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 / Unclassified / H2Te / GoodeveStein(1931)_298K_203.4-401.2nm(meas)

DATAFILE: H2Te_GoodeveStein(1931)_298K_203.4-401.2nm(meas).txt
NAME: hydrogen telluride
FORMULA: H2Te
AUTHOR(YEAR): GoodeveStein(1931)
T: 298K
λ: 203.4-401.2nm(meas)
BIBLIOGRAPHY: C.F. Goodeve and N.O. Stein, "The absorption spectra and the optical dissociation of the hydrides of the oxygen group", Trans. Faraday Soc. 27, 393-402 (1931); DOI: 10.1039/TF9312700393
COMMENTS: Absorption measurements by photographic photometry, the light sources used were a "Pointolite" for the visible, a mercury arc lamp for the visible and near ultra-violet, a tungsten-steel spark and an aluminium spark for the far ultra-violet

Data points for the absorption coefficients k (Torr, 298 K)-1 cm-1 (base 10) vs. wavenumbers have been digitized from Fig. 3 and converted to absorption cross sections (conversion factor 7.11×10-17) vs. wavelengths

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