集团异化与亚太区域经济合作

集团异化现象是集团化进程中的一种逆反行为,集中反映在经互会的解体和围绕“赫一伯法”而导致的北美集团成员国之间制裁与反制裁的公开对抗。冷战结束后这种现象异常活跃,而且具有广泛的世界意义。文章阐述了集团异化的概念和当代的集团异化现象和异化效应;分析了集团异化产生的国际背景与内因。作者进而指出,在新的国际形势下,集团异化构成为集团化进程中的一种新现象和新问题,并非偶然;最后探讨了它对于发展亚太区域经济合作的理论意义和现实意义。     

三峡库区农业生态经济系统的预警分析

从系统与环境相统一的角度,研究了农业生态经济系统的模型、特征、预警分析的意义和内容;以三峡库区为例,从系统序化的观点,确定了这个系统的社会、经济、环境功能和状态的主要指标的警戒线;并与这些指标的现状、过去与未来趋势值进行对比;分别对现状预警、趋势预警和突变预警进行了评价;最后作了简易的对策探讨．     

多点入流汇流计算法在北京城市洪水计算中的应用与研究

根据北京城市化水平,城市汇流特点,通过用多点入流汇流计算法模拟实测洪水过程线,分析了北京城市河道的汇流特点与规律,初步提出了一种适合于北京城市洪水计算的方法,为城市防洪排水工程规划,设计提供依据。     

我国水电地下工程围岩分类系统支护方案探讨

在对我国水电地下工程围岩分类评价系统（ＳＤ系统）和Ｂａｒｔｏｎ的Ｑ系统的分析比较研究的基础上,针对水电工程,探讨了ＳＤ系统和Ｑ系统的相关关系,细化和发展了我国ＳＤ系统的支护设计方案,弥补了其支护类型偏少和简单的不足。     

An Improved Perturbation Mechanism for Simulated Annealing Simulation

Simulated annealing (SA) is being increasingly used for the generation of stochastic models of spatial phenomena because of its flexibility to integrate data of diverse types and scales. The major shortcoming of SA is the extensive CPU requirements. We present a perturbation mechanism that significantly improves the CPU speed. Two conventional perturbation mechanisms are to (1) randomly select two locations and swap their attribute values, or (2) visit a randomly selected location and draw a new value from the global histogram. The proposed perturbation mechanism is a modification of option 2: each candidate value is drawn from a local conditional distribution built with a template of kriging weights rather than from the global distribution. This results in accepting more perturbations and in perturbations that improve the variogram reproduction for short scale lags. We document the new method, the increased convergence speed, and the improved variogram reproduction. Implementation details of the method such as the size of the local neighborhood are considered.     

Geochemical Evolution and Environmental Changes of Qinghai—Xizang Plateau Since Late Cenozoic

Long-and short-term climatic curves were preliminarily established based on the comprehensive analysis of geochemical information since the Late Cenozoic in the Qinghai Xizang(Qinghai-Tibet)Plateau.The curves show that the climate in the plateau was alternatively dry-warm and cold-wet during the period of 30-3.4 Ma when the plateau was not uplifted to an enough altitude and the monsoon was not completely formed either,In the period of 3.4-0.73 Ma.the climate fluctuated between dry-cold and wet-warm when the plateau was rapidly uplifted and the Asian monsoon was consequently formed.Since 0.73 Ma.the climate became even drier when the plateau continuously rose.In the Holocene period.the climate alternatively changed with a complex model of being cool-dry,warm-wet and cold-wet.     

地震波测试技术在十三陵蓄能电站工程验收中的应用

介绍了地震波测试技术在钻孔中测试地层动弹模的原理、方法及效果,并计算出静弹模,为工程的质量评价和验收提供了依据。     

利用变参数回归方法反演泥质岩裂缝密度

本文利用变参数回归分析建立了多口井的泥质岩储层裂缝密度模型。该模型的平均相对误差为１３．５％,较常系数回归分析、ＢＰ网络模型进行裂缝预测的精度高（平均相对误差分别为３８．７％、１７．９％）。通过实际资料处理认为该油田在纵向上随时代变老,深度加深,裂缝密度降低。即从Ｎ２２、Ｎ１２到Ｎ１,平均裂缝密度从０．７８条／ｍ、０．５条／ｍ降低到０．３条／ｍ。在平面上,沿构造轴部裂缝最发育,平均裂缝密度Ｎ２２、Ｎ１２、Ｎ１层分别为０．５８条／ｍ、０．６条／ｍ、０．３条／ｍ。     

煤矸石合成莫来石熟料研究

研究了煤矸石加氢氧化铝及氧化铝合成莫来石熟料的可行性。实验表明,采用煤矸石和氢氧化铝可在１５００℃完成莫来石化反应,到１５５０℃可得到接近理论密度的莫来石熟料,采用煤矸石和工业氧化铝反应,可在１５５０℃全部合成莫来石,到１６００℃可得到接近理论密度的莫来石熟料,采用煤矸石加α－Ａｌ２Ｏ３所得样品性能良好,化学成分最纯。     

Mid-to-Far Infrared Spectral Energy Distribution of Galaxies in the Spitzer First Look Survey Field

We made model fitting to the mid-to-far infrared spectral energy distributions (SEDs) for different categories of galaxies in the main extragalactic field of the Spitzer First Look Survey with the aid of spectroscopic information from the Sloan Digital Sky Survey. We find that the mid-to-far infrared SEDs of HII galaxies, mixture type galaxies and LINERs can be well fitted by the one-parameter (α) dust model of Dale et al. plus the 13 Gyr dust-free elliptical galaxy model. The statistics of α values indicates that all these galaxies tend to be quiescent, although the HII galaxies are relatively more active than the LINERs. The mid- infrared SEDs of absorption galaxies are well fitted simply by the 13 Gyr dust-free elliptical galaxy template, and the near-to-mid infrared SEDs of QSOs can be represented by AGN NGC 5506.