Confinement suppresses the effect of rotation on convection
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| Format: | Preprint |
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2025
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| _version_ | 1866915149685719040 |
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| author | Tripathi, V. K. Joshi, P. |
| author_facet | Tripathi, V. K. Joshi, P. |
| contents | We perform direct numerical simulations (DNS) to study the effect of bi-lateral confinement, i.e., the effect of aspect ratio, on the Rayleigh number (Ra) for the onset of wall-mode convection ($Ra_{wm}$) in rotating Rayleigh-Bénard convection (RBC) for various Ekman number E ($10^{-2}{\le}E{\le}10^{-5}$) and aspect ratio $Γ$ ($0.08{\le}Γ{\le}5$). For a given E, as the aspect ratio is lowered from a large value, $Ra_{wm}$ initially decreases slowly, reaching a minimum at $Γ=Γ_{min}$ ($Γ_{min}{\sim}E^{0.09}$). As $Γ$ is decreased further below $Γ_{min}$, $Ra_{wm}$ increases rapidly and for sufficiently strong confinement, i.e., $Γ<Γ_{\ast}$ ($Γ_{\ast}{\sim}E^{\frac{1}{3}}$), becomes indistinguishable from $Ra_{c}$, the critical Rayleigh number for non-rotating RBC, at the same $Γ$. We designate the ranges $Γ_{min}<Γ<5$ as the 'confinement-affected' regime and $Γ<Γ_{\ast}$ as the 'spatially constrained' regime. For a given rotation rate, the spatially constrained regime extends to higher Ra as the aspect ratio is decreased. We propose that in this regime, strong lateral confinement suppresses the horizontal velocity, and hence the Coriolis force, rendering rotation ineffective over most of the domain. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2502_09174 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Confinement suppresses the effect of rotation on convection Tripathi, V. K. Joshi, P. Fluid Dynamics We perform direct numerical simulations (DNS) to study the effect of bi-lateral confinement, i.e., the effect of aspect ratio, on the Rayleigh number (Ra) for the onset of wall-mode convection ($Ra_{wm}$) in rotating Rayleigh-Bénard convection (RBC) for various Ekman number E ($10^{-2}{\le}E{\le}10^{-5}$) and aspect ratio $Γ$ ($0.08{\le}Γ{\le}5$). For a given E, as the aspect ratio is lowered from a large value, $Ra_{wm}$ initially decreases slowly, reaching a minimum at $Γ=Γ_{min}$ ($Γ_{min}{\sim}E^{0.09}$). As $Γ$ is decreased further below $Γ_{min}$, $Ra_{wm}$ increases rapidly and for sufficiently strong confinement, i.e., $Γ<Γ_{\ast}$ ($Γ_{\ast}{\sim}E^{\frac{1}{3}}$), becomes indistinguishable from $Ra_{c}$, the critical Rayleigh number for non-rotating RBC, at the same $Γ$. We designate the ranges $Γ_{min}<Γ<5$ as the 'confinement-affected' regime and $Γ<Γ_{\ast}$ as the 'spatially constrained' regime. For a given rotation rate, the spatially constrained regime extends to higher Ra as the aspect ratio is decreased. We propose that in this regime, strong lateral confinement suppresses the horizontal velocity, and hence the Coriolis force, rendering rotation ineffective over most of the domain. |
| title | Confinement suppresses the effect of rotation on convection |
| topic | Fluid Dynamics |
| url | https://arxiv.org/abs/2502.09174 |