Absolute IR band intensities of diacetylene in the 250 - 4300 cm-1 region: implications for Titan's atmosphere.

Details Absolute IR band intensities of diacetylene in the 250 - 4300 cm-1 region: implications for Titan's atmosphere. Absolute IR band intensities of diacetylene in the 250 - 4300 cm-1 region: implications for Titan's atmosphere.

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995jmosp.174..116k&link_type=abstract

Journal of Molecular Spectroscopy, Vol. 174, No. 1, p. 116 - 122

Physics

18

Titan Atmosphere: Organic Molecules, Infrared Spectra: Organic Molecules

Scientific paper

The infrared spectrum of C4H2, butadiyne (also called diacetylene), has been experimentally investigated in the region from 250 to 3300 cm-1 using a Fourier transform spectrometer. A total of 12 bands have been analyzed. For each band, the characteristic wavenumber has been deduced and the values of the absolute band intensities have been systematically determined together with their associated uncertainties. The results provide important data for planetary studies. In particular, a better estimate of the mean stratospheric abundance of butadiyne in Titan's atmosphere is obtained: its value is about 50% higher than previously reported.

Affiliated with

Also associated with

No associations

Rating

Absolute IR band intensities of diacetylene in the 250 - 4300 cm-1 region: implications for Titan's atmosphere. 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 Absolute IR band intensities of diacetylene in the 250 - 4300 cm-1 region: implications for Titan's atmosphere., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Absolute IR band intensities of diacetylene in the 250 - 4300 cm-1 region: implications for Titan's atmosphere. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1181577