- Abstract:
-
Saturn's moon Titan has a nitrogen atmosphere comparable to Earth's, with a surface pressure of 1.4 bar. Numerical models reproduce the tropospheric conditions very well but have trouble explaining the observed middle-atmosphere temperatures, composition and winds. The top of the middle-atmosphere circulation has been thought to lie at an altitude of 450 to 500 kilometres, where there is a layer of haze that appears to be separated from the main haze deck. This 'detached' haze was previously ...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1038/nature11611
-
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- Journal:
- Nature
- Volume:
- 491
- Issue:
- 7426
- Pages:
- 732-735
- Publication date:
- 2012-11-05
- DOI:
- EISSN:
-
1476-4687
- ISSN:
-
0028-0836
- URN:
-
uuid:2ef591b4-26c4-4d76-91cf-438b60d0bf8e
- Source identifiers:
-
365470
- Local pid:
- pubs:365470
- Language:
- English
- Copyright date:
- 2012
Journal article
Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan.
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