黑潮延伸体海域典型涡旋的次中尺度特征分析

本文基于卫星遥感资料和高分辨率ROMS(Regional Ocean Modeling System)数值模拟结果, 对黑潮延伸体海域典型中尺度涡旋的次中尺度特征进行了探讨。卫星观测和模拟结果显示, 黑潮延伸体涡旋海域伴随着活跃的次中尺度现象。涡旋演变与多尺度能量分析结果表明, 涡旋海域次中尺度动能的强弱与涡旋海域地转流动能有着密切联系, 锋生可能是涡旋边缘次中尺度动能增强的重要机制。次中尺度现象在中尺度涡旋海域具有沿地转流方向的复杂涡丝状结构特征, 意味着涡旋边缘较强的水平浮力梯度和地转流侧向剪切为次中尺度过程形成与发展提供了有利条件。此外, 垂向结构分析表明, 次中尺度过程能引起较大的垂向速度, 最大可达100m·day^-1, 该垂向速度可以影响至混合层下200m深度处, 对海洋内部的垂向物质能量交换、海—气相互作用等有着重要的影响。     

北极薄冰-煎饼冰区域中不同重力波驱动形成海流的敏感性分析

A coupled ocean-ice-wave model is used to study ice-edge jet and eddy genesis during surface gravity wave dissipation in a frazil-pancake ice zone. With observational data from the Beaufort Sea, possible wave dissipation processes are evaluated using sensitivity experiments. As wave energy dissipated, energy was transferred into ice floe through radiation stress. Later, energy was in turn transferred into current through ocean-ice interfacial stress. Since most of the wave energy is dissipated at the ice edge, ice-edge jets, which contained strong horizontal shear, appeared both in the ice zone and the ocean. Meanwhile, the wave propagation direction determines the velocity partition in the along-ice-edge and cross-ice-edge directions, which in turn determines the strength of the along-ice-edge jet and cross-ice-edge velocity. The momentum applied in the along-ice-edge(cross-ice-edge)direction increased(decreased) with larger incident angle, which is favorable condition for producing stronger mesoscale eddies, vice versa. The dissipation rate increases(decreases) with larger(smaller) wavenumber, which enhances(reduces) the jet strength and the strength of the mesoscale eddy. The strong along-ice-edge jet may extend to a deep layer(> 200 m). If the water depth is too shallow(e.g., 80 m), the jet may be largely dampened by bottom drag, and no visible mesoscale eddies are found. The results suggest that the bathymetry and incident wavenumber(magnitude and propagation direction) are important for wave-driven current and mesoscale eddy genesis.     

High-resolution simulation of upper-ocean submesoscale variability in the South China Sea: Spatial and seasonal dynamical regimes

Submesoscale processes in marginal seas usually have complex generating mechanisms, highly dependent on the local background flow and forcing. This numerical study investigates the spatial and seasonal differences of submesoscale activities in the upper ocean of the South China Sea (SCS) and the different dynamical regimes for sub-regions. The spatial and seasonal variations of vertical vorticity, horizontal convergence, lateral buoyancy gradient, and strain rate are analyzed to compare the submesoscale phenomenon within four sub-regions, the northern region near the Luzon Strait (R1), the middle ocean basin (R2), the western SCS (R3), and the southern SCS (R4). The results suggest that the SCS submesoscale processes are highly heterogeneous in space, with different seasonalities in each sub-region. The submesoscale activities in the northern sub-regions (R1, R2) are active in winter but weak in summer, while there appears an almost seasonal anti-phase in the western region (R3) compared to R1 and R2. Interestingly, no clear seasonality of submesoscale features is shown in the southern region (R4). Further analysis of Ertel potential vorticity reveals different generating mechanisms of submesoscale processes in different sub-regions. Correlation analyses also show the vertical extent of vertical velocity and the role of monsoon in generating submesoscale activities in the upper ocean of sub-regions. All these results suggest that the sub-regions have different regimes for submesoscale processes, e.g., Kuroshio intrusion (R1), monsoon modulation (R2), frontal effects (R3), topography wakes (R4).     

中新世黄河水系演化重建：来自钾长石Pb同位素的约束

自剥蚀地貌中形成的剥蚀产物搬运到沉积区或汇水盆地沉积下来的过程,称为“源-汇”系统。从这些“汇”中识别“源”的信息,结合地层的沉积时代,约束黄河的形成时代、水系格局演化、流域内构造运动以及环境变迁成为黄河水系演化研究的重要内容。然而,时至今日学者们对黄河何时出现的认识并不一致,存在“中新世内流黄河和中新世外流黄河”之争。为了解决这些争议,我们运用大河物源示踪研究中新兴的碎屑钾长石Pb同位素方法,对黄河中下游沉积物开展碎屑钾长石Pb同位素分析(n=378),将其与长江中下游和华夏板块已报道的碎屑和基岩钾长石Pb同位素结果进行对比,结果表明三者之间的钾长石Pb同位素组成明显不同。台湾岛是中国东部陆架海中新世地层出露最齐全的地区。因而,我们将黄河中下游与台湾岛中新统的钾长石Pb同位素比值进行对比,结果表明二者之间不存在物源联系。结合中国东部渤海湾盆地、南黄海盆地和东海盆地中新统的物源示踪研究结果,说明黄河物质在中新世未流入上述盆地。总体而言,中国北方中新世的构造活动控制了黄河的演化过程,导致其此时处于分段演化阶段。     

有限空间中三维壁面紊动射流流动特性试验研究

为了研究三维壁面紊动射流前方布置的垂直挡板对时均流动特性的影响,采用粒子图像测速技术对不同雷诺数和淹没水深条件下的流速场进行了测量,统计分析了U速度剖面分布、速度半宽值变化和最大速度衰减规律。结果表明:沿射流方向具有3个明显不同的衰减区,依次划分为自由边界下的三维壁面射流区（Ⅰ区）、垂直挡板影响区（Ⅱ区）和近壁区（Ⅲ区）。在重点分析的Ⅱ区内,3个特征物理量的分布规律均与雷诺数无关;在垂直挡板影响下,速度半宽值扩展率明显加快,发展更为充分;在水深H~1.75H范围内,射孔中垂面内速度半宽值扩展率为0.043,同时0.5H的递增对射孔中心水平面内速度半宽值的分布较为敏感,其扩展率由0.205增至0.270;最大速度衰减对水深的改变并不敏感,且在Ⅱ区加速衰减,衰减指数为1.095。通过与半无限空间中三维壁面射流径向型衰减区的流动特征比较,Ⅱ区与之相似,将Ⅱ区视为提前进入径向型衰减区。     

渤海主要汇入河流碎屑磷灰石地球化学特征及成因

渤海的碎屑物质详细记录了源区的地质信息,对其进行物源示踪研究有助于提高我们对周围造山带及黄河的演化、中国东部陆架海碎屑物质扩散等的认识。本文利用激光剥蚀电感耦合等离子质谱分别对辽东湾、渤海湾及莱州湾周围主要汇入河流的碎屑磷灰石进行原位微量元素分析,结合Kolmogorov-Smirnov统计方法的多维判别图与反向传播神经网络等方法,分析渤海主要汇入河流碎屑磷灰石的微量元素与稀土元素。结果表明在汇入渤海的主要河流中,碎屑磷灰石的微量元素主要以Sr元素与Y元素为主,且都出现较为明显的HREE富集,但在不同河流之间的碎屑磷灰石Sr元素与REE也存在一定差异,这可能与其母岩不同相关。     

基于夜间灯光影像数据的黄河流域中心城市建成区空间扩展及动力因子分析

研究黄河流域建成区扩展特征有助于透视用地开发效果和践行中心城市高质量发展规划。基于1992、1997、2002、2007、2012、2018年6期夜间灯光影像与统计数据,提取建成区范围,采用扩展强度指数、紧凑度指数、协调发展系数与灰色关联分析,探究1992—2018年黄河流域8个中心城市扩展的时空格局、质量及动力因子。结果表明：（1）黄河流域中心城市建成区面积分化明显,中下游城市扩展规模和强度大,扩展形态呈紧凑度普遍下降趋势。（2）夜间灯光影像数据刻画的西安建成区综合水平高、西宁水平低,银川综合发展快、兰州慢;除西宁、呼和浩特与太原外,其他中心城市平均夜间灯光指数在1997—2018年呈下降趋势,反映城市扩展水平降低。（3）中心城市人口-土地协调发展系数均呈波动下降趋势,除呼和浩特、太原和济南外,人口-土地由基本协调型向土地过快扩展型转变;中心城市经济-土地协调发展系数呈波动下降趋势,经济年均增长率降低,建成区面积年均扩展率增加,基本由经济过快增长型向经济-土地协调发展型转变。（4）中心城市空间扩展主要受经济发展（地区生产总值）影响;从中心城市整体看,全时段（1996—2018年）行政力（固定资产投资）和内源力（人口规模）影响作用较大,分时段（1996—2002年、2002—2012年与2012—2018年）行政力影响系数亦较高,市场力（社会消费品零售总额）与外向力（实际利用外资额）影响作用程度随时间增加明显。新时期黄河流域中心城市空间扩展应注重内部提质增效,提高建设用地利用效率,促进城市高质量发展。     

免疫多糖对栉孔扇贝酸性磷酸酶、碱性磷酸酶和超氧化物歧化酶活性的影响

在栉孔扇贝的血清、血细胞和肝脏提取液中均发现有酸性磷酸酶（ＡＣＰ）、碱性磷酸酶（ＡＬＰ）和超氧化物歧化酶（ＳＯＤ）活性,其中,ＡＣＰ和ＡＬＰ在肝脏中的活性最高。采用１．０％的虫草多糖或海藻多糖作为免疫药物,对栉孔扇贝进行注射刺激后,发现血清中的ＡＣＰ、ＡＬＰ和ＳＯＤ活性有显著提高,血细胞中的ＡＣＰ和ＳＯＤ活性也有所增加,而肝脏提取液的这三种酶活性的变化不很明显。研究认为这两种多糖具有增强栉孔扇贝免疫活性的作用,在水产养殖业中有一定的开发价值。     

Differences of granitic weathering at the northern and southern feet of Dabie Mountains,Central China: Implication for tectonic and climatic environments

Previous studies of weathering generally started with geochemistry[1—8] and mineralogy[9—12], and have been focused on chemical weathering rates[1—3], removability-enrichment of elements[3—6] during chemical weathering, and the age of weathering profi…     

Early cretaceous granitoids and their implications for the collapse of the Dabie orogen, eastern China: SHRIMP zircon U–Pb dating and geochemistry

Two stages of early Cretaceous post-orogenic granitoids are recognized in the Dabie orogen, eastern China, which recorded processes of extensional collapse of the orogen. The early stage granitoids ( 132 Ma) are foliated hornblende quartz monzonites and porphyritic monzogranites. They are of high-K calc-alkaline series and metaluminous to weakly peraluminous, with high K₂O and low MgO contents (Mg^# values: 32.0–46.0), they contain high Sr, low Y and heavy rare earth elements (HREE), and have high Sr/Y and (La/Yb)_N ratios, without clear negative Eu, Sr and Ti anomalies. The early stage deformed granitoids have adakitic geochemical compositions and are equilibrated with residues rich in garnet and poor in anorthite-rich plagioclase, and thus indicate the existence of an over-thickened (> 50 km) crustal root beneath the orogen at  132 Ma. The later stage granitoids ( 128 Ma) are undeformed fine-grained monzogranites, fine-grained K-feldspar granites and coarse-grained K-feldspar granite-porphyry. They belong to a peraluminous and high-K calc-alkaline to shoshonite series, and display a flat HREE pattern and have strong negative Eu, Sr and Ti anomalies, with low Sr/Y and (La/Yb)_N ratios. The late stage granitoids are equilibrated with residues rich in anorthite-rich plagioclase, hornblende, ilmenite/titanite and poor in garnet, indicating that the crust of the Dabie orogen became thinner (< 35 km) at  128 Ma. SHRIMP zircon U–Pb ages and changing compositional trends for these two stages of granitoids indicate that the over-thickened crust formed by the Triassic continental subduction/collision under the Dabie orogen remained until the early Cretaceous, and collapsed quickly in a few million years during the early Cretaceous.