Ammonia abundance in Jupiter's atmosphere derived from the attenuation of the Galileo probe's radio signal
- 25 September 1998
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 103 (E10), 22847-22855
- https://doi.org/10.1029/98je01635
Abstract
No abstract availableKeywords
This publication has 23 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
- Galileo probe measurements of thermal and solar radiation fluxes in the Jovian atmosphereJournal of Geophysical Research, 1998
- Solar and Thermal Radiation in Jupiter's Atmosphere: Initial Results of the Galileo Probe Net Flux RadiometerScience, 1996
- The Helium Mass Fraction in Jupiter's AtmosphereScience, 1996
- The Galileo Probe Mass Spectrometer: Composition of Jupiter's AtmosphereScience, 1996
- Structure of the Atmosphere of Jupiter: Galileo Probe MeasurementsScience, 1996
- Galileo Doppler Measurements of the Deep Zonal Winds at JupiterScience, 1996
- Laboratory Measurements of the Microwave Properties of H2S under Simulated Jovian Conditions with an Application to NeptuneIcarus, 1994
- Submillimeter, millimeter, and microwave spectral line catalogApplied Optics, 1985
- Transition from Resonant to Nonresonant Line Shape in Microwave AbsorptionPhysical Review Letters, 1965