基于3D+-TPR-tree的点目标全时段移动索引设计

在经典3D R-tree基础上提出新的3D R-tree索引,通过改变待索引数据项的结构并重新设计查询处理算法,减少包容矩形死区,提高查询效率;为了满足全时段查询要求,设计一种称为3D -TPR-tree的联合索引结构,并对其中TPR-tree的参数包容矩形的调整算法进行优化。通过测试,证明3D R-tree的查询效率明显高于普通3D R-tree;此外,测试结果也表明经过优化的参数包容矩形的调整算法也部分提升了TPR-tree的查询性能。     

上海世博会地下变电站基坑围护结构的动力反应分析

采用三维快速拉格朗日程序FLAC^3D,对上海世博会500kV地下变电站围护结构的动力反应问题进行了深入细致的分析和研究。所建立的模型采用摩尔一库伦本构关系,同时考虑了静力、动力以及地下承压水的影响,并且通过FLAC^3D软件的二次开发功能引入统一强度理论,来判别围护结构中钢筋混凝土的应力状态,力求更真实地反映围护结构在动力作用下的响应状态。分析结果表明,圆型围护结构的环向刚度比较大,受力时将大部分侧向荷载转移给其环向拱结构,从而使得基坑和周围土体无论在静力状态还是动力状态下,整体变形均较小;基坑整体在所研究的各种工况下,围护结构都处于安全状态。     

九瑞矿集区重磁三维约束反演及深部找矿意义

研究九瑞矿集区成矿地层和岩体的三维分布特征可为区域成矿背景和成矿规律研究提供新的信息,实现研究区深部及外围找矿突破.本文首先综合分析研究区区域地质及地层和岩石密度和磁化率特征,然后将区域地质和12条地质剖面信息利用自行开发的GIF2UBCmodel程序构建剩余密度和磁化率参考模型和上下边界约束模型,实现了带约束重磁数据三维反演.反演结果揭示九瑞矿集区剩余密度和磁化率三维分布特征,解译了矿集区主要地层和岩体分布特征.该区存在邓家山—东雷湾以及武山—丁家山两个大型岩体;盖层褶皱与结晶基底隆起方向一致,是深部基地隆起的继承.通过与矿集区已知矿床对比发现,高磁性岩体边缘和基底隆起(高密度体)两翼为成矿有利区.     

Geochemistry constraints of Mesozoic–Cenozoic calc-alkaline magmatism in the South Shetland arc, Antarctica

Geochemical data from basalts, basaltic andesites, and andesites of the Mesozoic–Cenozoic (143–44 Ma) from Livingston, Greenwich, Robert, King George, and Ardley Islands of the South Shetland archipelago, Antarctica, are presented. The rocks have variable SiO₂ of approximately 46–61 wt%, Al₂O₃ of 15–26 wt%, and total alkali (K₂O+Na₂O) of 2–6 wt%. Most samples have low Mg#, Cr, and Ni, which indicates that they have undergone significant fractional crystallization from mantle-derived melts. The presence of olivine cumulatic in the samples from Livingston and Robert Islands explains some high MgO, Ni, and Cr values, whereas low Rb, Zr, and Nb values could be related to undifferentiated magmas. N-MORB-normalized trace element patterns show that South Shetland Islands volcanic rocks have a geochemical pattern similar to that found for other island arcs, with enrichment in LILE relative to HFSE and in LREE relative to HREE. The geochemistry pattern and presence of calcic plagioclase, orthopyroxene, Mg-olivine, and titanomagnetite phenocrysts suggest a source related to the subduction process. The geochemical data also suggest magma evolution from the tholeiitic to the calc-alkaline series; some samples show a transitional pattern. Samples from the South Shetland archipelago show moderate LREE/HREE ratios relative to N-MORB and OIB, depletion in Nb relative to Yb, and high Th/Yb ratios. These patterns probably reflect magma derived from a lithospheric mantle source previously modified by fluids and sediments from a subduction zone.

Resumo

Dados geoquímicos de basaltos, andesitos basálticos e andesitos mesozóicos–cenozóicos (143–44 Ma) das ilhas Livingston, Greenwich, Robert, King George e Ardley do Arquipélago Shetland do Sul, Antártica são discutidas neste artigo. As rochas tem conteúdos de SiO₂ variando de 46 a 61%, Al₂O₃ de 15 a 26% e álcalis (K₂O+Na₂O) de 2 a 6%. A maior parte das amostras tem conteúdos baixos de Mg#, Cr e Ni, indicando que sofreram significante cristalização fracionada de fusões derivadas do manto. A presença de fases cumuláticas nas amostras das ilhas Livingston e Robert explicaria os elevados valores de MgO, Ni, Cr, enquanto que baixos valores de Rb, Zr e Nb observados nas amostras destas ilhas poderiam estar relacionados a magmas não diferenciados. Os padrões de elementos-traço normalizados pelo N-MORB mostram que as rochas vulcânicas das Ilhas Shetland do Sul têm padrão geoquímico similar àqueles encontrados em outros arcos de ilhas com enriquecimento em LILE em relação aos HFSE e em ETRL em relação aos ETRP. O padrão geoquímico e a ocorrência de fenocristais de plagioclásio cálcico, ortopiroxênio, olivina magnesiana e titanomagnetita sugerem origem relacionada a processos de subducção. Dados geoquímicos obtidos para as amostras do arquipélago Shetland do Sul sugerem um magma evoluindo de toleítico para cálcico-alcalino, observando-se em algumas amostras um padrão transicional. As amostras do arquipélago Shetland do Sul mostram em relação ao N-MORB e OIB, moderadas razões ETRL/ETRP, empobrecimento em Nb relativo a Yb e elevada razão Th/Yb Estes padrões refletem, provavelmente, magma derivado de uma fonte mantélica litosférica, que foi modificada por fluídos e sedimentos da zona de subducção.     

Timings of early crustal activity in southern highlands of Mars:Periods of crustal stretching and shortening

Extensional and compressional structures are globally abundant on Mars. Distribution of these structures and their ages constrain the crustal stress state and tectonic evolution of the planet. Here in this paper, we report on our investigation over the distribution of the tectonic structures and timings of the associated stress fields from the Noachis-Sabaea region. Thereafter, we hypothesize possible origins in relation to the internal/external processes through detailed morphostructural mapping. In doing so, we have extracted the absolute model ages of these linear tectonic structures using crater size-frequency distribution measurements, buffered crater counting in particular. The estimated ages indicate that the tectonic structures are younger than the mega impacts events(especially Hellas) and instead they reveal two dominant phases of interior dynamics prevailing on the southern highlands, firstly the extensional phase terminating around3.8 Ga forming grabens and then compressional phase around 3.5-3.6 Ga producing wrinkle ridges and lobate scarps. These derived absolute model ages of the grabens exhibit the age ca. 100 Ma younger than the previously documented end of the global extensional phase. The following compressional activity corresponds to the peak of global contraction period in Early Hesperian. Therefore, we conclude that the planet wide heat loss mechanism, involving crustal stretching coupled with gravitationally driven relaxation(i.e.,lithospheric mobility) resulted in the extensional structures around Late Noachian(around 3.8 Ga). Lately cooling related global contraction generated compressional stress ensuing shortening of the upper crust of the southern highlands at the Early Hesperian period(around 3.5-3.6 Ga).     

台湾海峡西部沉积物中碳的来源及埋藏

根据2005年夏季航次观测的沉积物中总有机碳(TOC)、无机碳(CaCO3)、总氮(TN)、悬浮体颗粒有机碳(POC)、沉积物粒度数据得出,台湾海峡西部表层沉积物TOC质量分数的范围为0.01～1.79,平均值为0.37±0.24,略高于20多年前台湾海峡南部海区,而低于台湾海峡中、北部海区;TOC的质量分数湾内比湾外...     

新丰江库区上地壳三维细结构层析成像

在新丰江库区布设一个范围约50 km×40 km、由50个地震临时台站组成的观测台阵,接收来自不同方位的人工震源产生的莫霍界面反射波;台阵中的20个台站和5个区域固定台还对2009年3月至2010年5月发生在库区的地方震进行了观测.本文联合利用人工地震莫霍面反射波走时和天然地震直达波走时,采用连续模型反演技术重建了库区上地壳P波、S波慢度扰动和Vp/Vs扰动分布图像.研究结果表明:新丰江库区东、西部地区上地壳结构存在明显的差异.库区东部地区构造复杂,多条断裂在该区呈交叉状分布.北西向的石角—新港—白田断裂带在库区段内具有复杂的岩性和构造特征,该断裂带在新港至双塘一线可能延伸至地下8 km左右;近北东向的断裂带切割地壳较深.峡谷区及大坝以东附近地区存在上、下贯通的波速比高值区,尤其是大坝以西的深水峡谷区,存在一条顺河走向的陡倾角断层裂隙带,为库水渗透提供了良好通道.库区西部地区为相对稳定构造区,完整坚硬的花岗岩体透水性能较差,受库水渗透影响很小.新丰江水库诱发地震的形成与深部构造环境密切相关.峡谷区及大坝以东附近地区上地壳介质性质呈现明显的横向不均匀性,微震分布在介质物性结构的特定部位,"软"、"硬"交错的介质环境是倾滑正断层型微小震产生的可能原因.     

台湾中西部沉积盆地三维密度结构及其重力异常

台湾中西部沉积盆地是台湾省海陆油气勘探的重点区域。本文利用石油钻井资料和重力观测数据,依据Kriging插值及台湾中国石油公司深度-密度经验公式,计算了该地区沉积地层三维密度及剩余密度结构,并依据三维有限元解泊松方程方法,通过求解重力位计算出三维剩余密度体产生的剩余重力异常。密度结构显示,在0~6km深度范围,自更新统到先中新统的沉积地层大致分为2.0~2.30g/cm3、2.30~2.45g/cm3、2.45~2.60g/cm3、2.60~2.70g/cm3等4个密度层。其中,台中盆地陆缘区中下部2~4km深度存在较大沉积凹陷,凹陷区密度比周围低0.05~0.10g/cm3.重力计算结果表明,本区沉积地层产生的剩余重力异常在-20~+15mGal之间,深部凹陷对应负异常低值圈闭,其形态和量值与实测重力异常一致。      

The star-forming content of the W3 giant molecular cloud

We have surveyed a ∼0.9 square degree area of the W3 giant molecular cloud (GMC) and star-forming region in the 850-μm continuum, using the Submillimetre Common-User Bolometer Array on the James Clerk Maxwell Telescope. A complete sample of 316 dense clumps were detected with a mass range from around 13 to  2500 M_⊙  . Part of the W3 GMC is subject to an interaction with the H  ii region and fast stellar winds generated by the nearby W4 OB association. We find that the fraction of total gas mass in dense, 850-μm traced structures is significantly altered by this interaction, being around 5–13 per cent in the undisturbed cloud but ∼25–37 per cent in the feedback-affected region. The mass distribution in the detected clump sample depends somewhat on assumptions of dust temperature and is not a simple, single power law but contains significant structure at intermediate masses. This structure is likely to be due to crowding of sources near or below the spatial resolution of the observations. There is little evidence of any difference between the index of the high-mass end of the clump mass function in the compressed region and in the unaffected cloud. The consequences of these results are discussed in terms of current models of triggered star formation.