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Fate of the nitrate radical at the summit of a semi-rural mountain site in Germany assessed with direct reactivity measurements
oleh: P. Dewald, C. M. Nussbaumer, J. Schuladen, A. Ringsdorf, A. Edtbauer, H. Fischer, J. Williams, J. Lelieveld, J. N. Crowley
| Format: | Article |
|---|---|
| Diterbitkan: | Copernicus Publications 2022-06-01 |
Deskripsi
<p>The reactivity of NO<span class="inline-formula"><sub>3</sub></span> plays an important role in modifying the fate of reactive nitrogen species at nighttime. High reactivity (e.g. towards unsaturated volatile organic compounds – VOCs) can lead to formation of organic nitrates and secondary organic aerosol, whereas low reactivity opens the possibility of heterogeneous NO<span class="inline-formula"><sub><i>x</i></sub></span> losses via the formation and uptake of N<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>5</sub></span> to particles.</p> <p>We present direct NO<span class="inline-formula"><sub>3</sub></span> reactivity measurements (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M7" display="inline" overflow="scroll" dspmath="mathml"><mrow><msup><mi>k</mi><mrow class="chem"><msub><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn></msub></mrow></msup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="24pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="e62469e350bfbd2e9f68c31f76725b79"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-22-7051-2022-ie00001.svg" width="24pt" height="13pt" src="acp-22-7051-2022-ie00001.png"/></svg:svg></span></span>) that quantify the VOC-induced losses of NO<span class="inline-formula"><sub>3</sub></span> during the TO2021 campaign at the summit of the Kleiner Feldberg mountain (825 m, Germany) in July 2021. <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M9" display="inline" overflow="scroll" dspmath="mathml"><mrow><msup><mi>k</mi><mrow class="chem"><msub><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn></msub></mrow></msup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="24pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="fc4d56c2b7a1cfe18d75d01c2d26ae04"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-22-7051-2022-ie00002.svg" width="24pt" height="13pt" src="acp-22-7051-2022-ie00002.png"/></svg:svg></span></span> was on average <span class="inline-formula">∼0.035</span> s<span class="inline-formula"><sup>−1</sup></span> during the daytime, <span class="inline-formula">∼0.015</span> s<span class="inline-formula"><sup>−1</sup></span> for almost half of the nights and below the detection limit of 0.006 s<span class="inline-formula"><sup>−1</sup></span> for the other half, which may be linked to sampling from above the nocturnal surface layer. NO<span class="inline-formula"><sub>3</sub></span> reactivities derived from VOC measurements and the corresponding rate coefficient were in good agreement with <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M16" display="inline" overflow="scroll" dspmath="mathml"><mrow><msup><mi>k</mi><mrow class="chem"><msub><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn></msub></mrow></msup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="24pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="62ef12770af628460499df482e0383ef"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-22-7051-2022-ie00003.svg" width="24pt" height="13pt" src="acp-22-7051-2022-ie00003.png"/></svg:svg></span></span>, with monoterpenes representing 84 % of the total reactivity. The fractional contribution <span class="inline-formula"><i>F</i></span> of <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M18" display="inline" overflow="scroll" dspmath="mathml"><mrow><msup><mi>k</mi><mrow class="chem"><msub><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn></msub></mrow></msup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="24pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="c33373a1e3ca7af4a5044bc1f50ef98b"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-22-7051-2022-ie00004.svg" width="24pt" height="13pt" src="acp-22-7051-2022-ie00004.png"/></svg:svg></span></span> to the overall NO<span class="inline-formula"><sub>3</sub></span> loss rate (which includes an additional reaction of NO<span class="inline-formula"><sub>3</sub></span> with NO and photolysis) were on average <span class="inline-formula">∼16</span> % during the daytime and <span class="inline-formula">∼50</span> %–60 % during the nighttime. The relatively low nighttime value of <span class="inline-formula"><i>F</i></span> is related to the presence of several tens of parts per trillion by volume (pptv) of NO on several nights. NO<span class="inline-formula"><sub>3</sub></span> mixing ratios were not measured, but steady-state calculations resulted in nighttime values between <span class="inline-formula"><i><</i>1</span> and 12 pptv. A comparison of results from TO2021 with direct measurements of NO<span class="inline-formula"><sub>3</sub></span> during previous campaigns between 2008 and 2015 at this site revealed that NO<span class="inline-formula"><sub>3</sub></span> loss rates were remarkably high during TO2021, while NO<span class="inline-formula"><sub>3</sub></span> production rates were low.</p> <p>We observed NO mixing ratios of up to 80 pptv at night, which has implications for the cycling of reactive nitrogen at this site. With O<span class="inline-formula"><sub>3</sub></span> present at levels of mostly 25 to 60 ppbv (parts per billion by volume), NO is oxidized to NO<span class="inline-formula"><sub>2</sub></span> on a timescale of a few minutes. We find that maintaining NO mixing ratios of, e.g., 40 pptv requires a ground-level NO emission rate of 0.33 pptv s<span class="inline-formula"><sup>−1</sup></span> (into a shallow surface layer of 10 m depth). This in turn requires a rapid deposition of NO<span class="inline-formula"><sub>2</sub></span> to the surface (vd<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M33" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi/><mrow class="chem"><msub><mi mathvariant="normal">NO</mi><mn mathvariant="normal">2</mn></msub></mrow></msub><mo>∼</mo><mn mathvariant="normal">0.15</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="52pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="4a273752f2992f916e30a02eaa5ce3b7"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-22-7051-2022-ie00005.svg" width="52pt" height="14pt" src="acp-22-7051-2022-ie00005.png"/></svg:svg></span></span> cm s<span class="inline-formula"><sup>−1</sup></span>) to reduce nocturnal NO<span class="inline-formula"><sub>2</sub></span> levels to match the observations.</p>