Worldview2数据在西昆仑老并—赞坎矿集区铁矿调查中的应用

正赞坎—老并矿集区位于新疆塔什库尔干县,属于西昆仑成矿带塔合曼—西若达坂铁矿成矿区,研究区高寒缺氧,地形切割强烈,人烟稀少,交通极为不便,面积性的野外矿产地质调查工作面临挑战,难以获取系统、全面、翔实的资料(王俊峰等,2013)。遥感技术作为当今矿产调查的主要技术手段之一,越来越得到重视,特别是高分辨率的WorldView-Ⅱ数据能够提供全色0.46 m和多光谱     

Volcanic and Scientific Activity at Kick ’em Jenny Submarine Volcano 2001–2002: Implications for Volcanic Hazard in the Southern Grenadines,Lesser Antilles

Kick em Jenny submarine volcano, ~8 km north of Grenada, has erupted at least 12 times since it was first discovered in 1939, making it the most frequently active volcano in the Lesser Antilles arc. The volcano lies in shallow water close to significant population centres and directly beneath a major shipping route, and as a consequence an understanding of the eruptive behaviour and potential hazards at the volcano is critical. The most recent eruption at Kick em Jenny occurred on December 4 2001, and differed significantly from past eruptions in that it was preceded by an intensive volcanic earthquake swarm. In March 2002 a multi-beam bathymetric survey of the volcano and its surroundings was carried out by the NOAA ship Ronald H Brown. This survey provided detailed three-dimensional images of the volcano, revealing the detailed morphology of the summit area. The volcano is capped by a summit crater which is breached to the northeast and which varies in diameter from 300 to 370 m. The depth to the summit (highest point on the crater rim) is 185 m and the depth to the lowest point inside the crater is 264 m. No dome is present within the crater. The crater and summit region of Kick em Jenny are located at the top of an asymmetrical cone which is about 1300 m from top to bottom on its western side. It lies within what appear to be the remnants of a much larger arcuate collapse structure. An evaluation of the morphology, bathymetry and eruptive history of the volcano indicates that the threat of eruption-generated tsunamis is considerably lower than previously thought, mainly because the volcano is no longer thought to be growing towards the surface. Of more major and immediate concern are the direct hazards associated with the volcano, such as ballistic ejecta, water disturbances and lowered water density due to degassing.     

等值线追踪生成等值面过程中的算法策略

等值面的生成可以通过等值线追踪来实现。现有的等值线追踪方法不但缺少对具体等值线追踪策略的详细描述,而且还缺少岛的拓扑关系分析及等值面属性的判断过程。本文通过分析等值面生成过程中的等值线追踪方法,提出了一种基于等值线追踪的等值面快速生成算法,并给出了追踪过程中的几个重要的数据结构及追踪策略,能够解决多种情况下的等值面生成问题,并重点对等值线追踪过程中岛的处理、 拓扑关系分析、 等值面属性判断等方面进行剖析。实际应用表明,该算法具有较好的鲁棒性,并能得到较高的算法追踪效率。     

阿尔金山北缘冰沟蛇绿混杂岩中辉长岩锆石SHRIMP U-Pb定年及其地质意义

冰沟蛇绿混杂岩是阿尔金山红柳沟蛇绿混杂岩带的东段部分,岩石组合包括蛇纹岩、方辉橄榄岩、辉石岩和辉长岩等。蛇纹岩具高Mg,Mg/Fe值大于9,低Al、Ca、Na、K为特征,从稀土元素和微量元素特征来看,基性辉长岩和洋壳以及洋中脊玄武岩极为相似,而超基性岩与原始地幔较为接近。辉长岩获得锆石SHRIMP年龄为449.5±10.9Ma。蛇绿混杂岩的围岩为一套巨厚的碎屑岩、火山碎屑岩、火山岩,以及部分碳酸盐岩构成,其中含有具有洋中脊特征的枕状构造玄武岩,以及放射虫硅质岩,放射虫时代为奥陶纪中晚期,与辉长岩的SHRIMP年龄一致。这些证据进一步证实了红柳沟一带存在早古生代洋盆的地质事实。     

云南地区波速比异常图像的南北差异

动态追踪了云南地区第4 强震活跃期6 .3 级以上强震前波速比异常图像,显示出明显的南北差异:滇西南的1988 年11 月6 日澜沧- 耿马7 .6 、7 . 2 级和1993 年1 月27 日普洱6 .3 级强震发生在低波速比异常区内; 中缅边境上的1992 年4 月23 日6 .7 、6 .8 级和1995 年7 月12 日孟连西7 .2 级强震发生在低波速比异常区边缘;而滇西北的1996 年2 月3 日丽江7 .0 级、1976 年11 月7 日、12 月14 日宁蒗6 .7 、6 .4 级和滇东的1995 年10 月24 日武定6 .5 级强震却都发生在高波速比异常区内.强震前近震震级 ML 与持续时间震级 MD 的震级差的南北差异也进一步证实了波速比异常的差别.     

代表性人口空间分布数据集的精度评价——以2010年广东省为例

以人口密度差异显著的广东省为研究区,比较Worldpop、GPW v4和2种中国公里网格人口分布数据集的空间分布一致性,并以第六次全国人口普查数据为真值,按人口密度分为高、中、低3组,从误差的数值分布和空间分布两方面定量评价4种数据集的精度,最后讨论估算误差的可能来源及数据适用性。结果表明,4种网格人口数据集中Worldpop整体精度最高,且在人口密集区的精度也是最高;GPW v4在低人口密度和中人口密度区域精度略高于Worldpop,但对镇街内人口分布细节刻画不够详细;2种中国公里网格人口分布数据集精度较前两者低,主要受空间化方法和模型变量的选择所限制。Worldpop适合用于人口密度中等及人口密度高区域的精细化研究,GPW v4适合用于长时序、最小研究单元大于镇街的研究,第一种中国公里网格人口分布数据集适合用于需要考虑镇街内人口分布和空间异质性的研究,第二种中国公里网格人口分布数据集适用于需要考虑人口分布细节和空间格局变化的长时序研究。     

新疆西准噶尔萨尔托海蛇绿混杂岩形成时代及构造环境分析

萨尔托海蛇绿混杂岩是西准噶尔地区达拉布特蛇绿混杂岩带的重要组成部分,其形成时代和构造环境颇具争议。通过LA-ICP-MS锆石微区原位U-Pb同位素测年,获得其中辉长辉绿岩的 206Pb/238U 加权平均年龄为388.8±1.1 Ma,确定该蛇绿混杂岩形成于中泥盆世。岩石地球化学分析表明,纯橄岩(蛇纹岩)属于低Si、低碱、高Mg的变质橄榄岩,REE呈∑REE 偏低的平坦型分布模式,Cr、Ni和Co含量较高,变玄武岩属于高Ti、富Mg、富Fe、偏碱的拉斑系列,REE分布模式呈现 ∑REE 偏低、Eu异常不明显的平坦型曲线,微量元素分布模式为K、Cs、Th、Nb和P相对亏损的平坦型曲线,Zr/Nb比值低,总体表现出与E-MORB相似的特征。综合判断认为,萨尔托海蛇绿混杂岩形成于大陆裂谷向洋盆转化的构造环境,类似于"红海式"洋盆,为进一步深入认识新疆地区众多蛇绿混杂岩的形成构造环境提供了新思路。     

雅鲁藏布江缝合带东段白垩纪混杂岩归属及其构造意义

采用野外地质点观察、岩相分析及碎屑锆石U-Pb定年方法,对雅鲁藏布江缝合带东段南侧的朗县白垩纪混杂岩（KL）进行研究。分析结果显示,以乃东-金东-莫洛断裂为界,该断裂南侧具有以板岩/千枚岩为主夹砂岩、粉砂岩的特征,属于海底扇沉积,其碎屑锆石年龄谱有230Ma和530Ma 2个峰值,与南部的上三叠统复理石郎杰学群极其相似;而该断裂北侧狭长地带的KL则主要为陆棚相板岩与大理岩,属于拉萨南缘沉积。为此认为,南部主体属于上三叠统郎杰学群,暗示印度大陆与欧亚大陆在西藏东南部的缝合碰撞边界可能是乃东-金东-莫洛断裂,而不是北侧的泽当-加查-朗拉岗则断裂或南侧的乃东-曲松-白露断裂。     

新疆伊吾阿勒吞昆多蛇绿混杂岩特征

前人将唐巴勒-卡拉麦里缝合线置于伊吾县以南哈尔里克山塔水河一线。1993年巴瑞士等在伊吾西北大黑山发现超镁铁岩-镁铁岩洋壳残片,认为卡拉麦里蛇绿岩从伊吾西北大黑山一带向东延伸。2009年笔者参与伊吾县阿尔通盖一带1∶5万区域地质矿产调查工作,于伊吾县以北阿勒吞昆多一带发现阿勒吞昆多蛇绿混杂岩,该蛇绿岩中斜长花岗岩形成于早石炭世((351±6)Ma),大地构造为哈萨克斯坦-准噶尔板块及准噶尔微板块、唐巴勒-卡拉麦里古生代沟弧体系。在研究前人资料基础上,提出阿勒吞昆多蛇绿混杂岩为卡拉麦里蛇绿岩(属唐巴勒-卡拉麦里缝合线)向东延伸部分,唐巴勒-卡拉麦里缝合线(沟弧体系)西起唐巴勒,向东经达拉布特-卡拉麦里-塔克扎勒-大黑山至伊吾县阿勒吞昆多一带,可能延伸至蒙古境内。     

Present Observational Status of the Intermediate Mass Stars: δ Sct Stars, γ Dor Stars and roAp Stars

The present observational status of the Sct stars, Dor stars and roAp stars is discussed. The Sct stars are the most intensively observed of the three groups, but it has become clear that there are severe problems in extracting asteroseismic information from them. Dozens of frequencies are observed, but hundreds of frequencies are predicted from the models; unique matches of observation and theory still elude us. The Sct stars are observationally complex – some recent `best case' campaigns are discussed. It is possible that substantial observational advances for Sct stars may need to await upcoming satellite missions. New Dor stars are beingdiscovered frequently, and new behaviour is being found for them. They constitutean observationally young field. Their pulsational frequency range is being expanded, their position in the HR diagram is becoming better known (but is yet to be fully constrained), and the possibility exists of hybrid Dor – Sct stars that have greatasteroseismic promise, although it is clear such stars are rare, if they do exist. It has been observationally challenging to extract more than a fewfrequencies for any Dor star so far. Exciting spectroscopic discoveries of new behaviour in roAp stars promise unprecedented information about the structure of the peculiar atmospheres ofthose stars – pulsation amplitude and phase in 3D, magnetic field structurein 3D, abundance stratification in 3D, realistic T- for the most peculiarstars – as well as entirely new information about the interaction of pulsation,rotation and magnetic fields. Recent theoretical work has led to new understandingof the previously inexplicable frequency spacing of HR 1217 with new Whole Earth Telescope observations supporting this theory. An `improved oblique pulsator model' has been developed in which the pulsationaxis is not the magnetic axis; this model has passed several observationaltests and new ones are being devised to examine it further.