底栖有孔虫(Florilus decors)壳体微量元素/钙比值的LA-ICP-MS原位微区分析方法及应用——以长江口外海域为例

深海沉积物中有孔虫壳体的微量元素、同位素测试技术已较为成熟,而河口近海沉积物中有孔虫壳体元素微区测试却鲜有报道。本文报道了一种利用激光剥蚀电感耦合等离子体质谱（LA-ICP-MS）分析法测试取自长江口外沉积物中的有孔虫壳体元素/钙比值的技术,研究了氦气载气流量、能量密度、束斑大小、激光剥蚀频率等参数对测试结果的影响,优化了活体有孔虫原位分析方法。应用确定的测试条件对2016年7月取自长江口外的底栖有孔虫优美花朵虫样品（Florilus decors）进行测试,发现Mg、Sr等元素/钙比值在壳体不同位置上无显著差异,而Mn的数据较为离散,可能与有孔虫生长过程中经历的水环境及其变化有关。     

浙江朱家尖岛东沙海滩对热带风暴“娜基莉”的响应及风暴后的恢复

海滩对风暴的响应及风暴后海滩的恢复过程一直以来都是国内外海滩研究的热点。本文通过对浙江舟山市朱家尖岛东沙海滩地形地貌的现场调查,对比分析了热带风暴"娜基莉"影响下东沙海滩剖面的蚀积变化,探讨了海滩在热带风暴发生后的恢复情况。结果表明,在"娜基莉"影响期间,因风暴浪为向岸浪,东沙海滩几乎遭受全线侵蚀,12个剖面单宽侵蚀总量为73.46 m3/m,其中海滩直线段较两个遮蔽段侵蚀显著。由于海滩在风暴前进方向的左侧,且"娜基莉"距东沙较远,使得东沙海滩普遍侵蚀但强度较小。东沙海滩在热带风暴后的恢复过程中,不同部位的地貌调整和冲淤变化不同,下岬角遮蔽段基本趋于稳定,直线段和上岬角遮蔽段在恢复过程中因受海滩季节性调整的影响呈现持续侵蚀。     

东海陆架外缘区构造特征及其成因机制

东海陆架边缘的构造特征记录了有关冲绳海槽张裂过程的关键信息,对于进一步理解海槽的形成演化以及弧后张裂与弧-陆碰撞之间的相互作用至关重要。本文基于多道地震和重磁资料,分析了东海陆架边缘的地形和构造特征,并对冲绳海槽早期张裂过程、北西向断裂带的分隔控制作用、钓鱼岛隆起带南北构造差异和冲绳海槽的向西前展等问题进行了探讨。结果表明,冲绳海槽西侧陆坡存在的分段性,各分段在地形地貌、地层展布和构造特征等方面的不同,体现了其构造演化和现今构造活动性的差异。冲绳海槽中—北段的张裂始于陆架前缘坳陷,在晚中新世向东扩展至整个海槽,晚中新世至今以分散式张裂为主。北西向断裂带对东海陆架边缘不同分段的构造特征和构造活动起到了分隔控制和转换协调作用,控制了不同类型陆坡的形成和发育。受冲绳海槽在全宽度上向西前展的影响,钓鱼岛隆起带南段的基底隆起及其支撑的陆架边缘发生了破坏和沉降,形成基底起伏较大、地形崎岖不平的陆坡。     

海洋气团对沿海城市大气环境影响与识别研究

本研究通过识别海洋气团特征及沿海城市大气受到海洋气团的影响方式与程度,为评价沿海城市空气环境质量提供科学依据。以青岛市为例,收集大气气溶胶样品中放射性核素~(210)Pb、40K数据及采集时段当地大气颗粒物数据;分析~(210)Pb活度浓度与气溶胶颗粒物浓度变化;对当地当时大气气团进行溯源分析。研究表明:(1)研究期间青岛沿岸地区2015年4月至2016年6月与2016年6月至2017年6月大气污染特征显著不同,前者~(210)Pb活度浓度与污染颗粒物浓度显著相关,而后者~(210)Pb活度浓度与污染颗粒物无相关关系;(2)穿越海洋的陆地气团呈现出高活度浓度、低颗粒物浓度的特征;来自海洋气团的气溶胶呈现出低活度浓度、低颗粒物浓度的特征;(3)海洋气团气溶胶中~(210)Pb活度浓度较低。临近大陆的海洋(黄海、东海)上层大气受到大陆气团的影响,其海洋气团的特征有所减弱。~(210)Pb活度浓度、颗粒物浓度(PM2.5)可作为判断海洋气团的指标,识别"来自海洋的气团"与"经过海洋的气团"。     

Explicit stress–strain equations for modeling frictional materials

In this paper, a comprehensive study on simulating the shearing behavior of frictional materials is performed. A set of two explicit equations, describing the relationship among the shear stress ratio and the distortional strain and the volumetric strain, are formulated independently. The equations contain three stress parameters and three strain parameters and another parameter representing the nonuniformity of stress and strain during softening. All the parameters have clear physical significance and can be determined experimentally. It is demonstrated that the proposed equations have the capacity of simulating the complicated shearing behavior of many types of frictional materials including geomaterials. The proposed equations are used to simulate the stress–strain behavior for 27 frictional materials with 98 tests. These materials include soft and stiff clays in both reconstituted and structured states, silicon sands and calcareous sands, silts, compacted fill materials, volcanic soils, decomposed granite soils, cemented soils (both artificially and naturally cemented), partially saturated soils, ballast, rocks, reinforced soils, tire chips, sugar, wheat, and rapeseed. It has been demonstrated that the proposed explicit constitutive equations have the capacity to capture accurately the shearing behavior of frictional materials both qualitatively and quantitatively. A study on model parameters has been performed.     

山东沂水太古宙麻粒岩区年代学研究成果简介

本文以详细研究本区麻粒岩-斜长角闪岩等表壳岩的岩石学、地球化学和 Sm-Nd 同位素定年为重点。所取得的成果，对华北陆台古老地层的分布和古构造格局的探索提供了实际资料。     

An algorithm to resolve γ-rays from charged cosmic rays with DAMPE

The DArk Matter Particle Explorer(DAMPE),also known as Wukong in China,which was launched on 2015 December 17,is a new high energy cosmic ray and γ-ray satellite-borne observatory.One of the main scientific goals of DAMPE is to observe Ge V-Te V high energy γ-rays with accurate energy,angular and time resolution,to indirectly search for dark matter particles and for the study of high energy astrophysics. Due to the comparatively higher fluxes of charged cosmic rays with respect to γ-rays,it is challenging to identify γ-rays with sufficiently high efficiency,minimizing the amount of charged cosmic ray contamination. In this work we present a method to identify γ-rays in DAMPE data based on Monte Carlo simulations,using the powerful electromagnetic/hadronic shower discrimination provided by the calorimeter and the veto detection of charged particles provided by the plastic scintillation detector. Monte Carlo simulations show that after this selection the number of electrons and protons that contaminate the selected γ-ray events at～10 Ge V amounts to less than 1% of the selected sample.Finally,we use flight data to verify the effectiveness of the method by highlighting known γ-ray sources in the sky and by reconstructing preliminary light curves of the Geminga pulsar.     

Petrogenesis of Early Cretaceous hornblende gabbro in Khanka Massif: evidence from geochronology and geochemistry

The authors report zircon U-Pb geochronological,whole-rock geochemical and zircon Lu-Hf isotope data for the hornblende gabbro within the Khanka Massif,with the aim of constraining its formation time and petrogenesis. The zircon U-Pb dating shows that ~(206)Pb/~(238)Pb ages of zircons from the hornblende gabbro range from 120 to 129 Ma,yielding a weighted mean age of 123 ± 2 Ma,i. e.,the Early Cretaceous. The hornblende gabbro has SiO_2 of 44. 77%--46. 58% and belongs to the tholeiitic series on FeO~t/MgO-SiO_2 diagram. It displays a right-inclined REE pattern with( La/Yb)_N ratios of 3. 44 to 4. 42. The trace element spidergram shows that they are enriched in large ion lithophile elements( LILE) such as Rb,Th,U,K and Pb,and depleted in high field strength elements( HFSE) such as Nb,Ta,Ti and P,indicating an affinity to arc igneous rocks.The ε_(Hf)( t) values of zircons vary from -2. 6 to + 3. 9 and Hf model ages( T_(DM1)) range from 622 to 883 Ma.These geochemical characteristics indicate that primary magma of the hornblende gabbro could be derived from partial melting of young mantle material accreted during the Neoproterozoic. Combined with the Early Cretaceous igneous rock assemblages in NE Asia. It is concluded that the hornblende gabbro formed in an active continental margin related to the westward subduction of the Paleo-Pacific Plate beneath the Khanka Massif.     

Helmert方差分量估计在GPS/GLONASS/BDS组合定位权比确定中的应用

因GNSS系统间观测噪声、轨道精度的差异,采用经验权比进行组合定位难以得到最优结果。基于此,在GPS/GLONASS/BDS组合定位中引入Helmert方差分量估计,对GPS/GLONASS/BDS组合单点定位和基线解算中各系统观测值进行合理定权。实验表明,采用该方法确定的伪距观测值最佳权比为5∶1∶1,相位观测值最佳权比为1∶1∶1,有效提高了GPS/GLONASS/BDS组合定位的精度和可靠性。     

Submarine landslide identified in DLW3102 core of the northern continental slope,South China Sea

In this paper, we take DLW3101 core obtained at the top of the canyon(no landslide area) and DLW3102 core obtained at the bottom of the canyon(landslide area) on the northern continental slope of the South China Sea as research objects. The chronostratigraphic framework of the DLW3101 core and elemental strata of the DLW3101 core and the DLW3102 core since MIS5 are established by analyzing oxygen isotope, calcium carbonate content, and X-Ray Fluorescence(XRF) scanning elements. On the basis of the information obtained by analyzing the sedimentary structure and chemical elements in the landslide deposition, we found that the DLW3102 core shows four layers of submarine landslides, and each landslide layer is characterized by high Si, K, Ti, and Fe contents, thereby indicating terrigenous clastic sources. L1(2.15–2.44 m) occurred in MIS2, which is a slump sedimentary layer with a small sliding distance and scale. L2(15.48–16.00 m) occurred in MIS5 and is a debris flow-deposited layer with a scale and sliding distance that are greater than those of L1. L3(19.00–20.90 m) occurred in MIS5; its upper part(19.00–20.00 m) is a debris flow-deposited layer, and its lower part(20.00–20.90 m) is a sliding deposition layer. The landslide scale of L3 is large. L4(22.93–24.27 m) occurred in MIS5; its upper part(22.93–23.50 m) is a turbid sedimentary layer, and its lower part(23.50–24.27m) is a slump sedimentary layer. The landslide scale of L4 is large.