Voyager ultraviolet stellar occultation measurements of the composition and thermal profiles of the Saturnian upper atmosphere
- 1 October 1982
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 9 (10) , 1147-1150
- https://doi.org/10.1029/gl009i010p01147
Abstract
Occultation of the star δ‐Scorpii by Saturn as recorded by the Voyager Ultraviolet Spectrometer yields the value of the exospheric temperature in the equatorial region to be 800 (+150, −120) K at an altitude of 1540 km above the 1‐bar atmospheric pressure level; the H2‐density at 1540 km is determined to be 5 (+3.6, −1.8) × 109 cm−3. Temperature gradient in the thermosphere is found to be 1.25 (+0.05, −0.07) K km−1. Methane volume mixing ratio at 965 km above the 1‐bar pressure level is determined to be 1.5 × 10−4.Keywords
This publication has 9 references indexed in Scilit:
- Eddy mixing coefficient on SaturnPlanetary and Space Science, 1982
- Lizards in CaptivityIchthyology & Herpetology, 1982
- Radio Science with Voyager 2 at Saturn: Atmosphere and Ionosphere and the Masses of Mimas, Tethys, and IapetusScience, 1982
- Extreme Ultraviolet Observations from the Voyager 2 Encounter with SaturnScience, 1982
- Saturn ionosphere: theoretical interpretationNature, 1981
- Jupiter - Structure and composition of the upper atmosphereThe Astrophysical Journal, 1981
- Composition and thermal profiles of the Jovian upper atmosphere determined by the Voyager Ultraviolet Stellar Occultation ExperimentJournal of Geophysical Research, 1981
- Radio Science Investigations of the Saturn System with Voyager 1: Preliminary ResultsScience, 1981
- Infrared Observations of the Saturnian System from Voyager 1Science, 1981