Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005dps....37.3026s&link_type=abstract
American Astronomical Society, DPS meeting #37, #30.26; Bulletin of the American Astronomical Society, Vol. 37, p.682
Astronomy and Astrophysics
Astronomy
Scientific paper
The Composite Infrared Spectrometer (CIRS) on the Cassini spacecraft has obtained high spectral resolution mid to far-infrared spectra of Saturn's atmosphere. In particular, long integrations were obtained with 0.3 cm-1, unapodized, spectral resolution at 15, 45, 60 and 75 S and high emission angles. These observations are optimal for detecting stratospheric emission from a variety of molecules. We present abundance gradients determined for benzene, carbon dioxide and propane for comparison with previous estimates from ISO and ground-based observations.
Achterberg Richard K.
Bjoraker Gordon L.
Cassini CIRS Team
Conrath Barney J.
Jennings Donald E.
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