Line widths of (N-14)H3 and (N-15)H3 applicable to planetary atmospheric observations

Details Line widths of (N-14)H3 and (N-15)H3 applicable to planetary atmospheric observations Line widths of (N-14)H3 and (N-15)H3 applicable to planetary atmospheric observations

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jqsrt..49..383v&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 49, no. 4, p. 383-388.

Physics

4

Absorption Spectra, Ammonia, Jupiter Atmosphere, Spectral Line Width, Spectrum Analysis, Electron States, Laser Spectrometers, Molecular Interactions, Spectral Resolution

Scientific paper

The collision-broadened half-widths of sP(1,0), sP(3,2), sP(4,1), sP(4,2), and sP(4,3) in the v2 sup s-fundamental bands of (N-14)H3 and (N-15)H3 have been measured at 198, 245, and 295 K employing the Doppler-limited spectral resolution of a tunable diode laser spectrometer. The temperature dependence of the collision-broadened half-widths of these lines broadened by H2 and N2 has been determined. In addition, we have also measured the air-broadened line widths of all of these lines at 295 K and the half-width of the sP(3,2) line of (N-15)H3 broadened by (N-14)H3 at 198, 245, and 295 K.

Affiliated with

Also associated with

No associations

Rating

Line widths of (N-14)H3 and (N-15)H3 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 Line widths of (N-14)H3 and (N-15)H3 applicable to planetary atmospheric observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Line widths of (N-14)H3 and (N-15)H3 applicable to planetary atmospheric observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1373022