Penetrative Convection in Partly Stratified Rapidly Rotating Spherical Shells

Many celestial objects are thought to host interfaces between convective and stable stratified interior regions. The interaction between both, e.g., the transfer of heat, mass, or angular momentum depends on whether and how flows penetrate into the stable layer. Powered from the unstable, convective...

Full description

Bibliographic Details
Main Authors: Wieland Dietrich, Johannes Wicht
Format: Article
Language:English
Published: Frontiers Media S.A. 2018-11-01
Series:Frontiers in Earth Science
Subjects:
Online Access:https://www.frontiersin.org/article/10.3389/feart.2018.00189/full
id doaj-d8f6f21667b743b8a26f02ebf741c4af
record_format Article
spelling doaj-d8f6f21667b743b8a26f02ebf741c4af2020-11-24T22:09:11ZengFrontiers Media S.A.Frontiers in Earth Science2296-64632018-11-01610.3389/feart.2018.00189414726Penetrative Convection in Partly Stratified Rapidly Rotating Spherical ShellsWieland DietrichJohannes WichtMany celestial objects are thought to host interfaces between convective and stable stratified interior regions. The interaction between both, e.g., the transfer of heat, mass, or angular momentum depends on whether and how flows penetrate into the stable layer. Powered from the unstable, convective regions, radial flows can pierce into the stable region depending on their inertia (overshooting). In rapidly rotating systems, the dynamics are strongly influenced by the Coriolis force and radial flows penetrate in stratified regions due to the geostrophic invariance of columnar convection even in the limit of vanishing inertia. Within this study, we numerically investigate both mechanisms and hence explore the nature of penetrative convection in rapidly rotating spherical shells. The study covers a broad range of system parameters, such as the strength of the stratification relative to the Coriolis force or the inertia. Guided by the application to Saturn, we model a sandwiched stable stratified layer (SSL) surrounded by two convective zones. A comprehensive analysis of the damping behavior of convective flows at the edges of the SSL showed that the mean penetration depth is controlled by the ratio of stratified and unstratified buoyancy gradients and is hence independent of rotation. A scaling law is derived and suggests that the penetration depth decreases with the square root of the ratio of unstabilizing and stabilizing entropy gradients. The influence of the Coriolis force, however, is evident by a modulation of the penetration depth along latitude, since convective columns are elongated vertically and hence pierce predominantly into the SSL around mid-latitudes and outside the tangent cylinder. Our result also show that the penetration depth decreases linearly with the flow length scale (low pass filter), confirming predictions from the linear theory of rotating partially stratified convection.https://www.frontiersin.org/article/10.3389/feart.2018.00189/fullstable stratificationrapidly rotating spherical shellspenetrative convectionnumerical simulationscaling laws
collection DOAJ
language English
format Article
sources DOAJ
author Wieland Dietrich
Johannes Wicht
spellingShingle Wieland Dietrich
Johannes Wicht
Penetrative Convection in Partly Stratified Rapidly Rotating Spherical Shells
Frontiers in Earth Science
stable stratification
rapidly rotating spherical shells
penetrative convection
numerical simulation
scaling laws
author_facet Wieland Dietrich
Johannes Wicht
author_sort Wieland Dietrich
title Penetrative Convection in Partly Stratified Rapidly Rotating Spherical Shells
title_short Penetrative Convection in Partly Stratified Rapidly Rotating Spherical Shells
title_full Penetrative Convection in Partly Stratified Rapidly Rotating Spherical Shells
title_fullStr Penetrative Convection in Partly Stratified Rapidly Rotating Spherical Shells
title_full_unstemmed Penetrative Convection in Partly Stratified Rapidly Rotating Spherical Shells
title_sort penetrative convection in partly stratified rapidly rotating spherical shells
publisher Frontiers Media S.A.
series Frontiers in Earth Science
issn 2296-6463
publishDate 2018-11-01
description Many celestial objects are thought to host interfaces between convective and stable stratified interior regions. The interaction between both, e.g., the transfer of heat, mass, or angular momentum depends on whether and how flows penetrate into the stable layer. Powered from the unstable, convective regions, radial flows can pierce into the stable region depending on their inertia (overshooting). In rapidly rotating systems, the dynamics are strongly influenced by the Coriolis force and radial flows penetrate in stratified regions due to the geostrophic invariance of columnar convection even in the limit of vanishing inertia. Within this study, we numerically investigate both mechanisms and hence explore the nature of penetrative convection in rapidly rotating spherical shells. The study covers a broad range of system parameters, such as the strength of the stratification relative to the Coriolis force or the inertia. Guided by the application to Saturn, we model a sandwiched stable stratified layer (SSL) surrounded by two convective zones. A comprehensive analysis of the damping behavior of convective flows at the edges of the SSL showed that the mean penetration depth is controlled by the ratio of stratified and unstratified buoyancy gradients and is hence independent of rotation. A scaling law is derived and suggests that the penetration depth decreases with the square root of the ratio of unstabilizing and stabilizing entropy gradients. The influence of the Coriolis force, however, is evident by a modulation of the penetration depth along latitude, since convective columns are elongated vertically and hence pierce predominantly into the SSL around mid-latitudes and outside the tangent cylinder. Our result also show that the penetration depth decreases linearly with the flow length scale (low pass filter), confirming predictions from the linear theory of rotating partially stratified convection.
topic stable stratification
rapidly rotating spherical shells
penetrative convection
numerical simulation
scaling laws
url https://www.frontiersin.org/article/10.3389/feart.2018.00189/full
work_keys_str_mv AT wielanddietrich penetrativeconvectioninpartlystratifiedrapidlyrotatingsphericalshells
AT johanneswicht penetrativeconvectioninpartlystratifiedrapidlyrotatingsphericalshells
_version_ 1725813198812086272