Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003dps....35.1611v&link_type=abstract
American Astronomical Society, DPS meeting #35, #16.11; Bulletin of the American Astronomical Society, Vol. 35, p.1484
Astronomy and Astrophysics
Astronomy
Scientific paper
We report high-resolution (0.005 cm-1), low-temperature (87-300 K), measurements of the spectral line parameters in the 1-0, 2-0, and 3-0 bands of CO. The line parameters are the absolute intensities, collision-broadened half-widths, collision-induced line shifts,and the variation of these parameters with temperature. By using N2, O2, air, H2, and CO2 as the broadening gases we have obtained data that are directly applicable to the spectrosocpic observations of the atmospheres of the terrestrial and Jovian planets.It is interesting to observe that, while the collision-broadened half-widths of lines with the same rotational quantum numbers in the three bands are practically the same, the collision-induced line shifts show a marked increase that is progressive with the upper vibrational quantum number of the band. This observation may prove crucial in astronomical and atmospheric observations.
Sung Kevin
Varanasi Prasad
No associations
LandOfFree
Infrared Spectral Line Parameters of CO Applicable to Planetary Atmospheric Observations. 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 Infrared Spectral Line Parameters of CO Applicable to Planetary Atmospheric Observations., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Infrared Spectral Line Parameters of CO Applicable to Planetary Atmospheric Observations. will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-878768