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Studying the vertical aerosol extinction coefficient by comparing in situ airborne data and elastic backscatter lidar

机译:通过比较原位机载数据和弹性后向散射激光雷达研究垂直气溶胶消光系数

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摘要

Vertical profiles of aerosol particle optical properties were explored in a case study near the San Pietro Capofiume (SPC) ground station during the PEGASOS Po Valley campaign in the summer of 2012. A Zeppelin NT airship was employed to investigate the effect of the dynamics of the planetary boundary layer at altitudes between ∼  50 and 800 m above ground. Determined properties included the aerosol particle size distribution, the hygroscopic growth factor, the effective index of refraction and the light absorption coefficient. The first three parameters were used to retrieve the light scattering coefficient. Simultaneously, direct measurements of both the scattering and absorption coefficient were carried out at the SPC ground station. Additionally, a single wavelength polarization diversity elastic lidar system provided estimates of aerosol extinction coefficients using the Klett method to accomplish the inversion of the signal, for a vertically resolved comparison between in situ and remote-sensing results. Note, however, that the comparison was for the most part done in the altitude range where the overlap function is incomplete and accordingly uncertainties are larger. First, the airborne results at low altitudes were validated with the ground measurements. Agreement within approximately ±25 and ±20 % was found for the dry scattering and absorption coefficient, respectively. The single scattering albedo, ranged between 0.83 and 0.95, indicating the importance of the absorbing particles in the Po Valley region. A clear layering of the atmosphere was observed during the beginning of the flight (until ∼  10:00 LT – local time) before the mixing layer (ML) was fully developed. Highest extinction coefficients were found at low altitudes, in the new ML, while values in the residual layer, which could be probed at the beginning of the flight at elevated altitudes, were lower. At the end of the flight (after ∼  12:00 LT) the ML was fully developed, resulting in constant extinction coefficients at all altitudes measured on the Zeppelin NT. Lidar estimates captured these dynamic features well and good agreement was found for the extinction coefficients compared to the in situ results, using fixed lidar ratios (LR) between 30 and 70 sr for the altitudes probed with the Zeppelin. These LR are consistent with values for continental aerosol particles that can be expected in this region.
机译:在2012年夏季的PEGASOS Po Valley战役期间,在San Pietro Capofiume(SPC)地面站附近进行了案例研究,探索了气溶胶颗粒光学特性的垂直剖面。使用Zeppelin NT飞艇来研究气溶胶动力学的影响。海拔约50至800 m的行星边界层。所确定的性质包括气溶胶粒径分布,吸湿性生长因子,有效折射率和光吸收系数。前三个参数用于检索光散射系数。同时,在SPC地面站直接测量了散射系数和吸收系数。此外,一个单波长偏振分集弹性激光雷达系统使用Klett方法提供了气溶胶消光系数的估计值,以完成信号的反演,从而实现了原位和遥感结果之间的垂直分辨比较。但是请注意,比较大部分是在重叠函数不完整且不确定性较大的海拔范围内完成的。首先,低空飞行结果通过地面测量得到验证。干散射和吸收系数分别在±25%和±20 %%之间。单个散射反照率在0.83至0.95之间,表明在波谷地区吸收粒子的重要性。在飞行开始之前(直到〜10:00 LT –当地时间),在混合层(ML)完全展开之前,观察到了清晰的大气层。在新的ML中,在低海拔处发现了最高的消光系数,而在海拔较高的飞行开始时可以探测到的残留层中的值较低。飞行结束时(约12:00 LT后),ML充分发育,在齐柏林飞艇NT上测得的所有高度上的消光系数保持恒定。激光雷达估计很好地捕获了这些动态特征,并且与齐普特林探测的海拔高度相比,使用固定的激光雷达比(LR)在30至70arsr之间,与原位结果相比,消光系数具有很好的一致性。这些LR与在该区域可以预期的大陆气溶胶颗粒值一致。

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