Chemyakin Eduard, Müller Detlef, Burton Sharon, Kolgotin Alexei, Hostetler Chris, Ferrare Richard
Appl Opt. 2014 Nov 1;53(31):7252-66. doi: 10.1364/AO.53.007252.
We present the results of a feasibility study in which a simple, automated, and unsupervised algorithm, which we call the arrange and average algorithm, is used to infer microphysical parameters (complex refractive index, effective radius, total number, surface area, and volume concentrations) of atmospheric aerosol particles. The algorithm uses backscatter coefficients at 355, 532, and 1064 nm and extinction coefficients at 355 and 532 nm as input information. Testing of the algorithm is based on synthetic optical data that are computed from prescribed monomodal particle size distributions and complex refractive indices that describe spherical, primarily fine mode pollution particles. We tested the performance of the algorithm for the "3 backscatter (β)+2 extinction (α)" configuration of a multiwavelength aerosol high-spectral-resolution lidar (HSRL) or Raman lidar. We investigated the degree to which the microphysical results retrieved by this algorithm depends on the number of input backscatter and extinction coefficients. For example, we tested "3β+1α," "2β+1α," and "3β" lidar configurations. This arrange and average algorithm can be used in two ways. First, it can be applied for quick data processing of experimental data acquired with lidar. Fast automated retrievals of microphysical particle properties are needed in view of the enormous amount of data that can be acquired by the NASA Langley Research Center's airborne "3β+2α" High-Spectral-Resolution Lidar (HSRL-2). It would prove useful for the growing number of ground-based multiwavelength lidar networks, and it would provide an option for analyzing the vast amount of optical data acquired with a future spaceborne multiwavelength lidar. The second potential application is to improve the microphysical particle characterization with our existing inversion algorithm that uses Tikhonov's inversion with regularization. This advanced algorithm has recently undergone development to allow automated and unsupervised processing; the arrange and average algorithm can be used as a preclassifier to further improve its speed and precision. First tests of the performance of arrange and average algorithm are encouraging. We used a set of 48 different monomodal particle size distributions, 4 real parts and 15 imaginary parts of the complex refractive index. All in all we tested 2880 different optical data sets for 0%, 10%, and 20% Gaussian measurement noise (one-standard deviation). In the case of the "3β+2α" configuration with 10% measurement noise, we retrieve the particle effective radius to within 27% for 1964 (68.2%) of the test optical data sets. The number concentration is obtained to 76%, the surface area concentration to 16%, and the volume concentration to 30% precision. The "3β" configuration performs significantly poorer. The performance of the "3β+1α" and "2β+1α" configurations is intermediate between the "3β+2α" and the "3β."
我们展示了一项可行性研究的结果,其中使用了一种简单、自动化且无监督的算法(我们称之为排列平均算法)来推断大气气溶胶粒子的微物理参数(复折射率、有效半径、总数、表面积和体积浓度)。该算法使用355、532和1064纳米处的后向散射系数以及355和532纳米处的消光系数作为输入信息。算法测试基于从规定的单峰粒径分布和描述球形、主要是细模态污染粒子的复折射率计算得到的合成光学数据。我们针对多波长气溶胶高光谱分辨率激光雷达(HSRL)或拉曼激光雷达的“3个后向散射(β)+2个消光(α)”配置测试了该算法的性能。我们研究了通过该算法反演得到的微物理结果对输入后向散射和消光系数数量的依赖程度。例如,我们测试了“3β+1α”、“2β+1α”和“3β”激光雷达配置。这种排列平均算法有两种应用方式。首先,它可用于对激光雷达获取的实验数据进行快速数据处理。鉴于美国国家航空航天局兰利研究中心的机载“3β+2α”高光谱分辨率激光雷达(HSRL - 2)能够获取大量数据,快速自动反演微物理粒子特性非常必要。这对于越来越多的地基多波长激光雷达网络将证明是有用的,并且它将为分析未来星载多波长激光雷达获取的大量光学数据提供一种选择。第二个潜在应用是利用我们现有的使用带正则化的蒂霍诺夫反演的反演算法来改进微物理粒子表征。这种先进算法最近经过开发以实现自动化和无监督处理;排列平均算法可用作预分类器以进一步提高其速度和精度。排列平均算法性能的首次测试结果令人鼓舞。我们使用了一组48种不同的单峰粒径分布、复折射率的4个实部和15个虚部。总共针对0%、10%和20%的高斯测量噪声(一个标准差)测试了2880个不同的光学数据集。在具有10%测量噪声的“3β+2α”配置情况下,对于1964个(68.2%)测试光学数据集,我们将粒子有效半径反演到误差在27%以内。数量浓度的反演精度为76%,表面积浓度为16%,体积浓度为30%。“3β”配置的性能明显较差。“3β+1α”和“2β+1α”配置的性能介于“3β+2α”和“3β”之间。