Cassini-Huygens' exploration of the Saturn system: 13 years of discovery
L Spilker - Science, 2019 - science.org
The Cassini-Huygens mission to Saturn provided a close-up study of the gas giant planet, as
well as its rings, moons, and magnetosphere. The Cassini spacecraft arrived at Saturn in …
well as its rings, moons, and magnetosphere. The Cassini spacecraft arrived at Saturn in …
Dynamics and clouds in planetary atmospheres from telescopic observations
A Sánchez-Lavega, P Irwin, A García Muñoz - The Astronomy and …, 2023 - Springer
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 …
Venus, Mars, Jupiter, Saturn, Uranus and Neptune, the satellite Titan, and those of …
Long-lasting, deep effect of Saturn's giant storms
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 …
recorded occurrences of past eruptions, and the most recent one was in 2010, with its whole …
Phosphine on jupiter and saturn from cassini/cirs
The global distribution of phosphine (PH3) on Jupiter and Saturn is derived using 2.5 cm− 1
spectral resolution Cassini/CIRS observations. We extend the preliminary PH3 analyses on …
spectral resolution Cassini/CIRS observations. We extend the preliminary PH3 analyses on …
Saturn's deep atmospheric flows revealed by the Cassini grand finale gravity measurements
How deep do Saturn's zonal winds penetrate below the cloud level has been a decades‐
long question, with important implications not only for the atmospheric dynamics but also for …
long question, with important implications not only for the atmospheric dynamics but also for …
Methane and its isotopologues on Saturn from Cassini/CIRS observations
High spectral resolution observations from the Cassini Composite Infrared Spectrometer
[Flasar, FM, and 44 colleagues, 2004. Space Sci. Rev. 115, 169–297] are analysed to derive …
[Flasar, FM, and 44 colleagues, 2004. Space Sci. Rev. 115, 169–297] are analysed to derive …
[图书][B] Giant planets of our solar system: atmospheres, composition, and structure
P Irwin - 2009 - books.google.com
This book reviews the current state of knowledge of the atmospheres of the giant gaseous
planets: Jupiter, Saturn, Uranus, and Neptune. The current theories of their formation are …
planets: Jupiter, Saturn, Uranus, and Neptune. The current theories of their formation are …
[HTML][HTML] Mechanisms of jet formation on the giant planets
J Liu, T Schneider - Journal of the Atmospheric Sciences, 2010 - journals.ametsoc.org
Mechanisms of Jet Formation on the Giant Planets in: Journal of the Atmospheric Sciences
Volume 67 Issue 11 (2010) Jump to Content Jump to Main Navigation Logo Logo Logo Logo …
Volume 67 Issue 11 (2010) Jump to Content Jump to Main Navigation Logo Logo Logo Logo …
Saturn's zonal wind profile in 2004–2009 from Cassini ISS images and its long-term variability
E García-Melendo, S Pérez-Hoyos, A Sánchez-Lavega… - Icarus, 2011 - Elsevier
Five years of Cassini Imaging Science Subsystem images, from 2004 to 2009, are analyzed
in this work to retrieve global zonal wind profiles of Saturn's northern and southern …
in this work to retrieve global zonal wind profiles of Saturn's northern and southern …
Saturn's atmosphere in northern summer revealed by JWST/MIRI
LN Fletcher, ORT King, J Harkett… - Journal of …, 2023 - Wiley Online Library
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 …
(4.9–27.9 µm) in November 2022, tracing the seasonal evolution of temperatures, aerosols …