Analysis of spatial clustering optimization

Spatial clustering is widely used in many fields such as WSN (Wireless Sensor Networks), web clustering, remote sensing and so on for discovery groups and to identify interesting distributions in the underlying database. By discussing the relationships between the optimal clustering and the initial seeds, a clustering validity index and the principle of seeking initial seeds were proposed, and on this principle we recommend an initial seed-seeking strategy: SSPG (Single-Shortest-Path Graph). With SSPG strategy used in clustering algorithms, we find that the result of clustering is optimized with more probability. At the end of the paper, according to the combinational theory of optimization, a method is proposed to obtain optimal reference k value of cluster number, and is proven to be efficient.     

某可溶性软弱基座型斜坡的破坏方式及变形破坏机制

以仁义河特大桥南桥台南侧斜坡为例,分析研究了可溶性软弱基座型斜坡的破坏方式及其变形破坏力学机制,认为该斜坡的失稳破坏主要为崩塌破坏,并存在倾倒(外倾型)、倾滑(内倾型)和基座倾滑3种崩塌破坏方式,形成不同崩塌破坏方式的内在变形机制有弯曲一拉裂、弯曲一层间滑动和拉裂一滑移3种模式,从而为解决该类特殊斜坡工程问题提供了理论依据。     

海洋灾害地质风险评价在辽东湾浅海油气开发区的应用

基于在辽东湾浅海油田多年调查获取的地质地球物理资料,构建以油气开发区潜在灾害地质类型为基础的灾害地质风险评价指标体系,确定潮流冲刷槽、浅滩、埋藏古河道、易液化砂层、软弱地层和浅层气等6个评价指标,利用层次分析法(AHP)确定各指标的权重值,采用模糊数学评判法对海区灾害地质风险性作定量评价。评价结果划为5级风险区(风险高、较高、中等、较低和低),其中,潮流冲刷槽为本区的高风险区,地势平缓的潮滩为低风险区。评价结果与区内已建海洋工程的评价分析相互印证,对海上工程建设具有实际应用价值。     

浅谈灰土挤密桩与DDC桩在工程实践中应用与发展

DDC桩是挤密桩的一种新型桩。根据宝鸡某大型电厂中DDC桩与灰土挤密桩地基处理工程实例,从挤密机理、挤密效果、复合地基承载力与抗变形性状及复合地基浸水稳定性等诸方面进行了系统地分析对比,进而探讨挤密桩地基的应用与发展。     

关于垃圾填埋场渗滤系统渗透性能经时变化的研究

利用模拟实验对垃圾填埋场中渗滤系统的渗透性能与填埋时间的关系进行了研究。采用焚烧灰、土工织物和碎石导流层组成渗透系统,研究了实验时间对渗滤系统的渗透系数以及结晶物颗粒直径的影响。结果表明:由于垃圾焚烧灰中硅酸钙和铝酸钙的结晶作用,随着渗透时间的增加,吸附在土工织物表面的物质逐渐增多,使颗粒之间更紧密,导致空隙减小影响渗滤系统的渗透性能。根据研究结果,在垃圾焚烧灰填埋时,垃圾焚烧灰压实密度不要太高,这样有利于渗滤液的排放。     

Temporal and spatial dynamical simulation of groundwater characteristics in Minqin Oasis

Application scope of geostatistics has been gradually extended from original geologic field to soil science and ecological field, etc. and its successful application results have been widely demonstrated. But little information is reported as to the direct use of geostatistical method to work out the distribu- tion map of groundwater characteristics. In this paper the semivariogram of geostatistics, in combina- tion with GIS, was used to quantitatively study the spatial variation characteristics of groundwater table depth and mineralization degree and their relation to the landuse changes. F test of the used spherical model reached a very significant level, and the theoretical model can well reflect the spatial structural characteristics of groundwater table depth and mineralization degree and achieve an ideal result. This shows that the application of the method in the dynamical simulation of groundwater is feasible. And this paper also provides useful reference for the application of geostatistics in the study of the dy- namical variations of groundwater resources in the oasis.     

RG-1测汞仪软件介绍

RG1测汞仪操作软件使用VC++5.0工具研制,在Windows95下运行。通过AD/DA接口实现对RG1的控制和对基准电压的自动跟踪校正。完全的可视化操作。具有4种可选的标准曲线拟合方法以用于不同浓度样品的峰值和积分值测量,并直接给出汞浓度及各种统计数据     

按新旧规范设计的多层住宅砖房地震易损性的对比

本文采用概率方法借助于拉丁超立方采样技术和非线性地震反应时程分析对按现行规范设计的多层住宅砖房的地震易损性进行分析,并与按上一代规范设计的多层住宅砖房的地震易损性分析结果[1]进行了比较,为进一步研究这类结构的地震安全性、未来地震的损失预测以及防震减灾对策奠定基础。     

Dark energy model in anisotropic Bianchi type-III space-time with variable EoS parameter

A new dark energy model in anisotropic Bianchi type-III space-time with variable equation of state (EoS) parameter has been investigated in the present paper. To get the deterministic model, we consider that the expansion θ in the model is proportional to the eigen value s² ₂\sigma^{2}_{~2} of the shear tensor s^j _i\sigma^{j}_{~i}. The EoS parameter ω is found to be time dependent and its existing range for this model is in good agreement with the recent observations of SNe Ia data (Knop et al. in Astrophys. J. 598:102, 2003) and SNe Ia data with CMBR anisotropy and galaxy clustering statistics (Tegmark et al. in Astrophys. J. 606:702, 2004). It has been suggested that the dark energy that explains the observed accelerating expansion of the universe may arise due to the contribution to the vacuum energy of the EoS in a time dependent background. Some physical aspects of dark energy model are also discussed.