20颗依巴谷碳星的近红外测光

对20颗依巴谷(Hipparcos)卫星所观测的碳星作了近红外JHK测光，由近红外观测结果估算了其在K波段的热改正BCK和视热星等mbpl以及有效温度Te，结合依巴谷卫星所得视差，得到其中一些星的绝对热星等Mbol。     

用陆地卫星—5近红外图像观测胶州海况

对海洋上卫星测得的近红外波辐射反映的信息进行理论分析，表明卫星近红外波段图像上反映的海况信息，１９９６年１１月５日陆地卫星ＴＭ６图像显示胶州湾海表温度的波状分布，ＴＭ２，ＴＭ３，ＴＭ４波段彩色合成图像显示胶州湾的悬浮泥沙含量分布和泥沙运动。ＴＭ４图像显示在海洋波动和风力作用下的海况，并用实测潮汐资料，气象信息解译胶州湾海况，在胶州湾中，西部，悬浮泥沙含量较高，而ＴＭ４波段辐射值较低，图像阴暗，较高     

近红外反射光谱学在岩石矿物研究中的应用Ⅱ.快速测定地质样品中有机质

利用偏最小二乘法回归的多变量校正方式,建立了应用近红外反射光谱学方法无损快速测定各种地质样品中有机质的模型.设计了多重散射光校正、标准正常变量转换及导数光谱,扣除额外基线和重叠信号的影响,分离出与有机质含量有关的光谱信息.大多数地质样品的有机质近红外反射光谱估算结果与化学法符合.     

微型近红外光谱仪测量北极积雪覆盖海冰内部太阳辐照度可行性研究

The extremely low temperature, high humidity and limited power supply pose considerable challenges when using spectrometers within the Arctic sea ice. The feasibility of using a miniature low-power near-infrared spectrometer module to measure solar radiation in Arctic sea ice environments was investigated in this study.Temperature and integration time dependences of the spectrometer module were examined over the entire target operating range of –50℃ to 30℃, well below the specified operating range of this spectrometer. Using these observations, a dark output prediction model was developed to represent dark output as a function of temperature and integration time. Temperature-induced biases in the saturation output and linear operating range of the spectrometer were also determined. Temperature and integration time dependences of the signal output were evaluated. Two signal output correction models were developed and compared, to convert the signal output at any temperature within the operating temperature range and integration time to that measured at the reference temperature and integration time. The overall performance of the spectrometer was evaluated by integrating it into a refined fiber optic spectrometry system and measuring solar irradiance distribution in the ice cover with thickness of 1.85 m in the Arctic during the 9th Chinese National Arctic Research Expedition. The general shape of the measured solar irradiance above the snow surface agreed well with that measured by other commercial oceanographic spectroradiometers. The measured optical properties of the sea ice were generally comparable to those of similar ice measured using other instruments. This approach provides a general framework for assessing the feasibility of using spectrometers for applications in cold environments.     

土壤粒径的光谱响应特性研究

以实验室制备的5个不同粒径水平的土壤样本和室内高光谱数据为基础,通过对光谱数据进行重采样、数学变换等预处理并进行单因素方差分析、相关性分析和回归分析,探讨土壤粒径的高光谱特性,建立了光谱数据预测土壤粒径的校正模型。结果表明,土壤粒径对反射光谱有显著的影响,波长越长影响越大;在全波段范围内土壤粒径和光谱数据都呈负相关关系,对原始光谱数据进行微分变换能增加其与土壤粒径的相关性;以反射率一阶微分建立的回归模型为反演土壤粒径的最佳模型,其建模决定系数■、预测决定系数■、预测相对偏差RPD分别为0.666,0.653,2.043,预测均方根误差RMSE为0.175。     

HEIFE绿洲区太阳总辐射和地表反射率的分光谱特征

太阳辐射的分光测量在许多研究和应用领域中都具有十分重要的意义．本文利用HEIFE临泽子站进行的太阳总辐射和反射辐射的分光观测资料，研究了黑河绿洲区太阳总辐射和地表反射率的光谱特征．研究结果表明：在太阳总辐射的光谱能量分布中，紫外和可见光部分的比倒偏小，近红外部分则偏太．在其从冬到夏的季节变化中紫外和可见光部分是由小到大，近红外部分剐是由大到小。在其日变化中0．5μm以下波段是中午大早晚小；0．7μm以上波段是中午小，早晚大；0．5-0．7μm波段的日变化不明显。紫外波段的相对日变化幅度最大．地表反射率的光谱特性有明显的季节变化，变化特征与地表植被状况有关．各波段地表反射率的日变化型有一定的季节差异，其中波长小于0．7μm部分较为明显，并与地表植被状况有关．在裸露地表各波段反射率与太阳高度角的关系中，近红外波段随太阳高度角增加而增大，紫外和可见光波段则随太阳高度角增大而减小．全波段反射率随太阳高度角增大而增大主要是近红外波段的贡献．这是裸露地表光谱反射率的重要特征之一。     

Sagnac型干涉成像光谱仪研制及干涉成像光谱实验

空间调制干涉成像（傅里叶变换）光谱仪（SMIFTS）是一种有重要的研究和应用价值的空间遥感器。依据应用要求和信噪比方程设计并研制了Sagnac型干涉成像（傅里叶变换）光谱仪原理样机。用该样机进行了实验室干涉成像光谱实验，获取了较为清晰的可见光、近红外谱段干涉成像图像。对其中各像元的干涉图进行数据处理和计算，提取出了光谱特征明显的成像光谱图像和与被测图样光谱特征相符的像元光谱。由实测光谱辐射亮度曲线反演计算出的光谱反射曲线与标准仪器测得的图样光谱反射特性曲线进行了比较，结果表明二者对应相似。     

用神舟三号中分辨率成像光谱仪数据反演大气水汽

2002年3月中国神舟三号飞船发射成功，所携带的中分辨率成像光谱仪获取了一批940nm波段的遥感数据。本文用其中的部分资料做了反演水汽的试验，给出一些结果和分析。     

基于ALOS光学影像的2008年汶川地震震害信息提取

本文基于ALOS光学影像对2008年5月12日发生的四川汶川大地震灾区进行了震害信息提取。由于本次地震造成了大范围的山体滑坡,我们尝试利用震前和震后获取的ALOS/AVNIR-2影像进行滑坡区域信息提取。首先利用分级方法提取植被和水体信息,对植被和水体进行掩膜之后通过基于像元的分类将裸地信息从震前和震后的影像中提取出来,两幅影像中裸地信息的差异则被认为是滑坡。同时在被滑坡阻塞的河流地区,水平面的上升情况也被提取出来。除此以外本文利用由SRTM获得的DEM数据对坡度和滑坡发生之间的关系进行了研究。     

Near—Infrared Imaging Observations of the Orion A—W Star Forming Region

We carried out near-infrared imaging observations of the Ori A-W region using the Italian 1.5m TIRGO infrared telescope at Gornergrat. A group of infrared objects is visible on the K band image, including an IRAS source (IRS 1). From its IRAS flux density the IRAS luminosity is derived to be 45L⊙, which shows that IRS 1 is a low-mass protostar. By superimposing the position of the VLA H2O maser on the K image, we can identify the less evolved object IRS 1 as the excitation source of the H2O maser, within a projected distance of 470AU. This would be evidence that the maser effect is associated with the youngest phase of stellar evolution. The first probable HH object candidate in the Ori A-W region is discovered from the H2 S(1) 1-0 observation. Comparing the position of the H2O maser with the direction of the molecular hydrogen emission in the region, we suggest that the observed H2O maser could be tracing the circumstellar disk of IRS 1.