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
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DATAFILE: | IO_JPL-2010(2011)_298K_339-417nm(rec).txt |
NAME: | iodine monoxide |
FORMULA: | IO |
AUTHOR(YEAR): | JPL-2010(2011) |
T: | 298K |
λ: | 339-417nm(rec) |
BIBLIOGRAPHY: |
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/
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COMMENTS: | JPL-2010 recommendation, adopting the earlier recommendation of
S.P. Sander, R.R. Friedl, D.M. Golden, M.J. Kurylo, G.K. Moortgat, H. Keller-Rudek, P.H. Wine, A.R. Ravishankara, C.E. Kolb, M.J. Molina, B.J. Finlayson-Pitts, R.E. Huie, V.L. Orkin, “Chemical Kinetics and Photochemical Data for Use in Atmospheric Studies. Evaluation Number 15“, JPL Publication 06-2, Jet Propulsion Laboratory, Pasadena, 2006; http://jpldataeval.jpl.nasa.gov/ :
(1) The spectra of M.H. Harwood, J.B. Burkholder, M. Hunter, R.W. Fox, and A.R. Ravishankara, "Absorption cross sections and self-reaction kinetics of the IO radical," J. Phys. Chem. 101, 853-863 (1997); DOI: 10.1021/jp962429b, and B. Laszlo, M.J. Kurylo, and R.E. Huie, "Absorption cross sections, kinetics of formation, and self-reaction of the IO radical produced via laser photolysis of N2O/I2/N2 mixtures," J. Phys. Chem. 99, 11701-11707 (1995); DOI: 10.1021/j100030a013, have been degraded to the resolution 1.13 nm of the spectrum of W.J. Bloss, S.L. Nickolaisen, R.J. Salawitch, R.R. Friedel, and S.P. Sander, Kinetics of the self-reaction and 210 nm absorption cross section of the ClO dimer," J. Phys. Chem. A 105, 11226-11239 (2001); DOI: 10.1021/jp012429y. (2) The degraded spectra of Harwood et al. and Laszlo et al. have been normalized to the (4,0) peak value of Bloss et al.. (3) The mean of the degraded and normalized spectra of Harwood et al. and Laszlo et al. and that of Bloss et al. has been calculated and averaged over 1-nm intervals |
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