Evolution and persistence of 5‐μm hot spots at the Galileo probe entry latitude
- 25 September 1998
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 103 (E10), 23051-23069
- https://doi.org/10.1029/98je00696
Abstract
No abstract availableKeywords
This publication has 34 references indexed in Scilit:
- Characteristics of the Galileo probe entry site from Earth‐based remote sensing observationsJournal of Geophysical Research, 1998
- Thermal structure of Jupiter's atmosphere near the edge of a 5‐μm hot spot in the north equatorial beltJournal 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
- Cloud structure and atmospheric composition of Jupiter retrieved from Galileo near‐infrared mapping spectrometer real‐time spectraJournal of Geophysical Research, 1998
- Observations and Analysis of Longitudinal Thermal Waves on JupiterIcarus, 1997
- Richardson number constraints for the Jupiter and outer planet wind regimeGeophysical Research Letters, 1995
- Are the Giant Planets Fully Convective?Icarus, 1994
- Planetary waves in Jupiter's equatorial atmosphereIcarus, 1990
- Jovian cloud structure and velocity fieldsNature, 1979
- The Effects of Latitudinal Shear on Equatorial Waves. Part II: Applications to the AtmosphereJournal of the Atmospheric Sciences, 1978