1993
DOI: 10.1006/icar.1993.1047
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Modeling Titan's Thermal Infrared Spectrum for High-Resolution Space Observations

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Cited by 76 publications
(53 citation statements)
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“…Furthermore, acetylene concentration in human breath has been identified as a biomarker for smoking [5]. Acetylene has been found as a trace constituent of the Titan atmosphere and in outer planetary atmospheres of Jupiter and Saturn [6,7]. Accurate measurements of important spectroscopic parameters such as linestrengths, collisional broadening coefficients and their temperature dependencies are crucial for precise measurements of acetylene concentration in a variety of environments.…”
Section: Introductionmentioning
confidence: 99%
“…Furthermore, acetylene concentration in human breath has been identified as a biomarker for smoking [5]. Acetylene has been found as a trace constituent of the Titan atmosphere and in outer planetary atmospheres of Jupiter and Saturn [6,7]. Accurate measurements of important spectroscopic parameters such as linestrengths, collisional broadening coefficients and their temperature dependencies are crucial for precise measurements of acetylene concentration in a variety of environments.…”
Section: Introductionmentioning
confidence: 99%
“…Allene has been the object of much investigation for its relevance to astrochemistry [1][2][3] and to studies of photodissociation dynamics. [4][5][6][7][8][9] Allene is also the smallest member of the cumulene family and one of the simplest representatives of the D 2d ͑M͒ molecular symmetry group.…”
Section: Introductionmentioning
confidence: 99%
“…Although allene was not observed by the infrared interferometer and spectrometer (IRIS) on board the Voyager spacecraft, an upper mole-fraction limit of 5 ϫ 10 Ϫ9 was implied from a fit of the spectroscopic data (3,4). Allene was not detected by the short/long wavelength grating spectrometer on the Infrared Space Observatory (ISO) either and the upper limit is yet to be derived.…”
Section: Introductionmentioning
confidence: 99%
“…Allene was not detected by the short/long wavelength grating spectrometer on the Infrared Space Observatory (ISO) either and the upper limit is yet to be derived. However, the composite infrared spectrometer (CIRS) abroad the Cassini mission that is currently on its way to Titan will be capable of detecting allene at much lower abundances owing to CIRS's much higher sensitivity (4). Candidate spectral regions for the observation of allene include the isolated weak 353 cm Ϫ1 11 band and the strong 10 band near 841 cm Ϫ1 (4).…”
Section: Introductionmentioning
confidence: 99%