Author
Listed:
- Nicholas A. Teanby
(School of Earth Sciences, University of Bristol, Wills Memorial Building, Queen’s Road, Bristol BS8 1RJ, UK)
- Patrick G. J. Irwin
(Atmospheric, Oceanic and Planetary Physics, University of Oxford, Clarendon Laboratory, Parks Road, Oxford OX1 3PU, UK)
- Conor A. Nixon
(Planetary Systems Laboratory, NASA Goddard Space Flight Center)
- Remco de Kok
(SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands)
- Sandrine Vinatier
(LESIA Observatoire de Paris, CNRS, UPMC Université Paris 06, Université Paris-Diderot, 5 place Jules Janssen, 92195 Meudon Cedex, France)
- Athena Coustenis
(LESIA Observatoire de Paris, CNRS, UPMC Université Paris 06, Université Paris-Diderot, 5 place Jules Janssen, 92195 Meudon Cedex, France)
- Elliot Sefton-Nash
(School of Earth Sciences, University of Bristol, Wills Memorial Building, Queen’s Road, Bristol BS8 1RJ, UK
University of California Los Angeles)
- Simon B. Calcutt
(Atmospheric, Oceanic and Planetary Physics, University of Oxford, Clarendon Laboratory, Parks Road, Oxford OX1 3PU, UK)
- F. Michael Flasar
(Planetary Systems Laboratory, NASA Goddard Space Flight Center)
Abstract
Observations of trace gases over the south pole of Titan indicate that the moon’s middle-atmospheric circulation extends to an altitude of at least 600 kilometres, which is higher than previously thought and requires active chemistry and dynamics in the upper atmosphere.
Suggested Citation
Nicholas A. Teanby & Patrick G. J. Irwin & Conor A. Nixon & Remco de Kok & Sandrine Vinatier & Athena Coustenis & Elliot Sefton-Nash & Simon B. Calcutt & F. Michael Flasar, 2012.
"Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan,"
Nature, Nature, vol. 491(7426), pages 732-735, November.
Handle:
RePEc:nat:nature:v:491:y:2012:i:7426:d:10.1038_nature11611
DOI: 10.1038/nature11611
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