Estimating economic losses of midrise reinforced concrete shear wall buildings in sedimentary basins by combining empirical and simulated seismic hazard characterizations     

Pouria Kourehpaz  Carlos Molina Hutt  Nasser A. Marafi  Jeffrey W. Berman  Marc O. Eberhard 《地震工程与结构动力学》2021,50(1):26-42

Studies of recorded ground motions and simulations have shown that deep sedimentary basins can greatly increase the intensity of earthquake ground motions within a period range of approximately 1–4 s, but the economic impacts of basin effects are uncertain. This paper estimates key economic indicators of seismic performance, expressed in terms of earthquake‐induced repair costs, using empirical and simulated seismic hazard characterizations that account for the effects of basins. The methodology used is general, but the estimates are made for a series of eight‐ to 24‐story residential reinforced concrete shear wall archetype buildings in Seattle, WA, whose design neglects basin effects. All buildings are designed to comply with code‐minimum requirements (i.e., reference archetypes), as well as a series of design enhancements, which include (a) increasing design forces, (b) decreasing drift limits, and (c) a combination of these strategies. As an additional reference point, a performance‐based design is also assessed. The performance of the archetype buildings is evaluated for the seismic hazard level in Seattle according to the 2018 National Seismic Hazard Model (2018 NSHM), which explicitly considers basin effects. Inclusion of basin effects results in an average threefold increase in annualized losses for all archetypes. Incorporating physics‐based ground motion simulations to represent the large‐magnitude Cascadia subduction interface earthquake contribution to the hazard results in a further increase of 22% relative to the 2018 NSHM. The most effective of the design strategies considered combines a 25% increase in strength with a reduction in drift limits to 1.5%.  相似文献   

Multiple sulfur isotope chemostratigraphy across the Permian–Triassic boundary at Chaotian,China: Implications for a shoaling model of toxic deep-waters     

Masafumi Saitoh  Yuichiro Ueno  Yukio Isozaki  Naohiro Yoshida 《Island Arc》2021,30(1):e12398

Previous studies on multiple sulfur isotopes (³²S, ³³S, and ³⁴S) in sedimentary pyrite at the end-Permian suggested a shoaling of anoxic/sulfidic deep-water contributing to the extinction. This scenario is based on an assumption that the sedimentary sulfur cycle was largely controlled by benthos activity, though a stratigraphic correlation between the sulfur records and ichnofabrics of the sediments at the end-Permian has not yet been examined. We report the multiple sulfur isotopic composition of pyrite in the Permian–Triassic boundary interval at Chaotian, South China. Our data can be generally explained by a mixing of sulfur in sulfide from two different sources: one produced via sulfate reduction in an open system with respect to sulfate and the other produced in a closed system. In particular, the former with the substantially low δ³⁴S (<−40 ‰) and high ∆³³S (up to +0.100 ‰) values was likely produced via water-mass sulfate reduction or via sulfate reduction in oxic sediments with common burrows. The frequent occurrence of small pyrite framboids (mostly <5 μm in diameter) in the Lopingian (Late Permian) Dalong Formation of deep-water facies supports the enhanced water-mass sulfate reduction in an anoxic deep-water mass. The negative ∆³³S values are observed only in the oxic limestones, and no substantial ∆³³S change is observed across the extinction horizon despite of the disappearance of bioturbation. Our results are apparently inconsistent with the previous shoaling model. We expand the model and infer that, when the deep-water was sulfidic and its shoaling rate was high, a substantial amount of hydrogen sulfide (H₂S) was supplied onto the shelf via the shoaling; that resulted in the positive ∆³³S value of the bulk sediments. The observed ∆³³S variation on a global scale suggests a substantial variation in H₂S concentration and/or in upwelling rate of shoaling deep-waters during the Permian–Triassic transition.  相似文献   

塔北、塔中地区碳酸盐岩及其原油中的二苯并噻吩类化合物   总被引：4，自引：0，他引：4  

李景贵  郑建京  刘文汇  陈国俊  孟自芳 《沉积学报》2004,22(2):348-353

塔里木盆地塔北、塔中地区四口井(库南1井,轮南46井,塔中12井和塔参1井)寒武-奥陶系12个碳酸盐岩烃源岩(泥灰岩,泥质灰岩和云岩)岩芯样品抽提物芳烃组分中的二苯并噻吩类化合物组成和丰度变化特征可分为三种类型:Ⅰ二苯并噻吩、甲基二苯并噻吩型;Ⅱ二苯并噻吩、甲基二苯并噻吩、二甲基二苯并噻吩+三甲基芴混合物型;Ⅲ二苯并噻吩、甲基二苯并噻吩、二甲基二苯并噻吩和三甲基二苯并噻吩型。研究的塔北、塔中隆起11个海相油二苯并噻吩类化合物分布类型均为二苯并噻吩、甲基二苯并噻吩、二甲基二苯并噻吩和三甲基二苯并噻吩型,和海相烃源岩二苯并噻吩类化合物第Ⅲ种分布类型完全相同。据此推断:塔北隆起8个海相油可能主要来源于塔北轮南地区下奥陶统;塔中隆起3个海相油可能来源于塔中地区中-上奥陶统。  相似文献   

混合热源与热泵联动空调技术及其在天津"975"工程中的应用   总被引：1，自引：1，他引：0  

何满潮  乾增珍  徐能雄 《吉林大学学报(地球科学版)》2004,34(2):247-250

混合热源与热泵联动空调技术以天然、廉价和低品位的资源为主,以高品位资源为尖峰负荷的系统能源配置设计新方法,实现以单投入多功能的新型能源利用方式替代多投入单功能传统的能源利用方式,使建筑物的空调系统具有经济、节能与环保等特点.该项技术能较好地应用于能源获取难度大、单一冷热源不能满足要求的工程.在天津"975"工程供暖及制冷系统中的应用结果表明:混合热源与热泵联动空调技术成功地解决了系统的冷热源、热(冷)负荷需求大等难题,具有明显的环境与经济效益.  相似文献   

Extragalactic X‐ray surveys: AGN physics and evolution     

A. Comastri  M. Brusa 《Astronomische Nachrichten》2008,329(2):122-126

We review the most important findings on AGN physics and cosmological evolution as obtained by extragalactic X‐ray surveys and associated multiwavelength observations. We briefly discuss the perspectives for future enterprises and in particular the scientific case for an extremely deep (2–3 Ms) XMM survey. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

The brightness of the galactic radio loops at 1420 MHz: Some indications for the existence of Loops V and VI     

V. Borka  J. Milogradov‐Turin  D. Uro&#x;evi&#x; 《Astronomische Nachrichten》2008,329(4):397-402

In this article we use 1420 MHz data to demonstrate the likely reality of Galactic radio Loops V and VI. We further estimate distances and spectral indices for both these and the four main radio loops. In the cases of Loops I–IV, radio spectral indices are calculated from the mean brightnesses at 1420 and 820/404 MHz. The spectral indices of Loops V and VI are obtained from T –T plots between 1420 and 408 MHz. Using the supernova remnant (SNR) hypothesis for the origin of radio loops, distances are calculated from the surface brightnesses and the angular diameters at 1420 MHz. We also study how results for brightnesses and distances of radio loops agree with current theories of SNR evolution. For this purpose, the ambient density and initial explosion energy of the loops are discussed. We also discuss applications of different Σ–D relations. The results obtained confirm a non‐thermal origin and nearby locations for the Galactic radio loops. Therefore, we have indications that they are very old SNRs that evolve in low ambient densities, with high initial explosion energies. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Suzaku observations of clusters of galaxies     

K. Matsushita  Suzaku SWG team 《Astronomische Nachrichten》2008,329(2):139-142

We review results of Suzaku observations of the intracluster medium of clusters of galaxies whose O, Mg, Si, S and Fe abundances have been measured with good accuracy due to the good energy resolution and low background. Metal massto‐light ratios were derived and we will discuss the origin of the metals. We also review the results of the search for bulk motion and hard X‐ray emission. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

X‐rays from young stars: A summary of highlights from the XMM‐Newton Extended Survey of the Taurus Molecular Cloud (XEST)     

M. Güdel 《Astronomische Nachrichten》2008,329(2):218-221

The XMM‐Newton Extended Survey of the Taurus Molecular Cloud (XEST) is a survey of the nearest large star‐forming region, the Taurus Molecular Cloud (TMC), making use of all instruments on board the XMM‐Newton X‐ray observatory. The survey, presently still growing, has provided unprecedented spectroscopic results from nearly every observed T Tauri star, and from ≈50% of the studied brown dwarfs and protostars. The survey includes the first coherent statistical sample of high‐resolution spectra of T Tauri stars, and is accompanied by an U ‐band/ultraviolet imaging photometric survey of the TMC. XEST led to the discovery of new, systematic X‐ray features not possible before with smaller samples, in particular the X‐ray soft excess in classical T Tauri stars and the Two‐Absorber X‐ray (TAX) spectra of jet‐driving T Tauri stars. This paper summarizes highlights from XEST and reviews the key role of this large project. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

鄂尔多斯盆地西南缘砂岩型铀矿赋矿地层及矿化特征   总被引：1，自引：0，他引：1  

段晓华  张君弟 《铀矿地质》2019,(2):88-94

通过对鄂尔多斯盆地西南缘泾源-华亭一带的地质调查和资料综合分析,笔者重点研究了该区砂岩型铀矿的成矿地质背景、含矿层及铀矿化的基本特征,认为下白垩统六盘山群是区内的主要赋矿层位,可分为上、下两个含矿层;铀矿化与有机质、黄铁矿、黄铜矿等含量关系密切,铀以沥青铀矿或残余铀黑、硅钙铀矿、钙(铜)铀云母等矿物形式为主,部分呈分散吸附状,与Cu、 Pb、 Mn、V、 Ni、 Co等呈正相关关系。这些特征显示,研究区具有较好的砂岩型铀矿找矿前景,值得进一步开展工作。  相似文献   

塔里木盆地塔中北坡奥陶系微生物碳酸盐岩储层形成机制与评价          下载免费PDF全文

王玉伟  陈红汉  曹自成  云露 《地球科学》2019,44(2):559-571

微生物岩储层是当前的研究热点之一.通过对塔中北坡微生物岩样品的岩芯以及铸体薄片的观察,发现研究区域的微生物岩储层以裂缝-孔隙型储层为主.对其进行全直径孔渗性检测发现,微生物岩储层具有较好的天然气储集物性.通过对微生物岩的形成机制及特点的分析,结合应力敏感实验和成像测井资料,总结出微生物岩储集空间发育的优势因素.原生白云石的生成可以促进方解石的溶解,而塔中北坡微生物岩发生早成岩岩溶作用,部分地区叠加晚期深成热液改造,提高了储集物性;有机质含量较丰富不仅可以在埋藏成岩阶段生成有机酸造成溶蚀,还能够降低微生物岩的极限强度从而容易在构造作用下发生断裂形成裂缝,因此塔中北坡微生物岩储集空间主要以次生作用为主.通过岩石压缩系数的测定,得出微生物岩的抗压实能力一般,但藻屑骨架对藻孔的保护有利,抗压实能力最强的是受到热液作用而硅化的微生物岩,其次是白云石化微生物岩.  相似文献