Comparatively little is known about atmospheric chemistry on Uranus and Neptune,
because remote spectral observations of these cold, distant 'Ice Giants' are challenging, and …

A major motivation for multiple atmospheric probe measurements at Uranus is the
understanding of dynamic processes that create and maintain spatial variation in thermal …

Planetary-scale giant storms erupt on Saturn quasiperiodically. There have been at least six
recorded occurrences of past eruptions, and the most recent one was in 2010, with its whole …

Despite being one of the weakest dimers in nature, low-spectral-resolution Voyager/IRIS
observations revealed the presence of (H 2) 2 dimers on Jupiter and Saturn in the 1980s …

Saturn's quasi-periodic planet-encircling storms are the largest convecting cumulus
outbursts in the Solar System. The last eruption was in 1990 (Sánchez-Lavega, A.[1994] …

Giant planets acquire gas, ices and rocks during the early formation stages of planetary
systems and thus inform us on the formation process itself. Proceeding from inside out …

Saturn's polar stratosphere exhibits the seasonal growth and dissipation of broad, warm
vortices poleward of~ 75° latitude, which are strongest in the summer and absent in winter …

The transformation of Jupiter's South Equatorial Belt (SEB) from its faded, whitened state in
2009-2010 (Fletcher et al., 2011b) to its normal brown appearance is documented via …

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 have developed and optimized a seasonal, radiative–convective model of Saturn's
upper troposphere and stratosphere. It is used to investigate Saturn's radiatively-forced …