396 citations · 1.2k across the 24 of their papers we have counts for
24 papers
From gas to ice giants: A unified mechanism for equatorial jets
Keren Duer-Milner, Nimrod Gavriel, Eli Galanti +2
The equatorial jets dominating the dynamics of the Jovian planets exhibit two distinct types of zonal flows: strongly eastward in the gas giants (superrotation) and strongly westwa…
Depth Dependent Dynamics Explain the Equatorial Jet Difference Between Jupiter and Saturn
Keren Duer, Eli Galanti, Yohai Kaspi
Jupiter's equatorial eastward zonal flows reach wind velocities of ~100 m/s, while on Saturn they are three times as strong and extend about twice as wide in latitude, despite the…
NeuralCMS: A deep learning approach to study Jupiter's interior
Maayan Ziv, Eli Galanti, Amir Sheffer +3
NASA's Juno mission provided exquisite measurements of Jupiter's gravity field that together with the Galileo entry probe atmospheric measurements constrains the interior structure…
Gas Giant Simulations of Eddy-Driven Jets Accompanied by Deep Meridional Circulation
Keren Duer, Eli Galanti, Yohai Kaspi
Jupiter's atmosphere comprises several dynamical regimes: the equatorial eastward flows and surrounding retrograde jets; the midlatitudes, with the eddy-driven, alternating jet-str…
The Shape of Jupiter and Saturn Based on Atmospheric Dynamics, Radio Occultations and Gravity Measurements
Eli Galanti, Yohai Kaspi, Tristan Guillot
The shape of the two gas giants, Jupiter and Saturn, is determined primarily by their rotation rate, and interior density distribution. It is also affected by their zonal winds, ca…
Jupiter Science Enabled by ESA's Jupiter Icy Moons Explorer
Leigh N. Fletcher, Thibault Cavalié, Davide Grassi +47
ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital…