排序方式： 共有124条查询结果，搜索用时 15 毫秒
41.
利用相似性度量的不同比例尺地图数据网状要素匹配算法 总被引：1，自引：0，他引：1
提出了一种基于相似性度量的不同比例尺地图数据网状要素匹配算法。首先进行结点、弧段的粗匹配,然后利用结点-弧段拓扑关系的相似性和离散Fréchet距离进行精确匹配,匹配过程将几何、语义、拓扑、结点和弧段匹配有效结合起来,最后以可视化方式将不同匹配结果进行显示,以便人机交互。实验表明,该算法可有效地匹配各种复杂情况下的同名道路,并提高匹配的正确率和速度。 相似文献
42.
The low detection limits and multi‐element capability of inductively coupled plasma‐mass spectrometry (ICP‐MS) makes it an attractive option in a wide range of environmental, medical, biological, industrial and archaeological applications. Quadrupole ICP‐MS is used to determine element concentrations in a diverse range of sample types, often very different from the geological applications for which ICP‐MS was originally developed. Whilst modern instruments are robust and capable of a high degree of automation, it is essential that users of both instrumentation and data are aware of the strengths and limitations of the technique. Many people who are now involved with the operation and application of ICP‐MS instruments are not specialists in the field, as was usually the case amongst early operators. This back‐to‐basics review is aimed at the novice user and includes a guide to ICP‐MS instrumentation and performance. Whilst solids, liquids and gases can all be measured by ICP‐MS, discussion of sample introduction is limited to liquids. Requirements for producing good quality data, including aspects of sample preparation, calibration, and methods of interference limitation are also discussed. 相似文献
43.
广西十万大山前陆冲断推覆构造 总被引：8，自引：0，他引：8
通过十万大山盆地内地震剖面资料和ＴＭ遥感图象的地质构造解译,结合重力资料和野外地质观察及构造分析,阐述了十万大山前陆冲断推覆构造的发育特征和前陆盆地的构造演化。前陆冲断推覆构造由３个不同的构造变形带组成：卷入海西和印支期花岗岩体的逆冲断裂带、充填中生代陆相沉积并发生构造滑脱的前陆盆地和对应于华南准地台的前陆腹地。冲断推覆构造的形成和演化是与中、晚古生代钦州海槽晚二叠世的褶皱回返和中生代相继的构造复活密切联系的,它经历了３期主要构造应力作用事件：晚二叠世海西运动晚幕为冲断推覆构造的雏形期,晚三叠世印支运动晚幕的近ＳＮ向挤压是陆相前陆盆地的发育期;早白垩世末期燕山运动主幕ＮＷ—ＳＥ向挤压是现今十万大山前陆冲断推覆构造的成型期。 相似文献
44.
西准噶尔巴尔雷克蛇绿混杂岩带中玄武岩地球化学特征及大地构造意义 总被引：6，自引：0，他引：6
西准噶尔地区巴尔雷克蛇绿混杂岩中的玄武岩与蛇纹岩、放射虫硅质岩和晚泥盆世铁列克提组的泥质粉砂岩与沉凝灰岩形成混杂堆积。对玄武岩进行详细的岩石地球化学研究表明,SiO2含量为42.15%～44.71%,高TiO2(3.17%～3.77%)、Na2O(1.73%～2.28%),低Al2O3(13.54%～14.31%)、K2O(1%～1.82%),MgO含量相对稳定(6.75%～8.14%),Mg#为43～46,属于碱性玄武岩系列。稀土总量∑REE=186×10-6～219.06×10-6,轻、重稀土分馏较为明显((La/Yb)N=11.37～12.62),无明显Eu异常(Eu/Eu*=0.96～1),稀土配分模式类似于OIB。相对富集LILE(如Rb、Ba、Th),亏损HFSE(如Zr、Hf),没有明显的Nb和Ta异常,具有高的Ti/Yb(7395～8724)和Zr/Yb(120～136)比值,为典型的OIB地球化学特征。综合研究认为玄武岩形成于弧后盆地的海山环境,其岩浆源区可能为EMI型富集地幔,即软流圈的上涌导致尖晶石相二辉橄榄岩地幔源区大比例部分熔融形成的玄武岩。在区域上,蛇绿混杂岩中的玄武岩所代表的泥盆纪古洋盆是西准噶尔古洋盆向北收缩的残余洋盆。 相似文献
45.
基于冰川区地形图和实地GPS测量数据,总结4种用于计算冰川末端变化量的方法:主流线法、中心线法、周长法和特征点法,并提出基于GIS的操作思路.分析了各种方法的优缺点,阐述了各种方法在使用中的注意事项.建议使用最短距离的特征点法计算冰川末端变化量,并且以前一期的特征点向后一期的冰川边界搜索最短距离.通过把方法应用在北极Austre Lovénbreen冰川,结果表明,自2005年观测以来北极Austre Lovénbreen冰川末端呈现退缩趋势,年均退缩量为9.44m.a-1,年际变差系数为0.40,冰川末端变化量年际变化较大. 相似文献
46.
弯岛湖蛇绿混杂岩带是金沙江缝合带西段的重要组成部分。蛇绿岩混杂于上三叠统变质碎屑岩夹变质火山岩中,成份主要为镁铁质-超镁铁质杂岩,岩石类型有变质橄榄岩、变质堆晶质辉长岩及其伴生的岛弧型花岗岩系。岩石化学及地球化学特征表明:蛇绿岩主要为低Ti(岛弧-弧后)型、富集型洋中脊(E-MORB)拉斑玄武岩;与之共(伴)生的基性喷出岩、辉绿岩脉属板内洋岛型裂谷型碱性玄武岩及其过渡类型系列。在变质辉长岩获得全岩Sm-Nd等时线年龄值为232±11Ma,代表了镁铁质-超镁铁质杂岩的形成年龄,可能为洋壳初始俯冲变质的时间。在蛇绿岩上覆的硅质岩中发现有中三叠世拉丁晚期至晚三叠世卡宁早期的放射虫化石,表明弯岛湖镁铁质-超镁铁质杂岩可能形成于中三叠世多岛洋盆或弧后盆地构造环境。 相似文献
47.
Ali Pourmand François L. H. Tissot Monica Arienzo Arash Sharifi 《Geostandards and Geoanalytical Research》2014,38(2):129-148
We present an open‐source algorithm in Mathematica application (Wolfram Research) with a transparent data reduction and Monte Carlo simulation of systematic and random uncertainties for U‐Th geochronometry by multi‐collector ICP‐MS. Uranium and thorium were quantitatively separated from matrix elements through a single U/TEVA extraction chromatography step. A rigorous calibrator‐sample bracketing routine was adopted using CRM‐112A and IRMM‐035 standard solutions, doped with an IRMM‐3636a 233U/236U ‘double‐spike’ to account for instrumental mass bias and deviations of measured isotope ratios from certified values. The mean of 234U/238U and 230Th/232Th in the standard solutions varied within 0.42 and 0.25‰ (permil) of certified ratios, respectively, and were consistent with literature values within uncertainties. Based on multiple dissolutions with lithium metaborate flux fusion, U and Th concentrations in USGS BCR‐2 CRM were updated to 1739 ± 2 and 5987 ± 50 ng g?1 (95% CI), respectively. The measurement reproducibility of our analytical technique was evaluated by analysing six aliquots of an in‐house reference material, prepared by homogenising a piece of speleothem (CC3A) from Cathedral Cave, Utah, which returned a mean age of 21483 ± 63 years (95% CI, 2.9‰). Replicate analysis of ten samples from CC3A was consistent with ages previously measured at the University of Minnesota by single‐collector ICP‐MS within uncertainties. 相似文献
48.
Geological reference materials (RMs) with variable compositions and NIST SRM 612 were analysed by isotope dilution mass spectrometry for bulk rock concentrations of chalcogen elements (sulfur, selenium and tellurium), rhenium and platinum‐group elements (PGEs: Ru, Pd, Os, Ir and Pt), including the isotope amount ratios of 187Os/188Os. All concentrations were obtained from the same aliquot after HCl‐HNO3 digestion in a high pressure asher at 320 °C. Concentrations were determined after chemical separation by negative TIMS, ICP‐MS and hydride generation ICP‐MS (Se, Te). As in previous studies, concentrations of the PGEs in most RMs were found to be highly variable, which may be ascribed to sample heterogeneity at the < 1 g level. In contrast, S, Se and Te displayed good precision (RSD < 5%) in most RMs, suggesting that part of the PGE budget is controlled by different phases, compared with the chalcogen budget. The method may minimise losses of volatile chalcogens during the closed‐system digestion and indicates the different extent of heterogeneity of chalcogens, Re and PGEs in the same sample aliquot. OKUM, SCo‐1, MRG‐1, DR‐N and MAG‐1 are useful RMs for the chalcogens. NIST SRM 612 displays homogenous distribution of S, Se, Te, Pt and Pd in 30 mg aliquots, in contrast with micro‐scale heterogeneity of Se, Pd and Pt. 相似文献
49.
Paul F. Schofield Andrew D. Smith J. Frederick W. Mosselmans Hendrik Ohldag Andreas Scholl Simone Raoux Gordon Cressey Barbara A. Cressey Paul D. Quinn Caroline A. Kirk Simon C. Hogg 《Geostandards and Geoanalytical Research》2010,34(2):145-159
This work describes the application of microfocus X-ray absorption spectroscopy (XAS) and X-ray photo-emission electron microscopy (XPEEM) to the study of the complex mineralogical intergrowths within the Santa Catharina meteorite. The Santa Catharina meteorite of this study (BM52283 from the meteorite collection of the Natural History Museum, London, UK) primarily comprises a taenite bulk host phase (Fe:Ni ratio = 70.9 ± 0.8%:29.1 ± 0.8%) with a set of oxide-bearing cloudy zone textured regions (Fe:Ni:O ratio = 40.4 ± 0.3%:49.0 ± 0.7%:10.6 ± 0.8% at the core and Fe:Ni:O ratio = 34.4 ± 1.5%:42.7 ± 0.6%:22.9 ± 1.8% towards the rims) and numerous schreibersite (Fe:Ni:P ratio = 38.6 ± 1.6%:38.4 ± 0.9%:23.0 ± 0.5%) inclusions. Between the schreibersite and the taenite are rims up to 50 μm across of Ni-rich kamacite (Fe:Ni ratio = 93.4 ± 0.4%:6.6 ± 0.5%). No chemical zoning or spatial variations in the Fe and Ni speciation was observed within either the schreibersite or the kamacite phases. The oxide-bearing cloudy zone textured regions mostly comprise metallic Fe–Ni alloy, predominantly tetrataenite. Within the oxide phases, the Fe is predominantly, but not entirely, tetrahedrally co-ordinated Fe3+ and the Ni is octahedrally co-ordinated Ni2+. Structural analysis supports the suggestion that non-stoichiometric Fe2NiO4 trevorite is the oxide phase. The trevorite:tetrataenite ratio increases at the edges of the oxide-bearing cloudy zone textured regions indicating increased oxidation at the edges of these zones. The spatial resolution of the XPEEM achieved was between 110 and 150 nm, which precluded the study of either the previously reported ∼ 10 nm precipitates of tetrataenite within the bulk taenite or any antitaenite. 相似文献
50.
John Eliades Xiaolei Zhao William E. Kieser Albert E. Litherland 《Geostandards and Geoanalytical Research》2010,34(2):107-115
Preliminary tests of a prototype radio-frequency quadrupole (RFQ) collision cell system, known as an isobar separator for anions (ISA), for the removal of isobaric interferences for accelerator mass spectrometry (AMS) and for studies of anion–gas interactions are reported. The ISA decelerated a mass-analysed beam of anions from an energy (∼ 20 keV) typically generated by an AMS ion source to < 10 eV. RFQs and electrostatic lenses then guided the ions through the collision cell where ion-gas collisions reduced both the energy and energy spread of the ion beam (cooled the ions) and ion-gas reactions attenuated most of the unwanted isobars. The anions were then re-accelerated to their original energy for injection into the rest of the AMS system. With the ISA installed on a full 3 MV AMS system, attenuations of 32S-, 12C3- and 39K- by six, seven and greater than ten orders of magnitude, respectively were achieved using 0.7–1 Pa NO2 gas in the collision cell, while maintaining approximately 10–30% of the chlorine anion transmission. A further measurement of a 36Cl/Cl = 4.1 × 10-11 RM is also described. The results suggest that the 36Cl/Cl lower detection limit of the current system was 10-14–10-15 for samples that could be prepared with S/Cl ratios below 10 μg g-1. 相似文献