Journal article
Mapping the zonal structure of Titan’s northern polar vortex
- Abstract:
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Saturn exhibits an obliquity of 26.7° such that the largest moon, Titan, experiences seasonal variations including the formation of a polar vortex in the winter hemisphere. Titan's polar vortex is characterised by cold stratospheric temperatures due to the lack of insolation over the winter pole, and an increase in trace gas abundance as a result of complex organic chemistry in the upper atmosphere combined with polar subsidence. Meridional variations in temperature and gas abundance across t...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
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(Accepted manuscript, pdf, 7.9MB)
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- Publisher copy:
- 10.1016/j.icarus.2019.113441
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Authors
Funding
Bibliographic Details
- Publisher:
- Elsevier Publisher's website
- Journal:
- Icarus Journal website
- Volume:
- 337
- Article number:
- 113441
- Publication date:
- 2019-10-05
- Acceptance date:
- 2019-09-10
- DOI:
- ISSN:
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0019-1035
- Source identifiers:
-
1052877
Item Description
- Language:
- English
- Keywords:
- Pubs id:
-
pubs:1052877
- UUID:
-
uuid:a803d317-4ea7-4d05-b642-654703d661db
- Local pid:
- pubs:1052877
- Deposit date:
- 2019-09-10
Terms of use
- Copyright holder:
- Elsevier
- Copyright date:
- 2019
- Rights statement:
- © 2019 Elsevier Inc. All rights reserved.
- Notes:
- This is the accepted manuscript version of the article, available under the terms of a Creative Commons, Attribution, Non-Commercial, No Derivatives licence. The final version is available online from Elsevier at: https://doi.org/10.1016/j.icarus.2019.113441
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