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Infrared limb sounding of Titan with the Cassini Composite InfraRed Spectrometer: effects of the mid-IR detector spatial responses.

Abstract:
The composite infrared spectrometer (CIRS) instrument on board the Cassini Saturn orbiter employs two 1x10 HgCdTe detector arrays for mid-infrared remote sensing of Titan's and Saturn's atmospheres. In this paper we show that the real detector spatial response functions, as measured in ground testing before launch, differ significantly from idealized "boxcar" responses. We further show that neglecting this true spatial response function when modeling CIRS spectra can have a significant effect on interpretation of the data, especially in limb-sounding mode, which is frequently used for Titan science. This result has implications not just for CIRS data analysis but for other similar instrumental applications.
Publication status:
Published

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Publisher copy:
10.1364/ao.48.001912

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Author


Publisher:
Optical Society of American (OSA)
Journal:
Applied optics More from this journal
Volume:
48
Issue:
10
Pages:
1912-1925
Publication date:
2009-04-01
DOI:
EISSN:
1539-4522
ISSN:
0003-6935


Language:
English
Pubs id:
pubs:17078
UUID:
uuid:fb118aa5-26a3-4761-b4a0-7cd5eec5599b
Local pid:
pubs:17078
Source identifiers:
17078
Deposit date:
2012-12-19

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