Titan’s atmosphere from ISO mid-infrared spectroscopy
Authors:
- Athena CoustenisACAthena Coustenis
- A SalamaASA Salama
- B SchulzBSB Schulz
- S OttSOS Ott
- E LellouchELE Lellouch
- T.H EncrenazTET.H Encrenaz
- D GautierDGD Gautier
- H FeuchtgruberHFH Feuchtgruber
Abstract
No abstract availableKeywords
This publication has 42 references indexed in Scilit:
- The D/H Ratio in Methane in Titan: Origin and HistoryIcarus, 2002
- Europa: Tidal heating of upwelling thermal plumes and the origin of lenticulae and chaos meltingGeophysical Research Letters, 2002
- An Evolutionary Turbulent Model of Saturn's Subnebula: Implications for the Origin of the Atmosphere of TitanIcarus, 2002
- The Structure of Titan's Stratosphere from the 28 Sgr OccultationIcarus, 1999
- Vertical distribution of Titan's atmospheric neutral constituentsJournal of Geophysical Research, 1996
- Titan: Evidence for seasonal change—A comparison of Hubble space telescope and voyager imagesIcarus, 1992
- Plasma discharge in N2 + CH4 at low pressures: Experimental results and applications to TitanIcarus, 1991
- Titan's atmosphere from Voyager infrared observationsIcarus, 1989
- The abundance of CH3D in the atmosphere of Titan, derived from 8- to 14-μm thermal emissionIcarus, 1982
- Kinetic inhibition of CO and N2 reduction in circumplanetary nebulae - Implications for satellite compositionThe Astrophysical Journal, 1981