Structure and Composition of Titan's ATMOSPHERE:CYCLE 1

Details Structure and Composition of Titan's ATMOSPHERE:CYCLE 1 Structure and Composition of Titan's ATMOSPHERE:CYCLE 1

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1289c&link_type=abstract

HST Proposal ID #1289

Physics

Hst Proposal Id #1289

Scientific paper

Titan will be observed both with ultraviolet imaging and spectroscopy. The ultraviolet imaging is to look for very high altitude atmospheric structure that might be associated with details of the UV spectroscopy. The UV spectroscopy will include a search for discrete absorption features and continuum Rayleigh scattering. Rayleigh scattering has not previously been detected from Titan, despite the very thick atmosphere there, because of strong absorption by quasi-organic material.

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