Infrared signature of linear carbon chains on Titan

Details Infrared signature of linear carbon chains on Titan Infrared signature of linear carbon chains on Titan

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1128j&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1128

Physics

Scientific paper

Our laboratory experimental study of HC3N [1] has shown that band intensities had to be revised and that including hot bands was necessary to model the observed spectra. A new extended line list was obtained and due to the precision of the new spectroscopic data, 13C isotopologues of HC3N have been detected and quantified for the first time in the atmosphere of Titan using CIRS data [2]. The detection of the 15N isotopologue of HC3N was also considered but not possible at 663 cm-1 as the spectral resolution of CIRS was not sufficient to separate the nitrogen isotope band from the main band emission.

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