Fault Characteristics in Longmen Mountain Thrust Belt,Western Sichuan Foreland Basin,China

Through field geological survey,the authors found that abundant thrust faults developed in the Longmen (龙门) Mountain thrust belt.These faults can be divided into thrust faults and strike-slip faults according to their formation mechanisms and characteristics.Furthermore,these faults can be graded into primary fault,secondary fault,third-level fault,and fourth-level fault according to their scale and role in the tectonic evolution of Longmen Mountain thrust belt.Each thrust fault is composed of several secondary faults,such as Qingchuan (青川)-Maowen (茂汶) fault zone is composed of Qiaozhuang (乔庄) fault,Qingxi (青溪) fault,Maowen fault,Ganyanggou (赶羊沟) fault,etc..The Longmen Mountain thrust belt experienced early Indosinian movement,Anxian (安县) movement,Yanshan (燕山)movement,and Himalayan movement,and the faults formed gradually from north to south.     

柴达木盆地东部36～18kaB.P.期间的孢粉记录及其气候环境

对柴达木盆地察尔汗古贝壳堤剖面的沉积物进行孢粉分析,结果显示这个地区植被与气候在晚更新世中晚期经历以下几个阶段的变化:36.2～31.2kaB.P.(未校正14C年代,下同)期间,以禾本科、藜科、蒿属、莎草科为主,发育草原-草甸植被,气候温和湿润,盘星藻出现较多,反映淡水湖泊,水深在10m左右;31.2～27.6kaB.P.期间,松属、云杉属、桦属等为主的木本植物的含量增加,周围山地森林发育,表明气候温暖,降水量增多。但由于蒸发量大,有效湿度下降,荒漠成分柽柳属等增加,盘星藻在30kaB.P.以后消失,反映湖泊盐度增大;27.6～23.3kaB.P.期间,植被中荒漠成分显著增加,周围山地森林萎缩,气候趋向相对寒冷干旱,湖面积缩小;23.3～18.0kaB.P.,孢粉浓度很低,蒺藜科、藜科等荒漠成分明显增加,植被稀疏,已趋向荒漠化草原,反映气候寒冷干旱。从整个剖面来看,主要的陆生植物孢粉类型为禾本科、柽柳属、蒺藜科、麻黄属、松属、云杉属、柏科、胡桃属和桦属等,藜科和蒿属含量很少,这与柴达木盆地东部地区的表土分析结果完全不同,也与其他草原以及荒漠草原的表土花粉结果相异。这说明晚更新世中晚期柴达木盆地东部地区的植被和现在无法进行比较,气候环境与现在显著不同。     

Applications of AnnAGNPS model for soil loss estimation and nutrient loading for Malaysian conditions

The study evaluated the performance and suitability of AnnAGNPS model in assessing runoff, sediment loading and nutrient loading under Malaysian conditions. The watershed of River Kuala Tasik in Malaysia, a combination of two sub-watersheds, was selected as the area of study. The data for the year 2004 was used to calibrate the model and the data for the year 2005 was used for validation purposes. Several input parameters were computed using methods suggested by other researchers and studies carried out in Malaysia. The study shows that runoff was predicted well with an overall R² value of 0.90 and E value of 0.70. Sediment loading was able to produce a moderate result of R² = 0.66 and E = 0.49, nitrogen loading predictions were slightly better with R² = 0.68 and E = 0.53, and phosphorus loading performance was slightly poor with an R² = 0.63 and E = 0.33. The erosion map developed was in agreement with the erosion risk map produced by the Department of Agriculture, Malaysia. Rubber estates and urban areas were found to be the main contributors to soil erosion. The simulation results showed that AnnAGNPS has the potential to be used as a valuable tool for planning and management of watersheds under Malaysian conditions.     

地震瞬时属性分析技术在岩溶勘查中的应用

介绍地震瞬时属性分析技术的原理及处理方法,分别对岩溶在地震剖面、瞬时振幅剖面、瞬时频率剖面、瞬时相位剖面上的表现特征作了说明.并结合实际资料进行多参数解释,进而确定地下岩溶的发育情况、分布范围和规模,同时对异常进行钻井验证,结果表明,地震瞬时属性分析技术比常规地震处理方法能更好地排除干扰,确定岩溶异常.     

应用混合分布研究银川平原地下水埋深对植被的影响

银川平原地处西北干旱地区,自然生态环境在西北地区具有典型性。研究银川平原的生态环境,需要研究植被,它反映多种因素的作用。在影响植被的各种因素中,地下水对植被生长的影响非常重要,但将地下水对植被生长的影响进行定量化分离并不容易。近年来,用混合分布函数处理大量数据的方法受到越来越多的关注,但是混合分布函数的参数求解一直比较困难。文章提出了一种基于混合分布函数和数据直方图之间的关系,用最小二乘法估计参数的新方法;并用这种方法,结合银川平原遥感数据中的归一化植被指数NDVI,对地下水埋深与植被生长的关系进行定量分析,得到地下水埋深对植被影响所服从的正态分布密度函数。     

Zircon M257 ‐ a Homogeneous Natural Reference Material for the Ion Microprobe U‐Pb Analysis of Zircon

We introduce and propose zircon M257 as a future reference material for the determination of zircon U‐Pb ages by means of secondary ion mass spectrometry. This light brownish, flawless, cut gemstone specimen from Sri Lanka weighed 5.14 g (25.7 carats). Zircon M257 has TIMS‐determined, mean isotopic ratios (2s uncertainties) of 0.09100 ± 0.00003 for ²⁰⁶pb/²³⁸U and 0.7392 ± 0.0003 for ²⁰⁷pb/²³⁵U. Its ²⁰⁶pb/²³⁸U age is 561.3 ± 0.3 Ma (unweighted mean, uncertainty quoted at the 95% confidence level); the U‐Pb system is concordant within uncertainty of decay constants. Zircon M257 contains ～ 840 μg g^?1 U (Th/U ～ 0.27). The material exhibits remarkably low heterogeneity, with a virtual absence of any internal textures even in cathodoluminescence images. The uniform, moderate degree of radiation damage (estimated from the expansion of unit‐cell parameters, broadening of Raman spectral parameters and density) corresponds well, within the “Sri Lankan trends”, with actinide concentrations, U‐Pb age, and the calculated alpha fluence of 1.66 × 10¹⁸ g^?1. This, and a (U+Th)/He age of 419 ± 9 Ma (2s), enables us to exclude any unusual thermal history or heat treatment, which could potentially have affected the retention of radiogenic Pb. The oxygen isotope ratio of this zircon is 13.9%o VSMOW suggesting a metamorphic genesis in a marble or calc‐silicate skarn.     

煤矿区沉降与遥感监测方法探讨

以晋城市煤矿区沉降研究为例,介绍了应用遥感图像调查与数字高程模型相结合的方法进行煤矿区沉降研究及监测。监测结果表明,沉降区主要集中在该区域的西北部,沉降区面积较大,沉降原因是大矿开采3#煤层,导致地面沉降,只有2处沉降由小煤矿开采9#煤层引起。经验证,具体位置虽有差异,但沉降区基本与实际吻合。依据当前合成孔径雷达干涉测量技术的发展,对煤矿区遥感综合监测方法进行了讨论。     

南黄海北部前陆盆地的构造演化与油气突破

南黄海北部盆地是我国近海海域中唯一由中生代陆-陆碰撞造山作用形成的前陆盆地。其构造演化经历了4个阶段:(1)前造山期大陆边缘盆地阶段(Z—T2);(2)苏鲁造山带晚期前陆盆地阶段(J3—K);(3)造山期后陆内断陷盆地阶段(K2t—E);(4)区域沉降覆盖阶段(N—Q)。对其中陆内断陷盆地的详细调查研究结果表明,盆地内晚白垩世泰州组烃源岩发育,具有4套储盖组合,圈闭构造多,成藏配套条件好,计算其石油资源量约20×108t,是当前在南黄海获取油气重要突破的首选区域。     

CSU－RAMS模式在区域气侯模拟中的应用

将ＣＳＵ－ＲＡＭＳ（中尺度）数值模式改造成“区域气候数值模式”以及进行区域气候数值模拟的试验研究。说明将有限区域中尺度数值模式与ＧＣＭ模式嵌套应用到区域气候数值模拟研究上能够取得有意义的结果。它能在一定程度上改善ＧＣＭ模式的不足。可以更为细致地描述大气环流的变化特征,是了解区域气候变化的有效方法之一。     

Nonthermal radio emission from hot star winds

Nonthermal radio emission has been observed from some of the most luminous hot star winds. It is understood to be synchrotron radiation of the relativistic electrons in the winds. To understand how the electrons are accelerated to such high energies and to correctly explain the observed radio flux and spectra require an exhaustive investigation of all the relevant physical processes involved and possibly point to a complex wind structure. In this paper we discuss the logical path toward a comprehensive model of the nonthermal radio emission from hot star winds. Based on the available observational data and fundamental theoretical considerations, we found that the only physically viable and self-consistent scenario is:the nonthermal radio emission is synchrotron radiation of relativistic electrons the electrons are accelerated by shocks via the first-order Fermi mechanism the acceleration has to be in situ in the radio emitting region the shocks formed at the base of the winds have to propagate to beyond the radio photosphere).