Chudamani S, Spinhirne J D, Clarke A D
Appl Opt. 1996 Aug 20;35(24):4812-9. doi: 10.1364/AO.35.004812.
Lidar backscatter cross-sectional measurements at 1.064, 0.532, and 1.54 μm were acquired during November 1989 and May-June 1990 around the Pacific region by the NASA DC-8 aircraft as part of the Global Backscatter Experiment. The primary motivation for the Global Backscatter Experiment was the study of lidar backscatter cross sections for the development of a spaceborne wind-sensing lidar. Direct backscatter measurements obtained by the NASA Goddard Space Flight Center visible and infrared lidar are compared with backscatter cross sections calculated from aerosol size distributions obtained by particle counters. Results for one flight with pronounced aerosol layers in the upper troposphere southeast of Japan are presented. Because 2-μm region wavelengths are possible candidates for a spaceborne wind-sensing lidar, the visible and infrared lidar backscatter cross sections at 1.064, 0.532, and 1.54 μm are extrapolated to the 2-μm region. The extrapolated 2-μm cross sections are compared with lidar measurements at 9 μm. A significant range in the ratio of 2-9-μm backscatter cross sections is found, but a large number of points concentrate near ratios of three to ten. A large number of 1.064- and 1.54-μm cross sections were binned to provide an estimate of backscatter for various percentiles for the flight. The ratio of the 50-percentile backscatter values at 1.064 and 1.54 μm suggest a λ(-1.9) to λ(-3.0) wavelength dependence of aerosol backscatter cross section in the near infrared for the observational case.
1989年11月以及1990年5月至6月期间,美国国家航空航天局(NASA)的DC - 8飞机在太平洋地区进行了1.064、0.532和1.54微米处的激光雷达后向散射截面测量,这是全球后向散射实验的一部分。全球后向散射实验的主要动机是研究激光雷达后向散射截面,以开发星载测风激光雷达。将美国国家航空航天局戈达德太空飞行中心可见和红外激光雷达获得的直接后向散射测量结果,与根据粒子计数器获得的气溶胶粒径分布计算出的后向散射截面进行比较。给出了一次飞行的结果,此次飞行在日本东南部对流层上部有明显的气溶胶层。由于2微米区域波长可能是星载测风激光雷达的候选波长,因此将1.064、0.532和1.54微米处的可见和红外激光雷达后向散射截面外推到2微米区域。将外推得到的2微米截面与9微米处的激光雷达测量结果进行比较。发现2 - 9微米后向散射截面的比值范围很大,但大量数据点集中在三到十的比值附近。对大量1.064微米和1.54微米的截面进行了分组,以估算该次飞行中不同百分位数的后向散射。1.064微米和1.54微米处50百分位后向散射值的比值表明,在该观测情况下,近红外区域气溶胶后向散射截面的波长依赖性为λ(-1.9)至λ(-3.0)。