汞在地壳、岩石和疏松沉积物中的分布

20世纪80年代以来分析测试技术取得了突破性的进展,积累了汞在岩石和疏松沉积物大量可靠的分析数据,发现引用20世纪70年代前发表的有关汞的地壳丰度及岩石和沉积物中的平均含量作为衡量标准已不适宜.本文根据近20年来发表的有关汞在地壳、岩石和疏松沉积物中含量的文献,结合作者在地壳元素丰度研究中积累的大量岩石中汞含量的可靠数据以及IGCP360"全球地球化学基准"计划获得的国外沉积物中汞含量的可靠数据,综合给出了汞在地壳、出露岩石地壳的丰度分别为7 ng/g和13 ng/g,岩石、火成岩、沉积岩、变质岩的平均含量分别为12.5 ng/g、6.9 ng/g、22.6 ng/g和8.6 ng/g,大陆疏松沉积物、水系沉积物、泛滥平原沉积物、土壤和浅海沉积物的平均含量分别为60 ng/g、60 ng/g、60 ng/g、65 ng/g和25ng/g.     

湖盆数据未知的湖泊动态库容遥感监测方法

针对现有库容遥感监测方法对无湖盆数据区域的湖泊动态库容难以直接测算问题,提出了未知湖泊水下地形数据的遥感湖泊动态库容监测方法。该方法通过多源遥感数据,匹配相对时相的湖泊面积和水位信息,构建并模拟湖盆DEM数据,据此来估算湖泊的动态库容。在算法实现上,首先采用分布迭代水体提取从遥感影像提取湖泊的多期动态边界;其次,从ICEsat GLAS激光测高数据中反演出湖泊的动态水位高程;第三,依据时间水位信息,通过邻近时相匹配,将水位高程赋给湖泊边界线,生成湖泊等水位线;第四,通过等水位线构建TIN(triangulated irregular network)和Kriging插值,得到模拟湖盆数字高程模型;最后,依据模拟湖盆DEM和水体面积分布、水位信息,计算湖泊动态库容。试验通过对博斯腾湖的多年动态库容监测与真实性检验,结果显示:最大误差为2.21×108 m3,最小误差为0.000 02×108 m3,平均误差为0.044×108 m3,均方根为0.59,相关系数达到0.99。     

A k - *epsiv Turbulence Closure Model For The Atmospheric Boundary Layer Including Urban Canopy

A numerical model for the computation of the wind field,air temperature and humidity in the atmospheric boundary layer (ABL) including the urbancanopy was developed for urban climate simulation. The governing equations of the modelare derived by applying ensemble and spatial averages to the Navier–Stokes equation, continuityequation and equations for heat and water vapour transfer in the air. With the spatial averagingprocedure, effects of buildings and other urban structures in the urban canopy can be accounted for byintroducing an effective volume function, defined as the ratio between the volume of air in acomputational mesh over the total volume of the mesh. The improved k - model accounts for the anisotropyof the turbulence field under density stratification. In the improved k - model, the transportof momentum and heat in the vertical direction under density stratification is evaluated based onthe assumption of a near-equilibrium shear flow where transport effects on the stresses andheat fluxes are negligible. The heating processes at surfaces of buildings and ground are alsomodelled. The comparison of the computational results obtained with the present modeland existing observational data and numerical models shows that the present model is capableof predicting the structure of turbulence in the urban canopy layer under density stratification.Numerical experiments with the new model show that the flow behaviour of the air in the urbancanopy layer is strongly affected by the existence of buildings and density stratification.     

延长油田郭旗西区长6储集条件及油气成藏控制因素分析

通过对延长油田郭旗西区长6油层组储层的沉积微相、储层的岩石学特征、成岩作用、孔隙结构特征和物性条件研究，探讨了影响储集条件和油气成藏的主要因素.延长油田郭旗西区三叠系延长组长6早期沉积微相以三角洲前缘水下分流河道为主，长6晚期以三角洲平原分流河道沉积为主，储集层发育.受成岩后生作用影响，形成了低孔隙度、特低-超低渗透率的储集层.油藏分布主要受沉积微相和储层物性控制，为典型的岩性油藏。     

半干旱半湿润地区洪水预报模型适用性研究

针对半干旱半湿润地区的流域特性和产汇流特点,比较了河北雨洪模型和新安江模型的模型原理和模型特性,以滦河支流老牛河流域为例,开展了洪水预报适用性研究。结果表明,河北雨洪模型的预报精度较高,更适用于半干旱半湿润地区的洪水预报。     

中国煤中的汞

煤中的汞是人们最为关注的环境有害元素之一。由于汞具有强挥发性,燃烧时容易排放到大气中,从而对大气产生污染。我国多数煤中含汞处于0.01～1mg/kg之间,平均0.15mg/kg。煤中黄铁矿是汞的主要载体,其它硫化物、方解石和粘土矿物也可能含汞。燃煤向大气排放汞的问题正日益受到重视。     

Fission track dating obsidians in Central and Northern Anatolia

Twenty obsidian samples from Central and North Anatolia were dated by the fission track method. Split samples analyzed in two different laboratories give consistent results. Data presented refer to three volcanic fields and are summarized as follows: Orta-Sakaeli (Northern Anatolia) obsidians with ages from 21–23 Ma; Göllü Dagi dome complex near Çiftlik (Central anatolia) has given ages between 1.33–0.98 Ma; Acigöl caldera (Central Anatolia) shows three age groups: (1) Eruptions of precaldera (Bogazköy) obsidians with ages 0.18–0.15 Ma; (2) Formation of the large intracaldera dome Kocadag-Taskesiktepe at about 0.08 Ma (uncorrected apparent age of 0.075 Ma); and (3) Acigöl peripheral obsidian domes with plateau ages of 0.020 and 0.019 Ma, and an additional uncorrected age of 0.018 Ma form a distinct age group. This fission track parameters discriminate between the various obsidian sources of prehistoric obsidian artifacts.     

Low energy γ-ray events in imaging Čerenkov telescope arrays

One of the major goals in VHE--ray astronomy is to open the energy range below 100 GeV with earthbound detectors. This paper demonstrates a new method for analyzing erenkov light of a shower in a erenkov telescope array. This method is successful for showers in this low energy regime where previous techniques (e.g. alpha analysis) are not applicable. A Monte Carlo simulation is applied to a system of 19 Whipple type [3, Cawley 1990] Imaging Atmospheric erenkov telescopes (IAT), each built as a 10 m diameter reflector and equipped with a 109 photomultiplier tube camera. The energy threshold for a single detector of this type is given [5, Kerrick et al. 1995] as 250 GeV. Analysis of simulated coincident events of the system for those events not having enough light to apply a standard imaging analysis [4, Hillas 1985], leads to a considerably lower threshold of 85 GeV. With a new analysis method of these events it is shown that it should be possible to distinguish between -ray induced and proton induced showers. The improvement of sensitivity (Q = figure of merit) of this analysis method is found to be Q=2.9.     

A new octuple Earth-crossing meteoroid stream

It was shown that the orbit of Virginid meteors is an octuple Earth-crosser so that the stream can produce eight related meteor showers. Of these eight theoretical showers five are identified in the catalogues; one of these is the Cygnids.