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 / Nitrogen oxides / N2O5 / Kritten(2014)_230K_200-420nm

DATAFILE: N2O5_Kritten(2014)_230K_200-420nm.txt
NAME: dinitrogen pentoxide
FORMULA: N2O5
AUTHOR(YEAR): Kritten(2014)
T: 230K
λ: 200-420nm
BIBLIOGRAPHY: L. Kritten, A. Butz, M.P. Chipperfield, M. Dorf, S. Dhomse, R. Hossaini, H. Oelhaf, C. Prados-Roman, G. Wetzel, and K. Pfeilsticker, "Constraining the N2O5 UV absorption cross section from spectroscopic trace gas measurements in the tropical mid-stratosphere", Atmos. Chem. Phys. 14, 9555–9566 (2014); DOI: 10.5194/acp-14-9555-2014
COMMENTS: The absorption cross sections of N2O5 were investigated by balloon-borne observations of the relevant trace gases in the tropical mid-stratosphere

The method relies on the observation of the diurnal variation of NO2 by limb scanning DOAS (differential optical absorption spectroscopy) measurements supported by detailed photochemical modelling of NOy (NOx(= NO+NO2) +NO3 + 2N2O5 + ClONO2 + HO2NO2 + BrONO2 +HNO3) photochemistry and a non-linear least square fitting of the model result to the NO2 observations

Best agreement between the simulated and observed diurnal increase of NO2 is found if the absorption cross sections of N2O5, as recommended by

S.P. Sander, J. Abbatt, J. R. Barker, J. B. Burkholder, R. R. Friedl, D. M. Golden, R. E. Huie, C. E. Kolb, M. J. Kurylo, G. K. Moortgat, V. L. Orkin and P. H. Wine "Chemical Kinetics and Photochemical Data for Use in Atmospheric Studies, Evaluation Number 17", JPL Publication 10-6, Jet Propulsion Laboratory, Pasadena, 2011. http://jpldataeval.jpl.nasa.gov,

are scaled by a factor of 1.6 ± 0.8 in the UV-C (200–260 nm) and by a factor of 0.9 ± 0.26 in the UV-B/A (260–350 m)

Absorption cross sections have been obtained by personal communication from Lena Kritten (January 2015)

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