Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan
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 winds1, 2. The top of the middle-atmosphe...
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Online Access: | https://hdl.handle.net/1983/5f9a976d-7bdf-4417-a48a-ded12f57b470 https://research-information.bris.ac.uk/en/publications/5f9a976d-7bdf-4417-a48a-ded12f57b470 https://doi.org/10.1038/nature11611 |
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ftubristolcris:oai:research-information.bris.ac.uk:publications/5f9a976d-7bdf-4417-a48a-ded12f57b470 2024-05-19T07:48:40+00:00 Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan Teanby, Nick A Irwin, Patrick G. J. Nixon, Conor A. de Kok, R Vinatier, S Coustenis, A Sefton-Nash, Elliot Calcutt, SB Flasar, FM 2012-11-29 https://hdl.handle.net/1983/5f9a976d-7bdf-4417-a48a-ded12f57b470 https://research-information.bris.ac.uk/en/publications/5f9a976d-7bdf-4417-a48a-ded12f57b470 https://doi.org/10.1038/nature11611 eng eng https://research-information.bris.ac.uk/en/publications/5f9a976d-7bdf-4417-a48a-ded12f57b470 info:eu-repo/semantics/restrictedAccess Teanby , N A , Irwin , P G J , Nixon , C A , de Kok , R , Vinatier , S , Coustenis , A , Sefton-Nash , E , Calcutt , SB & Flasar , FM 2012 , ' Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan ' , Nature , vol. 491 , pp. 732-735 . https://doi.org/10.1038/nature11611 article 2012 ftubristolcris https://doi.org/10.1038/nature11611 2024-04-30T23:39:44Z 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 winds1, 2. 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 deck3. This ‘detached’ haze was previously explained as being due to the co-location of peak haze production and the limit of dynamical transport by the circulation’s upper branch4. Here we report a build-up of trace gases over the south pole approximately two years after observing the 2009 post-equinox circulation reversal, from which we conclude that middle-atmosphere circulation must extend to an altitude of at least 600 kilometres. The primary drivers of this circulation are summer-hemisphere heating of haze by absorption of solar radiation and winter-hemisphere cooling due to infrared emission by haze and trace gases5; our results therefore imply that these effects are important well into the thermosphere (altitudes higher than 500 kilometres). This requires both active upper-atmosphere chemistry, consistent with the detection of high-complexity molecules and ions at altitudes greater than 950 kilometres6, 7, and an alternative explanation for the detached haze, such as a transition in haze particle growth from monomers to fractal structures8. Article in Journal/Newspaper South pole University of Bristol: Bristol Research Nature 491 7426 732 735 |
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Open Polar |
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University of Bristol: Bristol Research |
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ftubristolcris |
language |
English |
description |
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 winds1, 2. 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 deck3. This ‘detached’ haze was previously explained as being due to the co-location of peak haze production and the limit of dynamical transport by the circulation’s upper branch4. Here we report a build-up of trace gases over the south pole approximately two years after observing the 2009 post-equinox circulation reversal, from which we conclude that middle-atmosphere circulation must extend to an altitude of at least 600 kilometres. The primary drivers of this circulation are summer-hemisphere heating of haze by absorption of solar radiation and winter-hemisphere cooling due to infrared emission by haze and trace gases5; our results therefore imply that these effects are important well into the thermosphere (altitudes higher than 500 kilometres). This requires both active upper-atmosphere chemistry, consistent with the detection of high-complexity molecules and ions at altitudes greater than 950 kilometres6, 7, and an alternative explanation for the detached haze, such as a transition in haze particle growth from monomers to fractal structures8. |
format |
Article in Journal/Newspaper |
author |
Teanby, Nick A Irwin, Patrick G. J. Nixon, Conor A. de Kok, R Vinatier, S Coustenis, A Sefton-Nash, Elliot Calcutt, SB Flasar, FM |
spellingShingle |
Teanby, Nick A Irwin, Patrick G. J. Nixon, Conor A. de Kok, R Vinatier, S Coustenis, A Sefton-Nash, Elliot Calcutt, SB Flasar, FM Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan |
author_facet |
Teanby, Nick A Irwin, Patrick G. J. Nixon, Conor A. de Kok, R Vinatier, S Coustenis, A Sefton-Nash, Elliot Calcutt, SB Flasar, FM |
author_sort |
Teanby, Nick A |
title |
Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan |
title_short |
Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan |
title_full |
Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan |
title_fullStr |
Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan |
title_full_unstemmed |
Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan |
title_sort |
active upper-atmosphere chemistry and dynamics from polar circulation reversal on titan |
publishDate |
2012 |
url |
https://hdl.handle.net/1983/5f9a976d-7bdf-4417-a48a-ded12f57b470 https://research-information.bris.ac.uk/en/publications/5f9a976d-7bdf-4417-a48a-ded12f57b470 https://doi.org/10.1038/nature11611 |
genre |
South pole |
genre_facet |
South pole |
op_source |
Teanby , N A , Irwin , P G J , Nixon , C A , de Kok , R , Vinatier , S , Coustenis , A , Sefton-Nash , E , Calcutt , SB & Flasar , FM 2012 , ' Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan ' , Nature , vol. 491 , pp. 732-735 . https://doi.org/10.1038/nature11611 |
op_relation |
https://research-information.bris.ac.uk/en/publications/5f9a976d-7bdf-4417-a48a-ded12f57b470 |
op_rights |
info:eu-repo/semantics/restrictedAccess |
op_doi |
https://doi.org/10.1038/nature11611 |
container_title |
Nature |
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491 |
container_issue |
7426 |
container_start_page |
732 |
op_container_end_page |
735 |
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1799466981129191424 |