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首页> 外文期刊>Atmospheric chemistry and physics >Characterization of forest fire smoke event near Washington, DC in summer 2013 with multi-wavelength lidar
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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表征2013年夏季华盛顿特区附近的森林火灾烟雾事件

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摘要

The multi-wavelength lidar technique was applied to the study of a smoke event near Washington, DC on 26-28 August 2013. Satellite observations combined with transport model predictions imply that the smoke plume originated mainly from Wyoming/Idaho forest fires and its transportation to Washington, DC took approximately 5 days. The NASA Goddard Space Flight Center (GSFC) multi-wavelength Mie-Raman lidar was used to measure the smoke particle intensive parameters such as extinction and backscatter Angstrom exponents together with lidar ratios at 355 and 532 nm wavelengths. For interpretation of the observed vertical profiles of the backscatter Angstrom exponents gamma beta at 355-532 and 532-1064 nm, numerical simulation was performed. The results indicate that, for fine-mode dominant aerosols, the Angstrom exponents gamma beta (355-532) and gamma beta (5321064) have essentially different dependence on the particle size and refractive index. Inversion of 3 beta + 2 alpha lidar observations on 27-28 August provided vertical variation of the particle volume, effective radius and the real part of the refractive index through the planetary boundary layer (PBL) and the smoke layer. The particle effective radius decreased with height from approximately 0.27 mu m inside the PBL to 0.15 mu m in the smoke layer, which was situated above the PBL. Simultaneously the real part of the refractive index in the smoke layer increased to m(R) approximate to 1.5. The retrievals demonstrate also that the fine mode is predominant in the particle size distribution, and that the decrease of the effective radius with height is due to a shift of the fine mode toward smaller 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烟雾事件。卫星观测结果与运输模型预测相结合,表明烟雾羽流主要来自怀俄明州/爱达荷州的森林大火及其向大气中的运输华盛顿特区花费了大约5天的时间。美国宇航局戈达德太空飞行中心(GSFC)多波长Mie-Raman激光雷达用于测量烟雾颗粒强度参数,例如消光和后向散射埃斯特朗姆斯指数,以及355和532 nm波长的激光雷达比率。为了解释在355-532和532-1064 nm处观察到的反向散射Angstrom指数γ的垂直分布,进行了数值模拟。结果表明,对于精细模式的优势气溶胶,埃数指数γβ(355-532)和γβ(5321064)对颗粒大小和折射率具有根本不同的依赖性。 8月27日至28日对3 beta + 2 alpha激光雷达观测结果的反演提供了通过行星边界层(PBL)和烟层的粒子体积,有效半径和折射率的实部的垂直变化。粒子的有效半径随着高度的增加而从PBL内部的约0.27μm降低到位于PBL上方的烟层中的0.15μm。同时,烟气层中折射率的实部增加到m(R)大约为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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