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dc.contributor.authorGough, DO
dc.date.accessioned2017-10-03T07:41:42Z
dc.date.available2017-10-03T07:41:42Z
dc.date.issued2012-02-29
dc.identifier.citationD. O. Gough, “On Estimating Fluxes due to Small-Scale Turbulent Convection in a Rotating Star,” ISRN Astronomy and Astrophysics, vol. 2012, Article ID 987275, 10 pages, 2012. doi:10.5402/2012/987275
dc.identifier.issn2090-4738
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/267574
dc.description.abstract<jats:p>The way in which turbulent fluxes are usually represented in computations of large-scale flow in the convection zones of the sun and other stars is briefly described. A model of an ensemble of eddies that is capable of generalization to circumstances more complicated than the usual essentially spherically symmetrical convection zone is outlined. Generalization usually requires the introduction of new postulates, and, in so doing, also lays bare some of the assumptions, often implicit, in the usual mixing-length formalisms.</jats:p>
dc.publisherHindawi Limited
dc.rightsAll Rights Reserved
dc.rights.urihttps://www.rioxx.net/licenses/all-rights-reserved/
dc.titleOn Estimating Fluxes due to Small-Scale Turbulent Convection in a Rotating Star
dc.typeArticle
dc.date.updated2017-07-13T08:40:14Z
dc.description.versionPeer Reviewed
dc.language.rfc3066en
dc.rights.holderCopyright © 2012 D. O. Gough. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
prism.publicationNameISRN Astronomy and Astrophysics
dc.identifier.doi10.17863/CAM.13513
rioxxterms.versionofrecord10.5402/2012/987275
dc.contributor.orcidGough, DO [0000-0002-6086-2636]
dc.identifier.eissn2090-4746


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