From Newsgroup: sci.space.news
http://saturn.jpl.nasa.gov/mission/flybys/titan20160201/
Cassini
Titan Flyby T-116: Multiple Occultations
Feb. 01, 2016
The Ultraviolet Imaging Spectrograph (UVIS) will observe two stars as
they disappear behind Titan's atmosphere, which will provide detailed
vertical profiles of composition and temperature in the high atmosphere
not possible with any other instrument. UVIS also will take advantage
of solar occultations to probe both northern and southern latitudes. The
solar occultation is also observed by Visible and Infrared Mapping Spectrometer
(VIMS) to provide detailed vertical profiles of composition and aerosols
in the atmosphere below 200 km.
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Titan Flyby at a Glance
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Date
Feb. 1, 2016
Altitude
870 miles (1,400 kilometers)
Speed (rel. to Titan)
12,974 mph (5.8 km/sec)
SEEN-BY: 154/30 2320/100 0 1 227/0