Abstract

<strong class="journal-contentHeaderColor">Abstract.</strong> An instrument based on 20 m open-path incoherent broadband cavity-enhanced absorption spectroscopy (IBBCEAS) was established at the Jülich SAPHIR chamber in spring 2011. The setup was optimized for the detection of HONO and NO<span class="inline-formula"><sub>2</sub></span> in the near-UV region 352–386 nm, utilizing a bright hot-spot Xe-arc lamp and a UV-enhanced charge-coupled device (CCD) detector. A 2<span class="inline-formula"><i>σ</i></span> detection limit of 26 pptv for HONO and 76 pptv for NO<span class="inline-formula"><sub>2</sub></span> was achieved for an integration time of 1 min. Methacrolein (MACR) was also detected at mixing ratios below 5 ppbv with an estimated 2<span class="inline-formula"><i>σ</i></span> detection limit of 340 pptv for the same integration time. The IBBCEAS instrument's performance for HONO and NO<span class="inline-formula"><sub>2</sub></span> detection was compared to that of extractive wet techniques, long-path absorption photometry (LOPAP), and chemiluminescence spectrometry (CLS) <span class="inline-formula">NO<sub><i>x</i></sub></span> detection, respectively. For the combined data sets an overall good agreement for both trend and absolute mixing ratios was observed between IBBCEAS and these established instruments at SAPHIR. Correlation coefficients <span class="inline-formula"><i>r</i></span> for HONO range from 0.930 to 0.994 and for NO<span class="inline-formula"><sub>2</sub></span> from 0.937 to 0.992. For the single measurement of MACR <span class="inline-formula"><i>r</i>=0.981</span> is found in comparison to proton-transfer-reaction mass spectrometry (PTRMS).

Highlights

  • Photolysis of nitrous acid (HONO + h ( < 400 nm OH + NO) leads to the formation of the most important daytime 25 oxidant in the atmosphere, the hydroxyl radical (OH)

  • Measurements of time-dependent mixing ratios of HONO, NO2 and MACR using open-path incoherent broadband cavity-enhanced absorption spectroscopy (IBBCEAS) were taken during Summer and Autumn 2011, and compared with those utilizing long-path absorption photometry (LOPAP), chemiluminescence 190 spectrometry (CLS) and proton transfer reaction mass spectrometry (PTRMS), respectively

  • After cleaning and humidifying the SAPHIR chamber HONO formation by unknown photo-induced reactions on the Teflon chamber walls and degradation was studied in experiments always including light-induced and dark reactions of HONO formation or destruction – the experimental protocols 200 concerning changes in chamber conditions are given in the figure captions

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Summary

Introduction

Photolysis of nitrous acid (HONO + h ( < 400 nm OH + NO) leads to the formation of the most important daytime 25 oxidant in the atmosphere, the hydroxyl radical (OH). HONO indirectly affects the oxidative potential of the troposphere and strongly influences degradation mechanisms of a vast variety of natural and urban pollutants. The mechanisms of HONO formation in the troposphere are still not fully understood (Calvert et al 1994, Finlayson-Pitts et al 2003, Ramazan et al 2004, Liu et al 2019). Many atmospheric studies revealed elevated HONO mixing ratios during daytime under specific conditions that cannot be fully explained (Staffelbach et al 1997, Zhou et al 2002a, Zhou et al 2003, Kleffmann et al 2003, Vogel et al 30 2003, Kleffmann et al 2005, Acker et al 2006, Spataro and Ianniello, 2014).

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