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121.
甘肃省地热资源丰富,其地热资源的开发利用具有较大的潜力。本文介绍了甘肃省地热资源分布概况,结合地区构造、地热水化学特征、地热资源量及开发利用现状探讨了甘肃隆起山地对流型与沉积盆地传导型地热资源的赋存特征,并对两种类型地热资源潜力进行了分析评价。结果表明,沉积盆地地热资源分布于河西、陇西及陇东盆地等,热储类型为裂隙型和孔隙型,热储层自元古宙至新生代均有发育,岩性以砂岩为主;隆起山地型地热资源主要分布于祁连山和西秦岭造山带,热储类型为断裂破碎带,岩性以花岗岩为主;通过潜力计算得知,全省热量开采系数≥0.4的仅占29.17%,表明目前甘肃地热资源开采程度较低,开采潜力较大。 相似文献
122.
2017年河套盆地临河坳陷油气勘探取得重要发现,基于区域中生代以来大地构造演化系统梳理,以钻井与地震对照、研究区与邻近盆地类比为研究方法,划分河套盆地临河坳陷南部吉兰泰凹陷中生代构造层,并绘制其分布范围,探讨其赋存特征与意义。结果表明:研究区中生界除三叠系外发育齐全,厚度巨大,且白垩系自上而下可细分为K1 I、K1 II和K1III三个构造层;除K1I构造层全区广覆式发育外,其它构造层呈楔状—缓楔状,长轴沿主控断裂NNE向延伸;研究区自中生代以来盆地性质经历了早中侏罗世断陷、早白垩世早期断陷、早白垩世中期断拗转换和早白垩世晚期拗陷的演化过程;F 3和F 7断层之间的K1 II和K1 III构造层、F 7断层东部的J构造层均具良好的油气勘探前景。 相似文献
123.
烃源岩中的有机酸来源于有机质,但有机质具有不同的赋存形式,有机酸具有不同性质,这将影响有机酸与不同赋存有机质的关系,进而影响分离和检测方法。文章在总结前人对有机质赋存形式和有机酸性质等特征的基础上,提出烃源岩中的有机酸并以非单一的形式存在,具有水溶性、脂溶性和难溶性有机酸三种类型,游离有机质中存在水溶性和脂溶性有机酸,而结合有机质中存在水溶性、脂溶性和难溶性有机酸。因此在检测方法上需采取分步分离的方法,且根据有机酸的性质选取合适的检测方法,即水溶性有机酸利用离子色谱检测,索氏抽提得到的脂溶性有机酸利用气相色谱—质谱检测,通过酸解抽提残渣得到的难溶性有机酸利用红外光谱检测,全面系统地认识烃源岩中有机酸含量和类型等特征。这对进一步探讨烃源岩各种类型有机酸特征和演化规律,深化烃源岩有机质生烃以及有机—无机相互作用等机理都具有重要意义。 相似文献
124.
This paper presents a copula technique to develop time-variant seismic fragility curves for corroded bridges at the system level and considers the realistic time-varying dependence among component seismic demands. Based on material deterioration mechanisms and incremental dynamic analysis, the time-evolving seismic demands of components were obtained in the form of marginal probability distributions. The time-varying dependences among bridge components were then captured with the best fitting copula function, which was selected from the commonly used copula classes by the empirical distribution based analysis method. The system time-variant fragility curves at different damage states were developed and the effects of time-varying dependences among components on the bridge system fragility were investigated. The results indicate the time-varying dependence among components significantly affects the time-variant fragility of the bridge system. The copula technique captures the nonlinear dependence among component seismic demands accurately and easily by separating the marginal distributions and the dependence among them. 相似文献
125.
Influence of lunar phases,winds and seasonality on the stranding of mesopelagic fish in the Strait of Messina (Central Mediterranean Sea) 下载免费PDF全文
Pietro Battaglia Giovanni Ammendolia Mauro Cavallaro Pierpaolo Consoli Valentina Esposito Danilo Malara Ignazio Rao Teresa Romeo Franco Andaloro 《Marine Ecology》2017,38(5)
The shore stranding of mesopelagic fauna is a recurrent phenomenon in the Strait of Messina (Central Mediterranean Sea). The aim of this paper is to test the influence of lunar phases, winds and seasons upon the frequency of occurrence of strandings of mesopelagic fish. Species abundance in relation to these factors was quantified for the first time. Specimens were collected stranded on the shore along the Sicilian coast of the Strait of Messina between 2008 and 2016. Overall 32 species belonging to seven families (Gonostomatidae, Microstomatidae, Myctophidae, Paralepididae, Phosichthyidae, Sternoptychidae, Stomiidae) were found stranded. Myctophidae was the family including the highest number of species (16), whereas Gonostomatidae was the most abundant in terms of total number of individuals (47.2%), mainly thanks to the species Cyclothone braueri. The moon, which influences the strength of currents (highest during full and new moon phases) and irradiance (higher in some lunar phases, such as the full moon), affected the abundance of stranded mesopelagic fish in the study area. The highest number of stranding events was recorded during the new moon: 34.6% of the total relative abundance of stranded mesopelagic fish. Wind blowing from the sea towards the coastline (southeasterly and easterly winds) created the best conditions for strandings. The highest abundance of stranded specimens was recorded during the winter season. 相似文献
126.
127.
A framework for the evaluation of ground motion selection and modification procedures 总被引:1,自引:0,他引:1 下载免费PDF全文
This study develops a framework to evaluate ground motion selection and modification (GMSM) procedures. The context is probabilistic seismic demand analysis, where response history analyses of a given structure, using ground motions determined by a GMSM procedure, are performed in order to estimate the seismic demand hazard curve (SDHC) for the structure at a given site. Currently, a GMSM procedure is evaluated in this context by comparing several resulting estimates of the SDHC, each derived from a different definition of the conditioning intensity measure (IM). Using a simple case study, we demonstrate that conclusions from such an approach are not always definitive; therefore, an alternative approach is desirable. In the alternative proposed herein, all estimates of the SDHC from GMSM procedures are compared against a benchmark SDHC, under a common set of ground motion information. This benchmark SDHC is determined by incorporating a prediction model for the seismic demand into the probabilistic seismic hazard analysis calculations. To develop an understanding of why one GMSM procedure may provide more accurate estimates of the SDHC than another procedure, we identify the role of ‘IM sufficiency’ in the relationship between (i) bias in the SDHC estimate and (ii) ‘hazard consistency’ of the corresponding ground motions obtained from a GMSM procedure. Finally, we provide examples of how misleading conclusions may potentially be obtained from erroneous implementations of the proposed framework. Copyright © 2014 John Wiley & Sons, Ltd. 相似文献
128.
Intensity measures for probabilistic assessment of non‐structural components acceleration demand 下载免费PDF全文
Marco De Biasio Stephane Grange Frederic Dufour Frederic Allain Ilie Petre‐Lazar 《地震工程与结构动力学》2015,44(13):2261-2280
A fundamental issue in the framework of seismic probabilistic risk analysis is the choice of ground motion intensity measures (IMs). Based on the floor response spectrum method, the present contribution focuses on the ability of IMs to predict non‐structural components (NSCs) horizontal acceleration demand. A large panel of IMs is examined and a new IM, namely equipment relative average spectral acceleration (E‐ASAR), is proposed for the purpose of NSCs acceleration demand prediction. The IMs efficiency and sufficiency comparisons are based on (i) the use of a large dataset of recorded earthquake ground motions; (ii) numerical analyses performed on three‐dimensional numerical models, representing actual structural wall and frame buildings; and (iii) systematic statistical analysis of the results. From the comparative study, the herein introduced E‐ASAR shows high efficiency with respect to the estimation of maximum floor response spectra ordinates. Such efficiency is particularly remarkable in the case of structural wall buildings. Besides, the sufficiency and the simple formulation allowing the use of existing ground motion prediction models make the E‐ASAR a promising IMs for seismic probabilistic risk assessment. Copyright © 2015 John Wiley & Sons, Ltd. 相似文献
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130.
基于CALIPSO星载激光雷达的中国沙尘气溶胶观测 总被引:2,自引:0,他引:2
基于2006年6月至2012年5月无云条件下CALIPSO星载激光雷达观测资料,分析中国典型地区(塔克拉玛干沙漠、柴达木盆地、戈壁区和华北)沙尘气溶胶分布。结果表明:塔克拉玛干沙漠和戈壁区为沙尘天气发生频率高值区,且前者在各高度层的沙尘发生频率都大于后者。沙尘发生呈季节性分布。塔克拉玛干沙漠在春季沙尘发生频率最大,抬升最高可至10 km,冬季频率最小,高度最低,主要分布在3 km以下。戈壁区在春季沙尘发生频率、抬升高度最大,冬季抬升高度最低,但低层发生频率大于夏、秋两季。在塔克拉玛干沙漠,沙尘光学厚度春季最大约为0.44,冬季最小约为0.17,春,冬季消光系数峰值最大,可达0.25 km-1,且随高度的递减率大于夏,秋季。在戈壁区和柴达木盆地,沙尘光学厚度春季最大、秋季最小。在华北,沙尘光学厚度春季最大、夏季最小,消光系数在2 km以上春季最大,这主要是由于春季远距离高空传输到华北的沙尘量最多。塔克拉玛干沙漠与柴达木盆地的退偏比为0.2~0.35,戈壁区为0.16~0.28,可能是由于塔克拉玛干沙漠的物质组成与柴达木盆地相同,而与戈壁区不同。华北因低层沙尘与其他气溶胶混合导致退偏振比廓线随高度递增。4个区域对流层上部退偏比全为0.2,表明高空气溶胶可能为来自相同源区的沙尘。 相似文献