针对应急救援的强余震特征统计          下载免费PDF全文

管丽倩    戴君武    杨永强    许德峰   《世界地震工程》2022,38(3):212-220

大地震后强余震活跃,震后快速判断最大余震震级和强余震发生可能性对提高应急救援效率有重大意义。针对震后应急救援,本文根据救援存活率将震后救援期分为8个时段:震后12 h、震后24 h、震后48 h、震后72 h、震后96 h、震后120 h、震后144 h和震后168 h。对我国大陆地区1966年以来6级及以上地震强余震资料进行分时段统计,分别拟合出8个时段的最大余震震级和主震震级的经验公式;并提出震后强余震发生可能性的经验判断方法,通过本文提出的可能性指数a,依据主震震级,震后可以快速判定强余震发生的可能性。  相似文献   

基于IDA的层间隔震结构失效模式研究          下载免费PDF全文

李天明  刘德稳  罗晓轩  霍一然  杨忠楠  雷敏 《世界地震工程》2022,38(4):132-142

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。  相似文献   

场地韧性的概念及有关问题的讨论          下载免费PDF全文

薄景山    张毅毅  薄涛  王玉婷    赵鑫龙  陈亚男 《世界地震工程》2022,38(3):001-9

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。  相似文献   

一种亮星识别算法及其在天文定向中的应用     

詹银虎  郑勇  张超  李铸洋  张中凯 《测绘学报》2015,44(3):257-263

基于全站仪对任意亮星的观测采样,提出了一种利用高度角序列和水平角速率进行联合匹配的任意亮星识别算法。通过引入天体地平坐标计算程序,算法可正确辨别行星和恒星。本文分析了任意亮星高度角和水平角速率的观测误差和计算误差,以此给出了匹配阈值条件的设定依据,并在此基础上制定了有效的匹配策略。仿真计算及实际观测试验均表明,该算法具有100%的识别成功率,远优于现有算法。将此算法应用于任意亮星天文定向,定向结果的内符合精度达到2″,外部检核精度达到1.6″。采用多颗任意亮星进行定向,可有效减弱由测站位置误差引入的定向系统误差,提高绝对定向精度。本文提出的天文定向适用于多云及雾霾天气。  相似文献   

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

Yun-Ming Dong Lan-Wei Jia Xiao-Hong Zhao Yunnan Astronomical Observatory/National Astronomical Observatories  Chinese Academy of Sciences  Kunming  Graduate University of Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2006,6(1):69-76

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.  相似文献   

CCD Photometry of Asteroid （147） Protogeneia     

Xi-Liang Zhang  Xiao-Bin Wang  Li-Yun Zhang National Astronomical Observatories / Yunnan Observatory  Chinese Academy of Sciences  Kunming  Graduate School of Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2006,6(6):729-732

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.  相似文献   

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

Cong Yu National Astronomical Observatories / Yunnan Astronomical Observatory  Chinese Academy of Sciences  Kunming  Graduate School of Chinese Academy of sciences  Beijing 《中国天文和天体物理学报》2006,6(6):680-688

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.  相似文献   

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

Zhong-Quan Qu  Shuai Wang  Cheng-Lin Xu  XiaoYu Zhang  Ming-Guo Sun  Chun-Lan Jin National Astronomical Observatories/Yunnan Astronomical Observatory  Chinese Academy of Sciences  Kunming  zqqu@vip.km.net Graduate School of the Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2005,5(4):426-432

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.  相似文献   

计算空间VLBI天线面有效截面程的数学模型     

郑勇  钱志瀚 《中国科学院上海天文台年刊》1992,(13):140-144

本推导建立了计算空间VLBI天线面有效截面的数学模型，它将适用于确定空间VLBI站轨道所需的太阳光压、大气阻力、地球反照压等非引力摄动模型中面质比的计算。  相似文献   

Analysis on the decadal scale variation of the dust storm in North China   总被引：3，自引：0，他引：3  

KANG Dujuan  & WANG Huijun . NZC/LASG  Institute of Atmospheric Physics  Chinese Academy of Sciences  Beijing  China  . Environmental Fluid Mechanics Laboratory  Stanford University  Stanford CA  USA 《中国科学D辑(英文版)》2005,48(12):2260-2266

Dust storm is a disastrous weather that can cause serious environmental consequences and hazards. It causes excessive soil mass and nutrient loss in source areas, and air pollution in deposition area, which result in bad influence on agriculture, industry, traffic, and peoples’ daily life[1-4]. Dust storm can also affect the thermal balance of planetary radiation and then lead to meso- to macroscale climatic modification[5-7]. North- west China and North China are two high-frequency centers …  相似文献