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Characterization of forest fire smoke event near Washington, DC in summer 2013 with multi-wavelength lidar

机译:使用多波长激光雷达对2013年夏季华盛顿特区附近的森林火灾烟雾事件进行表征

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摘要

The multi-wavelength lidar technique was applied to the study of a smokeevent near Washington, DC on 26–28 August 2013. Satellite observationscombined with transport model predictions imply that the smoke plumeoriginated mainly from Wyoming/Idaho forest fires and its transportation toWashington, DC took approximately 5 days. The NASA Goddard Space Flight Center (GSFC) multi-wavelengthMie–Raman lidar was used to measure the smoke particle intensive parameterssuch as extinction and backscatter Ångström exponents together withlidar ratios at 355 and 532 nm wavelengths. For interpretation of theobserved vertical profiles of the backscatter Ångström exponentsγ at 355–532 and 532–1064 nm, numerical simulation wasperformed. The results indicate that, for fine-mode dominant aerosols, theÅngström exponents γ(355–532) and γ(532–1064) have essentially different dependence on the particlesize and refractive index. Inversion of 3 β + 2 α lidarobservations on 27–28 August provided vertical variation of the particlevolume, effective radius and the real part of the refractive index throughthe planetary boundary layer (PBL) and the smoke layer. The particle effective radius decreased withheight from approximately 0.27 μm inside the PBL to 0.15 μm inthe smoke layer, which was situated above the PBL. Simultaneously the realpart of the refractive index in the smoke layer increased to ≈ 1.5. The retrievals demonstrate also that the fine mode ispredominant in the particle size distribution, and that the decrease of theeffective radius with height is due to a shift of the fine mode towardsmaller radii.
机译:多波长激光雷达技术已用于研究2013年8月26日至28日在华盛顿特区附近的一次烟雾事件。卫星观测结果与运输模型预测相结合,表明烟雾主要来自怀俄明州/爱达荷州森林大火,其向华盛顿特区的运输大约5天。美国宇航局戈达德太空飞行中心(GSFC)多波长米厄-拉曼激光雷达用于测量烟粒密集型参数,例如消光和反向散射Ångström指数,以及在355和532 nm波长下的激光雷达比。为了解释在355–532和532–1064 nm处观察到的反向散射Ångström指数γ的垂直剖面,进行了数值模拟。结果表明,对于精细模式占优势的气溶胶,Ångström指数γ(355–532)和γ(532–1064)对颗粒大小和折射率的依赖性基本不同。 8月27日至28日对3β+ 2α激光雷达的反演提供了通过行星边界层(PBL)和烟气层的粒子体积,有效半径和折射率的实部的垂直变化。粒子的有效半径随高度的增加而从PBL内部的约0.27μm减小到位于PBL上方的烟层中的0.15μm。同时,烟气层中的折射率的实部增加到大约。 1.5。检索结果还表明,精细模式在粒度分布中占主导地位,有效半径随高度的减小是由于精细模式向较小半径的偏移。

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