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 …

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 …

The ice giants Uranus and Neptune have hydrogen-based atmospheres with several
constituents that condense in their cold upper atmospheres. A small number of bright cloud …

Deep elemental composition is a challenging measurement to achieve in the giant planets
of the solar system. Yet, knowledge of the deep composition offers important insights in the …

Abstract Jupiter's Great Red Spot (GRS), a giant anticyclone, is the largest and longest‐lived
of all the vortices observed in planetary atmospheres. During its history, the GRS has shrunk …

On May 31, 2020 a convective storm appeared in one small cyclone in the South Temperate
Belt (STB) of Jupiter. The storm, nicknamed as Clyde's Spot, had an explosive start and …

Imaging observations of Jupiter with high spatial resolution were acquired beginning in
2016, with a cadence of 53 days to coincide with atmospheric observations of the Juno …

Here we describe a cyclone at 50∘ N in the atmosphere of Saturn that was the source of
eight separate convective storms. The storm clouds that appeared bright in scattered …

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 …