Submillimeter Spectra of Low Temperature Gases and Gas Mixtures

Details Submillimeter Spectra of Low Temperature Gases and Gas Mixtures Submillimeter Spectra of Low Temperature Gases and Gas Mixtures

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nla..work..260w&link_type=abstract

NASA Laboratory Astrophysics Workshop, held May 1-3 2002 at NASA Ames Research Center, Moffett Field, CA 94035-1000. Publisher:

Astronomy and Astrophysics

Astrophysics

Scientific paper

Submillimeter absorption spectra of nitrogen, nitrogen-argon mixtures, and methane have been measured using temperatures and pressures near to those found in the atmospheres of Titan and Saturn. The experiments show the spectral signature of dimers which will likely appear in far-infrared spectra of Titan that will be obtained by the Composite Infrared Spectrometer (CIRS) onboard the Cassini spacecraft. The recent CIRS spectrum of Jupiter shows far-infrared spectral lines of methane and the corresponding lines are observed in the laboratory. We are extending this work to lower frequencies using a new differential Michelson interferometer that operates over the frequency region 3-30 cm-1.

Affiliated with

Also associated with

No associations

Rating

Submillimeter Spectra of Low Temperature Gases and Gas Mixtures 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 Submillimeter Spectra of Low Temperature Gases and Gas Mixtures, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Submillimeter Spectra of Low Temperature Gases and Gas Mixtures will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1193062