4.4 Article

Chiral pattern in nonrotating spherical convection

Journal

PHYSICAL REVIEW FLUIDS
Volume 7, Issue 1, Pages -

Publisher

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevFluids.7.013502

Keywords

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Funding

  1. JSPS KAKENHI [17H02998]
  2. NIFS Collaboration Research Program [NIFS15KNSS062]
  3. Grants-in-Aid for Scientific Research [17H02998] Funding Source: KAKEN

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When the Rayleigh number is low, Rayleigh-Benard convection in a nonrotating spherical shell with central gravity has symmetric solutions in terms of three-dimensional discrete rotation. We found an alternative type of steady convection in a nonrotating spherical shell by computer simulations, which has the discrete rotational symmetry of a regular tetrahedron with no reflection symmetry.
When the Rayleigh number is low, Rayleigh-Benard convection in a nonrotating spherical shell with central gravity has symmetric solutions in terms of three-dimensional discrete rotation. All the known patterns with the regular polyhedral symmetries accompany reflection symmetry. We found an alternative type of steady convection in a nonrotating spherical shell by computer simulations. The pattern has the discrete rotational symmetry of a regular tetrahedron with no reflection symmetry. The convection consists of six pairs of spiral rolls placed on 12 faces of a spherical dodecahedron. Depending on the winding of the spirals, there are two possible configurations that are mirror images of one another.

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