Abstract Before Cassini, scientists viewed Saturn's unique features only from Earth and from
three spacecraft flying by. During more than a decade orbiting the gas giant, Cassini studied …

The outer planets of our Solar System display a myriad of interesting cloud features, of
different colors and sizes. The differences between the types of observed clouds suggest a …

Numerical studies of small-scale forced, two-dimensional turbulent flows on the surface of a
rotating sphere have revealed strong large-scale anisotropization that culminates in the …

Numerical Simulations of Forced Shallow-Water Turbulence: Effects of Moist Convection on
the Large-Scale Circulation of Jupiter and Saturn in: Journal of the Atmospheric Sciences …

Three-dimensional numerical simulations show that large-scale latent heating resulting from
condensation of water vapor can produce multiple zonal jets similar to those on the gas …

Abstract In December 2000, the Cassini fly-by near Jupiter delivered high-resolution images
of Jupiter's clouds over the entire planet in a band between 50° N and 50° S. Three daily …

The Cassini mission unveiled the intense and diverse activity in Saturn's atmosphere:
banded jets, waves, vortices, equatorial oscillations. To set the path towards a better …

We investigate the dynamics of Jupiter's upper troposphere and lower stratosphere using a
General Circulation Model that includes two-stream radiation and optional heating from …

The latitude‐altitude map of ammonia mixing ratio shows an ammonia‐rich zone at 0–5° N,
with mixing ratios of 320–340 ppm, extending from 40–60 bars up to the ammonia cloud …

We describe the use of Isca for the hierarchical modeling of Solar System planets, with
particular attention paid to Earth, Mars, and Jupiter. Isca is a modeling framework for the …