identifier.issue1-
dc.identifier.spagearticle no. 011701-
dc.identifier.epagearticle no. 011701-
dc.identifier.isiWOS:000274180800001-
dc.identifier.scopusauthoridLi, L=16304446000-
dc.identifier.scopusauthoridLiao, X=7202134147-
dc.identifier.scopusauthoridChan, KH=7406033542-
dc.identifier.scopusauthoridZhang, K=7404451892-
dc.identifier.issnl1070-6631-

Export via OAI-PMH Interface in XML Formats

OR

Export to Other Non-XML Formats