利用激光雷达资料分析兰州远郊气溶胶光学特性

利用2007年1～4月兰州大学半干旱气候与环境观测站激光雷达资料,反演了晴空无云典型日和沙尘过程大气气溶胶消光系数和光学厚度。结果表明,兰州远郊榆中地区,1km以下大气气溶胶消光系数较大,为0.01～0.1km-1;平均气溶胶光学厚度〈0.5,光学厚度日变化呈双峰型,峰值分别出现在12：00和20：00。采暖期与非采暖...     

基于光谱分类的太湖水体后向散射研究

由于时空变化而产生的水体后向散射系数参数化差异一直是影响水质参数遥感定量反演精度的一个重要因素。在对太湖遥感反射率光谱进行分类的基础上,针对影响太湖水体水色的不同主导因子,把太湖水体分为3种类型,分别利用半分析方法和光学闭合原理对后向散射系数进行模拟,在此基础上研究其光学特性及其与水体组分浓度的关系,最后针对3种不同主导类型的水体分别建立了后向散射系数参数化模型。将后向散射特性在不同时间和空间上的差异转化为水体不同主导因子在生物-光学上的差异,从而得到适用于太湖不同湖区及不同季节的后向散射系数参数化模型,为利用分析方法对太湖水质参数进行更为精确的遥感反演提供了基础。     

中国西北大气沙尘光学特性的数值试验

利用 1991年 2月下旬～ 5月中旬HEIFE张掖和沙漠站的大气浑浊度观测、地面辐射观测及同期卫星资料 ,借助NCARCCM 3中的辐射模式CRM ,模拟估算了我国西北大气沙尘气溶胶的部分光学参数 ,单次散射反照率 (ω0 )和光学厚度比 [k(τλ=8～ 14 /τλ=0 .55) ]。计算结果表明 ,清洁天ω0 和k(τλ =8～ 14 /(τλ =0 .55)在沙漠和绿洲均为 0 .94和 0 .1;浑浊天ω0 在绿洲为 0 .90 ,沙漠为 0 .84 ;k(τλ=8～ 14 /τλ =0 .55)在绿洲为 0 .3 ,沙漠为 0 .4。在气候模式中 ,可将我国西部沙尘源区大气沙尘的ω0 和k(τλ =8～ 14 /τλ=0 .55)分别取为 0 .88和 0 .3。     

四种海水透明度现场测量方法的对比分析及发展趋势研究

随着海洋探测的不断发展,海水透明度作为海水光学性质的一个重要参量,也越来越受到人们的关注。文章对比分析了4种海水透明度现场测量方法:透明度盘法~([1])、光纤式高光谱剖面测量法~([2])、激光衰减测量法~([3])和基于双光路原理的海水IOPs高光谱测量法~([4]),主要分析了4种方法的测量原理,对比各自的优缺点,并提出了海水透明度测量未来发展设想。     

Automatic registration of optical imagery with 3D LiDAR data using statistical similarity

The development of robust and accurate methods for automatic registration of optical imagery and 3D LiDAR data continues to be a challenge for a variety of applications in photogrammetry, computer vision and remote sensing. This paper proposes a new approach for the registration of optical imagery with LiDAR data based on the theory of Mutual Information (MI), which exploits the statistical dependency between same- and multi-modal datasets to achieve accurate registration. The MI-based similarity measures quantify dependencies between aerial imagery, and both LiDAR intensity data and 3D point cloud data. The needs for specific physical feature correspondences, which are not always attainable in the registration of imagery with 3D point clouds, are avoided. Current methods for registering 2D imagery to 3D point clouds are first reviewed, after which the mutual MI approach is presented. Particular attention is given to adoption of the Normalised Combined Mutual Information (NCMI) approach as a means to produce a similarity measure that exploits the inherently registered LiDAR intensity and point cloud data so as to improve the robustness of registration between optical imagery and LiDAR data. The effectiveness of local versus global similarity measures is also investigated, as are the transformation models involved in the registration process. An experimental program conducted to evaluate MI-based methods for registering aerial imagery to LiDAR data is reported and the results obtained in two areas with differing terrain and land cover, and with aerial imagery of different resolution and LiDAR data with different point density are discussed. These results demonstrate the potential of the MI and especially the CMI methods for registration of imagery and 3D point clouds, and they highlight the feasibility and robustness of the presented MI-based approach to automated registration of multi-sensor, multi-temporal and multi-resolution remote sensing data for a wide range of applications.     

传感光纤-砂土界面力学性质的试验研究

近年来分布式光纤感测技术在岩土与地质工程领域的应用研究已成为一个研究热点,但工程实践表明,埋入式传感光纤与被测岩土体之间的变形协调性会对监测结果产生显著的影响,该问题一直制约着光纤感测技术在工程监测中的推广。本文通过一系列室内拉拔试验,对比了3种预埋于砂土中的单模光纤在不同上覆压力的作用下的拉拔力-拉拔位移曲线,并建立了一个用于描述光纤-砂土界面力学性质的三段式的拉拔模型,分析峰值拉拔力、残余拉拔力、有效拉拔位移和残余拉拔位移4个参数在不同上覆压力作用下的变化情况。分析结果揭示传感光纤-砂土界面的力学特性和应力传递规律,为分布式光纤传感技术在岩土体变形监测中的应用,尤其在变形监测光纤的选用标准方面,提供了参考依据。     

15厘米太阳射电望远镜增益运算放大器的制作与调试

本文介绍了１５厘米太阳射电望远镜增益运算放大器的结构原理，调试检测及测试结果。     

Magnetic fields of sunspots based on combined optical and radio observations

In the present paper we present the results of measurement of magnetic fields in some sunspots at different heights in the solar atmosphere, based on simultaneous optical and radio measurements. The optical measurements were made by traditional photographic spectral observations of Zeeman splitting in a number of spectral lines originating at different heights in the solar photosphere and chromosphere. Radio observations of the spectra and polarization of the sunspot - associated sources were made in the wavelength range of 2–4 cm using large reflector-type radio telescope RATAN-600. The magnetic field penetrating the hot regions of the solar atmosphere were found from the shortest wavelength of generation of thermal cyclotron emission (presumably in the third harmonic of electron gyrofrequency). For all the eight cases under consideration we have found that magnetic field first drops with height, increases from the photosphere to lower chromosphere, and then decreases again as we proceed to higher chromosphere and chromosphere-corona transition region. Radio measurements were found to be well correlated with optical measurements of magnetic fields for the same sunspot. An alternative interpretation implies that different lines used for magnetic field measurements refer to different locations on the solar surface. If this is the case, then the inversion in vertical gradients of magnetic fields may not exist above the sunspots. Possible sources of systematic and random errors are also discussed.     

查找表方法确定气溶胶类型

针对传统气溶胶类型确定方法的局限性以及当前气溶胶类型确定存在的困难,提出一种使用多波段气溶胶光学厚度数据确定气溶胶类型的方法。基于大气颗粒物的散射与吸收特性分析,通过构建查找表的方法实现气溶胶类型的确定。该方法利用Mie散射理论通过正向模拟不同类型气溶胶粒子数量与多波段光学厚度之间的关系来构建查找表,基于该查找表,使用440 nm、670 nm、870 nm及1020 nm 4个波段的气溶胶光学厚度确定气溶胶类型。使用模拟的多波段气溶胶光学厚度数据开展了气溶胶类型的确定实验,分析了不同波段气溶胶光学厚度误差对气溶胶类型确定结果的影响。结果表明,该方法可根据4个波段的气溶胶光学厚度以较高的精度确定出沙尘性、水溶性和煤烟3种气溶胶粒子的数量,从而确定气溶胶类型。