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On microphysical processes of noctilucent clouds (NLC): Observations and modeling of mean and width of the particle size-distribution

机译:关于夜光云(NLC)的微物理过程:粒径分布的均值和宽度的观察和建模

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摘要

Noctilucent clouds (NLC) in the polar summer mesopause region have been observed in Norway (69° N, 16° E) between 1998 and 2009 by 3-color lidar technique. Assuming a mono-modal Gaussian size distribution we deduce mean and width of the particle sizes throughout the clouds. We observe a quasi linear relationship between distribution width and mean of the particle size at the top of the clouds and a deviation from this behavior for particle sizes larger than 40 nm, most often in the lower part of the layer. The vertically integrated particle properties show that 65% of the data follows the linear relationship with a slope of 0.42±0.02 for mean particle sizes up to 40 nm. For the vertically resolved particle properties (Δz = Combining double low line 0.15 km) the slope is comparable and about 0.39±0.03. For particles larger than 40 nm the distribution width becomes nearly independent of particle size and even decreases in the lower part of the layer. We compare our observations to microphysical modeling of noctilucent clouds and find that the distribution width depends on turbulence, the time that turbulence can act (cloud age), and the sampling volume/time (atmospheric variability). The model results nicely reproduce the measurements and show that the observed slope can be explained by eddy diffusion profiles as observed from rocket measurements.
机译:1998年至2009年之间,挪威使用3色激光雷达技术在极地夏季更年期地区的夜光云(NLC)中进行了观测(69°N,16°E)。假设单峰高斯尺寸分布,我们推论出整个云中颗粒尺寸的均值和宽度。我们观察到分布宽度与云层顶部平均粒径之间的准线性关系,以及对于大于40 nm的粒径(通常在层的下部)最大粒径的这种行为的偏差。垂直积分的粒子特性显示,对于平均粒径最大为40 nm的数据,有65%的数据遵循线性关系,斜率为0.42±0.02。对于垂直解析的粒子属性(Δz=组合双低线0.15 km),斜率是可比较的,约为0.39±0.03。对于大于40 nm的颗粒,分布宽度几乎与颗粒大小无关,甚至在层的下部减小。我们将我们的观察结果与夜光云的微观物理模型进行了比较,发现分布宽度取决于湍流,湍流作用的时间(云龄)和采样量/时间(大气可变性)。模型结果很好地重现了测量结果,并表明观察到的斜率可以用从火箭测量中观察到的涡流扩散曲线来解释。

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