大气紫外线传输和激光雷达返回

D. Hao, S. Yi, B. Hui
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引用次数: 0

摘要

利用Hitran2004数据库中的分子吸收截面对大气传输模型UVTRAN进行了修正。改进后的UVTRAN可用于计算大气透射率,具有高精度和超光谱分辨率。由于目前微型计算机用的FASCOD3不能用于紫外光谱,因此可以代替FASCOD3。作为实例,利用改进的UVTRAN计算了可见光和紫外光谱下6个激光波长的大气传输和返回信号。结果表明,激光波长为中紫外,如308nm的XeCl准分子激光,适合在对流层短距离工作。如果选择在深紫外波段工作的激光器,就需要具有很高灵敏度的紫外探测器。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Atmospheric ultraviolet transmission and Lidar returns
The atmospheric transmission model UVTRAN is modified by use of molecular absorption cross sections taken from Hitran2004 database. The modified UVTRAN can be utilized to calculate atmospheric transmission with both high accuracy and super spectral resolution. It can replace FASCOD3 model because the current FASCOD3 for micro-computer can not be used in the ultraviolet spectrum. As an example, atmospheric transmissions and return signals are calculated by the modified UVTRAN for the 6 laser wavelengths at visible and ultraviolet spectrum. The results show that the laser wavelength at medium ultraviolet, e.g. 308nm XeCl Excimer laser, is suitable for working at short distance in the troposphere. The ultraviolet detector with very high sensitivity is required if a laser is chosen to work in deep ultraviolet.
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