A new method to determine the aerosol optical properties from multiple-wavelength O<sub>4</sub> absorptions by MAX-DOAS observation

oleh: C. Xing, C. Liu, C. Liu, C. Liu, C. Liu, S. Wang, S. Wang, Q. Hu, H. Liu, W. Tan, W. Zhang, W. Zhang, B. Li, J. Liu, J. Liu

Format: Article
Diterbitkan: Copernicus Publications 2019-06-01

Deskripsi

<p>Ground-based multi-axis differential optical absorption spectroscopy (MAX-DOAS) observation was carried out from November 2016 to February 2017 in Beijing, China, to measure the <span class="inline-formula">O<sub>4</sub></span> absorptions in UV and visible bands and further to illustrate its relationship with aerosol optical properties (AOPs) under different weather types. According to relative humidity, visibility, and PM<span class="inline-formula"><sub>2.5</sub></span>, we classified the observation periods into clear, light-haze, haze, heavy-haze, fog, and rainy weather conditions. There are obvious differences for measured AOPs under different weather conditions, especially scattering coefficient (<span class="inline-formula"><i>σ</i><sub>sca</sub></span>) and absorption coefficient (<span class="inline-formula"><i>σ</i><sub>sca</sub></span>). It was also found that both the <span class="inline-formula">O<sub>4</sub></span> differential slant column densities (DSCDs) at the UV and visible bands varied in the order of clear days&thinsp;&gt;&thinsp;light-haze days&thinsp;&gt;&thinsp;haze days&thinsp;&gt;&thinsp;heavy-haze days&thinsp;&gt;&thinsp;fog days. The correlation coefficients (<span class="inline-formula"><i>R</i><sup>2</sup></span>) between <span class="inline-formula">O<sub>4</sub></span> DSCDs at 360.8 and 477.1&thinsp;nm mainly varied in the order of clear days&thinsp;&gt;&thinsp;light-haze days&thinsp;&gt;&thinsp;haze days&thinsp;&gt;&thinsp;heavy-haze days. Based on the statistics of <span class="inline-formula">O<sub>4</sub></span> DSCDs at an elevation angle 1<span class="inline-formula"><sup>∘</sup></span> with the corresponding linear regression between UV and visible bands of segmental periods, the relationships between <span class="inline-formula">O<sub>4</sub></span> DSCDs and AOPs were established. It should mainly be clear or light-haze days when the correlation slope is greater than 1.0, with a correlation coefficient (<span class="inline-formula"><i>R</i><sup>2</sup></span>) greater than 0.9, and <span class="inline-formula">O<sub>4</sub></span> DSCDs mainly greater than <span class="inline-formula">2.5×10<sup>43</sup></span>&thinsp;molec.&thinsp;cm<span class="inline-formula"><sup>−2</sup></span>. Meanwhile, <span class="inline-formula"><i>σ</i><sub>sca</sub></span> and <span class="inline-formula"><i>σ</i><sub>abs</sub></span> are less than 45 and 12&thinsp;Mm<span class="inline-formula"><sup>−1</sup></span>, respectively. For haze or heavy-haze days, the correlation slope is less than 0.6, with an <span class="inline-formula"><i>R</i><sup>2</sup></span> less than 0.8, and <span class="inline-formula">O<sub>4</sub></span> DSCDs mainly less than <span class="inline-formula">1.3×10<sup>43</sup></span>&thinsp;molec.&thinsp;cm<span class="inline-formula"><sup>−2</sup></span>, under which <span class="inline-formula"><i>σ</i><sub>sca</sub></span> and <span class="inline-formula"><i>σ</i><sub>abs</sub></span> are mainly located at 200–900 and 20–60&thinsp;Mm<span class="inline-formula"><sup>−1</sup></span>. Additionally, the determination method was well validated based on another MAX-DOAS measurement at Gucheng from 19 to 27 November 2016. For more precise and accurate inversion of AOPs, more detailed look-up tables for <span class="inline-formula">O<sub>4</sub></span> multiple-wavelength absorptions need to be developed. Since the ground surface AOPs were determined using MAX-DOAS observation at a 1<span class="inline-formula"><sup>∘</sup></span> elevation in this study, we hope to highlight the potential of retrieved vertical spatially resolved AOPs being expected when multiple elevation angles of MAX-DOAS observation are used together.</p>