基于IDA的层间隔震结构失效模式研究

层间隔震结构是由基础隔震结构发展而来的一种新型隔震结构。为研究层间隔震结构的倒塌,需先研究不同层间隔震结构的不同失效模式和失效位置,文章建立了3个不同结构参数的层间隔震结构有限元模型,选取20条与抗震规范反应谱吻合的地震动,采用增量动力分析（IDA）方法,分别对其失效模式和失效位置进行研究。研究表明:基于不同的结构参数,层间隔震的基本失效模式有三种,即隔震层水平位移超限导致结构失效、下部结构层间位移角超限导致结构失效、隔震层拉压应力超限导致结构失效;隔震层下部结构和隔震层最外边缘支座为结构的薄弱位置,应引起更多关注。此方法不仅可以研究结构的不同失效模式,还可以确定失效位置,可为下一步层间隔震结构的抗倒塌分析提供理论基础。     

场地韧性的概念及有关问题的讨论

在韧性城市和建筑抗震韧性等级评价中,需要对场地的韧性给出评价。场地韧性是一个新概念,场地韧性的概念和场地韧性等级评价在学术界还是空白。因此,对场地韧性的概念及有关问题开展讨论,对韧性城市和建筑抗震韧性评价具有重要的理论意义和工程应用价值。本文在分析韧性和场地概念的基础上,讨论了场地的稳定性和抗干扰问题;基于HOLLING建立的适应性循环理论,论述了建立场地韧性概念的理论基础;首次提出了场地韧性概念并解释了其内涵;考虑韧性城市和建筑抗震韧性评价的需求,初步讨论了与场地韧性等级评价有关的问题,提出了建立场地韧性等级评价指标体系的初步设想;建议了场地韧性等级评价的数学方法,为实现场地韧性等级评价提供了途径和方法。本文研究成果对从事韧性城市和建筑抗震韧性研究的科技工作者有一定的参考价值。     

河流相储层地震属性优选与融合方法综述

地震属性分析已广泛应用于河流相砂体预测并取得良好效果.地震属性分析技术主要包括属性提取、属性优选与属性融合,总结了河流相砂体预测中常见的地震属性提取方式、优选及融合方法,分析了由围岩干扰、地震分辨率限制导致的属性提取与分析误区,阐述了不同属性优选与融合方法的优缺点、适用条件与发展前景.总体而言,基于线性模型的地震属性融合提升效果较差,适用于少井区域;基于非线性模型的属性融合效果较好,但仅适用于钻井较多的地区,如油气开发阶段;无监督智能属性融合可应用于无井或少井区域,是未来无井或少井条件下属性融合的重要发展趋势之一.同时,重点阐述了新提出的分频属性融合与降低围岩干扰的属性融合方法.      

鄂尔多斯盆地陇东地区长7段重力流砂体构型及其主控因素

鄂尔多斯盆地陇东地区长7段重力流砂体规模巨大、油气资源丰富,但不同层系不同地区砂体的形态、规模及叠置关系差异巨大,砂体构型特征及发育规律认识程度低,制约了其油气滚动勘探和开发效率。在岩心观察基础上,基于单井砂体构型界面识别和区域性连井砂体对比,结合砂体沉积微相类型开展了砂体构型划分和发育特征研究。研究认为陇东地区长7段重力流砂体规模较大,主要发育西南物源体系,其次为东北物源。发育典型的重力流水道—湖底扇沉积,可细分为侵蚀型水道、过渡型水道、沉积型水道、溢岸、沟道化朵叶体、板状朵叶体和浊积席状砂7种沉积微相。自三角洲前缘斜坡至深湖沉积中心,除砂体形态从条带状向扇形转换外,砂体规模、垂向叠置关系、横向迁移方式等构型特征亦呈现规律性变化,平面上呈现良好的分带性。在靠近三角洲前缘斜坡的近岸半深湖区,单砂体厚度小,呈孤立条带状分布,叠置关系以薄互层或单层型为主;向盆地内部,单砂体厚度增大,横向连通性增强,砂体叠置导致垂向连通性增强,逐渐向连续叠加型转化;靠近沉积中心地区,单砂体厚度略有减小,但横向连通性显著增强,连片性明显,呈间隔叠加型。综合分析认为,该区重力流砂体构型受控于重力流沉积微相、基准面旋回变化以及物源供给速率。     

Different Features of Jets and Isotropic Fireballs in Gamma-ray Burst Phase

We investigated physical quantities including the spectrum,emission lines and pulse profiles expected from a uniform jet,a spherical fireball and the 1/Γ region (the portion of the spherical fireball with opening angle 1/Γ)in the prompt emission phase,after taking into consideration of the Doppler effect under the fireball frame- work.Our study shows that:a)for these physical quantities the spherical fireball and the uniform jets do not present obvious differences,so we cannot use these to distinguish a spherical fireball from a uniform jet;b)for the spherical fireball and a uniform jet,the observed quantities mainly come from the 1/Г region,so we can simply use the 1/Г region in approximate calculations;c)broadening of emission lines is a general phenomena,which mainly comes from the curvature effect;d)the 1/Γ region plays different roles in different frequency ranges,and the radiation from the 1/Γ region is greater in the higher than in the lower frequencies.     

CCD Photometry of Asteroid （147） Protogeneia

We measured the light-curve of the asteroid (147) Protogeneia in November 2004, with a CCD detector attached to the 1-meter telescope at the Yunnan Observatory, China. The synodic period and maximum amplitude of (147) at this apparition are 7.852 hours and 0.25 mag, respectively. The value of a/b for (147), from a preliminary estimation, is not less than 1.26:1.     

An Efficient High-Resolution Shock-Capturing Scheme for Multi-Dimensional Flows I. Hydrodynamics

Many problems at the forefront of theoretical astrophysics require a treatment of dynamical fluid behavior. We present an efficient high-resolution shock-capturing hydrody-namic scheme designed to study such phenomena. We have implemented a weighted, essentially non-oscillatory (WENO) scheme to fifth order accuracy in space. HLLE approximate Riemann solver is used for the flux computation at cell interface, which does not require spectral decomposition into characteristic waves and so is computationally friendly. For time integration we apply a third order total variation diminishing (TVD) Runge-Kutta scheme. Extensive testing and comparison with schemes that require characteristic decomposition are carried out demonstrating the ability of our scheme to address challenging open questions in astrophysics.     

Magneto-induced Line Broadening of Magneto-sensitive Lines in Solar Magnetized Atmospheres

We analyze the spectral line broadening of those magneto-sensitive lines in solar magnetized atmospheres. The broadening at the line wings is due to the increase of the effective width of energy levels involved in Zeeman splitting, and the broadening at the line core also originated in Zeeman splitting under the condition that the Zeeman components are mixed. Therefore, the magnetoinduced or Zeeman broadening take effects on the whole line. The observed Stokes parameter data in a sunspot and outside it acquired by Solar Stokes Spectrum Telescope (S3T) are analyzed for the demonstration of this mechanism, and the Zeeman broadening rates are calculated for FeI6302.5 under some assumptions. Our result shows that the broadening is increased as the magnetic field strength becomes stronger, but the rate of increase at the line core is decreased as the field strength increases, while the rate at the wing does not show such an obvious regularity. The broadening is more effective in the line core than in the wings.     

平山县经济社会科技发展战略

本文运用区位、层位和生态经济理论,阐述平山县的发展战略目标、重点、布局及对策。