Earth-Based Radio Tracking of the Galileo Probe for Jupiter Wind Estimation
- 31 January 1997
- journal article
- other
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 275 (5300) , 644-646
- https://doi.org/10.1126/science.275.5300.644
Abstract
Although the Galileo probe was designed to communicate only to the orbiter, the probe radio signal was detected at two Earth-based radio observatories where the signal was a billion times weaker. The measured signal frequency was used to derive a vertical profile of the jovian zonal wind speed. Due to the mission geometry, the Earth-based wind estimates are less sensitive to descent trajectory errors than estimates based on probe-orbiter Doppler measurements. The two estimates of wind profiles agree qualitatively; both show high wind speeds at all depths sampled.Keywords
This publication has 12 references indexed in Scilit:
- Penetrative Convection and Zonal Flow on JupiterScience, 1996
- Solar and Thermal Radiation in Jupiter's Atmosphere: Initial Results of the Galileo Probe Net Flux RadiometerScience, 1996
- Structure of the Atmosphere of Jupiter: Galileo Probe MeasurementsScience, 1996
- Comparison of Galileo-Probe and Earth-Based Translation Rates of Jupiter's Equatorial CloudsScience, 1996
- Retrieval of a Wind Profile from the Galileo Probe Telemetry SignalPublished by Springer Nature ,1992
- Jupiter: New estimates of the mean zonal flow at the cloud levelIcarus, 1986
- Jovian Winds from Voyager 2. Part I: Zonal Mean CirculationJournal of the Atmospheric Sciences, 1982
- Zonal and meridional circulation of the lower atmosphere of Venus determined by radio interferometryJournal of Geophysical Research, 1980
- A simple model of convection in the Jovian atmosphereIcarus, 1976
- Differential Rotation in Stellar Convection ZonesThe Astrophysical Journal, 1970