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Bifurcations of rotating waves in rotating spherical shell convection

  • The dynamics and bifurcations of convective waves in rotating and buoyancy-driven spherical Rayleigh-Benard convection are investigated numerically. The solution branches that arise as rotating waves (RWs) are traced by means of path-following methods, by varying the Rayleigh number as a control parameter for different rotation rates. The dependence of the azimuthal drift frequency of the RWs on the Ekman and Rayleigh numbers is determined and discussed. The influence of the rotation rate on the generation and stability of secondary branches is demonstrated. Multistability is typical in the parameter range considered.

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Author details:Fred Feudel, L. S. Tuckerman, Marcus Gellert, Norbert SeehaferORCiD
DOI:https://doi.org/10.1103/PhysRevE.92.053015
ISSN:1539-3755
ISSN:1550-2376
Pubmed ID:https://pubmed.ncbi.nlm.nih.gov/26651787
Title of parent work (English):Physical Review E
Publisher:American Physical Society
Place of publishing:Woodbury
Publication type:Article
Language:English
Date of first publication:2015/11/20
Publication year:2015
Publishing institution:Universität Potsdam
Release date:2017/03/17
Tag:flow; fluid shells; hopf-bifurcation; magnetoconvection; nonsymmetric linear-systems; number; onset; thermal-convection
Volume:92
Issue:5
Organizational units:Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie
Peer review:Referiert
License (German):License LogoKeine öffentliche Lizenz: Unter Urheberrechtsschutz
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