This review presents an insight into our current knowledge of the atmospheres of the planets
Venus, Mars, Jupiter, Saturn, Uranus and Neptune, the satellite Titan, and those of …

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 …

Saturn's northern summertime hemisphere was mapped by JWST/Mid‐Infrared Instrument
(4.9–27.9 µm) in November 2022, tracing the seasonal evolution of temperatures, aerosols …

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 measured the horizontal winds in Jupiter's Great Red Spot (GRS) using data from the
WFC3/UVIS instrument on board the Hubble Space Telescope (HST). The data cover 11 …

Each of the giant planets, Jupiter, Saturn, Uranus, and Neptune, has been observed by at
least one robotic spacecraft mission. However, these missions are infrequent; Uranus and …

Moist convective storms in Jupiter develop frequently and can trigger atmospheric activity of
different scales, from localized storms to planetary-scale disturbances including convective …

This paper presents an analysis of large-scale vortices in the atmospheres of gas giants,
focusing on a detailed study conducted using the Saturn-DYNAMICO global climate model …

Saturn's convective storms usually fall in two categories. One consists of mid-sized storms∼
2,000 km wide, appearing as irregular bright cloud systems that evolve rapidly, on scales of …

We examine Saturn's atmospheric dynamics with observations in the visible range from
ground-based telescopes and Hubble Space Telescope (HST). We present a detailed …