博格达山东段苏吉山辉长岩LA-ICP-MS锆石U-Pb年龄、地质地球化学特征及构造意义

苏吉山辉长岩体位于博格达碰撞造山带东段,卡拉麦里蛇绿混杂岩带西南侧,出露面积约1.8 km~2,岩性为石英角闪辉长岩。苏吉山辉长岩体富含普通角闪石(20%)和磁铁矿物,表明原生岩浆富水、高氧逸度特征,岩石化学组成属于拉斑玄武岩系列,岩石弱富集大离子亲石元素Cs、Rb、Ba、Th、U,显著亏损Nb、Ta、Zr、Hf和弱亏损Ti,显示源区为受俯冲流体交代改造的岩石圈地幔,应是洋壳俯冲的产物。苏吉山辉长岩体锆石U-Pb年龄为308.1±3.3Ma,早于卡拉麦里混杂岩带内碱性花岗岩侵位,介于博格达裂谷活动期,是裂谷作用由全面伸展向局限伸展转换的标志。苏吉山辉长岩空间上位于古亚洲洋板块沿卡拉麦里蛇绿混杂岩带向准噶尔板块斜向俯冲的前进方向,时间上介于博格达裂谷活动期,地球化学上显示洋壳俯冲的特征,各种事实表明,古亚洲洋沿卡拉麦里碰撞带向准噶尔板块斜向俯冲作用形成撕裂型博格达裂谷,博格达裂谷由伸展机制向伸展-碰撞过渡机制的应力调整导致了苏吉山辉长岩体的侵位。     

华北克拉通乌拉山地区早前寒武纪岩浆作用和变质作用——锆石SHRIMP U-Pb定年及岩石地球化学研究

乌拉山地区位于大青山地区西侧,变泥砂质岩石大范围出露,并有一定数量变质岩浆侵入岩存在。本文对6个变质岩浆侵入岩进行了锆石SHRIMP U-Pb定年。片麻状闪长岩、片麻状英云闪长岩、片麻状花岗闪长岩和片麻状紫苏花岗岩等4个样品的锆石U-Pb数据点沿谐和线分散分布,n(~(207)Pb)/n(~(206)Pb)年龄从约2.5Ga到约1.8 Ga。变质辉长岩和眼球状石英二长岩锆石U-Pb数据点在谐和线上较集中分布,n(~(207)Pb)/n(~(206)Pb)年龄从约2.0Ga到约1.8 Ga。n(~(207)Pb)/n(~(206)Pb)年龄越小的锆石域通常显示越强烈的重结晶。结合已有研究和地球化学资料,可得出如下结论。(1)乌拉山地区存在新太古代晚期(约2.5 Ga)和古元古代中晚期(约2.0 Ga)岩浆侵入岩,后者形成于伸展构造环境。(2)乌拉山地区遭受新太古代晚期一古元古代早期和古元古代晚期两期构造热事件叠加改造。(3)乌拉山地区部分变泥砂质岩石形成于新太古代晚期,大青山地区原认为形成于古元古代早期的"大青山表壳岩"很可能也形成于新太古代晚期。(4)乌拉山地区和大青山具有类似或相同的早前寒武纪地质演化历史。     

Upper-Tropospheric Environment–Tropical Cyclone Interactions over the Western North Pacific: A Statistical Study

Based on 25-year(1987–2011) tropical cyclone(TC) best track data, a statistical study was carried out to investigate the basic features of upper-tropospheric TC–environment interactions over the western North Pacific. Interaction was defined as the absolute value of eddy momentum flux convergence(EFC) exceeding 10 m s~(-1)d~(-1). Based on this definition, it was found that 18% of all six-hourly TC samples experienced interaction. Extreme interaction cases showed that EFC can reach~120 m s~(-1)d~(-1) during the extratropical-cyclone(EC) stage, an order of magnitude larger than reported in previous studies.Composite analysis showed that positive interactions are characterized by a double-jet flow pattern, rather than the traditional trough pattern, because it is the jets that bring in large EFC from the upper-level environment to the TC center. The role of the outflow jet is also enhanced by relatively low inertial stability, as compared to the inflow jet. Among several environmental factors, it was found that extremely large EFC is usually accompanied by high inertial stability, low SST and strong vertical wind shear(VWS). Thus, the positive effect of EFC is cancelled by their negative effects. Only those samples during the EC stage, whose intensities were less dependent on VWS and the underlying SST, could survive in extremely large EFC environments, or even re-intensify. For classical TCs(not in the EC stage), it was found that environments with a moderate EFC value generally below ~25 m s~(-1)d~(-1) are more favorable for a TC's intensification than those with extremely large EFC.     

Factors controlling the interannual variations of MJO intensity

The interannual variations of intensity of the Madden-Julian Oscillation (MJO) during boreal winter are investigated by using the observed outgoing longwave radiation (OLR) and the reanalysis data of ECMWF and NCEP. The standard deviation of 20-80-day filtered OLR anomaly is used to measure the MJO intensity. The dominant spatial structure of the interannual variability is revealed by an EOF analysis of the MJO intensity field. It is found that the leading mode is associated with eastern Pacific type ENSO, whereas the second mode is related to central Pacific type ENSO. A simple atmospheric model is used to investigate the relative roles of background moisture and wind changes in affecting the overall strength of MJO. The numerical experiments indicate that the background moisture effect is dominant while the background wind change has a minor effect.     

含AgI焰剂成冰性能与物化特征的实验研究

利用CAMS的1 m~3等温云室系统筛选出新型高效AgI焰剂WMC-IN-001和WMG-IN-002。检测结果表明,它们具有较高的成核率,在-15℃时达到10~(15)g~(-1)AgI量级,尤其在-7℃时WMC-IN-001的成核率仍可达到10~(14)g~(-1)AgI量级。同时给出对节银剂配方和2011年市场上主要的几种催化剂的检测结果进行对比。WMC-IN-001和WMC-IN-002的成冰速率较慢,在各检测温度的成冰速率差异较小,均在40~55 min。利用冷场发射扫描电镜和能谱仪对WMC-IN-001燃烧产生的气溶胶粒子作了物化特征分析,粒子分布在0.02~0.60μm,具有两个典型的模态:0.02~0.10μm的较小的粒子和0.20~0.55μm的较大的粒子,均立方直径为0.2472μm。WMC-IN-001气溶胶粒子明显偏大,小粒子相对较少,这可能是其成冰速率偏慢的原因之一。