Area of research
Astronomy and Astrophysics · Molecular Biology
Research interest
Research focused on Jupiter (rocket family) and Planet, with related work in Saturn, Gravitational field, Differential rotation. Notable publications include 'Comparing Jupiter interior structure models to Juno gravity measurements and the role of a dilute core', 'The Juno Mission', and 'Jupiter’s interior and deep atmosphere: The initial pole-to-pole passes with the Juno spacecraft'.
Study of Jupiter’s interior: Comparison of 2, 3, 4, 5, and 6 layer models
Jupiter’s interior from Juno: Equation-of-state uncertainties and dilute core extent
Relation of Gravity, Winds, and the Moment of Inertia of Jupiter and Saturn
Jupiter’s inhomogeneous envelope
Revelations on Jupiter's formation, evolution and interior: Challenges from Juno results
Juno Spacecraft Measurements of Jupiter’s Gravity Imply a Dilute Core
Loss of a satellite could explain Saturn’s obliquity and young rings
Equilibrium Tidal Response of Jupiter: Detectability by the Juno Spacecraft
Updated Equipotential Shapes of Jupiter and Saturn Using Juno and Cassini Grand Finale Gravity Science Measurements
Measurement and implications of Saturn’s gravity field and ring mass
Jupiter’s atmospheric jet streams extend thousands of kilometres deep
Measurement of Jupiter’s asymmetric gravity field
A suppression of differential rotation in Jupiter’s deep interior
Comparing Jupiter interior structure models to <i>Juno</i> gravity measurements and the role of a dilute core
Jupiter’s interior and deep atmosphere: The initial pole-to-pole passes with the Juno spacecraft
The effect of differential rotation on Jupiter's low‐degree even gravity moments
Understanding Jupiter's interior
2013. Concentric Maclaurin Spheroid Models of Rotating Liquid Planets
2016cited by 77position: first
The Concentric Maclaurin Spheroid method with tides and a rotational enhancement of Saturn’s tidal response
The gravitational signature of internal flows in giant planets: Comparing the thermal wind approach with barotropic potential-surface methods
Differential rotation in Jupiter: A comparison of methods
DETECTING THE WIND-DRIVEN SHAPES OF EXTRASOLAR GIANT PLANETS FROM TRANSIT PHOTOMETRY
2015cited by 6position: last
On the convergence of the theory of figures
AB INITIO EQUATION OF STATE FOR HYDROGEN-HELIUM MIXTURES WITH RECALIBRATION OF THE GIANT-PLANET MASS-RADIUS RELATION
Atmospheric confinement of jet streams on Uranus and Neptune
HIGH-PRECISION MACLAURIN-BASED MODELS OF ROTATING LIQUID PLANETS