Increasing OH tied to increasing NOx in the Mt. Everest
ID:1946 View Protection:ATTENDEE Updated Time:2024-04-11 20:56:10 Hits:1698 Oral Presentation

Start Time:2024-05-19 12:15(Asia/Shanghai)

Duration:5min

Session:S13 主题13、气溶胶与大气环境 » S13-3主题13、气溶胶与大气环境 专题13.13(19日上午,214)

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Abstract
Tropospheric OH is buffered and thus relative stable in either a regional scale or global scale. Snow photochemistry in the high latitude amplifies the OH photochemical production in the low atmosphere following cross-boundary transport of snow impurities. As a result, the Antarctic pole OH and the Arctic pole OH resonate with emission inventory decline in the Europe since 1960s. Although the whole picture of snow photochemistry is not totally clear, intensive UV with high solar zenith angle and cross-boundary transport and deposition of HNO3/nitrate is known to favor a maximizing snow NOx emission flux and efficiency in the Mt. Everest. Consequently, the highest OH and highest growth slope of OH are revealed for the Mt. Everest with a nearly-explicit chemical model of MCM. Unlike relatively slow vertical mixing in the shallow boundary layer of the Antarctic and the Arctic, the Mt. Everest features the most intensive occurring of the deepest convection which effectively deliveries surface airmasses into the global circulation system. The global impacts on the oxidative capacity of the atmosphere is thus likely and needs further evaluation.
 
Keywords
OH,NOx,snow photochemistry
Speaker
张冲
博士研究生 北京大学

Submission Author
张冲 北京大学
叶春翔 北京大学环境科学与工程学院
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    2024

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    May 20

    2024

  • Mar 31 2024

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青年地学论坛理事会
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厦门大学近海海洋环境科学国家重点实验室
中国科学院城市环境研究所
自然资源部第三海洋研究所
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