Neogene Through Quaternary Tectonic Reactivation of SW Iberian Passive Margin   总被引：1，自引：0，他引：1  

N.?ZitelliniEmail author  M.?Rovere  P.?Terrinha  F.?Chierici  L.?Matias  Bigsets Team 《Pure and Applied Geophysics》2004,161(3):565-587

Southwest Portugal, the Gulf of Cadiz and Morocco are under the potential threat of natural hazards linked to seismicity and tsunami generation. We report the results of two multi-channel seismic (MCS) surveys carried out in 1992 and 1998 along the continental margin and oceanic crust of SW Iberia. This MCS data set shows the evidence of the compressional deformation which involves both the continental and the oceanic crust of the study area. The area of deformation extends from the southern border of the Tagus Abyssal Plain to the Seine Abyssal Plain, encompassing the continental margin of SW Portugal. Most of the structures observed are probably related to a Mid-Miocene phase of Africa-Europe plate convergence. In this paper we discuss the recent advances on the identification of the tectonic structures that are still active and that may generate great earthquakes and tsunamis. The tectonic structures identified are located respectively at the Guadalquivir Bank, along the eastern border of the Horseshoe Abyssal Plain and along the southern continental slope of SW Portugal.BIGSETS Team: L. Mendes Victor, C. Corela, A. Ribeiro, D. Cordoba, J. J. Danobeitia, E. Grácia, R. Bartolomé, R. Nicolich, G. Pellis, B. DellaVedova, R. Sartori, L. Torelli, A. Correggiari, L. Vigliotti.  相似文献   

四川大渡河金矿田成矿流体来源的氦氩硫氢氧同位素示踪   总被引：12，自引：3，他引：12       下载免费PDF全文

李晓峰毛景文  王登红罗辅勋 《地质学报》2004,78(2):203-210

四川大渡河金矿田位于扬子地台西缘金成矿带北段,受大渡河剪切带控制。本文以该矿田黄金坪、白金台子、黑金台子金矿为例,根据对黄铁矿流体包裹体氦氩同位素、黄铁矿硫同位素以及与黄铁矿共生的石英流体包裹体的氢氧同位素组成测定,讨论了大渡河金矿田成矿流体的来源。结果显示,该金矿田黄铁矿流体包裹体中的~3He/~4He变化较小,为0.16～0.86Ra,而~(40)Ar/~(36)Ar的变化较大,为298～3288;而黄铁矿δ~(34)S同位素变化范围较窄,一般为0.7‰～4.2‰,集中于2.5‰～3‰,显示硫地幔来源的特点;石英流体包裹体的氢、氧同位素分别为-2.6‰～ 3.64‰和-39.13‰～-108.23‰,说明成矿流体为岩浆水和大气降水的混合流体。本文认为大渡河金矿田成矿流体是地幔流体与地壳流体的混合作用的结果,而以地壳流体占主导地位。其中,地幔流体为与下伏隐伏岩体有关的岩浆水,而地壳流体端元则是含有一定放射成因Ar的大气降水,并且温度小于200℃。  相似文献   

新疆塔里木盆地艾协克—桑塔木南地区油气地球化学指标的多重分形性分析   总被引：1，自引：0，他引：1  

谢淑云鲍征宇  苏江玉贾先巧 《地质论评》2005,51(1):107-112

用分形与多重分形的方法研究地球化学场中地球化学指标的分布规律具有重要的意义。本文运用多重分形矩方法研究了新疆塔里木盆地艾协克一桑塔木南地区2000km^2内采集的2085个土壤样中20项油气化探指标的多重分形谱函数形态特征。结果表明，主要成油气指示指标的多重分形谱基本上呈单一“钩状”，显示较弱的多重分形或单一分形；而其他指标多显示较强的多重分形特征。这些性质在研究区广泛存在，将对区域含油性研究有重要的指示意义。  相似文献   

康定—泸定地区地震对策及破坏性地震应急反应预案     

余河生  杜江 《四川地震》1998,(Z1)

康定—泸定地区地震对策及破坏性地震应急反应预案余河生（甘孜州地震局）杜江（泸定县地震办公室）康定—泸定地区由于所处的特殊的地震构造和地震活动环境而面临严峻的地震形势。为了做好地震应急工作,甘孜州地震局和泸定县地震办公室分别代政府制定了破坏性地震应急反...  相似文献   

对东昆仑金水口地区高级变质岩的新认识     

刘永成  叶占福 《青海国土经略》1998,(1)

详细的构造岩石单位填图研究表明,东昆仑山金水口高级变质岩分布区,并非仅由早元古代金水口岩群白沙河岩组变质地层组成。由花岗闪长质—英云闪长质—奥长花岗质构成的灰色片麻岩,组成了高级变质岩分布区的主体。在灰色片麻岩中进一步还可解体出更古老的以包体形式产出的表壳岩组合系列。因此,以金水口地区为窗口,加深对东昆仑山高级变质岩的研究,有助于澄清变质杂岩的属性,正确认识造山带的形成与演化和提高1:5万地质填图质量。  相似文献   

湖南砂矿金刚石的颜色   总被引：4，自引：0，他引：4  

郭九皋  陈丰  邓华兴  谈逸梅  容振球  邓尔森 《矿物学报》1986,(2)

研究表明,湖南砂矿金刚石中存在着两类决定金刚石颜色(主要指黄、褐和绿色)的色心。一类是氮原子中心,有孤氮原子和N3中心。另一类是辐射损伤中心,有GR1、637、595、H3、H4和3H中心。文中还讨论了这些色心的地质意义。  相似文献   

湖南砂矿金刚石中顺磁氮的分配特点和金刚石归类问题   总被引：2，自引：1，他引：2  

蔡秀成  郭九皋  陈丰  富毓德  唐荣炳  谈逸梅  邓尔森 《矿物学报》1986,(3)

利用EPR检测了200多颗湖南砂矿金刚石。为53颗晶体测定了顺磁N的含量。阐明了砂矿金刚石中顺磁N分配的一般特点:具顺磁N信号者占30％,具较大顺磁N含量(10~(17)—10~(18)N原子/cm~3)者只占7％,属I_b型的晶体～2％。通过顺磋和红外光谱资料对比,发现了一些奇异现象,设想后者起因于混型晶的存在。为使金刚石正确归类,给出了一套测试方案,强调了紫外、红外光谱,紫外形貌照相和EPR等手段的联合使用。  相似文献   

Constraining the surface properties of Saturn's icy moons, using Cassini/CIRS emissivity spectra     

J.M. Carvano  A. Migliorini  A. Barucci  the CIRS Team 《Icarus》2007,187(2):574-583

We have conducted a search for emissivity features in the thermal infrared spectrum of the icy satellites of Saturn, Phoebe, Iapetus, Enceladus, Tethys, and Hyperion, observed by the Composite Infrared Spectrometer (CIRS) on board the Cassini spacecraft. Despite the heterogeneity of the composition of these bodies depicted by Earth-based and Cassini/VIMS observations, the CIRS spectra of all satellites are undistinguishable from black-body spectra, with no detectable emissivity feature. However, several materials, which have been detected on the surface of the same bodies, present emissivity features in the analyzed spectral range. In particular, water ice presents features with sufficient contrast to be detected by CIRS. Here we study the physical causes of the absence of features by simulating the effects of intimate mixtures using models of directional emissivity for optically thick surfaces for different particle sizes and abundances, and porosities. The simulations include a set of materials detected on the Phoebe's surface, like water ice, hydrated silicates, and organics. We find that featureless spectra can be produced in three scenarios: (1) ice particles with large sizes, (2) mixtures of ices dominated by dark contaminants, and (3) small particles with large porosity. Constraints imposed by the NIR spectra of the satellites favors the latter scenario as the more likely explanation to the absence of emissivity features on the icy satellites of Saturn.  相似文献   

Electrical properties of Titan's surface from Cassini RADAR scatterometer measurements     

Lauren C. Wye  Howard A. Zebker  Richard D. West  Ralph D. Lorenz  the Cassini RADAR Team 《Icarus》2007,188(2):367-385

We report regional-scale low-resolution backscatter images of Titan's surface acquired by the Cassini RADAR scatterometer at a wavelength of 2.18-cm. We find that the average angular dependence of the backscatter from large regions and from specific surface features is consistent with a model composed of a quasi-specular Hagfors term plus a diffuse cosine component. A Gaussian quasi-specular term also fits the data, but less well than the Hagfors term. We derive values for the mean dielectric constant and root-mean-square (rms) slope of the surface from the quasi-specular term, which we ascribe to scattering from the surface interface only. The diffuse term accommodates contributions from volume scattering, multiple scattering, or wavelength-scale near-surface structure. The Hagfors model results imply a surface with regional mean dielectric constants between 1.9 and 3.6 and regional surface roughness that varies between 5.3° and 13.4° in rms-slope. Dielectric constants between 2 and 3 are expected for a surface composed of solid simple hydrocarbons, water ice, or a mixture of both. Smaller dielectric constants, between 1.6 and 1.9, are consistent with liquid hydrocarbons, while larger dielectric constants, near 4.5, may indicate the presence of water-ammonia ice [Lorenz, R.D., 1998. Icarus 136, 344-348] or organic heteropolymers [Thompson, W.R., Squyres, S.W., 1990. Icarus 86, 336-354]. We present backscatter images corrected for angular effects using the model residuals, which show strong features that correspond roughly to those in 0.94-μm ISS images. We model the localized backscatter from specific features to estimate dielectric constant and rms slope when the angular coverage is within the quasi-specular part of the backscatter curve. Only two apparent surface features are scanned with angular coverage sufficient for accurate modeling. Data from the bright albedo feature Quivira suggests a dielectric constant near 2.8 and rms slope near 10.1°. The dark albedo feature Shangri-La is best fit by a Hagfors model with a dielectric constant close to 2.4 and an rms slope near 9.5°. From the modeled backscatter curves, we find the average radar albedo in the same linear (SL) polarization to be near 0.34. We constrain the total-power albedo in order to compare the measurements with available groundbased radar results, which are typically obtained in both senses of circular polarization. We estimate an upper limit of 0.4 on the total-power albedo, a value that is significantly higher than the 0.21 total albedo value measured at 13 cm [Campbell, D., Black, G., Carter, L., Ostro, S., 2003. Science 302, 431-434]. This is consistent with a surface that has more small-scale structure and is thus more reflective at 2-cm than 13-cm. We compare results across overlapping observations and observe that the reduction and analysis are repeatable and consistent. We also confirm the strong correlations between radar and near-infrared images.  相似文献   

Flow around sunspots from it p-mode frequency shift measurements     

Sun  Ming-Tsung  Chou  Dean-Yi  Lin  Chia-Hsien  Team  The TON 《Solar physics》1997,176(1):59-65

We use five-day helioseimic data from the Taiwan Oscillation Network to study the flow around a sunspot, NOAA 7887. The p-mode oscillations in an annular region centered at the sunspot are decomposed into the modes propagating toward and away from the sunspot. We find that the frequency of an outgoing mode is greater than that of the corresponding incoming mode. This indicates that the plasma is flowing outward from the sunspot. The outflow velocity is estimated to be about 40–80 m s^-1.  相似文献