胶北地体早前寒武纪重大岩浆事件、陆壳增生及演化

早前寒武纪重大岩浆事件是早期陆壳增生及演化的主要地质作用。本文通过系统总结最近几年胶北地体早前寒武纪重大岩浆事件代表性岩石的岩相学、锆石U-Pb年代学、岩石地球化学及锆石Hf同位素研究的最新成果,厘定出太古宙~2.9Ga、2.7Ga及2.5Ga三期以TTGs岩浆事件为代表的陆壳增生事件。这些TTGs具有典型太古宙高铝TTGs的地球化学特征及正的εHf(t)值,锆石Hf模式年龄主要集中在ca.3.2~2.7Ga。两种不同的构造模式被用来理解胶北太古宙TTGs(陆壳)的成因:(1)加厚基性下地壳的部分熔融;(2)俯冲洋壳的部分熔融。根据胶北TTGs在时间上呈事件性侵位,空间上呈面状分布,以及相对较低的Mg#、Cr及Ni含量,前者可能更适合胶北TTGs的成因。确定了胶北古元古代2.2~2.0Ga黑云母/角闪石二长花岗片麻岩及~1.8Ga以二长(正长)花岗岩为代表的多期陆壳重熔事件。综合这些研究结果,初步总结出胶北早前寒武纪陆壳形成及演化历史:1)2.9Ga,主要为基性地壳(洋壳)的增生,并可能存在规模有限的、被剥蚀殆尽的太古宙早期陆壳;2)在~2.9Ga、~2.7Ga及~2.5Ga,由于地幔(热)柱上涌,ca.3.3~2.7Ga新生的加厚基性玄武质下地壳发生事件性部分熔融,并伴随有早期陆壳的重熔,形成主要由TTGs及少量陆壳重熔型(高钾)花岗岩组成的太古宙陆壳;3)ca.2.2~2.0Ga,可能由于地幔物质上涌,陆壳伸展,形成裂谷,陆壳物质重熔,形成ca.2.2~2.0Ga花岗质岩石;4)ca.1.95~1.85Ga,发生强烈的挤压碰撞构造作用,裂谷闭合,卷入挤压作用的物质发生高角闪岩相到高压麻粒岩相变质;5)~1.8Ga,地幔物质上涌,陆壳伸展减薄,陆壳物质重熔,形成~1.8Ga花岗岩。     

滇西北衙斑岩型金多金属矿床成矿流体特征及其演化

北衙超大型金多金属矿床位于扬子陆块西缘与三江特提斯造山带的结合部位。本文通过对北衙矿区内的斑岩体石英斑晶、斑岩型矿化、矽卡岩矿化中的矽卡岩及外围似层状热液型铅锌银矿化的岩(矿)石中发育的流体包裹体进行了系统研究,发现北衙矿区内主要发育CO2、富CO2、含CO2、含子矿物三相、富气相水溶液及气液两相水溶液包裹体六类流体包裹体;与斑岩型矿化有关的成矿流体为中-高温Na Cl-H2O-CO2体系热液,矽卡岩矿化相关成矿流体为一种高温的Na Cl-H2O及Na Cl-H2O-CO2体系热液,而外围似层状铅锌银矿化相关的成矿流体则为中温的Na Cl-H2O-CO2体系热液。对比分析表明,矽卡岩矿化中的矽卡岩矿物(以绿帘石类矿物为主)形成较早,其中发育富气相的流体包裹体,可以推断岩浆侵位后先分异出富水蒸气的流体,此后CO2才从成矿流体中大量分异。斑岩型矿化及外围地层中似层状铅锌银矿化脉体中发育的流体包裹体与斑岩体石英斑晶内发育的流体包裹体组合类型基本一致,表明成矿流体主要来自斑岩体结晶分异出的岩浆热液。流体包裹体研究表明,北衙金多金属矿区内的矽卡岩型(金铜铁)、斑岩型(铜金钼)及外围碳酸盐岩等地层中的似层状热液型(铅锌银)矿床系列为与富碱斑岩体侵位活动有关的,由岩浆分异热液并逐渐演化形成的斑岩型金-铁铜-铅锌(银)多金属成矿系统。     

卵石地层的特殊性及其对基坑支护的影响分析

主要从卵石地层的特征分类、特殊结构及场内施工条件3个方面,对基坑支护结构选型及施工工艺选择进行深入、系统的分析论证,力求使在卵石地层中的基坑支护设计方案更科学、经济,使施工方法、工艺更具可操作性。     

珠江口盆地番禺低隆起东部珠江组沉积环境的恢复

对珠江口盆地番禺低隆起东部L16井中新统珠江组的岩心观察分析,岩性包括碎屑岩、碳酸盐岩以及碎屑-碳酸盐的混积岩。珠江组可划分为11种沉积微相类型;建立了三角洲—滨岸—碎屑与碳酸盐混积滨岸—碳酸盐台地—浅海陆棚(23.8 Ma~18.5 Ma)沉积演化序列。地震地质解释证实了珠江组早期东沙三角洲的存在;古珠江三角洲与东沙三角洲构成了研究区珠江组下段的沉积主体。恢复了研究区珠江组沉积相及其演化,重点刻画了SQ2—TST时期由陆到海的变迁,而海平面变化是这一变迁的主要控制因素。     

Kinematics of syn-tectonic unconformities and implications for the tectonic evolution of the Hala'alat Mountains at the northwestern margin of the Junggar Basin,Central Asian Orogenic Belt

The Hala’alat Mountains are located at the transition between the West Junggar and the Junggar Basin.In this area,rocks are Carboniferous,with younger strata above them that have been identified through well data and high-resolution 3D seismic profiles.Among these strata,seven unconformities are observed and distributed at the bases of:the Permian Jiamuhe Formation,the Permian Fengcheng Formation,the Triassic Baikouquan Formation,the Jurassic Badaowan Formation,the Jurassic Xishanyao Formation,the Cretaceous Tugulu Group and the Paleogene.On the basis of balanced sections,these unconformities are determined to have been formed by erosion of uplifts or rotated fault blocks primarily during the Mesozoic and Cenozoic.In conjunction with the currently understood tectonic background of the surrounding areas,the following conclusions are proposed:the unconformities at the bases of the Permian Jiamuhe and Fengcheng formations are most likely related to the subduction and closure of the Junggar Ocean during the late Carboniferous-early Permian;the unconformities at the bases of the Triassic Baikouquan and Jurassic Badaowan formations are closely related to the late Permian-Triassic Durbut sinistral slip fault;the unconformities at the bases of the middle Jurassic Xishanyao Formation and Cretaceous Tugulu Group may be related to reactivation of the Durbut dextral slip fault in the late Jurassic-early Cretaceous,and the unconformity that gives rise to the widely observed absence of the upper Cretaceous in the northern Junggar Basin may be closely related to large scale uplift.All of these geological phenomena indicate that the West Junggar was not calm in the Mesozoic and Cenozoic and that it experienced at least four periods of tectonic movement.     

一种亮星识别算法及其在天文定向中的应用

基于全站仪对任意亮星的观测采样,提出了一种利用高度角序列和水平角速率进行联合匹配的任意亮星识别算法。通过引入天体地平坐标计算程序,算法可正确辨别行星和恒星。本文分析了任意亮星高度角和水平角速率的观测误差和计算误差,以此给出了匹配阈值条件的设定依据,并在此基础上制定了有效的匹配策略。仿真计算及实际观测试验均表明,该算法具有100%的识别成功率,远优于现有算法。将此算法应用于任意亮星天文定向,定向结果的内符合精度达到2″,外部检核精度达到1.6″。采用多颗任意亮星进行定向,可有效减弱由测站位置误差引入的定向系统误差,提高绝对定向精度。本文提出的天文定向适用于多云及雾霾天气。     

基于时间序列雷达干涉测量的钱塘江海塘形变分析

形变监测是海塘安全运行的重要组成部分。本文利用杭州地区2006年—2010年获取的31景EnvisatASAR影像,根据MTInSAR(Multi-Temporal In SAR)方法,综合提取PS(Persistent Scatterer)和DS(Distributed Scatterer)点,得到密集的钱塘江海塘形变的In SAR测量结果。与28个点的水准数据对比表明,两者的平均误差为0.436 mm,最大误差为5.016 mm,验证了In SAR技术毫米级的测量精度和准确性。通过这两种数据的时间序列分析发现,海塘的沉降在空间上具有连续性,其空间分布呈现为单峰下沉曲线;在时间上,则具有明显的线性变化规律,并伴随有短时间范围的小幅度波动。     

Hemispheric asymmetry of sunspot area in solar cycle 23 and rising phase of solar cycle 24: Comparison of three data sets

Analysis of long-term solar data from different observatories is required to compare and confirm the various level of solar activity in depth. In this paper, we study the north–south asymmetry of monthly mean sunspot area distribution during the cycle-23 and rising phase of cycle-24 using the data from Kodaikanal Observatory (KO), Michelson Doppler Imager (MDI) and Solar Optical Observing Network (SOON). Our analysis confirmed the double peak behavior of solar cycle-23 and the dominance of southern hemisphere in all the sunspot area data obtained from three different resources. The analysis also showed that there is a 5–6 months time delay in the activity levels of two hemispheres. Furthermore, the wavelet analysis carried on the same data sets showed several known periodicities (e.g., 170–180 days, 2.1 year) in the north–south difference of sunspot area data. The temporal occurrence of these periods is also the same in all the three data sets. These results could help in understanding the underlying mechanism of north–south asymmetry of solar activity.     

Accuracy of the deep convection intensity from a limited number of casts

Deep convection is one of the key components of the Atlantic Meridional Overturning Circulation. The intensity of deep convection (DC) is traditionally estimated as the maximum mixed layer depth (MMLD). In this study, we developed a criterion of the minimum number of casts needed for obtaining the MMLD in the Greenland Sea with a pre-defined accuracy. The criterion depends on convection intensity.For gridded datasets, we introduce a complementary measure for the DC intensity: the area of the region with the mixed layer depth over a predefined value (800 m for the Greenland Sea, notated as S₈₀₀). For a weak or a moderate DC, variations of its intensity is more clear from variations of the MMLD (cluster 1 in the MMLD - S₈₀₀ parameter space). Then the MMLD can be obtained with the 25 % accuracy for at minimum 40 casts during winter. For a well developed DC (cluster 2), variations of the DC intensity are better accessed from variations of S₈₀₀ and minimum 10 casts are required.In the central Greenland Sea, the number of casts is sufficient for obtaining the interannual variations of the convection intensity only since 1986. If only Argo floats are available, minimum 4 floats should simultaneously operate in the Greenland Sea gyre during winter to reach the abovementioned accuracy. Up to present, the number of floats has been insufficient during most of the winters.     

基于FY-2G产品的江西省总云量最小二乘法建模与分析

使用2016年1月至2018年12月FY-2G卫星逐小时总云量产品和江西省26个测站的地面总云量观测资料,分析了两者在江西地区相关性的时空分布特征。结果表明:江西地区卫星总云量和地面观测总云量在数值和演变趋势上一致性较好,两者的总体相关系数超过0.60,但空间分布不均匀,大型水体(鄱阳湖和柘林湖)附近相关系数较低,低于0.45,江西省南部地区相关系数也不高,低于0.50。两者的相关系数在时间上也分布不均,其中14时的相关系数最高。此外,基于FY-2G卫星总云量产品和最小二乘法采用分段建模的方式,构建了江西省地面观测云的回归模型,且模拟的地面总云量在数值和演变趋势上更加接近观测的地面云量。