Shock metamorphism on the moon

Shock metamorphism of the lunar samples is discussed. All types of lunar glasses formed by various-size collision-type impact are found as impact glass, ropy glass and agglutinates. The agglutinates bonded by crystal and glassy materials contain hydrogen and helium from the solar wind components. Lunar shocked minerals of plagioclase and silica show anomalous compositions and densities. There are typical two formation processes on planetary materials formed by shock events; that is (1) shocked quartz formed by silica-rich target rocks (esp. on evolved planets of the Earth and Mars), and (2) shocked silica with minor Al contents formed from plagioclase-rich primordial crusts of the Moon. The both shocked silica grows to coarse-grain normal crystals after high-temperature metamorphism which cannot distinguish the original main formation event of impact process.     

星际分子正—NH3和He的超精细跃迁碰撞截面和速率系数的理论计算

本文采用Ｒ矩阵传播方法，通过求解ＣＳ近似下的耦合方程，计算了星际分子云条件下正－ＮＨ３分子和Ｈｅ碰撞的超精细跃迁碰撞截面和速率系数，为研究天体的信息提供需用的基础数据。     

An integrated linear/non-linear flow model for the conduit-fissure-pore media in the karst triple void aquifer system

Most karstic aquifer media may be characterized as the triple-void media with highly-varied hydraulic properties, including matrix pore, fissure and conduit, in which liner flow may co-exist with non-linear flow. In this paper, an attempt is made to couple linear flow with non-linear flow in a single unified flow governing equations by introducing the concept of equivalent hydraulic conductivity (EHC) and deriving a general Darcys law for various flow. The expression of EHC in the karst conduit and fissure are also derived. The procedures of numerical implementation are demonstrated via an ideal model and a case study of karst aquifer system in the Beishan Ore Formation area, Guangxi Autonomous Region, China.     

Binary collisions and the slingshot effect

We derive the equations for the gravity assist manoeuvre in the general 2D case without the constraints of circular planetary orbits or widely different masses as assumed by Broucke (AIAA/AAS 1988) and obtain the slingshot conditions and maximum energy gain for arbitrary mass ratios of two colliding rigid bodies. Using the geometric view developed in an earlier paper by the authors (Rica da Silva, A., Lemos, J.P.S.: Am. J. Phys. 74, 584–590, 2006) the possible trajectories are computed for both attractive or repulsive interactions yielding a further insight on the slingshot mechanics and its parametrization. . The general slingshot manoeuvre for arbitrary masses is explained as a particular case of the possible outcomes of attractive or repulsive binary collisions, and the correlation between asymptotic information and orbital parameters is obtained in general.     

论中国大陆复杂和混杂的碰撞带构造

中国大陆碰撞带是以结构复杂、形成过程复杂和物质成分趋于混杂为主要特征的。在构造特征上 ,表现为由构造岩片和混杂岩带所组成 ,形成扇状褶皱和对冲型逆掩断层。在剖面上常形成楔状(鳄鱼式 )构造 ,在平面上可构成嵌入构造 ,它们其实是两个板块在碰撞过程中互相挤压、缩短与穿插的、一个统一的三维共轭剪切断裂系统中的不同表现形式。绝大多数中国大陆碰撞带都不是一次形成的 ,而是经历了多期次、活动性质各不相同的、复杂的形成过程。为了进一步提高碰撞带的研究水平 ,应该把碰撞带及其两侧的板块当作一个整体来进行综合研究 ,应该大力加强碰撞带周邻板块的沉积古地理、生物古地理、古地磁学、地球化学和构造变形、变位资料的系统研究。碰撞作用时期是元素、岩石和构造单元趋于混杂的时期 ,而不是有利于元素、物质的分异和富集。碰撞带的主碰撞期形成的矿床是十分有限的。笔者推测有 4种类型的矿床可能将成为西部古碰撞带地区找矿的主要目标。     

华北新构造：印欧碰撞远场效应与太平洋俯冲地幔上涌之间的相互作用

作为大陆内部典型的伸展断陷区和强震活动区,华北地区处于东部太平洋板块俯冲构造和西部印欧大陆碰撞构造的双重大地构造背景之下,其新构造运动相当复杂:西部沿鄂尔多斯地块周缘两个地堑盆地系引张伸展断陷作用、中部太行山块体的局部断陷和整体隆升、东部华北平原区和渤海湾海域区的区域沉降,南缘沿秦岭构造带的左旋走滑拉张活动,东缘沿郯庐断裂带的右旋挤压走滑活动。这些不同类型的断裂构造在晚新生代的阶段性活动,产生了复杂的构造地貌组合特征。综合研究发现,华北晚新生代经历了3期伸展断陷-挤压隆升演化阶段:新近纪晚期(10～2.5 Ma)、早中更新世和晚更新世以来。地壳引张应力方向或NW-SE、或NE-SW向;地块隆升导致湖盆的消亡,挤压应力方向为NE-SW至W-E向。研究认为,华北地区新构造受两个岩石圈构造过程的相互影响:印欧碰撞产生的远程效应和东部岩石圈地幔的上涌。一方面,青藏高原东北缘地块的持续推挤及其构造应力向东的传递导致鄂尔多斯地块反时针旋转和秦岭山地的向东挤出逃逸,这个挤出构造动力学统治了华北地区晚新生代的引张伸展、斜张走滑和挤压变形。尤其是,新近纪晚期强烈的NW-SE向地壳伸展变形与青藏东缘挤出造山作用同步(10～9 Ma至4.2 Ma);上新世末期(约2.5 Ma)、晚更新世早期(约200～70 ka)和晚更新世晚期—全新世(约20 ka以来)3次构造挤压事件与青藏高原东缘构造事件基本对应。另一方面,岩石圈地幔上涌主导了华北东部平原区的区域地壳沉降,同时伴随着早、中更新世的5期幔源火山活动。这两个岩石圈构造作用力此消彼长,深刻统治着华北地区新构造与现今活动构造以及地震构造。     

塔里木地块上石炭统的古地磁研究

本文对塔里木地块西北缘柯坪地区的3条上石炭统康克林组剖面进行了古地磁研究。95个定向岩心样品的逐步热退磁和交变退磁揭示出3个磁性组分,第一个是具有低解阻温度谱或低矫顽力谱在现代地磁场作用下形成的粘滞剩磁A(D=10°;I=56°,α95=4°);第二个是红色石英砂岩的具有反极性的高温组分B(D=217°,I=-43°,λ=56°,Φ=184°E;A25=6°详细研究表明,该分量受附近晚二叠世脉岩侵入的重磁化;第三个是灰岩高矫顽力谱的反极性组分C（D=241°、I=-51°,λ=41°N,Φ=160°E,A（?）=4°）。这一分量通讨倾斜检验,在95%概率水平上明显不同于塔里木地块目前已有的石炭纪以后的古地磁方向,它代表了原生剩磁。研究结果表明:（1）晚石炭世塔里木地块已和哈萨克斯坦地块、苏联西天山地块以及西伯利亚地块发生碰撞:（2）苏联西天山地块相对塔里木地块曾逆时针旋转了70°（欧拉极位置λ=8°N,Φ=69°E）,而塔里木地块则相对西伯利亚地块逆时计旋转了21°（欧拉极位置λ=20°N,Φ=34°E）。从该区已有的晚古生代至早三叠世占地磁数据看,这些地块之间的相对旋转运动发生于早三叠世之后。     

Tectonic setting of the Azores Plateau deduced from a OBS survey

The studies of Azores seismicity generally show shocks with either normal faulting or right-lateral strike-slip along the ESE direction, compatible with a eastward relative motion of the Eurasian (EU) relative to the African (AF) plate. However, the 1 January 1980 earthquake was interpreted as a clear left-lateral strike-slip shock along the N150E direction. This pattern is difficult to explain in terms of the relative motion between the EU, AF and North American (NA) plates: all available models for the present day movement of this triple junction fail to explain the regional variability in the stress conditions of the area. Here we present data from a 34-day long Ocean Bottom Seismograph array deployment. We show that the seismicity is distributed along a band aligned with the island chain itself, and is concentrated along several faults with an approximate N150E strike, cutting the Azores plateau in all the area covered by the OBS network. The combination of these new results with other geophysical data permits us to conclude that the tectonic setting of the Azores plateau is characterised by the existence of two sets of faults, in the N120E and N150E directions, defining several crustal blocks, whose relative motion accommodates the interaction of the three megaplates. The deformation of these tectonic blocks is probably driven by the shear between the EU and AF plates. This model explains well the spatial variability of the stress conditions in the Azores domain, the combination of dextral and sinistral strike slip mechanisms and the observed seismotectonics of the Azores islands.     

Tectonic Evolution of the Lufilian Arc (Central Africa Copper Belt) During Neoproterozoic Pan African Orogenesis

The Lufilian arc of Central Africa (also called Katangan belt or Copperbelt) is a zone of low to highgrade metasedimentary (and subsidiary igneous) rocks of Neoproterozoic age hosting highgrade CuCoU and PbZn mineralizations. The Lufilian arc is located between the Congo and Kalahari cratons and defines a structure which is convex to the north. Three major phases of deformation characterize the construction of the Lufilian arc. The first phase (D1) called the “Kolwezian phase” developed folds and thrust sheets with a northward transport direction. D1 deformation occurred in the Lufilian arc between ca. 800 and 710 Ma, with a peak in the range 790–750 Ma. It is here correlated with the main deformation in the Zambezi belt. Southward-verging folds with the same trends as the D₁ structures were previously linked to a second tectonic event named Kundelunguian phase of the Lufilian orogeny. We show in this paper that they are backfolds developed during D1 along Katangan ramps and especially along the Kibaran foreland. The second phase (D2) of the Lufilian orogeny is the “Monwezi phase” including several large leftlateral strikeslip faults which have been activated successively. During this deformation phase, the eastern block of the belt rotated clockwise, giving the present day NWSE trend of D1 structures in this part of the Lufilian arc, and generating its convex geometry. The Mwembeshi dislocation, the major transcurrent shear zone separating the Zambezi and Lufilian arc, was mostly active during the D2 deformation phase. D2 deformation occurred between ca. 690 and 540 Ma. Such a long time interval is attributed to the migration of strikeslip faults developed sequentially from south to north, and probably to a slow convergence velocity during the collision between the Congo and Kalahari cratons. The third phase (D3) of the Lufilian orogeny is a late event called the “Chilatembo phase”, marked by structures transverse to the trends of the Lufilian arc. This deformation and the post-D_2′ uppermost Kundelungu sequence (Ks3 Plateaux Group), are younger than 540 Ma and probably early Paleozoic.