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The combined effects of buoyancy, rotation, and shear on phase boundary evolution

Abstract:
We use well-resolved numerical simulations to study the combined effects of buoyancy, pressure-driven shear and rotation on the melt rate and morphology of a layer of pure solid overlying its liquid phase in three dimensions at a Rayleigh number $Ra=1.25\times 10^5$ . During thermal convection, we find that the rate of melting of the solid phase varies non-monotonically with the strength of the imposed shear flow. In the absence of rotation, depending on whether buoyancy or shear dominates the flow, we observe either domes or ridges aligned in the direction of the shear flow, respectively. Furthermore, we show that the geometry of the phase boundary has important effects on the magnitude and evolution of the heat flux in the liquid layer. In the presence of rotation, the strength of which is characterized by the Rossby number, $Ro$ , we observe that for $Ro={O}(1)$ , the mean flow in the interior is perpendicular to the direction of the constant horizontal applied pressure gradient. As the magnitude of this pressure gradient increases, the geometry of solid–liquid interface evolves from the voids characteristic of melting by rotating convection, to grooves oriented perpendicular or obliquely to the direction of the pressure gradient.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1017/jfm.2022.304

Authors

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Role:
Author
ORCID:
0000-0001-9299-7570
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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0001-8450-2697
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Role:
Author
ORCID:
0000-0002-1676-9645


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Funder identifier:
10.13039/501100004359
Grant:
638-2013-9243


Publisher:
Cambridge University Press
Journal:
Journal of Fluid Mechanics More from this journal
Volume:
941
Pages:
a39
Article number:
A39
Publication date:
2022-05-03
DOI:
EISSN:
1469-7645
ISSN:
0022-1120


Language:
English
Keywords:
Pubs id:
1259548
Local pid:
pubs:1259548
Source identifiers:
W3176008146
Deposit date:
2026-04-24
ARK identifier:
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