吉林夹皮沟金矿稳定同位素地质及找矿方向

吉林夹皮沟金矿床成因,多年来一直存在变质热液和岩浆热液之争。在金矿带北侧海西期花岗岩内和南侧白山镇一带变质岩地区进行外围找矿始终没有突破性进展。在前人研究基础上,通过一些补测工作对夹皮沟金矿稳定同位素地质给予新的认识。Ｓ和Ｃ、Ｈ、Ｏ流体主要来自地幔,部分Ｓ和Ｓｉ、Ｐｂ、Ａｕ主要来自花岗岩和古老变质层状岩系,成矿远景区应重点选定在夹皮沟—大砬子深大断裂两侧中生代脉岩体附近。     

中建南盆地新生代层序地层特征

中建南盆地是在晚白垩世末南海中南部的一次张性构造运动──礼乐运动作用下开始形成的。盆地的发育经历了中、晚始新世之间的西卫运动造成区域抬升,使中建南盆地的下伏地层遭受变形、隆升和剥蚀;晚渐新世─中中新世的南海中央海盆扩张──南海运动;中中新世末期的万安运动和中新世末期南海整体沉降作用。共划分了6个层序组,8个层序,即A层序组(含A层序)、B层序组(含B层序)、C层序组(含C1层序和C2层序)、D层序组(含D层序)、E层序组(含E1层序和E2层序)和F层序组(含F层序)。     

湖北清江和尚洞风化岩壁放线菌分离及基于16S rRNA的种类分析

为探究湖北清江和尚洞岩壁放线菌物种组成及其与碳酸盐岩相互作用的关系,分别采集该洞穴无光区风化岩壁样品2份（W1和W2）和弱光区风化岩壁样品1份（W3）,采用经改良的5种已知放线菌分离培养基及1种自主设计的风化岩壁浸汁培养基两种策略优化设计分离培养基。采用稀释涂布法分离放线菌,并选择放线菌特异引物进行16S rRNA基因扩增和序列测定并构建系统发育树。结果表明,从3份风化岩壁样品中共纯化到放线菌72株,分属于放线菌纲（Actinobacteria）的4个属:链霉菌属（Streptomyces,69株）、红球菌属（Rhodococcus,1株）、冢村氏菌属（Tsukamurella,1株）和微杆菌属（Microbacterium,1株）,其中链霉菌属为优势菌属。无光区样品W1和W2分离到菌株较少,分别为9株和10株,而弱光区样品W3分离到菌株较多,为53株。研究结果为进一步研究放线菌与洞穴碳酸盐矿物相互作用的潜在关系奠定了基础。      

近30年夏季亚欧大陆中高纬度阻塞高压的统计特征

文中利用1970～2001年NCEP再分析500 hPa逐日高度场资料,根据阻塞高压的天气学定义,采用客观统计方法检索出近32 a亚欧中高纬度392个阻塞高压个例,对其进行了气候学分析.结果表明,亚欧中高纬地区夏季阻塞高压活动频繁,10 d以下的过程占绝对多数,地理分布主要集中在45～70°N之间,纬向上可划分5个高发区,其中乌拉尔山和贝加尔湖东部阻高活动频次最高,同时,每个区域中又存在着相应的阻高活跃区.亚欧中高纬地区夏季阻高活动具有明显的季节内变化特征.6月份,阻塞活动多发生在乌拉尔山地区和鄂霍次克海地区,以双阻为主要形势;7月份,欧洲区和贝加尔湖地区的阻塞活动有所增多,尤其贝加尔湖东部地区增多明显,而乌拉尔山地区的阻塞形势明显减少,鄂霍次克海地区的阻塞活动位置向北移动,多发生在60°N以北,双阻形势逐渐减弱,贝加尔湖地区的中阻形势有所增强.8月份,阻塞形势主要存在于贝加尔湖东西两区,中阻形势占据主导地位.亚欧中高纬地区夏季阻塞高压活动年际变化特征也很突出,且这种年际振荡有明显的地理差异.另外,研究表明亚洲北部的阻高活动多以稳定型为主,移动型阻高个例仅占6.6%.移动型阻高以起源于乌拉尔山地区最多,移距最长,生命期最长.偶极子类阻高多集中在贝加尔湖东部与乌拉尔山地区,约占该地区总阻高频次的62.0%和49.7%,平均生命期分别达到7 d/次和9 d/次以上.     

Post-Collisional Ductile Extensional Tectonic Framework in the UHP and HP Metamorphic Belts in the Dabie-Sulu Region, China

The present-day observable tectonic framework of the ultrahigh-pressure (UHP) and high-pressure (HP) metamorphic belts in the Dabie-Sulu region was dominantly formed by an extensional process, mostly between 200 and 170 Ma, following the Triassic collision between the Sino-Korean and Yangtze cratons. The framework that controls the present spatial distribution of UHP and HP metamorphic rocks in particular displays the typical features of a Cordilleran-type metamorphic core complex, in which at least four regional-scale, shallow-dipping detachment zones are recognized. Each of these detachment zones corresponds to a pressure gap of 0.5 to 2.0 GPa. The detachment zones separate the rocks exposed in the region into several petrotectonic units with different P-T conditions. The geometry and kinematics of both the detachment zones and the petrotectonic units show that the exhumation of UHP and HP metamorphic rocks in the Dabie-Sulu region was achieved, at least in part, by non-coaxial ductile flow in the mul     

塔里木盆地塔中地区志留系塔塔埃尔塔格组潮坪沉积中的遗迹化石

在塔里木盆地塔中地区志留系塔塔埃尔塔格组中共发现遗迹化石 11属 12种,包括Skolithoslinearis、Skolithosverticalis、Ophiomorphanodosa、Arenicolitesisp.、Cylindrichnusisp.、Thalassinoidessuevicus、Diplocraterionparallelum、Taenidi umsatanassi、Macaronichnussegregatis、Palaeophycustubularis、Planolitesbeverlegensis和Cochlichnusanguineus。这些遗迹化石主要是无脊椎动物的居住迹、进食迹和觅食迹,其中大部分呈全浮痕保存,少数呈上浮痕或下浮痕保存。按其古生态和沉积学特征,可划分出三个遗迹组合:①Skolithos-Thalassinoides遗迹组合,代表了平坦底型条件下的砂坪沉积环境;②Planolites-Palaeophycus遗迹组合,反映了潮间带砂泥坪沉积环境;③Cochlichnus-Planolites遗迹组合,代表了平均低潮线附近的泥坪沉积环境。     

峨眉山大火成岩省太和花岗岩的成因及构造意义

攀西地区的太和花岗质岩体和赋存超大型钒钛磁铁矿矿床的辉长岩体在空间上共生,成因上均与峨眉山地幔柱头的上升密切相关.太和花岗质岩体主要由超碱质花岗岩和石英正长岩及少量正长岩组成;富含高场强元素并具高Ga/Al值(3.74～5.63),显示典型A型花岗岩的特征.花岗岩、正长岩和辉长岩的Nb/Ta和Zr/Hf值与洋岛玄武岩(OIB)的相应比值近似.花岗质岩石具较低的87Sr/86Sr初始值(0.7025～0.7049)和正的εNd(t)值(1.9～3.5),与辉长岩的值相近[(87Sr/86Sr)i =0.7049～0.7052; εNd(t) =2.4～3.3].太和花岗质岩体的εNd(t)为正值,显示地幔柱来源的底侵玄武质岩浆对其形成起主要作用.辉长质和花岗质岩石具相似的钕同位素组成,表明其母岩浆来自于同一源区.我们认为太和花岗质侵入体主要由底侵于下地壳的玄武质岩浆分异出的花岗质熔体侵位及随后经结晶分异而形成.因此,晚古生代时幔源岩浆底侵造成的地壳增生在峨眉山大火成岩省中表现极为显著.     

巴西绿欧泊的宝石学特征

近期国内珠宝市场上出现一种产自巴西的绿欧泊,该类绿欧泊表现出的宝石矿物学特征与传统的欧泊有着明显差异。采用常规宝石学测试手段,并结合电子探针、X射线粉末衍射、扫描电子显微镜、红外吸收光谱、紫外吸收光谱等测试分析方法,就其化学成分、物相、微结构、谱学特征及颜色成因等问题展开初步研究。结果表明,巴西绿欧泊的主要矿物组成为蛋白石,含不等量的α-方石英和α-鳞石英等次要矿物,整体呈不规则胶柬状结构,局部微波纹理发育;该类欧泊主要由直径约10～30nm的SiO2球粒聚集而成;由H2O和M—OH倍频振动致近红外吸收谱带位于7000cm-1处,由H2O合频振动致近红外吸收谱带分别位于5200,5612cm叫处,由M—OH与[SiO4]合频振动致近红外吸收谱带位于4600-4100cm-1范围内。笔者还对巴西绿欧泊的呈色机理一并给予了探讨。     

RESEARCH ON THE RELATIONSHIP BETWEEN FRACTAL FACTORS AND TECTONIC ACTIVITY——A CASE STUDY OF SOUTHWESTERN YUNNAN BLOCK

Geomorphology could record long-term accumulation of tectonic movement and quantify it by relevant parameters.But because the influences of other factors such as climate and lithology,how to use the relevant parameters to reveal the relationship between geomorphology and tectonics is a research hot spot.In this paper,we utilize the variogram method and the cellular fractal model to estimate parameters such as the fractal dimension (D) and ordinate intercept (γ) from the SRTM3 DEM using a moving window operation.We compare the distribution characteristics of the parameters in different climate and lithology.The results indicate that the correlation between the parameters and lithology or climate is very poor.The fractal dimension (D) reveals a very good correlation with tectonics,which is low in tectonically inactive areas and high in active areas.It implies that fractal dimension (D) may be a new method for research of regional tectonic movement.     

Parameterization of the Absorption of the H_2O Continuum,CO_2,O_2,and Other Trace Gases in the Fu-Liou Solar Radiation Program

The absorption properties of the water vapor continuum and a number of weak bands for H2O, O2, CO2, CO, N2O, CH4, and O3 in the solar spectrum are incorporated into the Fu-Liou radiation parameterization program by using the correlated k-distribution method (CKD) for the sorting of absorption lines. The overlap absorption of the H2O lines and the H2O continuum (2500-14500 cm-1) are treated by taking the two gases as a single-mixture gas in transmittance calculations. Furthermore, in order to optimize the computation efforts, CO2 and CH4 in the spectral region 2850-5250 cm-1 are taken as a new single-mixture gas as well. For overlap involving other absorption lines in the Fu-Liou spectral bands, the authors adopt the multiplication rule for transmittance computations under which the absorption spectra for two gases are assumed to be uncorrelated. Compared to the line-by-line (LBL) computation, it is shown that the errors in fluxes introduced by these two approaches within the context of the CKD method are small and less than 0.48% for the H2O line and continuum in the 2500-14500 cm-1 solar spectral region, -1% for H2O (line) H2O (continuum) CO2 CH4 in the spectral region 2850-5250 cm-1, and -1.5% for H2O (line) H2O (continuum) O2 in the 7700-14500 cm-1 spectral region. Analysis also demonstrates that the multiplication rule over a spectral interval as wide as 6800 cm-1 can produce acceptable errors with a maximum percentage value of about 2% in reference to the LBL calculation. Addition of the preceding gases increases the absorption of solar radiation under all sky conditions. For clear sky, the increase in instantaneous solar absorption is about 9%-13% (~12 W m~2) among which the H2O continuum produces the largest increase, while the contributions from O2 and CO2 rank second and third, respectively. In cloudy sky, the addition of absorption amounts to about 6-9 W m-2. The new, improved program with the incorporation of the preceding gases produces a smaller solar absorption in clouds due to the reduced solar flux reaching the cloud top.