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利用宇宙成因35S探测平流层深层侵入

Detection of deep stratospheric intrusions by cosmogenic 35S.

作者信息

Lin Mang, Su Lin, Shaheen Robina, Fung Jimmy C H, Thiemens Mark H

机构信息

Department of Chemistry and Biochemistry, University of California, San Diego, La Jolla, CA 92093;

Environmental Science Programs, School of Science, Hong Kong University of Science and Technology, Clear Water Bay, Hong Kong, China.

出版信息

Proc Natl Acad Sci U S A. 2016 Oct 4;113(40):11131-11136. doi: 10.1073/pnas.1609919113. Epub 2016 Sep 21.

Abstract

The extent to which stratospheric intrusions on synoptic scales influence the tropospheric ozone (O) levels remains poorly understood, because quantitative detection of stratospheric air has been challenging. Cosmogenic S mainly produced in the stratosphere has the potential to identify stratospheric air masses at ground level, but this approach has not yet been unambiguously shown. Here, we report unusually high S concentrations (7,390 atoms m; ∼16 times greater than annual average) in fine sulfate aerosols (aerodynamic diameter less than 0.95 µm) collected at a coastal site in southern California on May 3, 2014, when ground-level O mixing ratios at air quality monitoring stations across southern California (43 of 85) exceeded the recently revised US National Ambient Air Quality Standard (daily maximum 8-h average: 70 parts per billion by volume). The stratospheric origin of the significantly enhanced S level is supported by in situ measurements of air pollutants and meteorological variables, satellite observations, meteorological analysis, and box model calculations. The deep stratospheric intrusion event was driven by the coupling between midlatitude cyclones and Santa Ana winds, and it was responsible for the regional O pollution episode. These results provide direct field-based evidence that S is an additional sensitive and unambiguous tracer in detecting stratospheric air in the boundary layer and offer the potential for resolving the stratospheric influences on the tropospheric O level.

摘要

平流层大尺度侵入对流层对对流层臭氧(O)水平的影响程度仍知之甚少,因为对平流层空气进行定量检测颇具挑战性。主要在平流层产生的宇宙成因硫有潜力识别地面的平流层气团,但这种方法尚未得到明确证实。在此,我们报告了2014年5月3日在南加州沿海站点收集的细硫酸盐气溶胶(空气动力学直径小于0.95微米)中硫浓度异常高(7390个原子/立方米;约为年平均值的16倍),当时南加州空气质量监测站(85个中的43个)的地面臭氧混合比超过了最近修订的美国国家环境空气质量标准(每日最大8小时平均值:70体积十亿分比)。空气污染物和气象变量的现场测量、卫星观测、气象分析以及箱式模型计算均支持了硫水平显著增强的平流层来源。这次平流层深度侵入事件是由中纬度气旋与圣安娜风的耦合驱动的,它导致了区域性臭氧污染事件。这些结果提供了基于实地的直接证据,表明硫是检测边界层平流层空气的另一种灵敏且明确的示踪剂,并为解决平流层对对流层臭氧水平的影响提供了可能性。

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Detection of deep stratospheric intrusions by cosmogenic 35S.利用宇宙成因35S探测平流层深层侵入
Proc Natl Acad Sci U S A. 2016 Oct 4;113(40):11131-11136. doi: 10.1073/pnas.1609919113. Epub 2016 Sep 21.

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