Abstract

Abstract. Accurate absorption spectra of gases in the near–ultraviolet (300 to 400 nm) are essential in atmospheric observations and laboratory studies. This paper describes a novel incoherent broadband cavity-enhanced absorption spectroscopy (IBBCEAS) instrument for measuring very weak absorption spectra from 335 to 375 nm. The instrument performance was validated against the 3B1-X1A1 transition of SO2. The measured absorption varied linearly with SO2 column density and the resulting spectrum agrees well with published spectra. Using the instrument, we report new absorption cross-sections of O3, acetone, 2-butanone, and 2-pentanone in this spectral region, where literature data diverge considerably. In the absorption minimum between the Huggins and Chappuis bands, our absorption spectra fall at the lower range of reported ozone absorption cross-sections. The spectra of the ketones agree with prior spectra at moderate absorptions, but differ significantly at the limits of other instruments' sensitivity. The collision-induced absorption of the O4 dimer at 360.5 nm was also measured and found to have a maximum cross-section of ca. 4.0×10−46 cm5 molecule−2. We demonstrate the application of the instrument to quantifying low concentrations of the short-lived radical, BrO, in the presence of stronger absorptions from Br2 and O3.

Highlights

  • Whereas large absorption cross-sections of atmospheric species are generally well established, weak absorption spectra are often poorly known

  • The near-ultraviolet (300 nm to 400 nm) absorption spectra of gases are relevant for understanding and modelling the chemistry of the atmosphere, since light in this spectral region drives most tropospheric photochemistry

  • Our aim in this paper is to demonstrate an incoherent broadband cavity-enhanced absorption spectroscopy (IBBCEAS) instrument for measuring weak absorption spectra of gases over the wavelength range 335 to 375 nm

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Summary

Introduction

Whereas large absorption cross-sections of atmospheric species are generally well established, weak absorption spectra are often poorly known. Weak absorptions, which occur when molecular absorption cross-sections are small or when the concentration of the species of interest is low, are a challenge to measure. Low gas concentrations are found for substances with low vapour pressures; as a result, the ultraviolet spectra of many low volatility organic species of atmospheric interest have yet to be determined. This includes the large group of compounds with carbonyl or nitro functional groups, for which the n → π transition occurs in the near-ultraviolet

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