A comparison of the atmospheres of Jupiter and Saturn: deep atmospheric composition, cloud structure, vertical mixing, and origin
- 1 October 1999
- journal article
- research article
- Published by Elsevier in Planetary and Space Science
- Vol. 47 (10-11) , 1243-1262
- https://doi.org/10.1016/s0032-0633(99)00047-1
Abstract
No abstract availableKeywords
This publication has 81 references indexed in Scilit:
- Thermal structure of Jupiter's atmosphere near the edge of a 5‐μm hot spot in the north equatorial beltJournal of Geophysical Research, 1998
- Ammonia abundance in Jupiter's atmosphere derived from the attenuation of the Galileo probe's radio signalJournal of Geophysical Research, 1998
- The Galileo probe mission to Jupiter: Science overviewJournal of Geophysical Research, 1998
- Analysis of Jupiter north equatorial belt hot spots in the 4–5 μm range from Galileo/near‐infrared mapping spectrometer observations: Measurements of cloud opacity, water, and ammoniaJournal of Geophysical Research, 1998
- Galileo probe measurements of thermal and solar radiation fluxes in the Jovian atmosphereJournal of Geophysical Research, 1998
- Evolution and persistence of 5‐μm hot spots at the Galileo probe entry latitudeJournal of Geophysical Research, 1998
- Helium in Jupiter's atmosphere: Results from the Galileo probe Helium Interferometer ExperimentJournal of Geophysical Research, 1998
- The clouds of Jupiter: Results of the Galileo Jupiter Mission Probe Nephelometer ExperimentJournal of Geophysical Research: Planets, 1998
- The Jovian atmospheric window at 2.7 μm: A search for H2SIcarus, 1984
- Eddy diffusion at Saturn's homopauseGeophysical Research Letters, 1982