沁水盆地南部潘庄区块废弃矿井煤层气地球化学特征及成因

为了研究废弃矿井中煤层气成因,以沁水盆地南部潘庄区块废弃矿井为例,抽采废弃矿井中煤层气并进行化学组分和同位素测试,并采集部分废弃矿井水样品测试水中离子浓度、pH值等进行研究。结果表明：潘庄区块废弃矿井中煤层气CH₄体积分数平均值为91.99%,CO₂为1.26%,N₂为6.73%;甲烷碳同位素（δ¹³C₁）值为-31.36‰~-33.53‰,平均-32.25‰,氢同位素（δD）值为-182.76‰~-193.20‰,平均-187.538‰。废弃矿井排采水中阴阳离子主要为Mg²⁺、K⁺、HCO₃^-、Cl^-、Na⁺、SO₄^2-和NO₃^-等,产出水型为Mg-（HCO₃）₂型,表明矿井水受到地表水的强烈影响。废弃矿井中煤层气主要以热成因气为主,少量次生生物气。与附近未开采煤储层相比,研究区废弃矿井中的环境更有利于次生生物气的生成。     

黔东地区变质核杂岩构造及其控矿作用

黔东地区的变质核杂岩构造其变质核杂岩为中元古界四堡群、梵净山群变质基底,其主滑脱面发育于新元古界底部的甲路组,同时在下江群、板溪群中出现一系列次级滑脱面,在其上的早古生代地层中则发育伸展剥离正断层系统。该类型构造形成于加里东期末,是该区加里东造山期后隆升背景的产物。变质核杂岩构造与该地区的金、铜、铅、锌、锑及汞等矿产关系十分密切,它们分别受控于主滑脱带、次级滑脱带及伸展剥离正断层系统,且在剖面上矿物组合、成矿温度出现有规律变化,反映出该地区金及多金属矿产是受控于变质核杂岩构造的一个完整的、相互有机联系的成矿系统。     

内蒙古萤石矿资源开发利用动态分析与建议

萤石是一种稀缺性战略资源。内蒙古萤石资源丰富,保有资源储量稳定。分析了内蒙古萤石资源储量动态、开发利用动态以及市场需求和发展动态,提出了加强萤石矿地质勘查工作,优化管理、节约资源,加快企业进步、抬升综合效益,改善下游消费结构、实现资源整体升值的未来发展建议。     

Constraints of Mantle and Crustal Sources Interaction during Orogenesis of Pre- and Post-collision Granitoids from the Northern Arabian-Nubian Shield: A Case Study from Wadi El-Akhder Granitoids,Southern Sinai,Egypt

The Egyptian older and younger granitic rocks emplaced during pre- and post-collision stages of Neoproterozoic Pan-African orogeny, respectively, are widely distributed in the southern Sinai Peninsula, constituting 70% of the basement outcrops. The Wadi El-Akhder, southwestern Sinai, is a mountainous terrain exposing two granitoid suites, namely the Wadi El-Akhder Older Granites (AOG) and the Homra Younger Granites (HYG). The AOG (granodiorites with subordinate tonalite compositions) have geochemical characteristics of medium-K calc-alkaline, metaluminous to mildly peraluminous granitoids formed in an island-arc environment, which are conformable with well-known Egyptian older granitoids rocks, whereas the HYG display calc-alkaline to slightly alkaline nature, peraluminous syeno-, monzogranites and alkali feldspar granites matching well those of the Egyptian younger granites. With respect to the AOG granitoids, the HYG granites contain lower Al2O3, FeO*, MgO, MnO, CaO, TiO2, Sr, Ba, and V, but higher Na2O, K2O, Nb, Zr, Th, and Rb. The AOG are generally characterized by enrichment in LILE and LREE and depletion in HFSE relative to N-MORB values (e.g., negative Nb and Ta anomalies). The geochemical features of the AOG follow assimilation-fractional crystallization (AFC) trends indicative of extensive crustal contamination of magma derived from a mantle source. The chemical characteristics of the AOG are remarkably similar to those of subduction-related granitoids from the Arabian-Nubian Shield (ANS). The compositional variations from monzogranites through syenogranites to alkali feldspar granite within HYG could not be explained by fractional crystallization solely. Correlating the whole-rock composition of the HYG to melts generated by experimental dehydration melting of meta-sedimentary and magmatic rocks reveals that they appear to be derived by extended melting of psammitic and pelitic metasediments, which is similar to the most of younger granitic suites in the ANS.     

Contrasting water–rock interaction behaviors of antimony and arsenic in contaminated rivers around an antimony mine,Hunan Province,China

Although antimony (Sb) and arsenic (As) exhibit similar geochemical behavior and toxicity in the environment, growing evidence suggests that their water–rock interaction behavior in contaminated rivers is quite different. Twenty-nine river water samples were collected between September and November 2018 from contaminated rivers around an antimony mine in Hunan Province, China. The concentrations of As and Sb were inversely proportional to the water flow distance. The rates and magnitudes of Sb decrease were more prominent than those of As. Silicate mineral dissolution from rocks such as silicified limestone increased the As and Sb concentration of in-mine-district (IMD) water. Dissolution of carbonate minerals, ion exchange, and competitive adsorption were the major water–rock interactions, resulting in rapidly decreasing As and Sb concentration in IMD direct impacted water and IMD indirect impacted water. The behaviors of As and Sb during water–rock interaction were dissimilar for areas dominated by carbonate and silicate minerals.     

Hydrodynamical simulations of Galactic fountains – I. Evolution of single fountains

The ejection of the gas out of the disc in late-type galaxies is related to star formation and is due mainly to Type II supernovae. In this paper, we studied in detail the development of the Galactic fountains in order to understand their dynamical evolution and their influence on the redistribution of the freshly delivered metals over the disc. To this aim, we performed a number of 3D hydrodynamical radiative cooling simulations of the gas in the Milky Way where the whole Galaxy structure, the Galactic differential rotation and the supernova explosions generated by a single OB association are considered. A typical fountain powered by 100 Type II supernovae may eject material up to ∼2 kpc which than collapses back mostly in the form of dense, cold clouds and filaments. The majority of the gas lifted up by the fountains falls back on the disc remaining within a radial distance  Δ R = 0.5 kpc  from the place where the fountain originated. This localized circulation of disc gas does not influence the radial chemical gradients on large scale, as required by the chemical models of the Milky Way which reproduce the metallicity distribution without invoking large fluxes of metals. Simulations of multiple fountains fuelled by Type II supernovae of different OB associations will be presented in a companion paper.     

The 2dF Galaxy Redshift Survey: luminosity dependence of galaxy clustering

We investigate the dependence of the strength of galaxy clustering on intrinsic luminosity using the Anglo-Australian two degree field galaxy redshift survey (2dFGRS). The 2dFGRS is over an order of magnitude larger than previous redshift surveys used to address this issue. We measure the projected two-point correlation function of galaxies in a series of volume-limited samples. The projected correlation function is free from any distortion of the clustering pattern induced by peculiar motions and is well described by a power law in pair separation over the range     . The clustering of     galaxies in real space is well-fitted by a correlation length     and power-law slope     . The clustering amplitude increases slowly with absolute magnitude for galaxies fainter than M *, but rises more strongly at higher luminosities. At low luminosities, our results agree with measurements from the Southern Sky Redshift Survey 2 by Benoist et al. However, we find a weaker dependence of clustering strength on luminosity at the highest luminosities. The correlation function amplitude increases by a factor of 4.0 between     and −22.5, and the most luminous galaxies are 3.0 times more strongly clustered than L * galaxies. The power-law slope of the correlation function shows remarkably little variation for samples spanning a factor of 20 in luminosity. Our measurements are in very good agreement with the predictions of the hierarchical galaxy formation models of Benson et al.     

青藏高原积雪异常与贵州东、西部旱、寒灾害关系的初步分析

利用 195 8— 1992年的有关资料 ,对青藏高原冬、春季积雪异常与贵州春、夏季不同区域干旱和低温灾害的强弱关系进行了统计分析。结果发现 :青藏高原冬、春季积雪异常与贵州春、夏季不同区域干旱和低温灾害的强弱间存在明显的相关关系 ,高原异常多雪年贵州西部 4月春旱偏重 ;东部夏旱偏重 ,春季低温灾害偏轻。反之 ,高原异常少雪年贵州西部春旱和东部夏旱都偏轻 ,春季低温灾害偏重。     

关于梅雨研究的回顾与展望

从梅雨的划分、梅雨的降水分型、梅雨与季风的关系及梅雨的影响因子几个方面,对前人的研究成果进行了回顾和讨论。最后,提出梅雨研究仍需解决的问题：（1）江淮流域梅雨季节的开始至今仍没有一个客观统一划定标准;（2）南海季风、印度季风等季风子系统对梅雨的影响大小及其机制尚需进一步研究讨论;（3）应针对梅雨季节内江淮流域不同的降水分布型,寻找其前期预兆信号进行深入研究;（4）应特别注意特定海温分布型对梅雨的影响,并从中找出影响梅雨的关键区域和影响的关键时段;（5）积冰和雪盖与梅雨异常的关系仍需进一步求证,影响机制还需进一步探索。