共查询到20条相似文献，搜索用时 46 毫秒
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元素硒早在1817年就被发现,但因产出稀少,数百年来只有几篇章报导了自然硒矿物。易爽庭等手1988年在新疆伊犁雅马渡地区发现了自然硒矿物,其产出环境是低变质烟煤中含硒黄铁矿于封闭缺氧条件下,在煤自燃过程中形成硒蒸汽经冷凝结晶而成。这是我国首次发现自然硒矿物。 相似文献
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1932—1937年间在周口店中国猿人产地及其他地点采得八十馀件节足动物化石,多破碎,完整者极少。颜色不一,由乳白而棕黄,兼有呈半透明玻璃状者。经初步观察,应属节足动物门,多足纲,倍脚目,马陆科,计一属两种: 一、山马陆(Julus of.terrestris)此种在第一,三,十五地点及山顶洞均有发现。此与现生的山马陆无甚差异,仅肛板及由二肛板所成之肛门沟稍大。二、裴氏小马陆(Julus peii Chia & Liu(sp.nov.)此种於第一,四,十五地点及山顶洞均有发现。由身体及头部形态,身体环节数目(三十个以上),知其与山马陆同属。但其决非幼小山马陆,因其体节数目多於长成之山马陆。但与现生於日本的一种 Nipponoiulus truncatus 近似,惟後者体节数较少,尾端钝圆。关於马陆属化石,据现在所知最早发现於始新统地层中,直到现在仍有生存,变异极小。以上所述二种若非与其他脊椎动物化石共生於周口店地点,则其年代颇难鉴定,因其有以後爬入岩隙死後石化之可能,不过上述之标本不但有共生脊椎动物为证,且有的已埋藏於固结的砾岩中,其属於更新统时期可无疑义。 相似文献
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1932—1937年间在周口店中国猿人产地及其他地点采得八十馀件节足动物化石,多破碎,完整者极少。颜色不一,由乳白而棕黄,兼有呈半透明玻璃状者。经初步观察,应属节足动物门,多足纲,倍脚目,马陆科,计一属两种: 一、山马陆(Julus of.terrestris)此种在第一,三,十五地点及山顶洞均有发现。此与现生的山马陆无甚差异,仅肛板及由二肛板所成之肛门沟稍大。二、裴氏小马陆(Julus peii Chia & Liu(sp.nov.)此种於第一,四,十五地点及山顶洞均有发现。由身体及头部形态,身体环节数目(三十个以上),知其与山马陆同属。但其决非幼小山马陆,因其体节数目多於长成之山马陆。但与现生於日本的一种 Nipponoiulus truncatus 近似,惟後者体节数较少,尾端钝圆。关於马陆属化石,据现在所知最早发现於始新统地层中,直到现在仍有生存,变异极小。以上所述二种若非与其他脊椎动物化石共生於周口店地点,则其年代颇难鉴定,因其有以後爬入岩隙死後石化之可能,不过上述之标本不但有共生脊椎动物为证,且有的已埋藏於固结的砾岩中,其属於更新统时期可无疑义。 相似文献
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本文通过系统对比分析前人研究成果,研究了南海边缘海多金属结核的成矿特征,结果表明：南海边缘海结核的矿物组成与大洋结核相似,均主要由锰相矿物和铁相矿物组成,其中锰相矿物主要为水羟锰矿和钡镁锰矿,铁相矿物主要以无定型铁氧化/氢氧化物形式存在,另外南海边缘海结核中含有大量硅酸盐矿物,表明在南海结核成矿过程中受到大量的陆源碎屑矿物混杂;相对于大洋主要经济成矿区的多金属结核,南海边缘海多金属结核中主要的经济元素如Mn、Cu、Co、Ni和Zn质量分数较低,而亲陆源性元素如Fe、Ti、P、Nb、Pb、Rb、Sc、Ta、Sr、Th和REY（REE和Y）等质量分数较高;南海边缘海多金属结核的元素地球化学特征和REE配分模式显示其为水成成因,并呈现更低的Mn/Fe值;同时南海边缘海结核也具有较快的平均生长速率及较高的δCe正异常,表明其生长在更为氧化的海水环境。虽然较快的沉积物沉积速率和动荡的海水环境影响了南海边缘海结核的成矿,但大量陆源物质进入海洋也为南海边缘海结核提供了丰富的成矿物质来源,便于南海边缘海结核的快速生长成矿。南海边缘海结核富集有Fe、Ti、Pb、Rb、Th和REY等金属元素,同样可以作为极具潜力的海洋矿产资源。南海边缘海多金属结核具有其独特的地球化学特征,与大洋多金属结核存在着明显差异。 相似文献
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路基下岩溶稳定性评价的模糊多层次多属性决策方法研究 总被引：1，自引：0，他引：1
影响高速公路路基下岩溶稳定性的因素很多,影响程度各不相同且包含各种模糊信息。基于实际工程资料,综合运用层次分析方法和模糊多属性决策方法,建立路基下岩溶顶板稳定性评价的模糊多层次多属性决策模型;采用Laagoven和Buckley关于层次分析方法中权重比矩阵元素模糊化的建议,推导出权重比矩阵元素为三角模糊数的模糊权值向量计算公式,再按照模糊平均加权方法（F-SAW）得到每个评语的模糊效应值;最后以此结果进行模糊集排序,得到岩溶顶板稳定性的评语。实际工程的应用结果表明了方法的可行性和有效性,为岩溶区路基稳定性评价提供了新的思路和方法。 相似文献
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We have modeled the dynamical evolution of small groups of N=3–18 stars in the framework of the gravitational N-body problem, taking into account possible coalescences of stars and the ejection of single and binary stars from the system. The distribution of states is analyzed for a time equal to 300 initial crossing times of the system. The parameters of the binaries and stable triple systems formed, as well as those of ejected single stars, are studied. In most cases, the evolution of the group results in the formation of a binary or stable triple system. The orbital eccentricities of the binaries formed are distributed according to the law f(e)=2e. As a rule, stable triple systems display pronounced hierarchy (the mean ratio of the semimajor axes of the outer and inner binaries is about 20:1). Stars are ejected with velocities from several km/s to several tens of km/s. The results of the modeling are compared with the parameters of observed wide binaries and triple systems. 相似文献
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Yu. A. Orlov 《Doklady Earth Sciences》2008,418(1):184-186
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A technique is developed for the analysis of multiple underream anchor systems resting in an elastic soil. This technique may be used to consider anchor systems involving arbitrary anchor inclination and depth beneath the soil surface, as well as arbitrary number, shape, size and spacing of underreams. The approach is largely analytical in nature and involves only a fraction of the computation required for a finite element analysis. Consideration is given to the effects of anchor depth and inclination to the soil surface, and the spacing and number of underreams upon the elastic response of anchor systems. On the basis of the result from this study, a simple, approximate method for estimating the response of multiple underream anchors is proposed. This approach involves the use of several interaction charts, which are presented in the paper, and can be used as a hand method for estimating the load–displacement behaviour of quite general anchor systems to sufficient accuracy for most practical purposes. The use of the approximate approach is illustrated by an example. 相似文献
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The chamber geometry is one of the key factors that influences the performance of a cone crusher. The design of the chamber geometry should take product quality and crushing efficiency into account. In this paper the kinematics of rock material in a crushing chamber, as interparticle breakage occurs, has been analyzed and the chamber division is achieved. Based on the chamber division and a population balance model, the method for chamber geometry design is presented. Combining the empirical model for predicting particle shape with the size distribution model, a flakiness prediction model is proposed. With the size reduction model and flakiness prediction model as constraints, an optimization of the crushing chamber is achieved. Finally, the validity of the crushing chamber optimization model has been verified by an appropriate prototype test. 相似文献
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Paul F. McCombie 《Computers and Geotechnics》2009,36(1-2):332-341
A method of slope stability analysis based upon multiple wedges is developed, accounting for kinematics in a similar way to proposals by [Srbulov M. On the influence of soil strength brittleness and nonlinearity on slope stability. Comput Geotech 1997;20(1):95--104] and [Donald IB, Chen Z. Modern wedge methods of slope analysis – their power and their versatility. In: Second international conference on landslides, slope stability & the safety of infra-structures; 1999. p. 13–24]. Instead of relying on almost arbitrary assumptions about stresses on wedge or slice boundaries to demonstrate an equilibrium of both forces and moments, the method works from simple assumptions about the kinematics of movement, increasing displacements and hence resisting forces iteratively until force equilibrium is attained. The procedure is simple and efficient, and ensures that inter-wedge forces developed by the movement are consistent with the shape of the sliding surface. 相似文献
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Simulation of interactions among multiple debris flows 总被引：3，自引：2，他引：1
Adjacent debris flows may interact in many ways: two or more concurrent debris flows may merge; one debris flow can run out over an existing debris flow fan. Such interactions may cause debris flow properties to change in the mixing process as well as more severe adverse effects than those caused by a single debris flow. This paper aims to investigate the interactions among channelized debris flows originated from adjacent catchments. Both concurrent and successive debris flows are considered. If several debris flows originate from different locations concurrently and merge, the volumetric sediment concentration (i.e., the ratio of the volume of solid material to the total volume of debris flow), C v, is a good index to capture the mixing process of these debris flows. The change in C v reflects where mixing occurs and the mixing degree. The debris flow properties (e.g., yield stress and dynamic viscosity) evolve in the mixing process and can be captured by the change in C v. The debris flow with a larger volume dominates the mixing process, and the properties of the mixed debris flow are more similar to those of the larger debris flow. The inundated areas and runout distances of successive debris flows are smaller than those of concurrent debris flows of the same total volume due to the smaller scales of the individual events and blockage by the earlier debris flows. However, the deposit depth in the interacting part of the debris flow fans of successive debris flows can be much larger than that of concurrent debris flows, leading to more destructive cascading hazards (e.g., the formation of debris barrier lakes). The sequence of successive debris flows not only significantly influences the runout characteristics of the debris flows but also substantially affects the cascading hazards. 相似文献
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Giulio Ottonello 《Physics and Chemistry of Minerals》1986,13(2):79-90
A thermodynamic model for multiple oxides with spinel structure based on the atomistic approach (lattice energy, enthalpy, bulk modulus) and semiempirical estimates (heat capacity functions, entropy, thermal expansion) is presented. The model fits the experimental high temperature free energy values of the reference compounds, with a mean absolute error of 0.65 percent (19 values). The standard state stable configuration of most reference compounds is shown to be achieved at a local minimum in the free energy vs. degree of inversion function. This is interpreted as evidence of internal consistency of the model. 相似文献