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The Dynamics of Jupiter's and Saturn's Weather Layers: A Synthesis After Cassini and Juno
PL Read - Annual Review of Fluid Mechanics, 2024 - annualreviews.org
Until recently, observations of the giant planets of our Solar System were confined to
sampling relatively shallow regions of their atmospheres, leaving many uncertainties as to …
sampling relatively shallow regions of their atmospheres, leaving many uncertainties as to …
Quenching of zonal winds in Jupiter's interior
UR Christensen, PN Wulff - Proceedings of the National Academy of …, 2024 - pnas.org
Gravity and magnetic field data obtained by the Juno mission show that Jupiter's strong
zonal winds extend a few thousand kilometers into the interior, but are quenched above the …
zonal winds extend a few thousand kilometers into the interior, but are quenched above the …
NeuralCMS: A deep learning approach to study Jupiter's interior
Context. NASA's Juno mission provided exquisite measurements of Jupiter's gravity field that
together with the Galileo entry probe atmospheric measurements constrains the interior …
together with the Galileo entry probe atmospheric measurements constrains the interior …
Io's tidal response precludes a shallow magma ocean
Io experiences tidal deformation as a result of its eccentric orbit around Jupiter, which
provides a primary energy source for Io's continuing volcanic activity and infrared emission …
provides a primary energy source for Io's continuing volcanic activity and infrared emission …
Testing general relativity with Juno at Jupiter
The Juno spacecraft has been orbiting Jupiter since 2016 July to deepen our
comprehension of the solar system by studying the gas giant. The radio science experiment …
comprehension of the solar system by studying the gas giant. The radio science experiment …
Contributions of Jupiter's deep‐reaching surface winds to magnetic field structure and secular variation
J Wicht, UR Christensen - Journal of Geophysical Research …, 2024 - Wiley Online Library
NASA's Juno mission delivered gravity data of exceptional quality. They indicate that the
zonal winds, which rule the dynamics of Jupiter's cloud deck, must slow down significantly …
zonal winds, which rule the dynamics of Jupiter's cloud deck, must slow down significantly …
Depth dependent dynamics explain the equatorial jet difference between Jupiter and Saturn
Jupiter's equatorial eastward zonal flows reach wind velocities of∼ 100 ms− 1, while on
Saturn they are three times as strong and extend about twice as wide in latitude, despite the …
Saturn they are three times as strong and extend about twice as wide in latitude, despite the …
Uranus Orbiter and Probe: A Radio Science Investigation to Determine the Planet's Gravity Field, Depth of the Winds, and Tidal Deformations
M Parisi, AJ Friedson, CR Mankovich… - The Planetary …, 2024 - iopscience.iop.org
Abstract The most recent Planetary Science and Astrobiology Decadal Survey has proposed
Uranus as the target for NASA's next large-scale mission. The interior structure and …
Uranus as the target for NASA's next large-scale mission. The interior structure and …
Determination of Jupiter's Pole Orientation from Juno Radio Science Data
The extreme accuracy of Juno radio science data allows us to perform very precise orbit
determination experiments. While previous works focused on the estimation of the …
determination experiments. While previous works focused on the estimation of the …
Characterizing Jupiter's interior using machine learning reveals four key structures
Context. The internal structure of Jupiter is constrained by the precise gravity field
measurements by NASA's Juno mission, atmospheric data from the Galileo entry probe, and …
measurements by NASA's Juno mission, atmospheric data from the Galileo entry probe, and …