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Characterising Saturn's vertical temperature structure from Cassini/CIRS

Abstract:

Thermal infrared spectra of Saturn from 10-1400 cm-1 at 15 cm-1 spectral resolution and a spatial resolution of 1°-2° latitude have been obtained by the Cassini Composite Infrared Spectrometer [Flasar, F.M., and 44 colleagues, 2004. Space Sci. Rev. 115, 169-297]. Many thousands of spectra, acquired over eighteen-months of observations, are analysed using an optimal estimation retrieval code [Irwin, P.G.J., Parrish, P., Fouchet, T., Calcutt, S.B., Taylor, F.W., Simon-Miller, A.A., Nixon, C.A.,...

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Publication status:
Published

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Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Atmos Ocean and Planet Physics
Irwin, PGJ More by this author
More by this author
Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Atmos Ocean and Planet Physics
Parrish, PD More by this author
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Journal:
ICARUS
Volume:
189
Issue:
2
Pages:
457-478
Publication date:
2007-08-05
DOI:
EISSN:
1090-2643
ISSN:
0019-1035
URN:
uuid:7bb42495-f3b5-4557-b7a7-6a2fdd903680
Source identifiers:
91
Local pid:
pubs:91
Language:
English
Keywords:

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