This dataset contains gravitational models using Slepian and spherical harmonic functions for Jupiter, derived from the high-precision Doppler measurements collected by NASA's Juno mission to Jupiter from periapsis 1 to 17. This dataset is intended to be paired with the following article submitted to the Journal of Geophysical Research-Planets: Marzia Parisi, Eli Galanti, William M. Folkner, Yohai Kaspi and Dustin R. Buccino. "Resolving the latitudinal short-scale gravity field of Jupiter using Slepian functions", Journal of Geophysical Research, 2020 (submitted Feb 2020). This dataset of gravity field models was produced in part at the Jet Propulsion Laboratory by the Juno Gravity Instrument Team and Interiors Working Group
This Doctoral Thesis reports on the analysis procedure for the data acquired by Juno and Cassini in ...
The Juno mission’s primary science objectives include the investigation of Jupiter interior structu...
Jupiter's spherical harmonic magnetic field and secular variation model coefficients with errors (68...
none19siThe combination of the Doppler data from the first two Juno science orbits provides an impro...
The latest estimation of Jupiter's gravitational field was obtained by processing the Doppler data f...
The upcoming Juno spacecraft measurements have the potential of improving our knowledge of Jupiter's...
Juno has been in a highly elliptical (average eccentricity e=0.95), nearly polar, 53-day orbit aroun...
The Juno gravity experiment, among the nine instruments onboard the spacecraft, is aimed at studying...
open27siThe gravity harmonics of a fluid, rotating planet can be decomposed into static components a...
The gravity harmonics of a fluid, rotating planet can be decomposed into static components arising f...
Juno is a NASA space mission to Jupiter, arriving at the planet in July 2016. Through accurate Doppl...
Juno is a NASA mission launched in 2011 with the goal of studying Jupiter. The probe will arrive to ...
The Juno spacecraft reached the mid‐point of its nominal mission in December 2018, after completing ...
The Juno spacecraft reached the mid-point of its nominal mission in December 2018, after completing ...
The Juno spacecraft has been collecting data to shed light on the planet's origin and characterize i...
This Doctoral Thesis reports on the analysis procedure for the data acquired by Juno and Cassini in ...
The Juno mission’s primary science objectives include the investigation of Jupiter interior structu...
Jupiter's spherical harmonic magnetic field and secular variation model coefficients with errors (68...
none19siThe combination of the Doppler data from the first two Juno science orbits provides an impro...
The latest estimation of Jupiter's gravitational field was obtained by processing the Doppler data f...
The upcoming Juno spacecraft measurements have the potential of improving our knowledge of Jupiter's...
Juno has been in a highly elliptical (average eccentricity e=0.95), nearly polar, 53-day orbit aroun...
The Juno gravity experiment, among the nine instruments onboard the spacecraft, is aimed at studying...
open27siThe gravity harmonics of a fluid, rotating planet can be decomposed into static components a...
The gravity harmonics of a fluid, rotating planet can be decomposed into static components arising f...
Juno is a NASA space mission to Jupiter, arriving at the planet in July 2016. Through accurate Doppl...
Juno is a NASA mission launched in 2011 with the goal of studying Jupiter. The probe will arrive to ...
The Juno spacecraft reached the mid‐point of its nominal mission in December 2018, after completing ...
The Juno spacecraft reached the mid-point of its nominal mission in December 2018, after completing ...
The Juno spacecraft has been collecting data to shed light on the planet's origin and characterize i...
This Doctoral Thesis reports on the analysis procedure for the data acquired by Juno and Cassini in ...
The Juno mission’s primary science objectives include the investigation of Jupiter interior structu...
Jupiter's spherical harmonic magnetic field and secular variation model coefficients with errors (68...