Convection patterns in a spherical fluid shell

F. Feudel, K. Bergemann, L. S. Tuckerman, C. Egbers, B. Futterer, M. Gellert, and R. Hollerbach
Phys. Rev. E 83, 046304 – Published 6 April 2011

Abstract

Symmetry-breaking bifurcations have been studied for convection in a nonrotating spherical shell whose outer radius is twice the inner radius, under the influence of an externally applied central force field with a radial dependence proportional to 1/r5. This work is motivated by the GeoFlow experiment, which is performed under microgravity condition at the International Space Station where this particular central force can be generated. In order to predict the observable patterns, simulations together with path-following techniques and stability computations have been applied. Branches of axisymmetric, octahedral, and seven-cell solutions have been traced. The bifurcations producing them have been identified and their stability ranges determined. At higher Rayleigh numbers, time-periodic states with a complex spatiotemporal symmetry are found, which we call breathing patterns.

    • Received 13 July 2010

    DOI:https://doi.org/10.1103/PhysRevE.83.046304

    ©2011 American Physical Society

    Authors & Affiliations

    F. Feudel and K. Bergemann

    • Institut für Physik und Astronomie, Universität Potsdam, Karl-Liebknecht-Strasse 24/25, D-14476 Potsdam-Golm, Germany

    L. S. Tuckerman

    • PMMH (UMR 7636 CNRS - ESPCI - UPMC Paris 6 - UPD Paris 7), 10 rue Vauquelin, 75005 Paris, France

    C. Egbers and B. Futterer

    • Department of Aerodynamics and Fluid Mechanics, BTU Cottbus, Siemens-Halske-Ring 14, D-03046 Cottbus, Germany

    M. Gellert

    • Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14467 Potsdam, Germany

    R. Hollerbach

    • Department of Applied Mathematics, University of Leeds, Woodhouse Lane, Leeds, LS2 9JT, United Kingdom

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    Issue

    Vol. 83, Iss. 4 — April 2011

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