Chiral Pattern in Nonrotating Spherical Convection
Akira Kageyama, Nobuaki Ohno

TL;DR
This paper reports the discovery of a novel steady convection pattern in nonrotating spherical shells, characterized by tetrahedral symmetry and spiral roll arrangements, differing from previously known symmetric solutions.
Contribution
The study reveals a new convection pattern with tetrahedral symmetry and no reflection symmetry, identified through computer simulations in nonrotating spherical shells.
Findings
Discovered a new steady convection pattern with tetrahedral symmetry.
Pattern consists of six pairs of spiral rolls on 12 faces.
Two mirror-image configurations depending on spiral winding.
Abstract
When the Rayleigh number is low, Rayleigh-B\'enard 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 a new 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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Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies · Geophysics and Gravity Measurements · Solar and Space Plasma Dynamics
