全球变暖、构造运动与沙漠化

采用统计分析与综合分析方法 ,研究了全球变暖、构造活动、地球 (以及月球和行星 )轨道效应、太阳活动等对降水的影响。认为构造活动、地震、气候变暖与降水或洪涝灾害有一定关系 ;地球的轨道效应是地球气候变化的重要因素 ,从而与旱涝相关 ;月球行星轨道效应和太阳活动均与旱涝有明显的对应关系。气候变冷和构造活动变弱是沙漠化的主要原因 ,人类活动则加速了沙漠化的进程     

Three-dimensional finite element modelling of stress relaxation tests in anisotropic clayey medium: direct problem and back analysis

This paper deals with a new strategy for initial stress identification by stress relaxation methods, coupled with finite element calculation, and applied to the overcoring test. The back-analysis of such a test uses an inversion method which consists in the minimisation, with a gradient-based algorithm, of a cost functional of least-squares type, which quantizes the difference between measured and computed strains. The computed strains are assessed by three-dimensional finite element modellings of the overcoring test. The inversion methodology is applied to a recent in situ overcoring test performed at Mont Terri laboratory, Switzerland. The inversion gave good results and allows us to validate the inversion methodology. The constitutive law considered for this application is transverse isotropic elasticity but the inversion method developed is applicable to most constitutive laws and every kind of in situ test.     

中新生代天山地区隆升历史的裂变径迹证据

本文对天山及其两侧盆地的8条典型地质剖面进行了大量的磷灰石裂变径迹测试,重点分析了天山地区不同区域的抬升历史的差异。结果表明天山主要经历4次构造抬升过程,每次抬升的范围并不相同,且存在东西差异:①早白垩世抬升,在天山南北两侧都有发生,且南边抬升早,北边抬升晚。本次抬升导致早中侏罗世天山地区准平原化状态开始解体,盆山分异开始出现;②晚白垩世抬升,从约96Ma开始,天山南侧为盆山同升的区域性隆升,天山北侧的抬升主要发生在东部地区;③古近纪抬升,从约46Ma开始,主要发生在中天山和南天山,造成天山两侧盆地物源区的重大变化,本次抬升为印度-亚洲碰撞在天山地区产生的最早的远程效应;④中新世以来的抬升,从约25Ma开始,主要发生在库车盆地北缘和北天山—准噶尔南缘。从抬升剥蚀量来看,从东向西逐渐变大。     

THE DYNAMICAL BASIS OF GEOSTROPHIC ADJUSTMENT MOTIONS IN TROPICS

Some dynamic constrains in the process of the tropical baroclinic geostrophic adjustment arediscussed.The dispersion equation of three-dimensional inertia-gravitational wave and the equation oftemporal conservation of potential vorticity are given,without considering the gradient of planetarypotential vorticity.It indicates that the motions will be horizontal,meaning that Taylor-Proudmantheorem is still right for tropics.At the same time,the semi-geostrophic balance is easier to appear inthe tropical belt.Therefore the motions are generally horizontal and non-divergent,but still arestratified after the geostrophic balance establishes.     

利用高程数据修正NOAA AVHRR轨道定位信息

在没有考虑高程数据的预处理方法得到的NOAA AVHRR资料中, 每条扫描线数据中的51点经纬度定位信息常常有误差, 尤其是在海拔较高、距卫星星下点较远的定位点, 其定位信息与实际差别很大。针对这种情况, 该文描述了一种引入高程数据并结合51点定位信息对2048个扫描点定位进行快速、简易的订正方法, 可有效地修正AVHRR资料预处理未考虑高程信息引起的经纬度定位偏差, 以便于对分辨率和定位精度要求不高的用户更好地使用AVHRR数据。     

硫镍矿晶体的人工合成与X射线衍射分析

本研究采用钛合金密封式高压釜,在温度为600℃,压力为888 atm下合成具有八面体晶形的硫镍矿单晶。实验证明,用淬火的方法保留硫镍矿高温相(β)结构是不可能的。 低温相(α)硫镍矿属三方菱面体类,空间群为R32。在536℃时低温相硫镍矿转变为高温相(β),并在805±2℃时熔化。β-硫镍矿(Ni_(3±x)S_2)属等轴晶系,立方面心格子(F),晶胞参数α=5.208A,可能的点群有m3,432,m3m。     

银河系疏散星团中的蓝离散星(英文)

作为目前研究复杂恒星系统的有力工具 ,星族合成方法是建立在单星演化理论基础之上的 ,因此 ,必然有其不完善性存在 ,尤其当系统中的双星成分不容忽视时。作为演化星族合成方法的基本单元 ,简单恒星星族模型的构成即排除了双星贡献。本文中 ,我们以银河系疏散星团为简单恒星星族模板 ,构造出一系列简单恒星星族积分光谱。从中我们可以看到 :蓝离散星这类理论上主要来源于双星系统的恒星 ,对星团积分光谱的紫外及蓝端有很大影响 ,从而造成简单恒星星族积分光谱能量分布的改变。这种改变势必影响对星团年龄及其它一些物理参量的判定 ,并最终影响星族合成的结果。同时 ,若以 (B -V )色指数进行度量 ,蓝离散星对简单恒星星族积分颜色的影响可达到 30 %。工作中 ,我们选取了 2 6个年龄在1x10 1 0 ～ 6x10 1 0 年之间的疏散星团为样本进行统计研究。     

宁强碳质球粒陨石的岩石、矿物特征研究

宁强碳质球粒陨石的结构复杂,有粒状、斑状和炉条状等结构。球粒分为玻璃质和晶质两种。聚合体含量丰富、形态各异,有钢性和塑性两种聚合体。目前已查明的矿物有20余种,主要是镁橄榄石、贵橄榄石、烦火辉石、普通辉石和黄长石类矿物等。在宁强陨石中出现罕见的方解石、白云石。不透明矿物有陨硫铁、铁纹石—镍纹石、镍铁矿、磁铁矿和非晶质碳质。Fe/SiO_2为0.71—0.72,SiO_2/MgO为1.37—1.40。根据化学及矿物特征,该陨石应属C_2群。     

Mapping and compositional analysis of mare basalts in the Aristarchus region of the Moon using Clementine data

The process of accurately defining and outlining mare basalt units is necessary for constraining the stratigraphy and ages of basalt units,which are used to determine the duration and the flux of lunar volcanism.We use a combination of Clementine’s five-band ultraviolet/visible data and TiO2and FeO abundance distribution maps to define homogenous mare basalt units and characterize their compositional variations(with maturity)in the Aristarchus region.With 20 groups of distinct mare basaltic soils identified using the method in this paper,six additional spectrally defined areas and five basaltic units are constructed,and their mineralogic quantization values provide new constraints on their temporal and spatial evolution.Our results indicate that the Aristarchus region has diverse basalt units and a complex history of volcanic evolution.We also demonstrate that the techniques,from which spectrally distinct mare basalts can be mapped,performed well in this study and can be confidently expanded to other mare regions of the Moon.     

Early Pliocene Paleoceanography of the Vityaz Fracture Zone, Central Indian Ridge

Planktic foraminifera from the calcareous substrate of a ferromanganese crust in the Vityaz Fracture Zone （VFZ）, Central Indian Ridge were studied to reconstruct the early Pliocene paleoceanography of this region. Eleven species of planktic foraminifera were encountered, among them Globorotalia menardii, Neogloboquadrina dutertrei, Globigerina bulloides and Globigerinoides tuber are prominent. Predominance of N. dutertrei in the top 3 cm of the carbonate substrate is attributed to an influx of fresh water which eventually triggered their productivity by increasing the nutrient level. The presence of G. bulloides and G. menardii in significant proportions in deeper layers suggests the prevalence of open ocean upwelling. The bulk chemical compositions of the substrate at different depth intervals indicates higher enrichment of trace metals in the upper sections which could have been supplied through oceanic water by the chemical weathering of terrestrial matter during the peak of Pliocene Asian monsoon. Thus, it is concluded that during the early Pliocene the biogenic components of the substrate were distinctly contributed by both upwelling and productivity triggered by an influx of fresh water originating from the intensification of the Asian monsoon during the early Pliocene Period.