1543—2001年北疆区域年降水量变化特征分析

征,同时200 a左右的周期变化特征也较为明显,且不同历史时期的周期变化特征存在明显差异.突变检验表明,均值突变尺度在50～100 a尺度上更为明显,公元1613-1643年,1731-1792年的突变表现为年降水量的增加,而公元1669-1712年的突变则表现为年降水量的减少;方差突变则以18世纪80年代最为明显.     

孔隙水压力静力触探动态贯入过程的有限元模拟

孔隙水压力静力触探作为一种新型的土体勘测技术已被广泛应用,但是,其机理的研究尚存在很大的不足。笔者系统分析了孔压触探的贯入特征,提出了“孔隙水压力体积基准值”的概念,借此推导出用土体体积变形量计算超孔隙水压力的公式。在此基础上,用轴对称有限单元法模拟探头的动态贯入过程,揭示应力－应变的变化特征,寻找超孔隙水压力生成与消散的规律,对孔压触探的机理进行了研究。     

采用土工合成材料的新型护岸结构的动态数值模拟

固化土和土工格栅护岸工法（SG-WALL工法）是一种采用固化土和土工格栅加固港口护岸结构的新型工法。它的抗震性能已经通过一系列振动台试验得到了确认。为了能够数值再现SG-WALL结构在地震荷载作用下的动力反应,对SG-WALL结构的振动台试验进行了动态数值模拟研究。试验和模拟结果的对比表明,数值模拟方法能够再现SG-WALL结构在振动荷载作用下的主要动力特征。模拟结果还表明：固化土的长度对SG-WALL抗震性能起到重要的影响;土工格栅的最大拉应变发生在与排桩的连接处,并且沿着远离排桩的方向逐渐减小。     

综合物探技术在煤系上覆薄硬岩矿区的应用初探——以山西潞安集团司马矿区为例

山西潞安集团司马矿区东高西低,西部延至长治盆地,矿区水系发育。主采3#煤层埋藏较浅,层位稳定。新生界不整合于下伏基岩之上,厚度变化较大,属典型的薄硬岩煤矿区。为准确提供矿区煤炭开采上限的地质依据,采用了综合勘探技术,其中利用三维地震勘探技术追踪新生界底面反射波及第四系"天窗"位置,利用直流电法与瞬变电磁法提供电性分层,并对其解释结果进行相互印证。勘探实例表明,三维地震勘探、电法勘探与钻探的综合运用不仅可解决薄硬岩煤矿区新生界厚度、含水层富水性及第四系缺失等问题,还可提供新生界含水层与基岩含水层之间的水力联系、制约因素等资料。     

Origin of the Neoproterozoic Baijianshan Banded Iron Formation at the Southeastern Margin of the Tarim Block in NW China: Implication for an Extremely Reducing Ocean

The Neoproterozoic banded iron formations(BIFs)were closely associated with the“Snowball Earth”during the breakup of the Rodinia,thus they played an important role in our understanding of the atmospheric and oceanic oxygen levels during this period.In this contribution,the Neoproterozoic(ca.737 Ma)Baijianshan BIF at Southeast Tarim,northwestern China was identified.Magnetite is the dominated iron-species,which occurs as the lamina interbedded with chert.The BIF contains low concentrations of trace elements,and is depleted in light rare earth elements(LREEs)based on comparison with the Post-Archean Australian Shale(PAAS).In addition,the BIF exhibits slightly positive La-Eu anomalies,negligible Ce anomalies,insignificant Y anomalies,chondritic Y/Ho ratios(23-32),and slightly chondritic initial ε_Nd(t=737 Ma)values(?0.45 to 1.46,averaging 0.37).All these features indicate that the precipitation of Baijianshan BIF was closely related to the submarine low-T hydrothermal fluids with little detrital contribution.Moreover,the Baijianshan BIF is characterized by the significant enrichment of heavy Fe isotopes,with δ⁵⁷Fe_IRMM-014 values ranging from 1.78‰ to 3.05‰,revealing the partial oxidation of Fe²⁺ into Fe³⁺ during the precipitation of this BIF.Our data suggest that the formation of Baijianshan BIF was closely associated with a significantly reducing ocean,which most likely was isolated from the oxidized atmosphere by a local ice sheet.This Neoproterozoic Baijianshan ocean has the initial oxygen levels as low as,or even lower than that of Archean and Paleoproterozoic oceans.     

内蒙古中部二叠纪碱性花岗岩及其地球动力学意义

西伯利亚板块南缘白音乌拉－东乌珠穆沁旗带的碱性花岗岩（Ｒｂ－Ｓｒ年龄２７６－２８６Ｍａ）生成于张性的构造环境，较西伯亚板块同中朝板块之间晚泥盆世－早石炭世的碰撞事件晚约６０Ｍａ，属于造山后的Ａ型花岗岩，可作为造山作用结束的标志。但在中朝板块北缘晚石炭世－二叠纪只发育钙碱性的晚造山花岗岩，直到三叠纪才出现碱性正长岩。相邻两大板块边缘之间岩浆活动的非对称性可能是受板块间面积和质量差别的制约。     

柴达木盆地东北缘中中新世以来古气候变化

全球变冷、青藏高原隆升以及特提斯洋海退被认为是控制亚洲大陆新生代气候变化的三大因素,然而由于长时间尺度古气候记录的匮乏,对于三者影响的认识并不清晰。柴达木盆地是青藏高原北部最大的一个封闭盆地,发育巨厚且连续的新生代地层,详细记录了周缘山体构造隆升过程和区域气候演化历史。本文通过柴达木盆地东北缘怀头他拉剖面的中中新世-早更新世沉积物气候代用指标碳酸盐、硫酸根和氯离子含量分析,显示该研究区中中新世以来气候变化经历了15.3~13.0Ma相对湿润、13.0~6.6Ma半干旱-半湿润和6.6~1.8Ma干旱的3个演化阶段。结合生物特征和前人研究成果,认为柴达木盆地干旱化历史可能从中中新世13Ma左右开始逐步发展,而真正意义上的干旱化始于6.6Ma以来。全球变冷是控制柴达木盆地干旱气候形成和发展的主导因素,同时青藏高原晚期持续阶段性的强烈隆升起到了催化剂的作用。     

Data‐driven taxonomy matching of asteroid and meteorite

The matching of asteroids and meteorites is a significant step toward a better understanding of the origin, structure, and history of the solar system. We propose a data‐driven approach for investigating common taxonomic structure between asteroids and meteorites; C‐, S‐, and V‐type for the former, and carbonaceous chondrite, ordinary chondrite, and howardite‐eucrite‐diogenite (HED) meteorite for the latter. In the numerical experiments, by checking whether the taxonomy information of meteorites improves classification for asteroid data, we examine the existence of common structure over the two domains. For this purpose, we compare the resultant accuracies of two clustering methods which are with/without the guidance of meteorite data. We observe that the guidance of meteorite taxonomy improves the accuracy for classifying asteroids, either with the reflectance spectra or major chemical compositions of meteorites. This fact serves as a piece of evidence that there is a common taxonomic structure and links between meteorites and asteroids, supporting a long‐standing hypothesis.