Stable stratification promotes multiple zonal jets in a turbulent Jovian dynamo model
arXiv:2012.06438 · doi:10.1016/j.icarus.2021.114514
Abstract
The ongoing NASA's Juno mission puts new constraints on the internal dynamics of Jupiter. Data gathered by its onboard magnetometer reveal a dipole-dominated surface magnetic field accompanied by strong localised magnetic flux patches. The gravity measurements indicate that the fierce surface zonal jets extend several thousands of kilometers below the cloud level before rapidly decaying below , being the mean Jovian radius at the one bar level. Several internal models suggest an intricate internal structure with a thin intermediate region in which helium would segregate from hydrogen, forming a compositionally-stratified layer. Here, we develop the first global Jovian dynamo which incorporates an intermediate stably-stratified layer between and . Analysing the energy balance reveals that the magnetic energy is almost one order of magnitude larger than kinetic energy in the metallic region, while most of the kinetic energy is pumped into zonal motions in the molecular envelope. Those result from the different underlying force hierarchy with a triple balance between Lorentz, Archimedean and ageostrophic Coriolis forces in the metallic core and inertia, buoyancy and ageostrophic Coriolis forces controlling the external layers. The simulation presented here is the first to demonstrate that multiple zonal jets and dipole-dominated dynamo action can be consolidated in a global simulation. The inclusion of an stable layer is a necessary ingredient that allows zonal jets to develop in the outer envelope without contributing to the dynamo action in the deeper metallic region. Stable stratification however also smooths out the small-scale features of the magnetic field by skin effect. These constraints suggest that possible stable layers in Jupiter should be located much closer to the surface ().
arXiv comment23 pages, 16 figures, 2 tables, accepted for publication in Icarus
References in corpus (32)
- Comparing Jupiter interior structure models to Juno gravity measurements and the role of a dilute core
- Efficient Spherical Harmonic Transforms aimed at pseudo-spectral numerical simulations
- Constraints on Deep-seated Zonal Winds Inside Jupiter and Saturn
- New models of Jupiter in the context of Juno and Galileo
- Spherical convective dynamos in the rapidly rotating asymptotic regime
- Effects of compressibility on driving zonal flow in gas giants
- Scaling regimes in spherical shell rotating convection
- Simulations of core convection in rotating A-type stars: Differential rotation and overshooting
- On differential rotation and overshooting in solar-like stars
- Scaling Laws for Planetary Dynamos
- Generation of equatorial jets by large-scale latent heating on the giant planets
- Approaching a realistic force balance in geodynamo simulations
- The Magnetic Furnace: Intense Core Dynamos in B-stars
- Force balance in numerical geodynamo simulations: a systematic study
- Explaining Jupiter's magnetic field and equatorial jet dynamics
- Energy Conservation and Gravity Waves in Sound-proof Treatments of Stellar Interiors: Part I Anelastic Approximations
- Theoretical seismology in 3D : nonlinear simulations of internal gravity waves in solar-like stars
- Understanding Jupiter's Interior
- Dynamo-based limit to the extent of a stable layer atop Earth's core
- Zonal Flow Magnetic Field Interaction in the Semi-Conducting Region of Giant Planets
- Zonal flow scaling in rapidly-rotating compressible convection
- Consistent scaling laws in anelastic spherical shell dynamos
- Combined magnetic and gravity measurements probe the deep zonal flows of the gas giants
- Anelastic spherical dynamos with radially variable electrical conductivity
- Relating force balances and flow length scales in geodynamo simulations
- Conduction in low Mach number flows: Part I Linear & weakly nonlinear regimes
- Dynamo Action of Jupiter's Zonal Winds
- Effects of a radially varying electrical conductivity on 3D numerical dynamos
- Characterising Jupiter's dynamo radius using its magnetic energy spectrum
- Penetrative Convection in Partly Stratified Rapidly Rotating Spherical Shells
- Dynamo Action in the Steeply Decaying Conductivity Region of Jupiter-like Dynamo Models
- Linking Zonal Winds and Gravity: The Relative Importance of Dynamic Self Gravity
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- Zonal jets experiments in the gas giants' zonostrophic regime
- Linking Zonal Winds and Gravity II: explaining the equatorially antisymmetric gravity moments of Jupiter
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- A Global Simulation of the Dynamo, Zonal Jets, and Vortices on Saturn
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- Gas Giant Simulations of Eddy-Driven Jets Accompanied by Deep Meridional Circulation
- Investigating Barotropic Zonal Flow in Jupiter's Deep Atmosphere using Juno Gravitational Data
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- A dynamo simulation generating Saturn-like small magnetic dipole tilts
- Global Turbulent Solar Convection: a Numerical Path Investigating Key Force Balances in the context of the Convective Conundrum
- Inflated hot Jupiters: Inferring average atmospheric velocity via Ohmic models coupled with internal dynamo evolution
- On the meaning of the dynamo radius in giant planets with stable layers
- Examining NHD vs QHD in the GCM THOR with non-grey radiative transfer for the hot Jupiter regime
- Westward hotspot offset explained by subcritical dynamo action in an ultra-hot Jupiter atmosphere
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- Non-linear saturation and energy transport in global simulations of magneto-thermal turbulence in the stratified intracluster medium
- Model of deep zonal flows in giant planets
- A Possible Mechanism to Explain the Prograde Equatorial Jet of a Jupiter-like Gaseous Giant