Tectono-magmatic evolution from accretion to collision in the southern margin of the Central Asian Orogenic BeltSCIEI北大核心CSCD

造山带演化及增生到碰撞的转变是板块构造与大陆动力学研究中的前沿科学问题。中亚造山带被认为是古亚洲洋长期俯冲-增生演化形成的显生宙最大的增生造山带,以发育巨量的面状展布的俯冲-增生相关的弧岩浆岩为特征。并且,由于中亚增生型造山带在潘吉亚最后聚合过程中发生弧弧(陆)碰撞,因此缺乏大规模且跨构造单元的碰撞相关的构造和变质等物质标志。显然,能否识别出大洋闭合期间碰撞作用的岩浆标志成为确定增生造山带增生过程终止的关键之一。本文系统研究确定:中亚造山带东南缘二叠纪到三叠纪钙碱性-碱钙性岩浆在空间分布上显示出由北西向南东迁移演化的特征;在岩浆性质上具有从二叠纪新生地壳来源的弧岩浆向早-中三叠世碰撞挤压背景下古老陆壳组分逐渐增多的高Sr/Y岩浆以及晚三叠世后造山伸展相关的A型花岗岩演化的特征。这些特征提供了俯冲-增生向碰撞造山演变的关键岩浆岩证据。结合区域资料,厘定出增生造山带最后碰撞相关的标志性岩浆为沿缝合带呈零星线性展布的增厚下地壳源区的高Sr/Y花岗岩类,构建了中亚造山带南缘从双向俯冲-增生到增生楔-增生楔碰撞及后造山伸展的三阶段构造-岩浆演化模型。系统对比研究,揭示出增生-碰撞相关的岩浆记录沿横向展布在中亚造山带南缘甘肃北山到吉林中部一带,表明碰撞挤压相关的岩浆作用在中亚造山带南缘具有一定的普适性。中亚造山带南缘从增生到碰撞的岩浆演化记录的厘定,证实显生宙最大的巨型增生造山带演化末期经历了碰撞造山作用,对进一步深入探索增生造山演化末期碰撞相关的标志性岩浆具有重要意义。     

Palynological constraints on the age of the Mississippi Valley-type Changdong Pb-Zn deposit,Sanjiang belt,West China

Mississippi Valley-type(MVT)Pb-Zn deposits serve as the world’s major supply of Pb-Zn resources.However,the age constraint of MVT Pb-Zn deposits has long been a big challenge,due to the lack of minerals that are unequivocally related to ore deposition and that can be used for radioisotopic dating.Here we show sporopollens can provide useful chronological information on the Changdong MVT Pb-Zn deposit in the Simao basin,Sanjiang belt,West China.The Pb-Zn ores in the Changdong deposit are hosted by internal sediments in paleo-karst caves of meteoric origin.Sphalerite and galena occur as replacements of carbonate minerals and void infillings in the internal sediments.The relations suggest that the Pb-Zn mineralization occurred after the deposition of the internal sediments.A palynological assemblage mainly composed of angiosperm pollen dominated by Castanea,Quercus,and Carya and fern spores dominated by Polypodiaceae,Pteris,and Athyriaceae was identified.These pollen and spores place the ore-hosting internal sediments and the Changdong paleo-karst at early to middle Oligocene.Consequently,the Changdong Pb-Zn deposit must have formed after the early Oligocene(~34 Ma).These age constraints,together with the geological characteristics,indicate that the Changdong Pb-Zn deposit is a paleo-karst-controlled MVT deposit related to fold-thrust systems in the Sanjiang belt.The Changdong deposit is similar to other MVT Pb-Zn deposits in the northern part of the Sanjiang belt,making it possible to extend this Pb-Zn belt 500 km further to the South.Results presented here highlights the potential of sporopollens in dating the age of MVT deposits related to paleo-karst formation in young orogenic belts.     

川东南盆缘常压区页岩裂缝脉体特征及古压力演化

为了查明川东南盆缘常压页岩气区五峰组页岩裂缝脉体记录的古温度及古压力特征,揭示常压页岩气区储层压力降低的主要影响因素和页岩气散失机理.以松坎地区五峰组黑色碳质页岩裂缝脉体内的流体包裹体为主要研究对象,通过显微镜光学观察、阴极发光测试、包裹体测温和激光拉曼分析,结合埋藏-生烃-热史模拟,对裂缝脉体中的气-液两相盐水包裹体和高密度甲烷包裹体进行了系统研究.研究表明:松坎地区五峰组裂缝中主要存在着两期脉体充填,M1裂缝脉体形成时间距今约103~86 Ma,脉体较宽、阴极发光颜色为橘红色,其内甲烷包裹体捕获压力为82.6~91.5 MPa,反映燕山中期盆缘地区页岩气藏处在超压状态;M2裂缝脉体生长于M1裂缝脉体两侧,形成时间距今约90~72 Ma,脉体较窄、阴极发光颜色为暗红色,其内甲烷包裹体捕获压力为43.6~47.3 MPa.综合分析认为,川东南盆缘松坎地区五峰组在燕山期经历了由超压至常压的转变.燕山期以来的抬升剥蚀与褶皱变形导致地层内大量页岩气沿着滑脱层发生侧向运移和散失,地层压力快速下降.燕山晚期时,盆内稳定构造区页岩气藏仍处于超压状态,而盆缘地区已降至常压.      

Experimental Study on Mechanical Properties Degradation and Acoustic Emission Characteristics of Coal Rock Caused by CO2 Injection

Geotechnical and Geological Engineering - Geological sequestration of greenhouse gases has gained extensive attentions in recent years, but the degradation law of mechanical parameters and the...     

澳大利亚中部Alice Spring红色表土磁学特征分析

炎热干旱的澳大利亚中部是现代正在形成红色地表的区域.围绕中部Alice Spring地区采集了一系列红色地表样品.这些红色样品按照岩性大致可以分为三类:砂土、沙丘砂和岩石.通过对这些样品详细的磁学测量,发现这三类样品存在明显磁学特征差异,红色砂土和沙丘砂样品磁化率较岩石样品高出许多(砂土和沙丘砂磁化率均值为93.82× 10-8m3/kg),红色岩石样品磁化率值最低(均值为23.2×10-8m3/kg);三者主要磁性矿物也不尽相同;磁颗粒均以超顺磁(SP)颗粒为主,而单畴(SD)颗粒含量少.研究区百分比频率磁化率xfd％均值为8.28％,较黄土高原西部表土(兰州为3.5％)高出许多.该区现代年降水量约300mm,比兰州(约330mm)还低,成土导致百分比频率磁化率增高却比兰州明显高出几倍.这可能反映了黄土高原表土频率磁化率增高与降水量密切相关;而在澳洲中部可能与持续高温成土条件和作用的时间存在更密切的关系.澳洲中部不论岩石还是表土均以红色为主.磁学实验表明,砂土和沙丘砂样品均以磁铁矿为主,三类样品普遍含一定量磁赤铁矿和赤铁矿的贡献,与地表红色外貌相符.说明澳洲红色地表过程很可能是黑色磁铁矿颗粒表面被长期氧化条件下形成的红色磁赤铁矿/赤铁矿所包裹的现象,使得澳洲中部广大地区岩石露头和地表沉积物,普遍形成一层红色染色层.     

博斯腾湖滨柽柳(Tamarix ramosissina)生长对湖水位的敏感性

基于博斯腾湖1955—2012年湖水位变化资料,利用树木年轮法分析了博斯腾湖年和月水位变化与湖滨柽柳(Tamarix ramosissina)年轮生长关系,利用敏感度指数得出博斯腾湖滨柽柳年轮生长的敏感水位范围。结果表明:(1)1955—2012年博斯腾湖年平均水位经历了3个明显变化阶段,即1955—1987年下降至最低,1987—2002年上升至最高。受向下游生态输水影响,2002—2012年博斯腾湖水位快速下降。输水对博斯腾湖月平均水位和季节性水位变化有影响。(2)博斯腾湖滨柽柳年轮指数与当年的湖水位变化和前1年的湖水位变化均显著相关(p0.05)。柽柳年轮指数与前1年10月至当年4月各个月份的湖水位表现出显著相关(p0.05)。柽柳年轮指数与前1年冬季湖水位相关显著(p0.05),与当年春季3—4月月平均湖水位相关性显著,与当年夏季和秋季湖水位的相关性不显著。(3)博斯腾湖滨柽柳年轮生长对月湖水位变化响应比较敏感。当湖水位在1045.3m时,柽柳年轮指数灵敏度指数(Sk)存在最低值;当湖水位在1 046.3m时,Sk出现最高值。     

网络数字雹雨分测仪技术试验研究

介绍了网络数字雹雨分测仪的传感器结构和工作原理:利用浮力定律,翻斗计量,微机记录,网络传输等工作原理,模拟实验了理论数值和实验数值间的计量误差,探讨了误差产生的原因及野外观测调节技术和蒸发补偿订正等.经试验表明,各种部件结构科学、稳定、误差小、整体性能良好.野外观测资料表明,网络雹雨分测仪所测雨量与自动站观测的雨量误差在可接受范围;由于能同时进行雹雨分测,对极端冰雹天气具有实时监测优势,在野外林果和农作物雹灾危害评估中有重要作用,具有与遥测雨量计和其他遥测气象要素仪器一样的现代化水平,可广泛应用于农业和林业灾害野外监测网络之中.     

Dynamics of the Jupiter Trojans with Saturn’s perturbation in the present configuration of the two planets

The dynamics of the two Jupiter triangular libration points perturbed by Saturn is studied in this paper. Unlike some previous works that studied the same problem via the pure numerical approach, this study is done in a semianalytic way. Using a literal solution, we are able to explain the asymmetry of two orbits around the two libration points with symmetric initial conditions. The literal solution consists of many frequencies. The amplitudes of each frequency are the same for both libration points, but the initial phase angles are different. This difference causes a temporary spatial asymmetry in the motions around the two points, but this asymmetry gradually disappears when the time goes to infinity. The results show that the two Jupiter triangular libration points should have symmetric spatial stable regions in the present status of Jupiter and Saturn. As a test of the literal solution, we study the resonances that have been extensively studied in Robutel and Gabern (Mon Not R Astron Soc 372:1463–1482, 2006). The resonance structures predicted by our analytic theory agree well with those found in Robutel and Gabern (Mon Not R Astron Soc 372:1463–1482, 2006) via a numerical approach. Two kinds of chaotic orbits are discussed. They have different behaviors in the frequency map. The first kind of chaotic orbits (inner chaotic orbits) is of small to moderate amplitudes, while the second kind of chaotic orbits (outer chaotic orbits) is of relatively larger amplitudes. Using analytical theory, we qualitatively explain the transition process from the inner chaotic orbits to the outer chaotic orbits with increasing amplitudes. A critical value of the diffusion rate is given to separate them in the frequency map. In a forthcoming paper, we will study the same problem but keep the planets in migration. The time asymmetry, which is unimportant in this paper, may cause an observable difference in the two Jupiter Trojan groups during a very fast planet migration process.