Chen Wei-Nai, Chiang Chih-Wei, Nee Jan-Bai
Department of Physics, National Central University, Chung-Li, Taiwan.
Appl Opt. 2002 Oct 20;41(30):6470-6. doi: 10.1364/ao.41.006470.
We report on studies of the lidar and the depolarization ratios for cirrus clouds. The optical depth and effective lidar ratio are derived from the transmission of clouds, which is determined by comparing the backscattering signals at the cloud base and cloud top. The lidar signals were fitted to a background atmospheric density profile outside the cloud region to warrant the linear response of the return signals with the scattering media. An average lidar ratio, 29 +/- 12 sr, has been found for all clouds measured in 1999 and 2000. The height and temperature dependences ofthe lidar ratio, the optical depth, and the depolarization ratio were investigated and compared with results of LITE and PROBE. Cirrus clouds detected near the tropopause are usually optically thin and mostly subvisual. Clouds with the largest optical depths were found near 12 km with a temperature of approximately -55 degrees C. The multiple-scattering effect is considered for clouds with high optical depths, and this effect lowers the lidar ratios compared with a single-scattering condition. Lidar ratios are in the 20-40 range for clouds at heights of 12.5-15 km and are smaller than approximately 30 in height above 15 km. Clouds are usually optically thin for temperatures below approximately -65 degrees C, and in this region the optical depth tends to decrease with height. The depolarization ratio is found to increase with a height at 11-15 km and smaller than 0.3 above 16 km. The variation in the depolarization ratio with the lidar ratio was also reported. The lidar and depolarization ratios were discussed in terms of the types of hexagonal ice crystals.
我们报告了对卷云的激光雷达和退偏振比的研究。光学厚度和有效激光雷达比是根据云的透过率推导出来的,透过率是通过比较云底和云顶的后向散射信号来确定的。将激光雷达信号与云区外的背景大气密度剖面进行拟合,以确保回波信号与散射介质的线性响应。对于1999年和2000年测量的所有云,已发现平均激光雷达比为29±12 sr。研究了激光雷达比、光学厚度和退偏振比随高度和温度的变化,并与LITE和PROBE的结果进行了比较。在对流层顶附近检测到的卷云通常光学厚度较薄,大多不可见。光学厚度最大的云出现在12公里附近,温度约为-55摄氏度。对于光学厚度较大的云,考虑了多次散射效应,与单次散射条件相比,这种效应会降低激光雷达比。对于高度在12.5 - 15公里的云,激光雷达比在20 - 40范围内,在高度超过15公里时小于约30。对于温度低于约-65摄氏度的云,通常光学厚度较薄,在该区域光学厚度往往随高度降低。发现退偏振比在11 - 15公里高度处随高度增加,在16公里以上小于0.3。还报告了退偏振比随激光雷达比的变化情况。根据六角形冰晶的类型讨论了激光雷达和退偏振比。