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Cassini UVIS observations of Titan ultraviolet airglow intensity dependence with solar zenith angle
DOI: 10.1002/2016GL071756 Bibcode: 2017GeoRL..44...88R

West, R. A.; Esposito, L. W.; Royer, E. M. +3 more

The Cassini Ultraviolet Imaging Spectrometer (UVIS) observed the airglow (dayglow and nightglow) of Titan over a range of solar zenith angles (SZA) from 14 to 150° on five separate observations obtained between 2008 and 2012. The modeling of the solar cycle normalized UVIS observations indicates that a Chapman layer function provides a satisfactor…

2017 Geophysical Research Letters
Cassini 1