66 citations · 99 across the 4 of their papers we have counts for
5 papers
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…
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's interior from Juno: Equation-of-state uncertainties and dilute core extent
S. Howard, T. Guillot, M. Bazot +10
The Juno mission has provided measurements of Jupiter s gravity field with an outstanding level of accuracy, leading to better constraints on the interior of the planet. Improving…
The Oscillatory Motion of Jupiter's Polar Cyclones Results From Vorticity Dynamics
Nimrod Gavriel, Yohai Kaspi
The polar cyclone at Jupiter's south pole and the five cyclones surrounding it oscillate in position and interact. These cyclones, observed since 2016 by NASA's Juno mission, prese…
Decoupling Jupiter's deep and atmospheric flows using the upcoming Juno gravity measurements and a dynamical inverse model
Eli Galanti, Yohai Kaspi
Observations of the flow on Jupiter exists essentially only for the cloud-level, which is dominated by strong east-west jet-streams. These have been suggested to result from dynami…