Titan’s atmosphere from ISO mid-infrared spectroscopy

By A. Coustenis, A. Salama, B. Schulz, S. Ott, E. Lellouch, T. Encrenaz, D. Gautier, H. Feuchtgruber. 2003

261 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/9891d8c591ad36b8197bb2b63ba0b8362db7e9d1

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In Astronomy and Astrophysics

Citations in the corpus

Vertical abundance profiles of hydrocarbons in Titan's atmosphere at 15° S and 80° N retrieved from Cassini/CIRS spectra (2007, methodology): “The mixing ratio we derive at 2 mbar for the 15◦ S-spectrum is in very good agreement with that retrieved from CIRS nadir spectra by Flasar et al. (2005) and Coustenis et al.”
The methane cycle on Titan (2008, methodology): “Benzene (C 6 H 6 ) has been detected in Titan's stratosphere by the Infrared Space Observator”
Laboratory Studies on the Irradiation of Methane in Interstellar, Cometary, and Solar System Ices (2006, background): “Coustenis et al. (2003) have analyzed the atmosphere of Saturn’smoonTitan using ISO and found that not only are methane, ethane, ethylene, and acetylene present, but also more complex hydrocarbons such as propane, propyne, benzene, allene, and diacetylene.”
Oxygen compounds in Titan's stratosphere as observed by Cassini CIRS (2007, methodology): “All previous analysis of CO2 either had lower spectral resolution (Coustenis and Bezard, 1995; Flasar et al., 2005 )o r lower spatial resolution ( Coustenis et al., 2003 ).”
The composition of Titan's stratosphere from Cassini/CIRS mid-infrared spectra (2007, methodology): “Our radiative transfer code is an update of the one used in the Voyager and ISO series papers (Coustenis and Bézard, 1995; Coustenis et al., 2003).”
The HITRAN 2008 molecular spectroscopic database (2005, background): “These species are also of importance for astronomical studies: benzene has been detected in the north polar auroral region of Jupiter [364] and in the stratospheres of Jupiter and Saturn [365] as well as in Titan’s atmosphere [366].”
Titan trace gaseous composition from CIRS at the end of the Cassini–Huygens prime mission (2010, background): “Besides these well-known trace species, a firm detection of benzene (C6H6), first reported in ISO data (Coustenis et al., 2003), was provided by CIRS at 674 cm .”
Analysis of Titan's neutral upper atmosphere from Cassini Ion Neutral Mass Spectrometer measurements in the Closed Source Neutral mode (2009, methodology): “For comparison, Coustenis et al. (2003) reported an H2O mixing ratio of 8 × 10−9 in Titan’s stratosphere (near 400 km), based on observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (ISO).”