Exploring The Saturn System In The Thermal Infrared: The Composite Infrared Spectrometer

By F. Flasar, V. Kunde, M. Abbas, R. Achterberg, P. Ade, A. Barucci, B. B'ezard, G. Bjoraker, J. Brasunas, S. Calcutt and 35 more. 2004

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High heat flow from Enceladus' south polar region measured using 10–600 cm−1 Cassini/CIRS data (2011, background): “Enceladus’ silicate interior and outer ice shell were decoupled by a global subsurface ocean or localized subsurface south polar sea [ Collins and Goodman, 2007; Nimmo et al., 2007; Tobie et al., 2008; Roberts and Nimmo, 2008], though the long‐term steady state upper limit discussed above still app”
Oxygen compounds in Titan's stratosphere as observed by Cassini CIRS (2007, methodology): “(2005) Stratosphere 45+15 −15 150–500 μm Flasar et al. (2005)”
Titan trace gaseous composition from CIRS at the end of the Cassini–Huygens prime mission (2010, background): “Hourdin et al. (2004) have shown that the meridional circulation on Titan, dominated by global Hadley cells, can be responsible for the accumulation of chemical species and aerosols at high northern latitudes and have also predicted the magnitude of the enrichment in stratospheric constituents to be”
The NEMESIS planetary atmosphere radiative transfer and retrieval tool (2008, methodology): “In some cases, other instrument functions are required, such as for example the Hamming function used in apodised CIRS spectra [10,11].”