异地异构天文数据资源的统一访问

天文观测数据资源具有时间跨度大,数据量大,存储、管理分散,管理工具驳杂等特点.如何提供给天文学家一个统一访问这些异地存放的异构数据资源的方案,是虚拟天文台的一个重要研究课题.本文提出了一种基于网格的解决方案.我们基于OGSA-DAI技术实现了对天文星表数据,图像数据和光谱数据的封装(DataNode).我们设计的虚拟天文台数据访问服务(VO-DAS)实现了对DataNode的自动资源发现以及异地异构数据库的联合访问.这将使天体的多波段交叉证认成为可能.VO-DAS支持国际虚拟天文台联盟(IVOA)的各项相关标准,使得它具有良好的互操作性.它的对外接口简单实用,可以针对不同需求的天文数据用户发展出多种网格应用产品.通过在两个科学范例中应用VO-DAS服务,证明了它的可行性.     

新疆塔里木河下游断流河道输水对地下水变化的影响分析

结合2000～2002年以来塔里木河下游间歇性输水后地下水变化的监测数据．用回归分析的方法对输水后地下水位动态响应变化过程进行分析,揭示输水量与地下水的响应范围之间的关系。结果表明：在横向上．随着向塔河生态输水次数和输水量的增加．地下水的响应范围逐渐扩大．但随远离输水河槽中轴线,响应程度减小．地下水位的抬升幅度减弱;纵向上,输水河段上游区段地下水位响应范围最大,中游区段次之,下游区段较小。在第二次输水过程中,靠近河岸地下水位出现急剧上升,而在第三次输水过程中,地下水的响应范围则有巨幅增加．输水量与输水持续时间与地下水位变化有着密切关系。     

Ejecta from impacts at 0.2-2.3 m/s in low gravity

Collisions between planetary ring particles and in some protoplanetary disk environments occur at speeds below 10 m/s. The particles involved in these low-velocity collisions have negligible gravity and may be made of or coated with smaller dust grains and aggregates. We undertook microgravity impact experiments to better understand the dissipation of energy and production of ejecta in these collisions. Here we report the results of impact experiments of solid projectiles into beds of granular material at impact velocities from 0.2 to 2.3 m/s performed under near-weightless conditions on the NASA KC-135 Weightless Wonder V. Impactors of various densities and radii of 1 and 2 cm were launched into targets of quartz sand, JSC-1 lunar regolith simulant, and JSC-Mars-1 martian regolith simulant. Most impacts were at normal or near-normal incidence angles, though some impacts were at oblique angles. Oblique impacts led to much higher ejection velocities and ejecta masses than normal impacts. For normal incidence impacts, characteristic ejecta velocities increase with impactor kinetic energy, KE, as approximately KE^0.5. Ejecta masses could not be measured accurately due to the nature of the experiment, but qualitatively also increased with impactor kinetic energy. Some experiments were near the threshold velocity of 0.2 m/s identified in previous microgravity impact experiments as the minimum velocity needed to produce ejecta [Colwell, J.E., 2003. Icarus 164, 188-196], and the experimental scatter is large at these low speeds in the airplane experiment. A more precise exploration of the transition from low-ejecta-mass impacts to high-ejecta-mass impacts requires a longer and smoother period of reduced gravity. Coefficient of restitution measurements are not possible due to the varying acceleration of the airplane throughout the experiment.     

东秦岭造山带"两阶段双带"区域成矿模式

东秦岭造山带总体上可划分为中元古代-古生代主要与裂谷、坳陷槽有关的海盆同生沉积成矿以及中生代与大规模陆内俯冲造山体制有关的后生热液成矿两大阶段,且中生代所形成的浅成和中深成两类热液矿床在横向上分带并呈相邻平行展布,成对共生,构成双成矿带,其形成机制是扬子地块及华北地块分别往秦岭发生陆内俯冲,使与挤压、转换挤压-变质变形、深成侵入-深源流体成矿系统有关的中深成热液型矿床形成于仰冲板片前缘的推覆-隆升带中;而使与伸展-高地热场(火山、浅成侵入)-地热流体成矿系统有关的浅成热液型矿床形成于推覆-隆升带后侧的同碰撞伸展带中.     

松辽盆地西部斜坡带油气运移示踪分析

利用天然气有机地球化学、油田水化学、原油中的有机物质及原油含氮化合物等油气运移示踪标志对松辽盆地西部斜坡带的油气运移路径进行了示踪分析,结果显示油气运移的主输导通道沿齐家古龙凹陷—新店—白音诺勒方向展布,之后分为两支,其一继续向西部的平洋方向运移,其二穿过阿拉新向北部的富拉尔基方向运移,而油气从齐家古龙凹陷穿过敖古拉—他拉哈断层直接向西部斜坡带的运移是非常局限的。该主输导通道同该区已发现的油气资源的匹配较完美。重点讨论了原油含氮化合物分析结果与其它示踪标志分析结果的差异及其产生的可能原因,指出对油气运移路径的分析应综合利用多种有机地球化学指标,而不应该过分依赖某一种或某两种示踪方法。     

城市生态安全水平的物元评判模型研究

作为人口高度集聚的人工生态系统,城市生态系统的安全性更加具有脆弱性。该文选取了若干公认的反映城市生态安全水平指标,建立了类型识别的物元评判模型。应用于我国十大城市,得出以下结论:处于"较安全"的城市有南京市、深圳市、大连市;处于"临界安全"的城市有上海市、广州市、南昌市、合肥市;处于"不安全"的城市有天津市、武汉市。评价结果基本与实地相符,说明建立的物元评判模型是可行的。     

地表的分形测量及其大地构造学意义

以湖北红安地区为例,采用投影覆盖法(projectivecoveringmethod)对地表进行了二维分形测量,结果表明,地表面积具有双分形(bifractal)关系,即具有小尺度的结构分形(texturalfractal)和大尺度的构造分形(structuralfractal),分叉点(breakpoint)的尺度为3610m,分维值都在2～3之间且结构分维值大于其构造分维值。可见,地表形态具有分形性质,分维值可以指示地表形态的复杂程度。构造分维值可作为构造活动强度的一个指标,可为大地构造单元的划分提供定量依据。复杂地表形态主要是由构造活动(内营力作用)和各种复杂表生地质作用(外营力作用)引起的,前者主要控制大尺度的地形起伏,后者则塑造小尺度的地表形态。地表分维值可以指示地表的发育成熟度,该地区小尺度的结构分维值大于大尺度的构造分维值表明其处于地表形态的发育晚期。此外,地表的分形尺度可以来用确定构造活动尺度,从而指导构造地质与找矿勘探研究。     

A Simple Monte Carlo Method for Locating the Three-dimensional Critical Slip Surface of a Slope

Based on the assumption of the plain-strain problem, various optimization or random search methods have been developed for locating the critical slip surfaces in slope-stability analysis, but none of such methods is applicable to the 3D case. In this paper, a simple Monte Carlo random simulation method is proposed to identify the 3D critical slip surface. Assuming the initial slip to be the lower part of a slip ellipsoid, the 3D critical slip surface is located by means of a minimized 3D safety factor. A column-based 3D slope stability analysis model is used to calculate this factor. In this study, some practical cases of known minimum safety factors and critical slip surfaces in 2D analysis are extended to 3D slope problems to locate the critical slip surfaces. Compared with the 2D result, the resulting 3D critical slip surface has no apparent difference in terms of only cross section, but the associated 3D safety factor is definitely higher.     

云南金满、水泄铜多金属矿床的Ar-Ar同位素年代学及其地质意义

滇西北兰坪中新生代盆地西缘铜多金属成矿带受澜沧江断裂带控制,赋矿围岩为二叠系至第三系,主要由下二叠统经上三叠统到上侏罗统砂岩、粉砂岩和页岩组成的碎屑岩建造、火山岩建造及含盐红色碎屑岩建造,矿体主要以脉状或透镜状产出。对该成矿带上的金满铜矿床和水泄铜(钴)矿床主成矿阶段的石英进行了^40Ar-^39Ar快中子活化法同位素地质年龄测定,获得坪年龄分别为56．7±1．0Ma和59．2±0．8Ma,且各自与对应的等时年龄在误差范围内完全一致,都可以代表矿石的形成年龄。综合已发表的有关兰坪盆地西缘及盆地内部铜、多金属矿床成岩成矿同位素年代学研究结果,表明两矿床与区域矿床具有一致的成矿时代,反映区域铜、多金属矿床均形成于喜马拉雅造山运动早期统一的地球动力学背景之下。     

Description and recognition of potassic-richterite,an amphibole supergroup mineral from the Pajsberg ore field,Värmland,Sweden

Mineralogy and Petrology - Potassic-richterite, ideally AKB(NaCa)CMg5TSi8O22W(OH)2, is recognized as a valid member of the amphibole supergroup (IMA-CNMNC 2017–102). Type material is from the...