电磁辐射异常分析方法研究

利用河北省电磁台网１９８８～１９９２年的观测资料，对不同台站不同方向的异常映震能力进行了分析研究。并运用信息论方法计算了各台信息水平作为其信息可信度的权系数，对各台资料采用加权平均的方法进行了合成处理，发现比平时采用的等权平均效果要好。同时对其异常频次的累加合成对应地震的异常特征进行了初步的探讨     

初析静力触探判别液化对标准贯入试验的优越性

结合7个勘察场地的标准贯入和静力触探原位测试数据,应用数理统计原理和方法对二者进行比较分析,得出用静力触探试验判别地基土液化的均方差和变异系数等均优越于标准贯入试验。     

中国地磁台环境场的计算与分析

根据国际参考地磁场(IGRF)模型,计算出1945年5月—1990年5月中国部分地磁台的计算年均值,并与相应观测年均值比较,计算出地磁台各个地磁要素的磁异常值以及地磁台异常场的模量,本文的计算结果将为认识地磁台的地磁场环境、地磁台站资料评比提供依据。     

A SPECTRUM OF LYAPUNOV EXPONENTS OBTAINED FROM A CHAOTIC TIME SERIES

A complete spectrum of Lyapunov exponents (LEs) is obtained from 1970— 1985 daily mean pressuremeasurements at Shanghai by means of a correlation matrix analysis technique and it is found that there exist LEs≥0,and <0. with their sum 0λ_i=K=0.110405 whereuponT=1 /K =9 is obtained as the predictable time scale, a result close to that acquired by the dynamic-statistical approachin early days and also in agreement with that present by the authors themselves(1991).     

相对点位中误差及其在工程测量中的作用

阐述相对点位中误差的概念及其在工程测量中的作用,介绍相对点位中误差及相对误差椭园计算方法,以示例说明点位中误差和相对点位中误差的意义和作用。     

粗差数学期望平移模型的理论研究

现有文献对数学期望平移模型的理论分析仅考虑了观测值统计独立的特殊情况。基于观测值统计相关的一般情况，导出了数学期望平移参数估值（Ｓｉ）的简明表达式。在此基础上，采用统计预测理论对Ｓｉ进行了直观的理论解释，扩展了统计学文献中的有关结论。借助于实例，分析了Ｓｉ与最小二乘残差的本质区别。     

海洋平均重力异常计算与精度估计

提出了一种简便实用的重力异常推值方法──方位距离加权中数法，给出了直接使用重力异常变化梯度作为衡量平均重力异常计算精度的尺度，并运用ＯＳＵ９１Ａ模型成功地建立起重力异常变化梯度与平均重力异常计算精度的相关关系，通过此关系可对海洋平均重力异常计算精度作出比较可靠的估计。     

Stochastic perturbation analysis of groundwater flow. Spatially variable soils,semi-infinite domains and large fluctuations

As is well known, a complete stochastic solution of the stochastic differential equation governing saturated groundwater flow leads to an infinite hierarchy of equations in terms of higher-order moments. Perturbation techniques are commonly used to close this hierarchy, using power-series expansions. These methods are applied by truncating the series after a finite number of terms, and products of random gradients of conductivity and head potential are neglected. Uncertainty regarding the number or terms required to yield a sufficiently accurate result is a significant drawback with the application of power series-based perturbation methods for such problems. Low-order series truncation may be incapable of representing fundamental characteristics of flow and can lead to physically unreasonable and inaccurate solutions of the stochastic flow equation. To support this argument, one-dimensional, steady-state, saturated groundwater flow is examined, for the case of a spatially distributed hydraulic conductivity field. An ordinary power-series perturbation method is used to approximate the mean head, using second-order statistics to characterize the conductivity field. Then an interactive perturbation approach is introduced, which yields improved results compared to low-order, power-series perturbation methods for situations where strong interactions exist between terms in such approximations. The interactive perturbation concept is further developed using Feynman-type diagrams and graph theory, which reduce the original stochastic flow problem to a closed set of equations for the mean and the covariance functions. Both theoretical and practical advantages of diagrammatic solutions are discussed; these include the study of bounded domains and large fluctuations.     

Differences between Mean Sea Levels for the Pacific,Atlantic and Indian Oceans From Topex/Poseidon Altimetry

Geopotential values W of the mean equipotential surfaces representing the mean ocean topography were computed on the basis of four years (1993 - 1996) TOPEX/POSEIDON altimeter data: W = 62 636 854.10m ² s ^–2 for the Pacific (P), W = 62 636 858.20m ² s ^–2 for the Atlantic (A), W = 62 636 856.28m ²s^–2 for the Indian (I) Oceans. The corresponding mean separations between the ocean levels were obtained as follows: A – P = – 42 cm, I– P = – 22 cm, I – A = 20 cm, the rms errors came out at about 0.3 cm. No sea surface topography model was used in the solution.     

The response of the azimuthal component of the ionospheric electric field to auroral arc brightening

We have analyzed the response of azimuthal component of the ionospheric electric field to auroral arc activity. We have chosen for analysis three intervals of coordinated EISCAT and TV observations on 18 February, 1993. These intervals include three kinds of arc activity: the appearance of a new auroral arc, the gradual brightening of the existing arc and variations of the arc luminosity. The arcs were mostly east-west aligned. In all cases, the enhancement of arc luminosity is accompanied by a decrease in the westward component of the ionospheric electric field. In contrast, an increase of that component seems to be connected with arc fading. The observed response is assumed to have the same nature as the short circuit of an external electric field by the conductor. The possible consequence of this phenomenon is discussed.