THE INTENSITY AND PRESSURE BROADENING OF THE 681.884NM METHANE ABSORPTION-LINE AT LOW-TEMPERATURES DETERMINED BY INTRACAVITY LASER SPECTROSCOPY

Citation
Bb. Radak et al., THE INTENSITY AND PRESSURE BROADENING OF THE 681.884NM METHANE ABSORPTION-LINE AT LOW-TEMPERATURES DETERMINED BY INTRACAVITY LASER SPECTROSCOPY, Journal of quantitative spectroscopy & radiative transfer, 52(6), 1994, pp. 809-818
Citations number
40
Categorie Soggetti
Spectroscopy
ISSN journal
00224073
Volume
52
Issue
6
Year of publication
1994
Pages
809 - 818
Database
ISI
SICI code
0022-4073(1994)52:6<809:TIAPBO>2.0.ZU;2-E
Abstract
The temperature dependence of the intensity and of the pressure broade ned width of the 681.884 nm ro-vibrational absorption line in the weak 681.5 nm band of methane is. studied experimentally using intracavity laser spectroscopy (ILS). These measurements are performed in the tem perature range between 77 and 295 K using equivalent absorption pathle ngths between 3.6 and 36 km. The collision-broadening data are measure d for cases in which CH4, N-2, H-2, and He are the collision partners at total pressures ranging between 100 and 500 torr. The intensity res ults obtained here are the first such data to be reported for the 681. 884 nm line. An analysis of the line intensity data based upon their d ependence on temperature suggests that the rotational quantum number J assignable to this line is 2. The 681.884 nm line examined here is fo und to be approximately 7 times weaker at ambient temperature than the 619.68 nm line studied previously using the ILS technique. The work p resented here, therefore, extends the limit of detection sensitivity f or quantitative spectroscopic applications of ILS in congested spectra l regions by almost an order of magnitude. The significance of the res ults with respect to observational spectroscopy of planetary atmospher es is also discussed.