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Seasonal evolution of C2N2, C3H4, and C4H2 abundances in Titan's lower stratosphere

Abstract:

Aims. We study the seasonal evolution of Titan’s lower stratosphere (around 15 mbar) in order to better understand the atmospheric dynamics and chemistry in this part of the atmosphere.

Methods. We analysed Cassini/CIRS far-IR observations from 2006 to 2016 in order to measure the seasonal variations of three photochemical by-products: C4H2, C3H4, and C2N2.

Results. We show t...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.1051/0004-6361/201630255

Authors


Sylvestre, M More by this author
Teanby, NA More by this author
Vinatier, S More by this author
Lebonnois, S More by this author
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Atmos Ocean & Planet Physics
Oxford college:
St Annes College
Cassini Project More from this funder
Publisher:
EDP Sciences Publisher's website
Journal:
Astronomy & Astrophysics Journal website
Volume:
609
Pages:
Article: A64
Publication date:
2018-01-08
Acceptance date:
2017-08-29
DOI:
EISSN:
1432-0746
ISSN:
0004-6361
Pubs id:
pubs:820980
URN:
uri:524e508f-ed96-4fa6-84ed-9b9640732129
UUID:
uuid:524e508f-ed96-4fa6-84ed-9b9640732129
Local pid:
pubs:820980

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