Cyanoacetylene (HC3N) Ice in Titan's Lower Stratosphere

Details Cyanoacetylene (HC3N) Ice in Titan's Lower Stratosphere Cyanoacetylene (HC3N) Ice in Titan's Lower Stratosphere

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ttt..work...67a&link_type=abstract

Through Time; A Workshop On Titan's Past, Present and Future, NASA Goddard Space Flight Center, April 6th - 8th, 2010. Edited b

Physics

Scientific paper

Cassini CIRS far infrared limb spectra of Titan reveal spectral evidence for the ν6 cyanoacetylene (HC3N) ice feature at 506 cm-1(~20 micron) at latitudes 62N and 70N. We derive particle size and column abundances in Titan's lower stratosphere with mean particle radii of 2.3 micron and 3.0 micron at 62N and 70N, respectively, and corresponding ice phase molecular column abundances in the range 1-10 mol cm-2. As a result of dynamical circulation, we expect stratospheric clouds with small particle radii to form principally at high northern latitudes in Titan's winter hemispheres, with much lower abundances at low latitudes.

Affiliated with

Also associated with

No associations

Rating

Cyanoacetylene (HC3N) Ice in Titan's Lower Stratosphere does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Cyanoacetylene (HC3N) Ice in Titan's Lower Stratosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cyanoacetylene (HC3N) Ice in Titan's Lower Stratosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1191464