Abstract Many organics likely to be present in Titan's atmosphere exhibit strong spectral signatures from the near to the far IR regions. Their number increases with their complexity, while their abundance decreases. Consequently, their detection requires IR instruments of higher sensitivity and, simultaneously, higher resolution. This is in the capabilities of the LWS and SWS of ISO. However there is also a need for more data on the absolute intensities of the main IR bands of these compounds.
Infrared spectra of gaseous organics of planetological interest: Implications for ISO capabilities
Advances in Space Research ; 12 , 11 ; 181-185
1992-01-01
5 pages
Article (Journal)
Electronic Resource
English
Infrared Spectroscopy of Organics of Planetological Interest at Low Temperatures
British Library Conference Proceedings | 1995
|Geology of Triton and some comparative-planetological implications
Elsevier | 1992
|British Library Conference Proceedings | 1995
|Infrared Spectroscopy of Organics of Planetological Interest at Low Temperatures
Online Contents | 1995
|