A simple model of convection in the Jovian atmosphere, Icarus, vol.29, pp.255-260, 1976. ,
Jovian atmospheric dynamics: an update after Galileo and Cassini, Reports on Progress in Physics, vol.68, issue.8, pp.1935-1996, 2005. ,
Effects of differential rotation on the gravitational figures of Jupiter and Saturn, Icarus, vol.52, pp.509-515, 1982. ,
, New Constraints on the Composition of Jupiter from Galileo Measurements and Interior Models, vol.130, pp.534-539, 1997.
The asymmetric gravity field of Jupiter, Nature, this issue, 2017. ,
Jupiter's deep atmosphere revealed by Juno's asymmetric gravity measurements, Nature, this issue, 2017. ,
Zonal flow magnetic field interaction in the semiconducting region of giant planets, Icarus, vol.296, pp.59-72, 2017. ,
Models and Outstanding Questions, Ann. Rev. Earth Plan. Sci, vol.33, pp.493-530, 2005. ,
URL : https://hal.archives-ouvertes.fr/hal-00388278
NOTE: Gravitational Signature of Jupiter's Deep Zonal Flows, Icarus, vol.137, pp.357-359, 1999. ,
The effect of differential rotation on Jupiter's low-degree even gravity moments, Geophys. Res. Let, vol.44, pp.5960-5968, 2017. ,
Jupiter internal structure: the effect of different equations of state, Astron. Astrophys, vol.596, p.114, 2016. ,
URL : https://hal.archives-ouvertes.fr/hal-02295779
Comparing Jupiter interior structure models to Juno gravity measurements and the role of an expanded core, Geophys. Res. Let, vol.44, pp.4649-4659, 2017. ,
Ab Initio Equation of State for Hydrogen-Helium Mixtures with Recalibration of the Giant-planet Mass-Radius Relation, Astrophys. J, vol.774, p.148, 2013. ,
Ab Initio Equations of State for Hydrogen (H-REOS.3) and Helium (He-REOS.3) and their Implications for the Interior of Brown Dwarfs, Astrophys. J. Suppl, vol.215, p.21, 2014. ,
Concentric Maclaurin Spheroid Models of Rotating Liquid Planets, Astrophys. J, vol.768, p.43, 2013. ,
Differential rotation in Jupiter: A comparison of methods, Icarus, vol.267, pp.315-322, 2016. ,
Physics of planetary interiors, Astronomy and Astrophysics Series, 1978. ,
, A&AS, vol.109, pp.109-123, 1995.
The Evolution and Internal Structure of Jupiter and Saturn with Compositional Gradients, Astrophys. J, vol.829, 2016. ,
Hydrogen-helium demixing from first principles: From diamond anvil cells to planetary interiors, PhRvB, vol.87, p.174105, 2013. ,
The dynamics and helium distribution in hydrogen-helium fluid planets, Astrophys. J. Suppl, vol.35, pp.239-261, 1977. ,
An exploration of double diffusive convection in Jupiter as a result of hydrogen-helium phase separation, MNRAS, vol.447, pp.3422-3441, 2015. ,
Bayesian Evolution Models for Jupiter with Helium Rain and Double-diffusive Convection, Astrophys. J, vol.832, p.113, 2016. ,
Cosmochemistry and structure of the giant planets and their satellites, Icarus, vol.62, pp.4-15, 1985. ,
The Fuzziness of Giant Planets' Cores, Astrophys. J, vol.840, p.4, 2017. ,
A Preliminary Jupiter Model, Astrophys. J, vol.820, p.80, 2016. ,
An Equation of State for Low-Mass Stars and Giant Planets, Astrophys. J. Suppl, vol.99, p.713, 1995. ,
Shock Compression of Deuterium and the Interiors of Jupiter and Saturn, Astrophys. J, vol.609, pp.1170-1180, 2004. ,
A new vision of giant planet interiors: Impact of double diffusive convection, A&A, vol.540, p.20, 2012. ,
The atmosphere of Neptune -an analysis of radio occultation data acquired with Voyager 2, AJ, vol.103, pp.967-982, 1992. ,
A comparison of the interiors of Jupiter and Saturn, P&SS, vol.47, pp.1183-1200, 1999. ,
Thermal structure of Jupiter's atmosphere near the edge of a 5-micron hot spot in the north equatorial belt, JGR, vol.103, pp.22857-22890, 1998. ,
Determining the Initial Helium Abundance of the Sun, Astrophys. J, vol.719, pp.865-872, 2010. ,
Helium in Jupiter's atmosphere: Results from the Galileo probe helium interferometer experiment, JGR, vol.103, pp.22815-22830, 1998. ,
,
,
,
, Extended Data Fig. 1. Validation of the calculation of gravitational moments with the CEPAM method. The four panels provide a comparison of gravitational moments J 2 to J 10 calculated with various methods: CEPAM models with 241 radial layers (black points), CMS models with 800 layers (grey points, CEPAM models with 1041 layers