爬山法在影像匹配中的应用

对传统的爬山法进行改进,通过两个方向的整体搜索来预测峰值可能出现的区域,使其能很快的找到峰值位置。试验表明这种方法减少了相关系数的计算,提高匹配的速度并且保证了匹配的精度。     

基于DEM的USLE土壤侵蚀方程地形因子获取与分析

坡长和坡度是研究水土流失问题中必须要考虑的重要地形因子,坡长的空间分布特征和规律、地貌发育对坡长的影响,以及坡长与坡度之间的关系,是研究水土流失、侵蚀规律的重要条件之一。利用GIS以及相关软件为平台,在黑龙江省通河地区建立USLE水土流失方程模型,研究LS因子在水土流失中的影响以及作用,并探讨DEM数据分辨率变化对LS值的影响。     

基于加权整体最小二乘的矿区平面坐标转换方法

常用的平面坐标系统转换模型四参数转换法在实际工程应用中,由于公共点一般分布在较小的范围内,点之间的距离较近,因此传统的四参数转换模型中旋转参数和平移参数之间的相关性较大,容易导致法方程病态,进而影响转换参数的精度,文中从重合点坐标重心化的转换模型出发,还原出重心化之前的四参数。通过加权整体最小二乘的转换分析及迭代计算,验证运用加权整体最小二乘(WTLS)方法转换的参数质量比最小二乘(LS)、整体最小二乘(TLS)方法得到的参数质量有显著改善。     

对分量进行联合解算的极移预报方法研究

为了提高极移预报的精度,该文提出结合极移的两个分量进行统一求解的极移联合预报方法:将极移的两个分量组成一个观测方程,并采用LS+AR模型对联合分量的确定项与随机项进行拟合。实验结果表明,文中采用的联合预报方法可以提高极移的预报精度。     

Gauss-Markov模型参数的部分根方估计

在分析根方估计，Stein均压缩估计，Sclove部分压缩估计各自特点的基础上，提出了一种新的有偏估计－部分根方估计，并讨论了它的优良性质。计算结果表明，在设计阵呈病态时，部分根方估计确能改善LS估计。     

First results of the Central-East-South European Binary Star Study Group (CESEB)

Several eclipsing binary systems have been selected for combined spectral and photometric observations using the Bulgarian NAO 2 m telescope and several smaller telescopes located at various places in the CESE region. Preliminary results, based on a pilot study started in 2001, about radial velocity and light curve variations of the active W UMa system LS Del are presented here.     

Correlated V/R and infrared photometric variations in the Be/X-ray binary LS I +61° 235/RX J0146.9+6121

We report on the long-term variability of the Be/X-ray binary LS I +61° 235/RX J0146.9+6121. New optical spectroscopic and infrared photometric observations confirm the presence of global one-armed oscillations in the circumstellar disc of the Be star, and allow us to derive a V R band quasi-period of 1240±30 d. Pronounced shell events, reminiscent of the spectacular variations in Be stars, are also seen. We have found that the J , H and K infrared photometric bands vary in correlation with the spectroscopic V R variations, implying that the one-armed disc oscillations are prograde. The effect of the oscillations is not only seen in the H α line but is also seen in the He  i λ 6678 and Paschen lines. As these lines are formed at different radii in the equatorial disc of the Be star, such effects confirm the global nature of the perturbation. The Keplerian disc has been found to be denser than the average for a sample of isolated Be stars, which may be indicative of some kind of interaction with the compact companion. Finally, from a Rossi X-ray Timing Explorer observation we derive a spin period of the neutron star of 1404.5±0.5 s.     

GPS高程异常拟合的稳健总体最小二乘算法

为解决控制点平面坐标与高程异常值中均含有误差的情况下求解模型参数的问题,对应用总体最小二乘算法(TLS)建立G-M模型求解拟合模型参数的方法进行讨论,重点对应用稳健总体最小二乘算法解决控制点之间观测值精度不等对参数求解有影响的问题进行探讨。对基于稳健估计思想的TLS迭代定权算法进行讨论,并通过算例与其他两种算法进行比较。结果表明,基于稳健估计的TLS算法能更好地解决含有误差的控制点已知坐标对GPS高程拟合模型参数求解有影响的问题。     

正则化方法的统一

对最小二乘估计作线性变换,使得新估计是真值的最优拟合,并且包含模型参数的先验误差协方差阵。从滤波因子的角度对正则化方法进行统一,提供了常见的Tikhonov正则化方法、截断奇异值法、广义岭回归方法等的滤波因子与对应的误差协方差阵的特征值。