卫星重力梯度向下延拓的频域最小二乘配置法

本文深入研究频域最小二乘配置法的基本原理及其在求解卫星重力梯度向下延拓问题中的应用。与一般空域最小二乘配置法相比，该方法具有高效稳定的特点，特别适合于大规模重力场数据处理，并为利用卫星重力梯度数据精化局部重力场提供了可供参考的方法。     

有限区域卫星云图资料变分分析的试验研究

资料分析在数值预报中的重要性受到越来越多的关注，星目前常规探测网的时空局限性，利用分辨率较高的非常规资料势在必行。该文利用一个有限区域中尺度模式ＭＭ４，采用变分分析技术对有限区域的常规探空资料和非常规云图资料进行变分分析和数值模拟。     

亚洲MAGSAT卫星磁异常图

使用２０多万个ＭＡＧＳＡＴ卫星磁测数据，编绘亚洲卫星标量（△Ｆ）和矢量（△Ｘ，△ｙ，△Ｚ）磁异常图（２０°ｓ－６０°Ｎ，５０°Ｅ－１６０°Ｅ）．为了提取岩石层卫星磁异常，首先对ＭＡＧＳＡＴ卫星数据进行了筛选，然后进行主磁场、磁层场、电离层场和感应场改正，并消除虚假测点．将卫星数据分成黎明组、黄昏组和联合组，分别绘制相应的卫星磁异常图．根据１°×１°的网点值，用计算机编绘亚洲卫星磁异常图．初步分析了卫星磁异常与大地构造的关系．     

结合卫星像影分析水库地震的形成原因

本文应用卫星影像分析了我国几个水库诱发地震震例,提出了库区内应力叠加模式,对水库地震的成因,做了探讨。     

便携式光电望远镜用于流星暴观测的探讨

本文介绍了便携式人卫光电望远镜的主要性能特点,探讨了将其应用于狮子座流星暴观测的可能性。     

The gravitational perturbation spectrum in linear satellite theory

A new method for calculating the perturbation spectrum in the framework of Kaula's linear satellite theory (LST) is introduced. The novelty of this approach consists in using recent results on the spectral decomposition of the perturbation frequencies in LST to provide a closed formulation for the amplitude and the phase of each line in the perturbation spectrum. The theory presented here can be applied to perturbations in the elements or in the radial and transverse directions due to the geopotential or to the tides. Separate algorithms are developed for application to orbits with circulating or frozen perigee.     

"2001.4.6"宁夏沙尘暴过程卫星图像分析

利用日本GMS-5地球同步气象卫星资料,结合常规气象资料,对2001年4月6日发生于宁夏的一次沙尘暴天气过程的影响系统、物理机制、运动学特征、发展演变过程和地形作用等进行了分析。结果表明：在GMS卫星图像上,这次过程有明显的特征,通过图像处理可以得到更多的细节信息。结合实测资料的分析表明：这次沙尘暴天气是高空强西北气流和地面急行冷锋共同影响的天气过程,在卫星云图上其热力与动力过程有明显的反映,而且随着时间的变化其作用不同。三种不同的地形在这次过程中具有不同的效应。这些结果对深入认识沙尘暴天气过程,提高监测预报能力有重要意义。     

Evaluation of pre-CHAMP gravity models `GRIM5-S1' and `GRIM5-C1' with satellite crossover altimetry

 The new GFZ/GRGS gravity field models GRIM5-S1 and GRIM5-C1, currently used as initial models for the CHAMP mission, have been compared with other recent models (JGM 3, EGM 96) for radial orbit accuracy (by means of latitude lumped coefficients) in computations on altimetry satellite orbits. The bases for accuracy judgements are multi-year averages of crossover sea height differences from Geosat and ERS 1/2 missions. This radially sensitive data is fully independent of the data used to develop these gravity models. There is good agreement between the observed differences in all of the world's oceans and projections of the same errors from the scaled covariance matrix of their harmonic geopotential coefficients. It was found that the tentative scale factor of five for the formal standard deviations of the harmonic coefficients of the new GRIM fields is justified, i.e. the accuracy estimates, provided together with the GRIM geopotential coefficients, are realistic. Received: 20 February 2001 / Accepted: 24 October 2001