The camera onboard the Cassini spacecraft has allowed us to observe many of Saturn's cloud features. We present observations of Saturn's south polar vortex (SPV) showing that it shares some properties with terrestrial hurricanes: cyclonic circulation, warm central region (the eye) surrounded by a ring of high clouds (the eye wall), and convective clouds outside the eye. The polar location and the absence of an ocean are major differences. It also shares properties with the polar vortices on Venus, such as polar location, cyclonic circulation, warm center, and long lifetime, but the Venus vortices have cold collars and are not associated with convective clouds. The SPV's combination of properties is unique among vortices in the solar system
2 Saturn inhabits a dynamical regime of rapidly rotating, internally heated atmospheres similar to J...
We analyze the potential vorticity of Saturn's polar regions, as it is a fundamental dynamical trace...
We analyze the potential vorticity of Saturn's polar regions, as it is a fundamental dynamical trace...
The camera onboard the Cassini spacecraft has allowed us to observe many of Saturn's cloud features....
100 allowed. It is shortened compared to the last version. Ulyana Most planets with an atmosphere ha...
Most planets with an atmosphere havelarge vortices. Here, we present obser-vations of Saturn’s south...
High-resolution images of Saturn's southern hemisphere acquired by the Cassini Imaging Science Subsy...
The Cassini Imaging Science Subsystem (ISS) began observing Saturn in early February 2004. From anal...
There have been many significant shifts in the dynamics on Jupiter and Saturn during the Cassini era...
Near-infrared spectral maps of Saturn's north polar vortex obtained at high spatial resolution provi...
Venus has no seasons, slow rotation and a very massive atmosphere, which is mainly carbon dioxide wi...
Initial images of Venus's south pole by the Venus Express mission have shown the presence of a brigh...
International audienceInitial images of Venus's south pole by the Venus Express mission have shown t...
Venus has no seasons, slow rotation and a very massive atmosphere, which is mainly carbon dioxide wi...
We examine Saturn's atmospheric dynamics with observations in the visible range from ground-based te...
2 Saturn inhabits a dynamical regime of rapidly rotating, internally heated atmospheres similar to J...
We analyze the potential vorticity of Saturn's polar regions, as it is a fundamental dynamical trace...
We analyze the potential vorticity of Saturn's polar regions, as it is a fundamental dynamical trace...
The camera onboard the Cassini spacecraft has allowed us to observe many of Saturn's cloud features....
100 allowed. It is shortened compared to the last version. Ulyana Most planets with an atmosphere ha...
Most planets with an atmosphere havelarge vortices. Here, we present obser-vations of Saturn’s south...
High-resolution images of Saturn's southern hemisphere acquired by the Cassini Imaging Science Subsy...
The Cassini Imaging Science Subsystem (ISS) began observing Saturn in early February 2004. From anal...
There have been many significant shifts in the dynamics on Jupiter and Saturn during the Cassini era...
Near-infrared spectral maps of Saturn's north polar vortex obtained at high spatial resolution provi...
Venus has no seasons, slow rotation and a very massive atmosphere, which is mainly carbon dioxide wi...
Initial images of Venus's south pole by the Venus Express mission have shown the presence of a brigh...
International audienceInitial images of Venus's south pole by the Venus Express mission have shown t...
Venus has no seasons, slow rotation and a very massive atmosphere, which is mainly carbon dioxide wi...
We examine Saturn's atmospheric dynamics with observations in the visible range from ground-based te...
2 Saturn inhabits a dynamical regime of rapidly rotating, internally heated atmospheres similar to J...
We analyze the potential vorticity of Saturn's polar regions, as it is a fundamental dynamical trace...
We analyze the potential vorticity of Saturn's polar regions, as it is a fundamental dynamical trace...