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

Home

Cross Sections

Quantum Yields

Errata

Contact, Imprint, Acknowledgements

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 / Oxygen / O2 / Preston(1940)_298K_121.57nm

DATAFILE: O2_Preston(1940)_298K_121.57nm.txt
NAME: oxygen
FORMULA: O2
AUTHOR(YEAR): Preston(1940)
T: 298K
λ: 121.57nm
BIBLIOGRAPHY: W.M. Preston, "The origin of radio fade-outs and the absorption coefficient of gases for light of wave-length 1215.7 Å", Phys. Rev. 57, 887-894 (1940); DOI: 10.1103/PhysRev.57.887
COMMENTS: Absorption coefficient at the Lyman α line, as quoted by

K. Watanabe, E. C.Y. Inn, and M. Zelikoff, "Absorption coefficients of gases in the vacuum ultraviolet", J. Chem. Phys. 20, 1969-1970 (1952); DOI: 10.1063/1.1700353,

converted to absorption cross section (conversion factor 3.72×10-20)

Search cross sections

Species search:
Identifier search:
Reference search:
Full text search:
Recent additions:
since ago