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NASA NTRS · 19880056661

Visible-ultraviolet absorption cross sections for NO2 as a function of temperature

Abstract

A redetermination of the temperature dependence of the absorption cross-section (sigma) of NO2 in the visible-ultraviolet region was made in order to provide a more reliable data base for the calculation of NO2 photolysis rates in the atmosphere. Experiments over a wide range of temperatures and NO2 concentrations were conducted. The integral of a plot of sigma versus the inverse of the wavelength was essentially independent of temperature. Increasing temperature produced a shift of the spectrum toward longer wavelengths, resulting in a small negative temperature dependence of sigma over the 264-400 nm range and a small positive dependence over the 450-649 nm range. Increasing temperature produced broadening of individual spectral features, resulting in a systematic lowering of peaks and filling of valleys. Recommended cross sections are presented for use in tropospheric NO2 photolysis rate calculations.

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Davidson, J. A., Cantrell, C. A., Mcdaniel, A. H., Shetter, R. E., Madronich, S.. 1988-06-20. Visible-ultraviolet absorption cross sections for NO2 as a function of temperature. https://ntrs.nasa.gov/citations/19880056661

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