水泥厂球磨机基础切割拆除控制爆破

介绍了基础切割拆除爆破的实践和经验。同时成功地应用了非电毫秒导爆管雷管孔外多级接力扩大雷管起爆段数的方法。     

Petrogenesis and tectonic setting of bimodal volcanism in the Sakoli Mobile Belt, Central Indian shield

The Sakoli Mobile Belt comprises bimodal volcanic rocks that include metabasalt, rhyolite, tuffs, and epiclastic rocks with metapelites, quartzite, arkose, conglomerate, and banded iron formation (BIF). Mafic volcanic rocks are tholeiitic to quartz‐tholeiitic with normative quartz and hypersthene. SiO₂ shows a large compositional gap between the basic and acidic volcanics, depicting their bimodal nature. Both the volcanics have distinct geochemical trends but display some similarity in terms of enriched light rare earth element–large ion lithophile element characteristics with positive anomalies for U, Pb, and Th and distinct negative anomalies for Nb, P, and Ti. These characteristics are typical of continental rift volcanism. Both the volcanic rocks show strong negative Sr and Eu anomalies indicating fractionation of plagioclases and K‐feldspars, respectively. The high Fe/Mg ratios for the basic rocks indicate their evolved nature. Whole rock Sm–Nd isochrons for the acidic volcanic rocks indicate an age of crystallization for these volcanic rocks at about 1675 ± 180 Ma (initial ¹⁴³Nd/¹⁴⁴Nd = 0.51017 ± 0.00017, mean square weighted deviate [MSWD] = 1.6). The εNd_t (t = 2000 Ma) varies between ?0.19 and +2.22 for the basic volcanic rock and between ?2.85 and ?4.29 for the acidic volcanic rocks. Depleted mantle model ages vary from 2000 to 2275 Ma for the basic and from 2426 to 2777 Ma for the acidic volcanic rocks, respectively. These model ages indicate that protoliths for the acidic volcanic rocks probably had a much longer crustal residence time. Predominantly basaltic magma erupted during the deposition of the Dhabetekri Formation and part of it pooled at crustal or shallower subcrustal levels that probably triggered partial melting to generate the acidic magma. The influence of basic magma on the genesis of acidic magma is indicated by the higher Ni and Cr abundance at the observed silica levels of the acidic magma. A subsequent pulse of basic magma, which became crustally contaminated, erupted as minor component along with the dominantly acidic volcanics during the deposition of the Bhiwapur Formation.     

Application of passive source surface-wave method in site engineering seismic survey

Site engineering seismic survey provides basic data for seismic effect analysis. As an important parameter of soil, shear-wave velocity is usually obtained through wave velocity testing in borehole. In this paper, the passive source surface-wave method is introduced into the site engineering seismic survey and practically applied in an engineering site of Shijingshan District. By recording the ubiquitous weak vibration on the earth surface, extract the dispersion curve from the surface-wave components using the SPAC method and obtain the shear-wave velocity structure from inversion. Over the depth of 42 m underground, it totally consists of five layers with interface depth of 3.31, 4.50, 7.23, 17.41, and 42.00 m; and shear-wave velocity of 144.0, 198.3, 339.4, 744.2, and 903.7 m/s, respectively. The inversion result is used to evaluate site classification, determine the maximum shear modulus of soil, provide basis for further seismic hazard analysis and site assessment or site zoning, etc. The result shows that the passive source surface-wave method is feasible in the site engineering seismic survey and can replace boreholes, shorten survey period, and reduce engineering cost to some extent.     

南海北部陆缘合浦盆地烃源岩特征与低熟油气及生物气勘探前景

南海北部陆缘广西合浦盆地油气勘探迄今尚未取得突破,其根本原因是对该区基本油气地质条件及油气地质规律认识尚不够深入。合浦盆地主要烃源岩与百色盆地一样,均属成熟度偏低的始新统中深湖相暗色泥质岩系,其低熟烃源岩与低熟油气特征及其成藏地质条件亦基本一致。在深入分析研究合浦盆地低熟烃源岩有机质丰度、生源母质类型及热演化特征的基础上,重点对其低熟油气及生物气的地球化学特征与百色盆地进行了类比,指出合浦盆地古近系具备低熟油气/生物气的基本地质条件,其油气勘探方向及勘探策略,应借鉴百色盆地的成功经验,重点勘探寻找低熟油气及生物气资源。     

微生物成矿

微生物对生命元素如碳、氮、硫、氧和金属离子的代谢作用能显著的改变微生物周边的外部环境和其内部环境。在一系列的生物地球化学过程中,微生物参与了矿产的沉积(生物成矿)或参与了矿石和岩石的溶解(生物风化)。生物成矿作用有两个途径：一个叫生物诱导成矿,通过这个过程,微生物分泌出代谢产物导致了之后的矿物颗粒的沉积;另一个叫生物控制成矿,在这个过程中,微生物在控制矿物成核和生长上起到了显著作用。微生物成因的矿物总体来说颗粒都很小和／或有着独特的同位素特征。最普遍的生物成因矿物有碳酸盐、硫化物和铁的氧化物。细胞表面和其分泌的胞外聚合物的结构可以为离子的浓缩、聚合和矿化提供模板,并起到重要作用。地球材料的仿生合成帮助我们了解了在人工条件下的生物成矿机制。此外,在地质环境中生物成因的矿物还可以作为一种生物信号,用来重建地球和其他行星的起源和演化。     

新疆小热泉子铜(锌)矿床同位素研究

小热泉子矿床是我国最近发现的一个中型富铜(锌)矿床,其矿床成因为众多的矿床学家所关注.本文对该矿床中不同类型矿石、矿物的S、O、H、Si及稀有(惰性)气体He、Ar同位素特征作了较祥细的论述,同时用K-Ar法对硫化物的年龄测定进行了初步尝试.该矿床硫化物的δ34S值为+1.5‰~+11.1‰,平均为6.15‰(46);3He/4He(初始)值为5×10-8~2.17×10-6,平均为0.64×10-6(6),40Ar/36Ar值为305.27~439.81,平均为353.57(6);容矿岩中石英的δ18O值为+7.5‰~+11.7‰,平均为9.23‰(8),δ30Si值为0~-0.8‰,平均为-0.3‰(8);δD值为-66‰~-121‰,平均为-97‰(3).硫化物的K-Ar法年龄主要为339.1Ma、230.2Ma及98.4Ma,这些数据均显示出该矿床的成矿物质具壳幔混合的特征,矿床的形成具同生及多次成矿作用的特点.上述资料为该矿床的成因研究提供了重要的同位素信息.     

云贵高原斜坡地带典型地下水富硫酸盐地区“越层找水”模式及其机理研究

地下水是中国西南云贵高原斜坡地带重要的饮用水源,其中黔中镇宁县北部存在大面积地下水中硫酸盐超标地区,导致了当地出现水质性缺水问题。本次研究通过岩相古地理分析、水化学分析、D、18O、34S同位素测试、岩样测试、岩心观察等技术手段,查明了研究区内地下水的补给源主要为大气降水,地下水中硫酸盐(SO_4~(2-))浓度在30～1100 mg/L,平均值为221.78 mg/L,呈现高度富集SO_4~(2-)的特点;在区域相对隔水层以上,不同类型地下水中SO_4~(2-)浓度大体具有机井上升泉下降泉溶潭地下河出口基岩裂隙泉表层岩溶泉的规律;探讨了地表水、地下水中SO_4~(2-)的来源,表层岩溶泉中硫酸根的来源主要为大气降水,高硫酸盐样品中硫酸根的来源主要为石膏溶解。在此基础上,结合钻井资料,掌握了研究区膏岩层分布及含水层结构特征,通过建立"越层找水"模式,采取下层低硫酸盐含水层,获取合格饮用水源,可有效解决当地水质性缺水问题。     

The geobiological formation process of the marine source rocks in the Middle Permian Chihsia Formation of South China

The Chihsia Formation is one of the four sets of regional marine hydrocarbon source rocks from South China.In the past two decades,detailed geochemical and sedimentological studies have been carried out to investigate its origination,which have demonstrated that the high primary productivity plays a primary role in the deposition of sediments enriched in the organic matter.However,the mechanism of this high productivity and the path of the deposition and burial of the organic matter have always been a mystery.Based on the previous studies on the Shangsi Section in Guangyuan City,Sichuan Province,we proposed that the development of the equatorial upwelling due to the sea level rise is responsible for the relatively high productivity in the Chihsia Formation.The sea waters with high nutrient were transported by the sub-surface currents along the equator.High organic carbon flux was deposited on the deeper shelf,and then decomposed by bacteria,leading to the occurrence of anaerobic respiration.The metabolism of the microorganisms consumed the dissolved oxygen in waters,which was in favor of the preservation of the organic matter.This suggested geobiological model integrating with paleoclimatology,paleoceanography and geomicrobiology will help us to understand the causes of this particular sedimentary sequence.     

X-ray absorption in the strong Fe ii narrow-line Seyfert 1 galaxy Markarian 507

We present results from spectral analysis of ASCA data on the strong Fe  ii narrow-line Seyfert 1 galaxy Mrk 507. This galaxy was found to have an exceptionally flat ROSAT spectrum among the narrow-line Seyfert 1 galaxies (NLS1s) studied by Boller, Brandt & Fink. The ASCA spectrum, however, shows a clear absorption feature in the energy band below 2 keV, which partly accounts for the flat spectrum observed with the ROSAT Position Sensitive Proportional Counter (PSPC). Such absorption is rarely observed in other NLS1s. The absorption is mainly the result of cold (neutral or slightly ionized) gas with a column density of (2–3) × 10²¹ cm⁻². A reanalysis of the PSPC data shows that an extrapolation of the best-fitting model for the ASCA spectrum underpredicts the X-ray emission observed with the PSPC below 0.4 keV if the absorber is neutral (which indicates that the absorber is slightly ionized), covers only part of the central source, or there is extra soft thermal emission from an extended region. There is also evidence that the X-ray absorption is complex; an additional edge feature marginally detected at 0.84 keV suggests the presence of an additional high-ionization absorber, which imposes a strong O  viii edge on the spectrum. After correction for the absorption, the photon index of the intrinsic continuum, Γ ≃ 1.8, obtained from the ASCA data is quite similar to that of ordinary Seyfert 1 galaxies. Mrk 507 still has one of the flattest continuum slopes among the NLS1s, but is no longer exceptional. The strong optical Fe  ii emission remains unusual in the light of the correlation between Fe  ii strengths and steepness of soft X-ray slope.     

HST Planetary Camera images of quasar host galaxies

We present Hubble Space Telescope ( HST ) images of seven low-redshift quasars (six taken with the Planetary Camera, one with the Wide Field Camera). These complete the sample of 14 quasars observed by the Faint Object Camera Investigation Definition Team (FOC IDT). Following subtraction of the quasar nuclear light, host galaxies can be seen in all seven cases. A combination of the optical morphology and luminosity profiles of the residual host galaxies and the results of 2D cross-correlation model fitting implies that five of the objects have elliptical host galaxies and two have disc host galaxies. The luminosities vary from slightly fainter than L ^* to about 1.3 mag brighter than L ^*.   We discuss the properties of the complete sample of 14 quasars. Nine of the objects appear to have elliptical host galaxies (all six of the radio-loud quasars in the sample as well as three radio-quiet quasars). Two further radio-quiet quasars appear to lie in disc galaxies. The other three objects (radio-quiet, ultraluminous infrared quasars) all lie in violently interacting systems. The sample as a whole has an average luminosity about 0.8 mag brighter than L ^*, although the radio-loud objects have hosts on average 0.7 mag brighter than the radio-quiet objects.   We compare our results with those from HST imaging of quasars by other authors. Taken together, our observations are in broad agreement with those of Bahcall et al. Radio-loud quasars appear to lie in luminous elliptical galaxies whereas radio-quiet quasars are found to lie in either elliptical or spiral hosts. Host galaxy luminosities (of radio-quiet and radio-loud quasars) are much brighter than would be expected if they followed a Schechter luminosity function.