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A. A. Simon-Miller, G. L. Bjoraker, D. E. Jennings (NASA GSFC), R. K. Achterberg (NASA/SSAI), B. J. Conrath (Cornell), C. A. Nixon (UMD), Cassini CIRS Team
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.
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Bulletin of the American Astronomical Society, 37 #3
© 2004. The American Astronomical Soceity.