From Newsgroup: sci.space.news
http://saturn.jpl.nasa.gov/mission/flybys/titan20160216/
Cassini
Titan Flyby T-117: One Flyby, Two Radio Science Experiments
Feb. 16, 2016
This is Cassini's 118th flyby of Titan and the third of 11 planned for
2016. This encounter will increase the inclination of Cassini's orbit
from 16 degrees to 20.6 degrees. The highest priority science is a grazing atmospheric occultation observed by Radio Science Subsystem (RSS), which
will profile the thermal structure of the atmosphere, with ingress and
egress latitudes of ~7S and ~30N degrees.The occultation is followed by
a short-duration high northern-latitude egress-only bistatic scattering
with ground track likely crossing small lakes, covering the region from
about (80N, 190W) to about (70N, 240W) degrees, and capturing near-grazing scattering angle decreasing from about 80 to 75 degrees.
On approach, the Composite Infrared Spectrometer (CIRS) will view the sub-Saturn hemisphere of Titan, the Visible and Infrared Mapping Spectrometer (VIMS) will do two mapping observations and the Imaging Science Subsystem (ISS) will search for clouds across Titan's Fensal-Aztlan region.
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Titan Flyby at a Glance
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Date
Feb. 16, 2016
Altitude
633 miles (1,018 km)
Speed (rel. to Titan)
20,132 mph (5.9 km/sec)
SEEN-BY: 154/30 2320/100 0 1 227/0