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Lyα Emissions from Titan’s Atmosphere and Exosphere

  • Authors: Devin Hoover, Panayotis Lavvas, Tommi Koskinen, Nathan Le Guennic, Dolon Bhattacharyya, Peter Stephenson

Devin Hoover et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 1.

Geometry of a UVIS scan during the T10 flyby (2006 January 15). The dark-orange region represents Titan’s nightside, while the light-orange region represents Titan’s dayside. The blue shaded area illustrates the region of Titan’s atmosphere below 1000 km altitude. Each white box corresponds to a spatial pixel on the UVIS detector. The white dots represent background stars. The top caption includes the date and time of the observation, as well as Cassini’s altitude.

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