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Aerosol optical properties in the southeastern United States in summer – Part?1: Hygroscopic growth

机译:夏季美国东南部的气溶胶光学特性-第一部分:吸湿性生长

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摘要

Aircraft observations of meteorological, trace gas, and aerosol properties were made during May–September?2013 in the southeastern United States (US) under fair-weather, afternoon conditions with well-defined planetary boundary layer structure. Optical extinction at 532?nm was directly measured at relative humidities (RHs) of ?~??15, ?~??70, and ?~??90?% and compared with extinction calculated from measurements of aerosol composition and size distribution using the iκ/i-K?hler approximation for hygroscopic growth. The calculated enhancement in hydrated aerosol extinction with relative humidity, if/i(RH), calculated by this method agreed well with the observed if/i(RH) at ?~??90?% RH. The dominance of organic aerosol, which comprised 65?±?10?% of particulate matter with aerodynamic diameter ?&??1?μm in the planetary boundary layer, resulted in relatively low if/i(RH) values of 1.43?±?0.67 at 70?% RH and 2.28?±?1.05 at 90?% RH. The subsaturated iκ/i-K?hler hygroscopicity parameter iκ/i for the organic fraction of the aerosol must have been ?&??0.10 to be consistent with 75?% of the observations within uncertainties, with a best estimate of iκ/i??=??0.05. This subsaturated iκ/i value for the organic aerosol in the southeastern US is broadly consistent with field studies in rural environments. A new, physically based, single-parameter representation was developed that better described if/i(RH) than did the widely used gamma power-law approximation.
机译:飞机在2013年5月至9月间于美国东南部(US)在晴朗的天气,下午的条件下进行了气象,微量气体和气溶胶特性的观测,并确定了行星边界层的结构。在相对湿度(RHs)为?〜?? 15,?〜?? 70和?〜?90?%的条件下,直接测量532?nm处的消光,并与使用气溶胶组成和尺寸分布的测量值计算得出的消光进行比较。吸湿生长的κ -K?hler近似。用这种方法计算出的相对湿度 f (RH)引起的水合气溶胶消光增强作用与在90℃〜90℃观察到的 f (RH)吻合得很好。相对湿度在行星边界层中占主导地位的有机气溶胶占空气动力学直径为φ<≤1≤μm的颗粒物的65?±?10?%,导致相对较低的 f (RH)相对湿度在70%时为1.43±±0.67,在相对湿度为90%时为2.28±1.05。气溶胶有机部分的亚饱和κ -K?hler吸湿性参数κ必须为≤0.10,与观测值的75%一致在不确定性范围内,最佳估计κ ?? = ?? 0.05。美国东南部有机气溶胶的亚饱和κ值与农村环境的田间研究基本一致。开发了一种新的基于物理的单参数表示形式,与广泛使用的伽马幂律近似法相比,它可以更好地描述 f (RH)。

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