Distribution of HCN in Titan's upper atmosphere from Cassini/VIMS observations at 3 μm

Details Distribution of HCN in Titan's upper atmosphere from Cassini/VIMS observations at 3 μm Distribution of HCN in Titan's upper atmosphere from Cassini/VIMS observations at 3 μm

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011icar..214..584a&link_type=abstract

Icarus, Volume 214, Issue 2, p. 584-595.

Physics

2

Scientific paper

We present the first concentration retrieval of HCN by
Cassini-VIMS limb observations of the Titan upper atmosphere. HCN is thought to play an important role in the chemistry and in
determining the thermal structure of Titan's thermosphere. A
model for non-LTE HCN emission in Titan atmospheric condition has been
developed for the purpose.

Affiliated with

Also associated with

No associations

Rating

Distribution of HCN in Titan's upper atmosphere from Cassini/VIMS observations at 3 μm 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 Distribution of HCN in Titan's upper atmosphere from Cassini/VIMS observations at 3 μm, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Distribution of HCN in Titan's upper atmosphere from Cassini/VIMS observations at 3 μm will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1680097