我国首次发现原生—自然硅

本文对自然硅进行了矿相学，矿物学研究，该矿物产于福建某地矽卡岩型硫，多金属矿床中，自然硅呈亮灰银白色、强金属光泽。性脆。镜下呈浑圆粒状、乳滴状，均质。实测比重ｄ＝２．３６８。硬度ＨＭ＝６．７６。反射率Ｒ：４７０ｎｍ３７０８；５４６ｎｍ３１．２７；６５０ｎｍ２９．９６。经扫描电镜能谱分析、电子探针分析，Ｓｉ９９．８７％～９９．９４％。含少许Ａｌ，Ｃａ，Ｆｅ机械混入物，Ｘ射线粉晶分析，主要Ｘ射线粉晶谱     

Neogene Through Quaternary Tectonic Reactivation of SW Iberian Passive Margin

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.     

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

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℃。     

康定—泸定地区地震对策及破坏性地震应急反应预案

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...     

对东昆仑金水口地区高级变质岩的新认识

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。     

湖南砂矿金刚石的颜色

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。     

湖南砂矿金刚石中顺磁氮的分配特点和金刚石归类问题

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。     

黑河流域水资源合理开发利用的研究

黑河流域是我国干旱区一个较大的内陆河流域,集水面积约13万平方公里,主流长821公里,发源于祁连山,穿越河西走廊,流泄于内蒙古西部高原。本文对黑河流域水资源、土地资源、草场资源的数显和质量进行评价。同时分析了流域水资源潜力及开发利用引起的环境变化。指出目前水资源开发已影响到中游绿洲建设规模和下游绿的安全。研究认为现阶段水资源开发利用应使经济发展和保护环境两者之间的关系相协调。实行以流域为整体的开发,采取有效的工程措施,加强中、下游水资源利用的宏观控制与管理,实行分区定量分配和综合治理,从而提高流域水资源利用的经济、环境和社会效益。     

中英联合洞穴探险及冠岩地下河系的新观察

<正> 洞穴探险是指使用某些专门的探洞装备和技术,考察一般情况下人们不能进入或不容易进入的洞穴。近十多年来,英、美等一些国家已利用洞穴探险技术,为洞穴学研究服务。他们的探洞技术发展很快,装备也不断更新。在洞穴测绘、洞穴摄影、洞穴潜水、攀登技术、洞内安全措施以及洞内生活方面积累了不少的经验,取得了大量洞穴学研究的资料和成果。我国的岩溶区面积和洞穴数量居世界之首,但洞穴考察程度还很低,尤其在南方岩溶峰丛山区,发育有较多危险的天窗、竖井、落水洞,以及一些充水的洞穴。      

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

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.