SWS observations and detection of water vapor on Titan

被引：0

作者：

Coustenis, A ^{[1
]}

Salama, A ^{[1
]}

Lellouch, E ^{[1
]}

Encrenaz, T ^{[1
]}

de Graauw, T ^{[1
]}

Kessler, MF ^{[1
]}

Feuchtgruber, H ^{[1
]}

Bjoraker, G ^{[1
]}

Samuelson, RE ^{[1
]}

Gautier, D ^{[1
]}

Orton, G ^{[1
]}

机构：

[1] Observ Paris, DESPA, F-92195 Meudon, France

来源：

UNIVERSE AS SEEN BY ISO, VOLS I AND II | 1999年 / 427卷

关键词：

ISO/SWS; infrared planetology; Titan; atmosphere; water vapor;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Titan ISO/SWS data were acquired in January and December 1997 in the grating mode with resolving powers between 1000-3000. Their analysis yielded information on the thermal and compositional structure of the satellite's atmosphere on a disk average basis with higher precision than the Voyager data. From a particular observational sequence around 40 mu m, the SWS data allowed the first detection of water vapor in Titan's upper atmosphere.

引用

页码：157 / 159

页数：3

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