The spectrum of Titan in the 1.06 and 1.28 micron windows

Details The spectrum of Titan in the 1.06 and 1.28 micron windows The spectrum of Titan in the 1.06 and 1.28 micron windows

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.338..353l&link_type=abstract

In ESA, Symposium on Titan p 353-358 (SEE N92-32348 23-91)

Astronomy and Astrophysics

Astronomy

4

Astronomical Spectroscopy, Atmospheric Chemistry, Infrared Spectroscopy, Methane, Satellite Atmospheres, Titan, Infrared Astronomy, Infrared Spectra, Infrared Windows, Near Infrared Radiation

Scientific paper

Observations of Titan at 1.0 to 1.4 microns at resolutions of 8/cm and 1/cm are reported. The spectra include two methane windows centered at 1.28 and 1.07 microns. A preliminary analysis of the 9050 to 9200/cm region of Titan is presented, using new laboratory data of methane recorded under long paths (about 500 m-am). The data in this range seem to be more consistent with a methane profile governed by saturation in most of the troposhere than with a uniform methane mixing ratio of 1 to 2 throughout the atmosphere.

Affiliated with

Also associated with

No associations

Rating

The spectrum of Titan in the 1.06 and 1.28 micron windows 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 The spectrum of Titan in the 1.06 and 1.28 micron windows, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The spectrum of Titan in the 1.06 and 1.28 micron windows will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1734695