中国北方沙漠地区第四纪研究的新进展

采用第四纪地质工作方法,通过近十年来的野外调查与室内分析工作,对中国北方沙漠地区古风成沙的分布、类型、特征,沙漠及沙漠化的形成时代、发展模式、性质、沉积环境、成因以及防治对策等方面取得了许多新认识。     

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STUDY ON THE INTERACTION BETWEEN NDVI PROFILE AND THE GROWING STATUS OF CROPS

Daily and ten-day Normalized Difference Vegetation Index(NDVI) of crops were retrieved from meteorological statellite NOAA AVHRR images ,The temporal variations of the NDVI were analyzed during the whole growing season,and thus the principle of the interaction between NDIV profile and the growing status of crops was discussed,As a case in point,the relationship between integral NDVI and winter wheat yield of Henan Province in 1999 had been analyzed.By putting integral NDVI values of 60 sample counties into the winter wheat yield-integral NDVI coordination,scattering map was plotted. It demonstrated that integral NDVI had a close relation with winter wheat yield.These relation could be described with linear,cubic polynomial ,and exponential regression,and the cubic polynomial regression was the best way,In general ,NDVI reflects growing status of green vegetation ,so crop monitoring and crop yield estimation could be realized by using remote sensing technique on the basis of time serial NDVI data together with agriculture calendars.     

A comparison of MODIS-derived cloud amount with visual surface observations

Two main sources for global cloud climatologies are visual surface observations and observations made by spaceborne sensors. Satellite observations compared with surface data show in most cases differences ranging from − 15% up to − 1%, depending on sensor and observation conditions. These differences are partially controlled by sensors' cloud detection capabilities — a higher number of spectral bands and higher spatial resolution are believed to allow discrimination of clouds from land/ocean/snow background. A Moderate-Resolution Imaging Spectroradiometer (MODIS) produces images of the atmosphere in 36 spectral bands with a spatial resolution of 250–1000 m, thus having a capacity for cloud detection far more advanced than other operating sensors. In this study, instantaneous MODIS cloud observations were compared with surface data for Poland for January (winter) and July (summer) 2004. It was found that MODIS observed 4.38% greater cloud amount in summer conditions and 7.28% in winter conditions. Differences were greater at night (7–8%) than in daytime (0.5–7%) and correlations ranged between 0.577 (winter night) and 0.843 (winter day, summer day and night).     

四川盆地川西坳陷高异常地层压力分布特征

本文通过分析川西坳陷２０多个含气构造的主要地层压力资料，对川坳陷高异常地层压力的分布特征有了一定的认识。认为川西高异常地层压力在纵向层位上主要分布于侏罗系和上三叠统，压力分段明显，相同的力段在不同的构造既不等时也不等深；在平面上高异常地层压力分布广泛，超高压区刚分布于川西北地区，并形成两个超高压中心，整个高异常地层压力的分布虽然总体上基本一致，但在不同层位，不同时期也存在着差异。     

秦岭造山带基本组成与结构及其构造演化

秦岭造山带主要由三大套构造岩石地层单元组成，经历了三个主要演化阶段：1．前寒武纪古老基底形成演化阶段，2．主造山期（Pt3—T2）板块构造演化阶段，3．中新生代陆内构造演化阶段。在早中元古代以扩张构造体制占主导，形成裂谷与小洋盆兼杂并存的基本构造格局，经10—8亿年晋宁期从扩张垂向加积增生构造体制为主向以侧向增生为主的板块构造体制的过渡，于晚元古代中晚期开始进入板块构造演化阶段。在晚古生代早期由于东古特提斯洋的形成，扬子板块北缘沿秦岭南部扩张打开，形成华北板块、扬子板块及其间的秦岭微板块，沿商丹和勉略二缝合带自南向北俯冲消减碰撞，于中三叠世最后全面陆陆碰撞造山，而后又发生了强烈陆内造山作用，终成今日之秦岭山脉面貌。现今的秦岭造山带岩石圈结构是一正在调整演化中的具流变学分层的“立交桥式”三维结构，上部地壳呈多层逆冲推覆迭置的不对称扇形几何学模式，岩石圈中部则是成水平状流变层，而深部地幔则是最新调整的近南北向的地球物理异常状态与结构，形成从下到上构造方向近乎正交的圈层非耦合关系。     

井间电阻率层析成象的平滑度约束反演

井间电阻率层析成象是一种探测地下浅部精细结构的物探方法，它主要用于解决工程地质问题。本文采用２．５－Ｄ有限元法，针对井间电阻率层析成象中的ＡＭ观测系统进行了反演成象计算。文中首先计算了灵敏度矩阵，然后给出了一种电阻率层析成象反演算法—平滑度约束反演，理论模型的计算和实际资料的处理，都证明了该算法的有效性     

北冰洋西部表层沉积物矿物学特征及其物质来源

对北冰洋西部79个表层沉积物样品进行了全岩X射线衍射矿物组成分析,结合洋流和地质背景,探讨各矿物分区的物质来源。矿物组合分区表明研究区物质来源变化较为复杂:(1)在楚科奇海的中部靠近白令海峡处长石含量很高,主要是阿纳德尔流携带的来自阿纳德尔河的沉积物;在楚科奇海的西侧的长石含量也较高,且与其他矿物组合分区相比,角闪石含量较高,这是因为受阿纳德尔流和东西伯利亚沿岸流的双重影响,沉积物来自西伯利亚陆地的一些高含长石的火山岩及沉积岩等。在楚科奇海的东侧,石英含量很高,来源为阿拉斯加沿岸流携带的育空河及卡斯奎姆河的沉积物。在阿拉斯加北部,碳酸盐岩和石英含量高,这与马更些河搬运的沉积物有关;(2)北冰洋西部深水区中加拿大海盆的南端和中部方解石和白云石的含量较低,说明受波弗特环流携带的加拿大北极群岛的碳酸盐影响相对较小,且与其他矿物组合分区相比,云母含量最高,说明沉积物主要来源为来自拉普捷夫海的海冰沉积物;此外,一些黏土级细粒物质可能由大西洋中层水携带而来。深水区的其他海域以方解石和白云石含量高为特点,主要受波弗特环流的影响,来源主要为加拿大北极群岛的班克斯岛和维多利亚岛;此外,还受来自西伯利亚陆架,主要是拉普捷夫海沉积物的影响。     

The tectono‐stratigraphic evolution of the Austral Basin and adjacent areas against the background of Andean tectonics,southern Argentina,South America

The Austral Basin (or Magallanes Basin) in southern Argentina is situated in a highly active tectonic zone. The openings of the South Atlantic and the Drake Passage to the east and south, active subduction in the west, and the related rise of the Andes have massively influenced the evolution of this area. To better understand the impacts of these tectonic events on basin formation to its present‐day structure we analysed 2D seismic reflection data covering about 95 000 km² on‐ and 115 000 km² offshore (Austral ‘Marina’ and Malvinas Basin). A total of 10 seismic horizons, representing nine syn‐ and post‐ rift sequences, were mapped and tied to well data to analyse the evolution of sedimentary supply and depocenter migration through time. 1D well backstripping across the study area confirms three main tectonic stages, containing (i) the break‐up phase forming basement graben systems and the evolution of the Late Jurassic – Early Cretaceous ancient backarc Austral/Rocas Verdes Basin (RVB), (ii) the inversion of the backarc marginal basin and the development of the foreland Austral Basin and (iii) the recent foreland Austral Basin. Synrift sedimentation did not exceed the creation of accommodation space, leading to a deepening of the basin. During the Early Cretaceous a first impulse of compression due to Andes uplift caused rise also of parts of the basin. Controlling factors for the subsequent tectonic development are subduction, balanced phases of sedimentation, accumulation and erosion as well as enhanced sediment supply from the rising Andes. Further phases of rock uplift might be triggered by cancelling deflection of the plate and slab window subduction, coupled with volcanic activity. Calculations of sediment accumulation rates reflect the different regional tectonic stages, and also show that the Malvinas Basin acted as a sediment catchment after the filling of the Austral Basin since the Late Miocene. However, although the Austral and Malvinas Basin are neighbouring basin systems that are sedimentary coupled in younger times, their earlier sedimentary and tectonic development was decoupled by the Rio Chico basement high. Thereby, the Austral Basin was affected by tectonic impacts of the Andes orogenesis, while the Malvinas Basin was rather affected by the opening of the South Atlantic.     

The masers of E-type methanol in orion KL and SGR B2

Using a simplified model the statistical equilibrium and radiative transfer equations of E-type-CH₃OH are solved for Orion KL and SgrB2. According to our calculation results and the observation data taken by Matsakiset al. (1980) and Morimotoet al. (1985a, b), the physical conditions of both sources are estimated. In theJ ₂-J ₁ E methanol maser region of Orion KL, the density, kinetic temperature, dust temperature, and the fractional abundance are 0.8–2×10⁶ cm^–3, 150, 30–90 K, 0.8–8×10^–6. In the 4_–1-3₀ E and 5_–1-4₀ E methanol maser region of Sgr B2 the correspondance physical conditions above are 10⁴ cm³, 45, 23 K, and 7×10^–7, respectively.