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The relationship between cloud condensation nuclei (CCN) concentration and light extinction of dried particles: indications of underlying aerosol processes and implications for satellite-based CCN estimates

机译:云凝结核浓度与干颗粒的消光之间的关系:潜在气溶胶过程的迹象以及对基于卫星的CCN估计的影响

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We examine the relationship between the number concentration ofboundary-layer cloud condensation nuclei (CCN) and light extinction toinvestigate underlying aerosol processes and satellite-based CCN estimates.For a variety of airborne and ground-based observations not dominated bydust, regression identifies the CCN (cm−3) at 0.4 ± 0.1%supersaturation with 100.3α +1.3σ0.75 where σ(Mm−1) is the 500 nm extinction coefficient by dried particles andα is the Angstrom exponent. The deviation of 1 kmhorizontal average data from this approximation is typically within a factorof 2.0. ∂logCCN / ∂logσ is less than unitybecause, among other explanations, growth processes generally make aerosolsscatter more light without increasing their number. This, barring specialmeteorology–aerosol connections, associates a doubling of aerosol opticaldepth with less than a doubling of CCN, contrary to previous studies basedon heavily averaged measurements or a satellite algorithm.
机译:我们研究了边界层云凝结核(CCN)的数量浓度与消光之间的关系,以研究潜在的气溶胶过程和基于卫星的CCN估计值。对于各种不受粉尘支配的机载和地面观测,回归分析确定了CCN( cm −3 )处于0.4±0.1%过饱和度,其中10 0.3α+1.3 σ 0.75 其中σ(Mm −1 )是干燥颗粒在500 nm处的消光系数,α是Angstrom指数。 1 km水平平均数据与该近似值的偏差通常在2.0的范围内。 ∂logCCN/∂logσ小于1,因为在其他解释中,生长过程通常使气溶胶散射更多的光而不增加其数量。除非特殊的气象学-气溶胶连接,否则将气溶胶光学深度的增加与CCN的增加相比要小得多,这与以前基于大量平均测量或卫星算法的研究相反。

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