Abstract

<strong class="journal-contentHeaderColor">Abstract.</strong> In the summer of 2018, a comprehensive field campaign, with measurements on HONO and related parameters, was conducted at the foot (150 m a.s.l.) and the summit of Mt. Tai (1534 m a.s.l.) in the central North China Plain (NCP). With the implementation of a 0-D box model, the HONO budget with six additional sources and its role in radical chemistry at the foot station were explored. We found that the model default source, NO <span class="inline-formula">+</span> OH, could only reproduce 13 % of the observed HONO, leading to a strong unknown source strength of up to 3 ppbv h<span class="inline-formula"><sup>−1</sup></span>. Among the additional sources, the NO<span class="inline-formula"><sub>2</sub></span> uptake on the ground surface dominated (<span class="inline-formula">∼</span> 70 %) nighttime HONO formation, and its photo-enhanced reaction dominated (<span class="inline-formula">∼</span> 80 %) daytime HONO formation. Their contributions were sensitive to the mixing layer height (MLH) used for the parameterizations, highlighting the importance of a reasonable MLH for exploring ground-level HONO formation in 0-D models and the necessity of gradient measurements. A <span class="inline-formula">Δ</span>HONO<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M10" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>/</mo><mi mathvariant="normal">Δ</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="16pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="70487647a1f237ca782af0f088ac6be0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-22-1035-2022-ie00001.svg" width="16pt" height="14pt" src="acp-22-1035-2022-ie00001.png"/></svg:svg></span></span>NO<span class="inline-formula"><sub><i>x</i></sub></span> ratio of 0.7 % for direct emissions from vehicle exhaust was inferred, and a new method to quantify its contribution to the observations was proposed and discussed. Aerosol-derived sources, including the NO<span class="inline-formula"><sub>2</sub></span> uptake on the aerosol surface and the particulate nitrate photolysis, did not lead to significant HONO formation, with their contributions lower than NO <span class="inline-formula">+</span> OH. <span id="page1036"/>HONO photolysis in the early morning initialized the daytime photochemistry at the foot station. It was also a substantial radical source throughout the daytime, with contributions higher than O<span class="inline-formula"><sub>3</sub></span> photolysis to OH initiation. Moreover, we found that OH dominated the atmospheric oxidizing capacity in the daytime, while modeled NO<span class="inline-formula"><sub>3</sub></span> appeared to be significant at night. Peaks of modeled NO<span class="inline-formula"><sub>3</sub></span> time series and average diurnal variation reached 22 and 9 pptv, respectively. NO<span class="inline-formula"><sub>3</sub></span>-induced reactions contribute 18 % of nitrate formation potential (<span class="inline-formula"><i>P</i></span>(HNO<span class="inline-formula"><sub>3</sub></span>)) and 11 % of the isoprene (C<span class="inline-formula"><sub>5</sub></span>H<span class="inline-formula"><sub>8</sub></span>) oxidation throughout the whole day. At night, NO<span class="inline-formula"><sub>3</sub></span> chemistry led to 51 % and 44 % of <span class="inline-formula"><i>P</i></span>(HNO<span class="inline-formula"><sub>3</sub></span>) or the C<span class="inline-formula"><sub>5</sub></span>H<span class="inline-formula"><sub>8</sub></span> oxidation, respectively, implying that NO<span class="inline-formula"><sub>3</sub></span> chemistry could significantly affect nighttime secondary organic and inorganic aerosol formation in this high-O<span class="inline-formula"><sub>3</sub></span> region. Considering the severe O<span class="inline-formula"><sub>3</sub></span> pollution in the NCP and the very limited NO<span class="inline-formula"><sub>3</sub></span> measurements, we suggest that besides direct measurements of HO<span class="inline-formula"><sub><i>x</i></sub></span> and primary HO<span class="inline-formula"><sub><i>x</i></sub></span> precursors (O<span class="inline-formula"><sub>3</sub></span>, HONO, alkenes, etc.), NO<span class="inline-formula"><sub>3</sub></span> measurements should be conducted to understand the atmospheric oxidizing capacity and air pollution formation in this and similar regions.

Highlights

  • Numerous field campaigns coupled with model simulations have been conducted worldwide to understand summertime atmospheric chemistry as it is linked to the regional air quality and global climate (Alicke et al, 2003; Elshorbany et al, 2012; Heard et al, 2004; Kanaya et al, 2009, 2013; Michoud et al, 2012; Ren et al, 2003; Rohrer and Berresheim, 2006; Tan et al, 2017; Travis et al, 2020)

  • Very few NO3 measurements are available in China (Lu et al, 2019; Suhail et al, 2019), while its high concentration and important role in chemical oxidation presented in this study indicate the necessity of direct NO3 measurements in the North China Plain (NCP), where summertime O3 levels are substantially increasing (Han et al, 2020; Li et al, 2019; Sun et al, 2016, 2019)

  • The present study was conducted mainly based on measurements at the foot station

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Summary

Introduction

Numerous field campaigns coupled with model simulations have been conducted worldwide to understand summertime atmospheric chemistry as it is linked to the regional air quality and global climate (Alicke et al, 2003; Elshorbany et al, 2012; Heard et al, 2004; Kanaya et al, 2009, 2013; Michoud et al, 2012; Ren et al, 2003; Rohrer and Berresheim, 2006; Tan et al, 2017; Travis et al, 2020). HONO photolysis is reported to be an important or even the major OH source in the lower atmosphere of polluted regions, with a contribution of 20 %–90 % (Alicke et al, 2003; Elshorbany et al, 2009; Kleffmann et al, 2005; Platt et al, 1980; Slater et al, 2020; Whalley et al, 2021; Xue et al, 2020). This process still needs more global quantification due to the incomplete understanding of HONO formation and its vertical distribution in the atmosphere (Kleffmann, 2007). A state-ofart summary of the reported HONO sources can be found in our recent study (Xue et al, 2020)

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