CFRP加固一字形竖缝耗能预制剪力墙抗震性能研究     

王宇亮  何斌  张玉敏  李祥  庞豹 《震灾防御技术》2021,16(3):544-553

以一字形竖缝耗能预制剪力墙作为研究对象,设计了3个装配式剪力墙试件及1个现浇剪力墙对比试件,进行低周往复荷载试验,并对破坏墙体进行CFRP加固,再次进行拟静力试验。试件变化参数包括轴压比、混凝土强度等级及配筋率,对比分析加固前后试件滞回性能、刚度退化、承载力和耗能能力等性能。试验结果表明,与现浇剪力墙相比,一字形竖缝耗能预制剪力墙工作性能良好,阻尼器屈服耗能提高了试件整体工作性能;CFRP加固可有效抑制墙体斜裂缝的发展,对墙体承载力及耗能能力均有显著改善作用;各试件均满足剪力墙弹塑性层间位移角限值要求,延性较好;试件整体表现出良好的抗震性能。  相似文献   

震源顶部条件-前兆优显层的讨论          下载免费PDF全文

郭增建  秦保燕 《地震工程学报》1982,4(2):1-6

在地震预报工作中,人们既期望直接观测到震源地方的情况,又期望观测手段易于实施以及干扰因素较小。但是这几个方面是不易得兼的。例如为了直接观测震源地方的情况,则探测深度就要深,此时测量手段不易实施;如观测震源在地表的间接表现,虽手段易于实  相似文献   

俯冲带中大理岩与榴辉岩的Mg-Fe-C-O同位素迁移     

闫伟豪  王勤  李伟强 《地质学报》2022,96(2):500-516

碳酸盐岩和碳酸盐化岩石是俯冲带中碳的主要地质载体.俯冲-折返的超高压变质岩记录了俯冲隧道中流体-岩石的相互作用与元素迁移,是研究地球内部元素循环的重要媒介.本文采集了大别造山带罗家岭互层状产出的大理岩和榴辉岩,建立了横跨岩性界面的矿物组成、显微结构和Mg-Fe-C-O同位素剖面.大理岩中主要组成矿物为白云石,其次为方解...  相似文献   

Formation blockage risk analysis of geothermal water reinjection:Rock property analysis,pumping and reinjection tests,and long-term reinjection prediction     

Liang Zhang  Songhe Geng  Linchao Yang  Ronghua Wen  Chuan He  Zhen Zhao  Guangxiong Qin 《地学前缘(英文版)》2022,(1):310-325

The blockage induced by particle migration and deposition is one of the main reasons for the decrease of reinjection capacity in the porous geothermal reservoir with a low and medium temperature.In this paper,a new drilled geothermal well in Xining basin China is taken as an example to investigate the formation blockage risk due to the movable clay and sand particles in pores.The physical properties of the reservoir rocks were analyzed,a series of pumping and reinjection tests were conducted,and the longterm reinjection performance of the well was predicted by numerical simulation based on the test fitting.The results show that the geothermal reservoir rocks are argillaceous and weakly cemented sandstones with a content of movable clay and sand particles up to 0.18–23.42 wt.%.The well presented a high productivity of 935–2186 m3?d-1 at a pressure difference of 0.7–1.62 MPa in the pumping tests associated with a large amount of clay and sand particles produced out,while in the reinjection test,only a low injectivity of 240–480 m3?d-1 was observed at an injection pressure of 0.2–0.6 MPa with the clay and sand particles near the wellbore move into deep.According to the prediction,under conditions of a blockage risk,the injectivity of the well will start to decline after 100 days of injection,and in the third year,it will decrease by 59.00%–77.09%.The influence of invasion of pretreated suspended particles and scale particles can be neglected.Under conditions of a high blockage risk,the injectivity of the well will decrease significantly in the first 20–30 days,with a decline of 75.39%–78.96%.Generally,the higher the injection pressure or rate,the greater the decrease in injectivity of the well caused by particle blockage.Pump lifting is an effective measure to remove the well blockage which can be used regularly.  相似文献   

山东东营凹陷古近系碎屑岩储层特征及控制因素   总被引：25，自引：10，他引：15       下载免费PDF全文

张琴  朱筱敏  钟大康  宋刚 《古地理学报》2004,6(4):493-502

通过对大量储层物性数据的分析和整理,结合薄片观察和扫描电镜分析结果,研究了不同构造背景、不同沉积类型及不同埋深的储层物性特征及其控制因素。东营凹陷近系碎屑岩储层类型多样,大多形成在冲积扇-河流、扇三角洲、近岸水下扇、深水浊积扇、三角洲前缘滑塌浊积扇以及滨浅湖滩坝等多种沉积环境中。碎屑岩储层类型主要包括砾岩、含砾砂岩、中粗砂岩、细砂岩及粉砂岩。其中中砂岩和细砂岩是最好的储层。但是不同地区、不同类型储层物性存在较大的差异。物性最好的储层为河道、（扇）三角洲前缘水下分流河道及河口坝砂体。在相同深度条件下,中央隆起带的物性最好,北部和南部次之。另外,本区随埋藏深度增加,碎屑岩储层物性逐渐变差（剔除次生孔隙的影响）。根据碎屑岩储层物性差异性分析和储层成岩演化研究结果,其储层物性主要受压实作用、碳酸盐溶蚀与胶结作用及沉积条件四大因素控制,其中压实作用、溶蚀作用及胶结作用是主要控制因素,而沉积条件对物性的影响主要表现在控制原生孔隙的发育程度,并进一步控制溶蚀、胶结等成岩作用。  相似文献   

The Effect of AGN and SNe Feedback on Star Formation, Reionization and the Near Infrared Background     

Lei Wangt Ji-Rong Mao Shou-Ping Xiang Ye-Fei Yuan 《中国天文和天体物理学报》2008,8(6)

Feedback from supernovae (SNe) and from active galactic nuclei (AGN) accom-panies the history of star formation and galaxy evolution. We present an analytic model to explain how and when the SNe and AGN exert their feedback effects on the star formation and galaxy evolution processes. By using SNe and AGN kinetic feedback mechanisms based on the Lambda Cold Dark Matter (LCDM) model, we explore how these feedback mecha-nisms affect the star formation history (SFH), the Near-Infrared Background (NIRB) flux and the cosmological reionization. We find the values of the feedback strengths, ∈AGN =1.0+0.50.3and ∈SN=0.04+0.02-0.02, can provide a reasonable explanation of most of the observational re-suits, and that the AGN feedback effect on star formation history is quite different from the SNe feedback at high redshifts. Our conclusions manifest quantitatively that these feedback effects decrease star formation rate density (SFRD) and the NIRB flux (in 1.4 - 4.0μm), and postpone the time of completion of the cosmological reionization.  相似文献   

Relationship between pulse width and energy in GRB 060124: from X-ray to γ-ray bands     

Fu-Wen Zhang  Yi-Ping Qin   《New Astronomy》2008,13(7):485-490

GRB 060124 is the first event that both prompt and afterglow emission were observed simultaneously by the three Swift instruments. Its main peak also triggered Konus-Wind and HETE-II. Therefore, investigation on both the temporal and spectral properties of the prompt emission can be extended to X-ray bands. We perform a detailed analysis on the two well identified pulses of this burst, and find that the pulses are narrower at higher energies, and both X-rays and γ-rays follow the same w–E relation for an individual pulse. However, there is no a universal power-law index of the w–E relation among pulses. We find also that the rise-to-decay ratio r/d seems not to evolve with E and the r/d values are well consistent with that observed in typical GRBs. The broadband spectral energy distribution also suggests that the X-rays are consistent with the spectral behavior of the γ-rays. These results indicate that the X-ray emission tracks the γ-ray emission and the emissions in the two energy bands are likely to be originated from the same physical mechanism.  相似文献   

全新世时期北京-张家口地区与黄土高原地区风成系统的差异   总被引：7，自引：3，他引：4  

秦小光  吴金水  蔡炳贵  顾兆炎  刘东生 《第四纪研究》2004,24(4):430-436

近年来,中国北方的沙尘暴对北京地区的影响越来越受到人们的重视,从地质记录上分析研究北京—张家口地区沙尘暴的粉尘来源对确定重点治理区、改善北京地区的大气环境质量具有积极意义。黄土是地质时期沙尘暴形成的风成沉积物,其粒径分布蕴含了粉尘搬运过程中的大气环境信息,本文利用黄土-古土壤沉积的粒径分布特征,分析了北京—张家口地区和黄土高原地区风成系统的差异,并根据粉尘动力学原理,结合遥感信息揭示的地面风蚀痕迹,探讨了北京—张家口地区黄土粉尘的主要来源,指出北京—张家口地区和黄土高原地区分属不同的风成系统,有不同的粉尘源区和不同的大气动力条件。北京—张家口地区大气动力强度大,粉尘源区近,粉尘主要来自阴山以北的内蒙古苏尼特右旗—二连浩特方向,与浑善达克沙地关系不大,也与黄土高原地区主要粉尘物源区不同  相似文献   

Energy transition,CO2 mitigation,and air pollutant emission reduction: scenario analysis from IPAC model     

Jiang  Kejun  Chen  Sha  He  Chenmin  Liu  Jia  Kuo  Sun  Hong  Li  Zhu  Songli  Pianpian  Xiang 《Natural Hazards》2019,97(3):1277-1295

The salinization of freshwater-dependent coastal ecosystems precedes inundation by sea level rise. This type of saltwater intrusion places communities, ecosystems, and infrastructure at substantial risk. Risk perceptions of local residents are an indicator to gauge public support for climate change adaptation planning. Here, we document residential perspectives on the present and future threats posed by saltwater intrusion in a rural, low-lying region in coastal North Carolina, and we compare the spatial distribution of survey responses to physical landscape variables such as distance to coastline, artificial drainage density, elevation, saltwater intrusion vulnerability, and actual salinity measured during a synoptic field survey. We evaluate and discuss the degree of alignment or misalignment between risk perceptions and metrics of exposure to saltwater intrusion. Risk perceptions align well with the physical landscape characteristics, as residents with greater exposure to saltwater intrusion, including those living on low-lying land with high concentrations of artificial drainages, perceive greater risk than people living in low-exposure areas. Uncertainty about threats of saltwater intrusion is greatest among those living at higher elevations, whose properties and communities are less likely to be exposed to high salinity. As rising sea levels, drought, and coastal storms increase the likelihood of saltwater intrusion in coastal regions, integrated assessments of risk perceptions and physical exposure are critical for developing outreach activities and planning adaptation measures.

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四川盆地震旦系灯影组白云岩成因   总被引：3，自引：1，他引：2  

金民东  谭秀成  李毕松  朱祥  曾伟  连承波 《沉积学报》2019,37(3):443-454

基于岩芯观察、薄片鉴定、地球化学分析,结合区域地质背景,系统研究了四川盆地震旦系灯影组白云岩成因。岩石学特征分析发现,灯影组白云岩可分为泥粉晶云岩、粒屑云岩、微生物云岩、岩溶角砾云岩4类,其结构类型一般为泥晶—粉晶,说明白云岩化时间较早,为准同生期。地球化学分析表明,灯影组白云岩δ^13C平均值与震旦纪原始海水较为接近,δ^18O值呈现中—高负偏的特征,有序度和Fe、Mn含量相对偏低,Na含量相对较高,稀土元素配分模式则与海水配分曲线类似,表明白云岩化主要受到海源流体的影响。盆地周缘的古陆和水下隆起使盆内海水极易封隔浓缩,盆内发育的富Ca^2+菌藻类可间接提高海水的Mg^2+/Ca^2+比值,加之灯影期干旱炎热的古气候让盆内蒸发作用强烈,可伴生石膏等蒸发性矿物,促进白云石化。综合上述特征,四川盆地灯影组白云岩成因为微生物参与的蒸发海水回流渗透白云石化。  相似文献