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.


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    Title :

    Infrared spectra of gaseous organics of planetological interest: Implications for ISO capabilities


    Contributors:
    Raulin, F. (author) / Khlifi, M. (author) / Dang-Nhu, M. (author) / Gautier, D. (author)

    Published in:

    Advances in Space Research ; 12 , 11 ; 181-185


    Publication date :

    1992-01-01


    Size :

    5 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



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