Evaluation of the seismic performance of a three‐story ordinary moment‐resisting concrete frame     

Sang Whan Han  Oh‐Sung Kwon  Li‐Hyung Lee 《地震工程与结构动力学》2004,33(6):669-685

This study focuses on the seismic performance of Ordinary Moment‐Resisting Concrete Frames (OMRCF) designed only for gravity loads. For this purpose, a 3‐story OMRCF was designed in compliance with the minimum design requirements in the American Concrete Institute Building Code ACI 318 (1999). This model frame was a regular structure with flexure‐dominated response. A 1/3‐scale 3‐story model was constructed and tested under quasi‐static reversed cyclic lateral loading. The overall behavior of the OMRCF was quite stable without abrupt strength degradation. The measured base shear strength was larger than the design base shear force for seismic zones 1, 2A and 2B calculated using UBC 1997. Moreover, this study used the capacity spectrum method to evaluate the seismic performance of the frame. The capacity curve was obtained from the experimental results for the specimen and the demand curve was established using the earthquake ground motions recorded at various stations with different soil conditions. Evaluation of the test results shows that the 3‐story OMRCF can resist design seismic loads of zones 1, 2A, 2B, 3 and 4 with soil types S_A and S_B . For soil type S_C , the specimen was satisfactory in seismic zones 1, 2A, 2B and 3. For soil type S_D , the OMRCF was only satisfactory for seismic zones 1 and 2A. Copyright © 2004 John Wiley & Sons, Ltd.  相似文献   

Origin of Mesozoic gold mineralization in South Korea   总被引：6，自引：0，他引：6  

Seon-Gyu  Choi  Sung-Tack  Kwon  Jin-Han  Ree  Chil-Sup  So  Sang Joon  Pak 《Island Arc》2005,14(2):102-114

Abstract   The Mesozoic gold–silver deposits in South Korea are closely associated with the Mesozoic granitoids. The Jurassic gold–silver deposits can be distinguished from the Cretaceous ones in terms of occurrence, alteration style, gold fineness, associated mineral assemblage, fluid inclusion and stable isotopic compositions. The Jurassic deposits were formed in mesozonal environments related to deep-seated granitoids, whereas the Cretaceous ones were formed in epizonal environments related to shallow-level granitoids. The Jurassic auriferous deposits (about 165–145 Ma) show fluid characteristics typical of an orogenic-type gold deposit, and were probably generated in a compressional regime caused by an orthogonal convergence of the Izanagi oceanic plate into the Asiatic margin. However, strike-slip faults and caldera-related fractures, together with subvolcanic to volcanic activity, may have played an important role in the formation of Cretaceous gold–silver lode deposits (about 110–45 Ma) under a continental arc setting.  相似文献   

云南兰坪白秧坪铜钴多金属矿集区矿石中石英的⁴⁰Ar-³⁹Ar年龄   总被引：6，自引：1，他引：6       下载免费PDF全文

何明勤  刘家军  李朝阳  李志明  刘玉平  杨爱平  桑海清 《地质科学》2006,41(4):688-693

云南兰坪白秧坪铜钴多金属矿集区矿石中石英的⁴⁰Ar-³⁹Ar快中子活化年龄谱呈马鞍形,坪年龄为56.53±0.43Ma,最小视年龄为55.52±1.78Ma,等时线年龄为55.90±0.29Ma,三者在误差范围内一致(1σ)。⁴⁰Ar/³⁶Ar初始值为294.7±1.14,与尼尔值(295.5±5)十分接近,坪年龄和等时线年龄均可作为石英的形成时代。因此,55.90~56.53Ma(喜马拉雅早期)代表了矿床的成矿年龄。  相似文献   

Genetic Environment of the Intrusion-related Yuryang Au-Te Deposit in the Cheonan Metallogenic Province, Korea     

Sang Joon Pak    Seon-Gyu Choi    Chang-Whan Oh  Chul-Ho  Heo  Sang-Hoon Choi  Sung-Won Kim 《Resource Geology》2006,56(2):117-132

Abstract. The Yuryang gold deposit, comprising a Te‐bearing Au‐Ag vein mineralization, is located in the Cheonan area of the Republic of Korea. The deposit is hosted in Precambrian gneiss and closely related to pegmatite. The mineralized veins display massive quartz textures, with weak alteration adjacent to the veins. The ore mineralization is simple, with a low Ag/Au ratio of 1.5:1, due to the paucity of Ag‐phases. Ore mineralization took place in two different mineral assemblages with paragenetic time; early Fe‐sulfide mineralization and late Fe‐sulfide and Au‐Te mineralization. The early Fe‐sulfide mineralization (pyrite + sphalerite) occurred typically along the vein margins, and the subsequent Au‐Te mineralization is characterized by fracture fillings of galena, sphalerite, pyrrhotite, Te‐bearing minerals (petzite, altaite, hessite and Bi‐Te mineral) and electrum. Fluid inclusions characteristically contain CO₂ and can be classified into four types (Ia, Ib, IIa and IIb) according to the phase behavior. The pressure corrected temperatures (≥500d?C) indicate that the deposit was formed at a distinctively high temperature from fluids with moderate to low salinity (<12 wt% equiv. NaCl) and CH₄ (1?22 mole %). The sphalerite geo‐barometry yield an estimated pressure about 3.5 ?2.1 kbar. The dominant ore‐deposition mechanisms were CO₂ effervescence and concomitant H₂S volatilization, which triggered sulfidation and gold mineralization. The measured and calculated isotopic compositions of fluids (δ¹⁸O_H2^O = 10.3 to 12.4 %o; δD_H2^O = ‐52 to ‐77 %o) may indicate that the gold deposition originated from S‐type magmatic waters. The physicochemical conditions observed in the Yuryang gold deposit indicate that the Jurassic gold deposits in the Cheonan area, including the Yuryang gold deposit are compatible with deposition of the intrusion‐related Au‐Te veins from deeply sourced fluids generated by the late Jurassic Daebo magmatism.  相似文献   

Genetic types of diamond mineralization   总被引：1，自引：0，他引：1  

A. A. Marakushev  Sang Longkang  You Zhendong  I. A. Zotov  N. N. Pertsev  N. A. Paneyakh 《中国地球化学学报》1998,17(1):12-28

The paper describes the proposed models of diamond formation both in meteorites and in kimberlite and lamproite bodies, metamorphic complexes and explosive-ring structures (“astroblemes”). The diamond distribution in meteorites (chondrites, iron meteorites and ureilites) is restricted to taenite-kamasite phase. The diamond generation here is tied up with the first stage of evolution of the planets. This stage is characterized by high pressure of hydrogen, leading to the formation of the planet envelope. The second stage of planet evolution began with the progressive impoverishment of their atmospheres in hydrogen due to its predominant emission into the space and to progressive development of oxidative conditions. The model appears to have proved the relict nature of diamond mineralization in meteorites. Diamond and other high-pressure minerals (its “satellites”) were crystallized without any exception in the early intratelluric stages of peridotite and eclogite-pyroxenite magma evolution just before the magma intrusion into the higher levels of the mantle and crust where diamond is not thermodynamically stable. The ultramafic intrusive bodies (bearing rich relict diamonds) in the base of a platform appear to be the substrata for the formation of kimberlite-lamproite magma chambers as a result of magmatic replacement. The model explains the polyfacial nature of diamondiferous eclogites, pyroxenites and peridotites and discusses the process of inheritance of their diamond mineralization by kimberlites and lamproites. Diamond productivity of metamorphic complexes is originated by the inheritance of their diamonds from the above-mentioned primary diamondiferous rocks. Large diamondiferous explosive-ring structures were formed by high-energy endogenic explosions of fluid which came from the Earth’s core. This high energy differs endogenic impactogenesis from explosive volcanism. It proceeds at very high temperature to create diaplectic glasses (monomineral pseudomorphs) —the product of isochoric melting, at the pressure high enough for the stable formation of very high-density minerals (coesite, stishovite, diamond, lonsdaleit, and chaoite). The research project was financially supported by the Russian Foundation of Fundamental Sciences (93-05-8566, 96-05-64307, and 96-05-00026c0) and China National Natural Science Foundation (No.49794041, No.49611121831).  相似文献   

恩施球粒陨石热历史及原始氩特征     

王松山  桑海清  裘冀 《地质论评》1997,43(3):303-309

H_s型恩施球粒陨石K-Ar年龄为4503±91Ma,~(40)Ar-~(39)Ar坪年龄为4518±8Ma,总气体年龄为4515±23Ma,等时线年龄为4505±16Ma,年龄的一致性表明该陨石未经受过明显的热扰动,它是我国首次发现的Ar保存年龄高达45亿年以上的陨石。陨石形成早期有过短期的快速冷却。陨石母体在4.66±0.04Ma时破裂。恩施球粒陨石原始捕获(~(40)Ar/~(36)Ar)_t为0.89±0.44,推测4.5Ga前太阳风中~(40)Ar/~(36)Ar近于l。  相似文献   

中国大陆与香港及周围地区的地震目录完全性分析     

陈龙生  陈棋福 《中国地震》1997,13(4):311-320

地震活动性中心Ｇｕｔｅｎｂｅｒｇ－Ｒｉｃｈｔｅｒ关系（ｌｏｇＮ＝ａ－ｂＭ）在确定地震发生率时起着重要作用，实际分析中存在的对Ｇ－Ｒ关系的偏离主要是由于地震目录的不完全性引起：即在低震级端因地震的监测能力有限，在高震级端因大震的稀少导致的统计涨落。  相似文献   

复杂地形上湍流扩散的数值模拟   总被引：2，自引：1，他引：2       下载免费PDF全文

桑建国 《气象学报》1988,46(2):219-226

本文采用准静力大气热力——动力学方程组和平流扩散方程的数值解方法,模拟了汾河河谷地区的流场、温度场和浓度场。所得结果和1984年春该地区进行的一次SF_6示踪试验资料做了对比。计算浓度场采用了三种方法:一般网格的数值模式、套网格数值模式和正态模式。和实测值的比较表明,套网格模式给出较好的计算结果,并且不需要增加过多的计算时间。  相似文献   

山西省代县高凡水系沉积物金异常及验证效果          下载免费PDF全文

桑华文 《地质找矿论丛》1988,(3):79-89

高凡Au异常受控于Nw向和NE向断裂构造交汇部位的特征,打破了前人局限于燕山期中酸性斑岩体内外接触带找Au—Ag矿的常规,为晋东北构造蚀变岩型Au—Ag矿的寻找提供了先例。另外,各种地球化学参数表明,高凡矿区Ag矿远景比Au矿更大。  相似文献   

迎风坡面上流场和温度场分布的分析解     

桑建国 《大气科学》1989,13(4):441-451

本文利用二层模式,分别得到低层大气稳定和不稳定时的大气波动方程表达式,并在特定的斜坡地形上,求出流线扰动的分析解。进一步讨论了不同上游大气条件下,地形造成的流场、温度场和湿度场分布,以及产生地形急流和地形云的判据。  相似文献