Zonal Flow Magnetic Field Interaction in the Semi-Conducting Region of Giant Planets

Abstract

All four giant planets in the Solar System feature zonal flows on the order of 100 m/s in the cloud deck, and large-scale intrinsic magnetic fields on the order of 1 Gauss near the surface. The vertical structure of the zonal flows remains obscure. The end-member scenarios are shallow flows confined in the radiative atmosphere and deep flows throughout the entire planet. The electrical conductivity increases rapidly yet smoothly as a function of depth inside Jupiter and Saturn. Deep zonal flows will inevitably interact with the magnetic field, at depth with even modest electrical conductivity. Here we investigate the interaction between zonal flows and magnetic fields in the semi-conducting region of giant planets. Employing mean-field electrodynamics, we show that the interaction will generate detectable poloidal magnetic field perturbations spatially correlated with the deep zonal flows. Assuming the peak amplitude of the dynamo alpha-effect to be 0.1 mm/s, deep zonal flows on the order of 0.1 - 1 m/s in the semi-conducting region of Jupiter and Saturn would generate poloidal magnetic perturbations on the order of 0.01% - 1% of the background dipole field. These poloidal perturbations should be detectable with the in-situ magnetic field measurements from the Juno mission and the Cassini Grand Finale. This implies that magnetic field measurements can be employed to constrain the properties of deep zonal flows in the semi-conducting region of giant planets.

38 pages, 12 figures, revised submission to Icarus

References in corpus (9)

• Magnetic Cycles in a Convective Dynamo Simulation of a Young Solar-type Star
• Constraints on Deep-seated Zonal Winds Inside Jupiter and Saturn
• Phase separation in hydrogen-helium mixtures at Mbar pressures
• Explaining Jupiter's magnetic field and equatorial jet dynamics
• Problems with kinematic mean field electrodynamics at high magnetic Reynolds numbers
• Large-scale Dynamo Action Driven by Velocity Shear and Rotating Convection
• Magnetic-field generation in helical turbulence
• Dynamics of cloud features on Uranus
• On Large-Scale Dynamo Action at High Magnetic Reynolds Number

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