The MPI-Mainz UV/VIS Spectral Atlas

of Gaseous Molecules of Atmospheric Interest

www.uv-vis-spectral-atlas-mainz.org

Hannelore Keller-Rudek1, Geert K. Moortgat2, Rolf Sander2, Rüdiger Sörensen1

1Satellite Group

2Atmospheric Chemistry Division

Max-Planck Institute for Chemistry
Mainz, Germany

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When referring to the Spectral Atlas, please cite our publication:

Keller-Rudek, H., Moortgat, G. K., Sander, R., and Sörensen, R.: The MPI-Mainz UV/VIS spectral atlas of gaseous molecules of atmospheric interest, Earth Syst. Sci. Data, 5, 365–373, (2013), DOI: 10.5194/essd-5-365-2013

Cross Sections / Organics (N-compounds) / Nitriles / HC3N / Benilan(1994)_293K_193.4-224.7nm(max)

DATAFILE: HC3N_Benilan(1994)_293K_193.4-224.7nm(max).txt
NAME: propynenitrile, cyanoacetylene
FORMULA: HC3N
AUTHOR(YEAR): Benilan(1994)
T: 293K
λ: 193.4-224.7nm(max)
BIBLIOGRAPHY: Y. Bénilan, P. Bruston, F. Raulin, C. Cossart-Magos, and J.-C. Guillemin, "Mid-UV spectroscopy of propynenitrile at low temperature: Consequences on expected results from observations of Titan's atmosphere", J. Geophys. Res. 99(E8), 17069-17074 (1994); DOI: 10.1029/94JE01087
COMMENTS: HC≡CC≡N

Maxima and other selected wavelengths of the absorption spectrum measured with a resolution of 0.02 nm as given by

T. Ferradaz, Y. Benilan, N. Fraya, A. Jollya, M. M.Schwell, M.-C. M.C.Gazeau, and H.W. Jochims, "Temperature-dependent photoabsorption cross-sections of cyanoacetylene and diacetylene in the mid-and vacuum-UV: Application to Titan's atmosphere", Planet. Space Sci. 57, 10-22 (2009); DOI: 10.1016/j.pss.2008.10.005

absorption coefficients in cm-1 amagat-1 (base e) have been converted to absorption cross sections (conversion factor 3.72×10-20)

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