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 / Halogens+mixed halogens / Cl2 / Maric(1993)_298K_255-488nm

DATAFILE: Cl2_Maric(1993)_298K_255-488nm.txt
NAME: chlorine
FORMULA: Cl2
AUTHOR(YEAR): Maric(1993)
T: 298K
λ: 255-488nm
BIBLIOGRAPHY: D. Maric, J.P. Burrows, R. Meller, and G.K. Moortgat, "Visible absorption spectra of molecular chlorine", J. Photochem. Photobiol. A: Chem. 70, 205-214 (1993); DOI: 10.1016/1010-6030(93)85045-A
COMMENTS: Measurements at 298 K in the wavelength range 200-550 nm with a spectral resolution of 0.2 nm

In the region 250-550 nm, the spectrum can be adequately described by the semi-empirical function (eqn. 12)

σ(λ,T) = 2.73×10-19 cm2 x tanh0.5
× exp{-99.0 x tanh x [ln(329.5 nm/λ)]2}
+ 9.32×10-21 cm2 x tanh0.5
× exp{-91.5 x tanh x [ln(406.5 nm/λ)]2}

with tanh = tanh(hcX559.751 cm-1/2KT) = tanh(402.7/T);
λ in nm, 250 < λ < 550 nm, and T in K; 300 K > T > 195 K

The absorption cross sections have been calculated at 0.2-nm intervals using this formula

Search cross sections

Species search:

Identifier search:

Reference search:

Full text search:

Recent additions:
since ago