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

Details Infrared spectra of gaseous organics of planetological interest - Implications for ISO capabilities Infrared spectra of gaseous organics of planetological interest - Implications for ISO capabilities

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992adspr..12..181r&link_type=abstract

(Planetary studies; Proceedings of Symposium 4 and the Topical Meeting of the Interdisciplinary Scientific Commission B /Meeting

Computer Science

Infrared Spectra, Organic Compounds, Satellite Atmospheres, Titan, Atmospheric Composition, Infrared Detectors

Scientific paper

Comments are presented concerning the search for new organics in Titan's atmosphere based on remote sensing techniques using Infrared Space Observatory (ISO) spectrometers. IR ISO spectrometers will provide a significantly higher resolution than that of IRIS even in the grating mode 0.5 compared to 4.3 per cm. The capabilities of ISO instruments will make it possible to observe the very far IR region, which includes signatures of several organics.

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