基于MODIS影像的超分辨率重建

针对4幅多时相250 m分辨率的MODIS影像,利用空间域中的超分辨率重建模型,进行了影像的匹配和运动参数估计,重建出采样率提高2倍的高分辨率影像。     

松花江干流（哈尔滨段）春季最低水位预测方法

利用1949~2003年松花江(哈尔滨段)最低水位资料,分析松花江干流(哈尔滨段)春季最低水位变化规律和典型枯水年成因,分析了其与松花江、嫩江等松花江流域面雨量的相关性,与拉尼娜、厄尔尼诺、太阳黑子等的关系。以松花江、嫩江、第二松花江流域7~11月面雨量总和及前一年松花江干流(哈尔滨段)最高水位为因子,预测2004~2013年松花江干流(哈尔滨段)最低水位。利用方差周期方法、均生函数方法对2004~2013年拉尼娜、厄尔尼诺、太阳黑子及松花江、嫩江、第二松花江流域月面雨量进行预测,并以此预测对2004~2013年松花江干流(哈尔滨段)最低水位进行订正,得出预测结论。     

地磁测量及其应用

地磁已广泛应用于地球科学、航天航空、交通通讯、地震预测、空间天气等诸多领域。鉴于地磁测量是地磁应用的基础，本文分析了现代地磁测量及其研究概况，展望了地磁应用发展趋势。     

温度、湿度对地磁Z基线值的影响及分析

仪器墩体受潮湿影响所产生的局部形变而引起的ZB磁变仪倾斜,是引起成都台CB3ZB变化幅度大,形成N字型年变化及其它类似形态变化的主要原因。实践证明,水泥墩湿引起的形变大,防潮效果差。而质地单纯均匀的石头墩受潮湿后引起的形变小,防潮效果好。     

The Spatial and Temporal Characteristics of Pc3 Geomagnetic Activity over Canada in 2000, as a Guide to Planning the Times of Aeromagnetic Surveys

Geomagnetic activity affects aeromagnetic surveys. Geomagnetic variations are quite complex and can be quantified in different ways. A measure of geomagnetic activity that is useful for planning aeromagnetic surveys is the Pc3 pulsation index developed by the Australian Space Weather Agency. Purposeful to developing guidelines for planning aeromagnetic surveys in Canada, we study the variations in Pc3 index amplitude over Canada in 2000. This study shows distinct patterns associated with the sub-auroral zone, the auroral zone, and the polar cap. Average Pc3 index activity is higher during the months of February, July, September, and November in the auroral and sub-auroral zones. The station in the polar cap exhibits maximum activity near midday during the summer months. Detailed analysis of a magnetic storm shows that Pc3 index amplitude during the beginning of the solar storm is least important at the polar cap. The mean Pc3 index also relates to solar wind parameters such as the solar wind velocity and the vertical polarity of the interplanetary magnetic field. Analysis of the morning maximum of the Pc3 index observed in the auroral zone can be used to develop guidelines for planning aeromagnetic surveys in Canada and other areas of the world affected by auroral zones.     

Seismic frame design via inverse mode design of frame-ground systems

A two-step stiffness design procedure is developed for a moment-resisting planar frame supported by a prescribed two-dimensional finite-element ground-pile system. In the first step, a hybrid inverse eigenmode problem is formulated and its solution is derived in an analytical form. A difficulty resulting from the existence of multiple interface nodes is overcome by incorporating a deformation constraint into a set of linear equations for finding the lowest-mode displacements at the interface nodes and in the ground. In the second step, the fundamental natural frequency of the combined system and the lowest mode-strain ratios in the frame specified in the first step are regarded as the parameters for adjusting the mean peak seismic member-end strains to their specified values. If the fundamental natural frequency of the frame with a fixed-base happens to be close to that of the ground, a difficulty arises in the two-step stiffness design procedure because of an irregular response amplification and of the non-predominance of the lowest-mode components. A new practical design procedure of rapid convergence is proposed such that an initial design is found for a stiff ground and that a sequence of stiffness designs is generated with respect to a ground stiffness parameter without any differential coefficient of series expansion. The accuracy of the model utilized in this paper and the validity of the present stiffness design procedure are verified through time-history response analysis.     

对AE指数的讨论：是否适用于磁层相空间重构

分析表明,目前广泛应用的ＡＥ指数虽然在一定程度能反映极区地磁活动特征,但其物理意义不清,不能描述亚暴活动的物理过程,不宜用来作磁层相空间重构等非线性过程的研究。ＡＵ和ＡＬ虽是不可缺少的描述极光电集流活动的指数,但仍须消除规则日变化ＳＲ的影响、改进推导方法（和台站布局）。     

瞬变电磁法二维逆时偏移

本文简要介绍了电磁偏移的基本原理和低频滤波的偏移处理方法,并详细论述了最佳极值时刻T的求取方法。电磁偏移以斯特莱顿-朱型积分为理论基础,借助于无限均匀介质中的格林函数,描述了似稳电磁场在下半空间的传播过程。利用电磁偏移方法处理TEM资料,能够较准确地确定局部导电地质体的空间位置,处理速度快,解释结果形象。     

A study of transient variations in the Earth’s electromagnetic field at equatorial electrojet latitudes in western Africa (Mali and the Ivory Coast)

In the framework of the French-Ivorian participation to the IEEY, a network of 10 electromagnetic stations were installed at African longitudes. The aim of this experiment was twofold: firstly, to study the magnetic signature of the equatorial electrojet on the one hand, and secondly, to characterize the induced electric field variations on the other hand. The first results of the magnetic field investigations were presented by Doumouya and coworkers. Those of the electric field experiment will be discussed in this study. The electromagnetic experiment will be described. The analysis of the electromagnetic transient variations was conducted in accordance with the classical distinction between quiet and disturbed magnetic situations. A morphological analysis of the recordings is given, taking into consideration successively quiet and disturbed magnetic situations, with the results interpreted in terms of the characterization of external and internal sources. Particular attention was paid to the effects of the source characteristics on the induced field of internal origin, and to the bias they may consequently cause to the results of electromagnetic probing of the Earth; the source effect in electromagnetic induction studies. During quiet magnetic situations, our results demonstrated the existence of two different sources. One of these, the S_R^E source, was responsible for most of the magnetic diurnal variation and corresponded to the well-known magnetic signature of the equatorial electrojet. The other source (the S_R*^E source) was responsible for most of the electric diurnal variation, and was also likely to be an ionospheric source. Electric and magnetic diurnal variations are therefore related to different ionospheric sources, and interpreting the electric diurnal variation as induced by the magnetic field diurnal variation is not relevant. Furthermore, the magnetotelluric probing of the upper mantle at dip equator latitudes with the electromagnetic diurnal variation is consequently impossible to perform. In the case of irregular variations, the source effect related to the equatorial electrojet is also discussed. A Gaussian model of equatorial electrojet was considered, and apparent resistivities were computed for two models of stratified Earth corresponding to the average resistive structure of the two tectonic provinces crossed by the profile: a sedimentary basin and a cratonic shield. The apparent resistivity curves were found to depend significantly on both the model used and the distance to the center of the electrojet. These numerical results confirm the existence of a daytime source effect related to the equatorial electrojet. Furthermore, we show that the results account for the observed differences between daytime and night-time apparent resistivity curves. In particular, it was shown that electromagnetic probing of the Earth using the classical Cagniard-Tikhonov magnetotelluric method is impossible with daytime recordings made at dip latitude stations.