Structure and Composition of Titan's ATMOSPHERE:CYCLE 3 High

Details Structure and Composition of Titan's ATMOSPHERE:CYCLE 3 High Structure and Composition of Titan's ATMOSPHERE:CYCLE 3 High

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.4965c&link_type=abstract

HST Proposal ID #4965

Physics

Hst Proposal Id #4965

Scientific paper

Titan will be observed with the FOS G270H, to search for discrete
absorption features and continuum Rayleigh scattering. Rayleigh
scattering has not previously been detected from Titan by the OAO-2 and
IUE spacecraft, despite the very thick atmosphere there, because of
strong absorption by quasi-organic material.

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