从ALADIN/Aeolus和CALIOP/CALIPSO激光雷达观测中获取的散射比曲线:瞬时重叠、统计比较和对高云的敏感性

A. Feofilov, H. Chepfer, V. Noel, M. Chiriaco
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引用次数: 0

摘要

云和气溶胶通过与太阳、大气和地面辐射以及空气湿度的复杂相互作用,在地球的能量收支中发挥着重要作用。光学厚度的云有效地反射入射的太阳辐射,在全球范围内,云对行星反照率的贡献约占三分之二。薄卷云阻挡了长波辐射,使地球保持温暖。气溶胶根据其大小和形状散射或吸收阳光,并以各种方式与云相互作用。由于云和气溶胶对地球能量收支的重要性,对其性质的全球卫星观测对于气候研究、约束气候模式和评估云参数化至关重要。利用激光雷达和雷达从太空主动探测是有利的,因为它能提供垂直分辨率的信息。CALIOP激光雷达从2006年开始观测地球大气层,已经证实了这一点。另一种类似的仪器,国际空间站上的CATS激光雷达从2015年初开始提供了超过33个月的测量。自2018年8月以来,ADM/Aeolus上的ALADIN激光雷达一直在测量水平风和气溶胶/云。计划在2022年发射更多的激光雷达——ATLID/EarthCare激光雷达,其他星载激光雷达正处于开发阶段。在这项工作中,我们比较了从ALADIN和CALIOP观测中获得的散射比产品。前者瞄准距最低点35度,测量距最低点355nm的大气后向散射,能够分离分子和特殊成分(HSRL),并提供垂直分辨率为~1km至20km高度的剖面。后者在532nm处工作,目标距离最低点3度,测量总后向散射达40公里。它的自然垂直分辨率高于ALADIN,但比较中使用的散射比产品是在~0.5km的垂直网格上提供的。我们对这两种仪器在2019年6月28日至2019年12月31日期间几乎同时进行的大气共同体积观测进行了搜索,并分析了并置数据。我们给出了散射比的纬向平均值,以及瞬时剖面比较和云探测的统计分析,云高度一致,以及这些特征的时间演变。从这一分析中可以得出的初步结论是,ALADIN和CALIOP观测反演的散射比曲线在6-7 km高度范围内的一致性较好,而在较高的大气层中,ALADIN对云的敏感性低于CALIOP。这种灵敏度的不足可以通过输入信号的进一步平均和/或使用本工作中提供的并置观测数据集更新检索算法来补偿。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Scattering ratio profiles retrieved from ALADIN/Aeolus and CALIOP/CALIPSO lidar observations: instantaneous overlaps, statistical comparison, and sensitivity to high clouds
Clouds and aerosols play an important role in the Earth’s energy budget through a complex interaction with solar, atmospheric, and terrestrial radiation, and air humidity. Optically thick clouds efficiently reflect the incoming solar radiation and, globally, clouds are responsible for about two thirds of the planetary albedo. Thin cirrus trap the outgoing longwave radiation and keep the planet warm. Aerosols scatter or absorb sunlight depending on their size and shape and interact with clouds in various ways. Due to the importance of clouds and aerosols for the Earth’s energy budget, global satellite observations of their properties are essential for climate studies, for constraining climate models, and for evaluating cloud parameterizations. Active sounding from space by lidars and radars is advantageous since it provides the vertically resolved information. This has been proven by CALIOP lidar which has been observing the Earth’s atmosphere since 2006. Another instrument of this kind, CATS lidar on-board ISS provided measurements for over 33 months starting from the beginning of 2015. The ALADIN lidar on-board ADM/Aeolus has been measuring horizontal winds and aerosols/clouds since August 2018. More lidars are planned – in 2022, the ATLID/EarthCare lidar will be launched and other space-borne lidars are in the development phase. In this work, we compare the scattering ratio products retrieved from ALADIN and CALIOP observations. The former is aimed at 35 deg from nadir, it measures the atmospheric backscatter at 355nm from nadir, is capable of separating the molecular and particular components (HSRL), and provides the profiles with a vertical resolution of ~1km up to 20km altitude. The latter, operating at 532nm is aimed at 3 deg from nadir and measures the total backscatter up to 40 km. Its natural vertical resolution is higher than that of ALADIN, but the scattering ratio product used in the comparison is provided at ~0.5km vertical grid. We have performed a search of nearly simultaneous common volume observations of atmosphere by these two instruments for the period from 28/06/2019 through 31/12/2019 and analyzed the collocated data. We present the zonal averages of scattering ratios as well as the instantaneous profile comparisons and the statistical analysis of cloud detection, cloud height agreement, and temporal evolution of these characteristics. The preliminary conclusion, which can be drawn from this analysis, is that the general agreement of scattering ratio profiles retrieved from ALADIN and CALIOP observations is good up to 6-7 km height whereas in the higher atmospheric layers ALADIN is less sensitive to clouds than the CALIOP. This lack of sensitivity might be compensated by further averaging of the input signals and/or by an updating of the retrieval algorithms using the collocated observations dataset provided in the present work.
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