Liu Dong, Zheng Zhuofan, Chen Weibiao, Wang Zhibin, Li Weijun, Ke Ju, Zhang Yupeng, Chen Sijie, Cheng Chonghui, Wang Shuaibo
Opt Express. 2019 Apr 15;27(8):A481-A494. doi: 10.1364/OE.27.00A481.
Cloud and aerosol contribute with great uncertainty in Earth's radiative budget. There is an urgent need for global 3-D observation of these atmospheric constituents. High-spectral-resolution Lidar (HSRL) can obtain vertical atmosphere profile with high accuracy, hence several space-borne HSRLs are planned to launch in few years. However, as far as we know, the performance evaluation of space-borne HSRL has not been reported yet. In this paper, we present the characteristics of a new designed space-borne HSRL for aerosol and cloud optical property profiling (ACHSRL), which is part of the Aerosol & Carbon Detection Lidar (ACDL) developed in China. The ACHSRL is essentially similar to the famous Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP), which is on board the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO). Moreover, the ACHSRL employs an iodine absorption filter as the spectral discriminator. The atmospheric optical properties data observed by CALIOP is used to estimate the performance of ACHSRL. We chose the level 2 profile data (version 4.10) in South Japan in June 2015 to compare the detection uncertainty of ACHSRL and CALIOP. The simulation calculates the uncertainties of ACHSRL and makes a statistic analysis. The analysis result demonstrates that 73.63% of the backscatter coefficient uncertainties are below 40% for ACHSRL. By contrast, the number is 30.72% for CALIOP. As for absolute extinction coefficient errors, the statistics shows that 76.01% of the extinction coefficient uncertainties are lower than 0.2 km for ACHSRL, while that for CALIOP are 56.97%. The assessment shows that ACHSRL could measure the particulate optical properties with better accuracy and compared with CALIOP. The estimation in this study reveals that the next generation space-borne HSRLs have a promising future.
云和气溶胶对地球辐射收支有着极大的不确定性影响。迫切需要对这些大气成分进行全球三维观测。高光谱分辨率激光雷达(HSRL)能够高精度获取垂直大气廓线,因此计划在未来几年发射几颗搭载HSRL的卫星。然而,据我们所知,尚未有关于星载HSRL性能评估的报道。在本文中,我们介绍了一种新设计的用于气溶胶和云光学特性探测的星载HSRL(ACHSRL)的特性,它是中国研制的气溶胶与碳探测激光雷达(ACDL)的一部分。ACHSRL本质上与搭载在云和气溶胶激光雷达与红外探路者卫星观测(CALIPSO)上的著名的正交偏振云和气溶胶激光雷达(CALIOP)相似。此外,ACHSRL采用碘吸收滤光片作为光谱鉴别器。利用CALIOP观测到的大气光学特性数据来评估ACHSRL的性能。我们选取了2015年6月日本南部的二级廓线数据(版本4.10)来比较ACHSRL和CALIOP的探测不确定性。通过模拟计算ACHSRL的不确定性并进行统计分析。分析结果表明,ACHSRL后向散射系数不确定性的73.63%低于40%。相比之下,CALIOP的这一比例为30.72%。至于绝对消光系数误差,统计显示ACHSRL消光系数不确定性的76.01%低于0.2 km,而CALIOP的这一比例为56.97%。评估表明,ACHSRL能够更精确地测量颗粒物光学特性,与CALIOP相比具有优势。本研究的评估结果表明,下一代星载HSRL具有广阔的前景。