Linking Zonal Winds and Gravity II: explaining the equatorially antisymmetric gravity moments of Jupiter
Wieland Dietrich, Paula Wulff, Johannes Wicht, Ulrich R., Christensen

TL;DR
This study proposes a new model for Jupiter's zonal winds that explains gravity measurements by suggesting winds are shallow near the equator and deeper at higher latitudes, aligning with magnetic and atmospheric constraints.
Contribution
It introduces an alternative wind structure that accounts for equatorial antisymmetry and matches gravity, magnetic, and atmospheric observations without artificial regularization.
Findings
Winds are shallow near the equator and deeper at higher latitudes.
The preferred wind structure is 50% deeper than previous models.
The model explains gravity moments while satisfying magnetic and atmospheric constraints.
Abstract
The recent gravity field measurements of Jupiter (Juno) and Saturn (Cassini) confirm the existence of deep zonal flows reaching to a depth of 5\% and 15\% of the respective radius. Relating the zonal wind induced density perturbations to the gravity moments has become a major tool to characterise the interior dynamics of gas giants. Previous studies differ with respect to the assumptions made on how the wind velocity relates to density anomalies, on the functional form of its decay with depth, and on the continuity of antisymmetric winds across the equatorial plane. Most of the suggested vertical structures exhibit a rather smooth radial decay of the zonal wind, which seems at odds with the observed secular variation of the magnetic field and the prevailing geostrophy of the zonal winds. Moreover, the results relied on an artificial equatorial regularisation or ignored the equatorial…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
