大气中性点区域偏振效应的地—气参量研究

随着中国多颗偏振遥感器搭载发射,偏振遥感成为对地观测领域一个新的增长点以及研究热点。由于大气散射具有较强的偏振效应,大气与地表偏振信号的分离是偏振对地进行有效观测和应用的一个现实问题与难点问题。本文利用晴空中有规律的偏振分布以及大气偏振中性点的性质,对利用大气中性点的偏振效应进行地表—大气偏振信息分离的可行性进行了论证。通过对大气中性点在辐射传输过程性质的计算,得出Babinet大气中性点区域的偏振效应以及基于Babinet中性点区域进行偏振对地观测的基本方法,研究重点阐述了从航空遥感和航天遥感两个层面对如何将大气中性点应用于遥感观测进行了讨论。结果表明:(1)Babinet中性点相比于其他两个中性点,更适合于偏振遥感对地观测中地—气偏振参量分离;(2)航空遥感搭载偏振传感器在Babinet中性点区域进行地表探测可以消除大气偏振,突出地物偏振信息,有效进行地—气偏振参量分离;(3)在太阳同步轨道的卫星遥感影像上能够有效识别偏振中性点区域;研究成果有效分离高分辨率偏振遥感地物反演中的大气偏振耦合效应,实现地表偏振反射信息最大化,对于偏振遥感的大气校正以及定量化水平的提升具有实践意义。     

利用常熟地震台同场地形变仪记录检测对比地球自由振荡信号

利用常熟地震台同场地观测的洞体应变仪、体应变仪、水管倾斜仪、垂直摆倾斜仪记录数据,采用小波变换与功率谱密度估计方法,检测2011年3月11日日本9.0级大地震激发的地球自由振荡信号,其中检测到47个球型基频振型（₀S₃—₀S₄₉）、15个环型基频振型（₀T₅—0T₂₅）以及部分球型谐频振型,与地球初步参考模型（PREM）理论频率值基本符合,表明检测结果较好。对比结果显示：水管倾斜仪检测球型振荡振型能力最强,垂直摆倾斜仪检测环型振荡振型能力最强;体应变仪可检测到清晰的环型基频振型,且信噪比较高;倾斜仪对自由振荡信号的检测能力优于应变仪。     

The Important Role Played by Atmospheric Angular Momentum in the Non-linear Prediction of the Variations in the Length of Day

The variation in the length of day has complicated time-varying characteristics and the traditional method for linear time series analysis is always difficult to obtain good effect of prediction. If the non-linear artificial neural network technique is adopted to predict the variation in the length of day, the topological structure of the network model is determined by the least square error method. By taking into account the close relation between the variation in the length of day and the general circulation of atmosphere, the axial sequence of atmospheric angular momentum is introduced into the forecasting model of neural network. The results show that the forecast accuracy is significantly improved by taking advantage of the combination of the length of day and the atmospheric angular momentum sequence in comparison with the individual adoption of the data of the length of day.     

Excitation of Annual Polar Wobble by Global Oceans

A reasonable and quantitative result on the variation of polar wobble excited by the oceans is not available at present. Numerous researches have shown that atmospheric motion is the greatest excitation source for the seasonal variations in the polar wobble and that oceanic motion is one of the main remaining excitation sources. The excitation of variation in the annual polar wobble caused by oceans from 1992 to 2004 both globally and in latitude dependence, have been studied in depth by means of the new generation of SODA oceanic data assimilation (SODA-1.4.2 and SODA-1.4.3) and the ECCO oceanic data assimilation. The result shows that the variation in the seasonal polar wobble excited by the SODA oceans is very close to that of the residual after the action of the atmosphere and land water is deducted from the geodesic excitation function for a large part of the investigated time interval, and that there is overall agreement between the two as regards the annual amplitude and phase. In addition, in comparison with the result of early SODA-Bata 7, the new generation of SODA oceanic excitation has achieved obvious improvements. The latitude distributions of the excitations of the annual polar wobble by the SODA and ECCO oceans are consistent in the Greenwich direction, while having obvious differences in the direction of 90° E.     

塔里木盆地肖尔布拉克剖面下寒武统底部硅质岩微量元素和稀土元素地球化学及其沉积背景

对塔里木盆地北部肖尔布拉克寒武系露头剖面中 8.8m厚的黑色页岩夹硅质岩组合中的硅质岩的系统采样分析表明,该硅质岩具有深源成因特征。其低的Th/U和Rb/Sr比也证明了其沉积时所具有的深部物源和热水注入迹象。硅质岩的稀土元素经北美页岩标准化后的Ce/Ce 从 0.4 2到 0.79,平均 0.5 7。Ce的负异常明显。这些稀土元素的参数特征与加利福尼亚弗朗希斯科杂岩 (FranciscanComplex)中沉积在大洋海底硅质岩的稀土元素特征十分相似。北美页岩标准化后的Eu/Eu 值从 8.0 5下降到 1.0 3。其相对较高的Eu/Eu 值很有可能反映了热水的注入。Eu/Eu 值从剖面底部到顶部的系统降低反映了剖面底部的热水作用最强烈,向上热水作用逐渐减弱。上述一系列的地球化学标志指示该硅质岩应沉积在离洋中脊不远的、具有深源物质/热水注入的远洋盆地背景中。结合区域地质和伴生黑色页岩地球化学的综合分析认为,该套硅质岩的形成与上升洋流的影响有关。上升洋流将形成于大洋盆地背景中的物质带到大陆边缘陆棚环境中发生沉积,造成了沉积在陆棚环境中的硅质岩,在地球化学组成上保留了其大洋盆地背景的特征     

地表的分形测量及其大地构造学意义

以湖北红安地区为例,采用投影覆盖法(projectivecoveringmethod)对地表进行了二维分形测量,结果表明,地表面积具有双分形(bifractal)关系,即具有小尺度的结构分形(texturalfractal)和大尺度的构造分形(structuralfractal),分叉点(breakpoint)的尺度为3610m,分维值都在2～3之间且结构分维值大于其构造分维值。可见,地表形态具有分形性质,分维值可以指示地表形态的复杂程度。构造分维值可作为构造活动强度的一个指标,可为大地构造单元的划分提供定量依据。复杂地表形态主要是由构造活动(内营力作用)和各种复杂表生地质作用(外营力作用)引起的,前者主要控制大尺度的地形起伏,后者则塑造小尺度的地表形态。地表分维值可以指示地表的发育成熟度,该地区小尺度的结构分维值大于大尺度的构造分维值表明其处于地表形态的发育晚期。此外,地表的分形尺度可以来用确定构造活动尺度,从而指导构造地质与找矿勘探研究。     

Geochemistry of Ore Fluids and Rb-Sr Isotopic Dating for the Wulong Gold Deposit in Liaoning, China

On the basis of detailed geological studies of the Wulong gold deposit, three metallogenic stages can be identified. With quartz fluid inclusions as an object of study, the authors investigated phase characteristics, compositional variations, temperature and pressure changes, fluid evolution, Pb isotope tracing and Rb-Sr isotopic dating of fluid inclusions entrapped in the above three metallogenic stages. The results show that Na+ is decreased obviously with metallogenic evolution, while K+ and other cations and gas compositions (H2, CO, CH4 and CO2) are increased slightly, and that the temperature and salinity vary in a pulsating manner along with the metallogenic evolution. Inverse calculation of hydrogen and oxygen isotopes indicate that at the first metallogenic stage the fluids were magmatic water, at the second stage they were dominated by magmatic water with a minor amount of meteoric water involved, and at the third stage, i.e., the final stage of metallogenesis, the fluids were composed complete     

山东招远金岭金矿埠南矿区1#脉流体特征及成矿物理化学条件研究

金岭金矿埠南矿区成矿流体成分特征显示流体为有幔源流体参与的岩浆水与大气水的混合流体。均一法测温表明成矿温度在 10 3～ 35 2℃ ,变化较大 ;通过Shenberger等和Hayashi等LogfO2 - pH图解 ,温度较低的成矿中期阶段 (2 5 0℃± )流体系统中的金明显比早期阶段 (30 0℃± )富集。成矿流体中金主要以Au(HS) -2 形式存在。根据含CO2 三相包体估算 ,流体压力在 5 1～ 70MPa之间。根据Sibson等断裂带流体垂直分带曲线 ,在流体压力为4 0～ 370MPa时 ,断裂带流体压力和深度之间为非线性关系 ,成矿深度既不能用静水压力梯度也不能用静岩压力梯度来计算 ,应该用特定的流体压力和深度关系式计算。通过分段拟合深度和压力之间的关系式计算出金岭金矿成矿深度在 5 .7～ 6 .78km之间 ;按照Gebre Mariam等提出太古代后生金矿深度分类 ,属典型中成脉型金矿。     

葡萄石的热膨胀性与压缩性及其地质意义

利用同步辐射X射线衍射及拉曼光谱技术对葡萄石分别进行了原位高温及原位高压实验。原位高温实验结果表明葡萄石的热膨胀系数为K=1. 77(3)×10~(-5)K~(-1),轴向热膨胀系数具有各向异性(α_aα_bα_c),葡萄石在1073K时开始发生脱水反应,分解为钙长石及硅灰石。原位高压X射线衍射实验结果表明,在大于12. 4GPa时,葡萄石的晶胞参数发生不连续变化,可能发生了相变;在24. 0GPa左右,葡萄石发生不可逆的非晶化转变。原位高压拉曼光谱表明,葡萄石在12. 6GPa左右发生相变,这一相变很可能与其[(Si,Al)O_4]四面体中的Si发生有序排列有关。结合葡萄石的热膨胀性及压缩性,我们确定了葡萄石在高温高压下的稳定范围,这一结果对认识上地幔中含水矿物的状态以及地幔中水的来源有重要意义。     

冈底斯岩浆弧东端石榴斜长角闪岩的晚白垩世岩浆与变质作用记录及构造意义

冈底斯岩浆弧位于青藏高原拉萨地体南部,形成在新特提斯洋向北俯冲的安第斯型造山和印度与欧亚大陆碰撞的喜马拉雅型造山过程中,是研究青藏高原中-新生代构造演化的理想地区。本文对冈底斯岩浆弧东端石榴斜长角闪岩进行了岩石学、相平衡模拟以及锆石U-Pb年代学研究。石榴斜长角闪岩主要由石榴石、角闪石、斜长石、绿帘石、白云母和石英组成,含少量金红石和钛铁矿,具有基性岩浆岩的化学成分。相平衡模拟结果表明,石榴斜长角闪岩经历了高压麻粒岩相变质作用和部分熔融,峰期变质作用的温度和压力条件为～820℃和～1.67GPa,形成深度相当于55km。石榴斜长角闪岩中的锆石具有继承的岩浆核和变质边。锆石岩浆核具有条带状环带,相对高的HREE含量(平均值为1150×10~(-6))和高的Th/U比值(0.51～0.95),给出了90.4±1.7Ma(MSWD=0.32)的原岩结晶年龄。锆石的变质边不具环带,具有较低的HREE含量(平均值为58.5×10~(-6))和低的Th/U比值(0.29～0.40),给出了86.7±5.7Ma(MSWD=0.15)的变质年龄。本文研究结果表明,冈底斯岩浆弧东端晚白垩世辉长岩经历了近侵入同期的高压高温变质作用和部分熔融,大体积幔源岩浆的底垫和增生导致岩浆弧发生了显著的新生地壳生长和加厚。