Penetrative magneto-convection of a rotating Boussinesq flow in $f$-planes
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arXiv
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2024
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| author | Xu, Fan Cai, Tao |
| author_facet | Xu, Fan Cai, Tao |
| contents | In this study, we conducted a linear instability analysis of penetrative magneto-convection in rapidly rotating Boussinesq flows within tilted f-planes, under the influence of a uniform background magnetic field. We integrated wave theory and convection theory to elucidate the penetration dynamics in rotating magneto-convection. Our findings suggest that efficient penetration in rapidly rotating flows with weakly stratified stable layers at low latitudes can be attributed to the resonance of wave transmission near the interface between unstable and stable layers. In the context of strongly stratified flows, we derived the scaling relationships of penetrative distances $Δ$ with the stability parameter $δ$. Our calculation shows that, for both rotation-dominated and magnetism-dominated flows, $Δ$ obeys a scaling of $Δ\sim O(δ^{-1/2})$. In rotation-dominated flows, we noted a general decrease in penetrative distance with increased rotational effect, and a minor decrease in penetrative distance with increased latitude. When a background magnetic field is introduced, we observed a significant shift in penetrative distance as the Elsasser number $Λ$ approaches one. The penetrative distance tends to decrease when $Λ\ll 1$ and increase when $Λ\gg 1$ with the rotational effect, indicating a transition from rotation-dominated to magnetism-dominated flow. We have further investigated the impact of the background magnetic field when it is not aligned with the rotational axis. This presents a notable contrast to the case where the magnetic field is parallel to the rotational axis. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2402_13736 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Penetrative magneto-convection of a rotating Boussinesq flow in $f$-planes Xu, Fan Cai, Tao Fluid Dynamics Solar and Stellar Astrophysics Atmospheric and Oceanic Physics Geophysics In this study, we conducted a linear instability analysis of penetrative magneto-convection in rapidly rotating Boussinesq flows within tilted f-planes, under the influence of a uniform background magnetic field. We integrated wave theory and convection theory to elucidate the penetration dynamics in rotating magneto-convection. Our findings suggest that efficient penetration in rapidly rotating flows with weakly stratified stable layers at low latitudes can be attributed to the resonance of wave transmission near the interface between unstable and stable layers. In the context of strongly stratified flows, we derived the scaling relationships of penetrative distances $Δ$ with the stability parameter $δ$. Our calculation shows that, for both rotation-dominated and magnetism-dominated flows, $Δ$ obeys a scaling of $Δ\sim O(δ^{-1/2})$. In rotation-dominated flows, we noted a general decrease in penetrative distance with increased rotational effect, and a minor decrease in penetrative distance with increased latitude. When a background magnetic field is introduced, we observed a significant shift in penetrative distance as the Elsasser number $Λ$ approaches one. The penetrative distance tends to decrease when $Λ\ll 1$ and increase when $Λ\gg 1$ with the rotational effect, indicating a transition from rotation-dominated to magnetism-dominated flow. We have further investigated the impact of the background magnetic field when it is not aligned with the rotational axis. This presents a notable contrast to the case where the magnetic field is parallel to the rotational axis. |
| title | Penetrative magneto-convection of a rotating Boussinesq flow in $f$-planes |
| topic | Fluid Dynamics Solar and Stellar Astrophysics Atmospheric and Oceanic Physics Geophysics |
| url | https://arxiv.org/abs/2402.13736 |