冀北榆树沟煤矿区褐煤地下气化地质条件分析

通过对冀北沽源县榆树沟煤矿白芈系青石砬组含煤地层地质条件进行分析,认为仵该矿区进行煤炭地下气化是可行的。研究区构造简单,为一轴向近东西向的舒缓向斜,主要煤层厚度大,最大平均厚度为24.31m。可采煤层顶板多为泥岩、炭质泥岩,尤其是煤系上覆的“三趾马红土”层,对气体有良好的圈闭作用。由于褐煤的灰分含量高,26％～49．03％,地下气化时对煤层顶板影响小,主要煤层埋藏浅200—300m,水文地质条件简单,根据诸多因素分析认为该矿区适合进行褐煤地下气化开采。     

Sedimentary characteristics of terrigenous debris at site MD05-2905 in the northeastern part of the South China Sea since 36 ka and evolution of the East Asian monsoon

Sediments with high sedimentation rate at site MD05-2905 in the Northeastern slope of the South China Sea provide unique materials for a high-resolution study on the paleoenvironment. Based on precise dating of AMS ¹⁴C, grain size analysis of terrigenous debris at core MD05-2905 was conducted after organic matter, biological carbonate and biogenic opal were removed. The results show that 15.5–63.5 μm coarse grain size ingredients may indicate East Asian winter monsoon changes and that 2–9 μm fine grain size ingredients may be used as a proxy of evolution of the East Asian summer monsoon. The results of grain size analysis, which suggest East Asian monsoon intensity, reveal that a winter monsoon dominated the glacial regime and a summer monsoon dominated the Holocene regime. It was also shown that the summer monsoon increased gradually, experienced several abrupt changes and reached a culmination in the early Holocene (11200–8500 a B.P.) since 36 ka. Controlled by precession periodicity, it may be related with the amount of solar radiation at the highest stage, which needs further study. __________ Translated from Advances in Earth Science, 2007, 22(10): 1012–1018 [译自: 地球科学进展]     

中国海相探矿权区块定量评价方法

在研究了我国海相油气探矿权区块基本油气地质条件、勘探程度、技术经济条件等要素和特点的基础上,给出了48个评价参数和归一化取值参照表,建立了探矿权区块评价工作流程、评分参数及计算公式。提出对我国海相勘探层探矿权区块评价应该注意:与国外海相碳酸盐岩评价的差别;与国内陆相碎屑岩评价的差别;成藏组合的划分;评价内容的有效性、不确定性和评价参数的可信度;成败经验的总结和勘探程度的研究。     

祁连山北缘—河西走廊西段晚新生代逆冲推覆断裂发育模式

祁连山北缘—河西走廊西段地处青藏高原东北缘,是我国新构造活动最强烈的地区之一。通过野外对研究区主要活动断裂的调查研究、结合年代学测试和综合分析,认为祁连山北缘—河西走廊西段地区的旱峡—大黄沟断裂、玉门断裂、新民堡断裂和阴洼山断裂都是晚更新世至全新世活动断裂。旱峡—大黄沟断裂形成于中新世晚期,一直活动至今;玉门断裂形成于上新世早期,在距今7.6ka左右和3.2ka左右发生过2次强烈的新构造活动(古地震),也是2002年玉门地震的发震断裂;阴洼山断裂形成于上新世晚期(3.0Ma左右),在距今19.9～21.0ka、8.6～10.0ka、4.1～5.0ka发生过3次强烈的新构造活动,也可能是1785年惠民堡(现新民堡)地震的发震断裂;但是位于近盆地中心的新民堡断裂形成时代明显晚的多,起始于中更新世晚期(0.17Ma左右),在距今28.3ka、4.4ka和1.2ka左右发生过强烈的3次新构造活动。在运动形式上,上述4条断裂均为自南南西向北北东的逆冲推覆。在变形性质上,新民堡断裂以非地震性的蠕滑为主,其他3条断裂主要为地震性的粘滑变形。在祁连山北缘—河西走廊西段的北北东剖面上,逆冲推覆断裂表现为前展-后展复合发育模式,即形成时代最新的是位于酒西盆地中心的新民堡断裂,在酒西盆地中心以南部分的剖面中断裂发育为前展式,由祁连山腹地向河西走廊盆地中心断裂形成时代越来越新,而酒西盆地中心以北部分的剖面中断裂发育为后展式,即从盆地中心到盆地北缘断裂形成时代越来越老。     

上海市长江口及邻近海域地质调查现状及展望

海洋区域地质调查近年来逐渐得到重视,海洋地质调查技术的发展也为开展海洋区域地质调查奠定了基础。上海地区社会经济发展对地质工作的需求,为摸清上海市长江口及邻近海域的地质现状提出了必然要求。本文在系统整理长江口及邻近海域地质资料的基础上,重点分析了区内存在的重点地质问题和研究存在的问题,根据海洋地质调查的技术发展,结合国内相关地区的调查经验,对长江口及邻近海域内区域地质调查进行了展望,提出了采用综合物探技术、地质取样和测试分析进行综合地质环境调查的建议,并对具体采用的调查技术和调查内容进行了论述。     

A quantitative model of coherent,stimulated emission in astrophysical jets

On the basis of issues raised by observations of BL Lac objects and the qualitative jet model proposed by Bakeret al. in 1988, we have been led to consider the quantitative role of coherent, stimulated emission in jets and construct a new jet model of blazars in which a relativistic electron beam with an axial symmetric, power-law distribution is injected from the central engine into the jet plasma. We study quantitatively the synchrotron emission of the relativistic electron beams. Using the weak turbulent theory of plasma, we discuss the interaction between relativistic electron beams and jet plasma, and the roles of stimulated emission. The main results are:

1. The synchrotron emission increases sensitively with the increase of the angle between the direction of the beam and the magnetic field. When the direction of the beam is vertical to the magnetic field, the synchrotron emission reaches its maximum, i.e. the emitted waves are beamed in the direction of the jet axis. We suggest that radio selected BL Lac objects belong to this extreme classification.
2. The synchrotron emission of the relativistic beam increases rapidly with the increase of the Lorentz factor of the relativistic electron,γ, whenγ ≤ 22.5, then decreases rapidly with increase ofγ.
3. The stimulated emission also increases with increasing Lorentz factorγ of the relativistic electrons whenγ ≤ 35 and then decreases with the increasingγ. The maximum stimulated emission and the maximum synchrotron emission occur at different frequencies. Stimulated emission is probably very important and reasonable flare mechanism in blazars.
4. The rapid polarization position angle (PA) swings may arise from the interaction between the relativistic electron beam and the turbulent plasma.

     

Densities of Huanghe River estuary and Bohai Bay waters

The densities of 36 water samples from the Huanghe River estuary and Bohai Bay were determinedby a magnetic float densimcter under three temperatures from 15℃ to 25℃.All the measured densities ofsamples were greater than that of the values calculated from the International Equation of State of Seawater.The differences between the measured and calculated densities increased with the decrease of salinities.The dif-ferences appeared exponentially correlated with[Ca~(2+)]/s,[Mg~(2+)]/s and[SO_4~(2-)]/s,and had"s"type curverelationship with the alkalinity in all salinity range.But in the salinity ranging from 25.72 to 31.57,therelationships were all linear.The density difference can be estimated from the equation △ρ（10~3kg·m~(-3)）=（-2.79+236.5([Ca~(2+)]/s)/(-9.7464×10~（-3）+[Ca~(2+)]/s).It was the high alkalinity and[Ca~(2+)]/s that resulted in the measured densi-ties of seawaters being higher than the calculated densities in the Huanghe estuary and Bohai Bay.     

全球不同构造环境蛇纹岩全岩和矿物微量元素组成及非传统稳定同位素(Fe- Zn- Cu同位素)特征

蛇纹岩对地球深部和浅部的元素循环以及氧化还原状态调节具有非常重要的作用。蛇纹岩中的流体活动性元素(fluid- mobile element, FME)是揭示地幔岩石水化、脱水以及元素循环的关键。本文系统收集和分析了前人报道的不同构造环境的蛇纹岩矿物化学、全岩微量元素和非传统稳定同位素(Fe、Zn、Cu)的组成特征，试图从多个角度总结蛇纹岩脱水过程的元素迁移规律及流体性质。蛇纹岩主要矿物蛇纹石微量元素含量具有以下主要特征：① 不同变质程度的蛇纹岩中的蛇纹石既包含轻稀土元素(light rare earth element, LREE)富集，又包含LREE亏损的特征；② 纤蛇纹石的REE和微量元素分布在利蛇纹石和叶蛇纹石的范围内，利蛇纹石重稀土元素(heavy rare earth element, HREE)整体上略高于叶蛇纹石且更加富集FME；③ 通过中度不相容元素与REE含量相结合，能够较好地区分橄榄石和辉石蛇纹石化所形成的蛇纹石，即辉石形成的蛇纹石富集相容元素(如Sc、Zn、Cr、Y和Ti等)并具有较高的HREE，而橄榄石形成的蛇纹石则表现为平坦且整体较低的REE分布型式。在蛇纹岩全岩微量元素和稀土元素(rare earth element, REE)含量方面，不同构造环境的蛇纹岩具有较大范围的重叠，但也有一定的差异：① 慢速扩张的印度洋中脊蛇纹岩REE和微量元素含量要整体高于快速扩张的大西洋中脊和太平洋中脊的蛇纹岩；② 马里亚纳蛇纹岩泥相比于蛇纹岩和蛇纹石化纯橄岩具有更高的REE和微量元素，而蛇纹石化纯橄岩相比于蛇纹岩则具有相对低的REE及流体不活动性元素含量。因此，利用微量元素的含量在区分不同环境的蛇纹岩方面存在一定的困难。但是，碱金属元素与U元素含量及其相应的比值，则可以较明显区分出大洋蛇纹岩和弧前蛇纹岩。目前已发表的蛇纹岩Fe、Zn、Cu同位素数据表明：① 蛇绿岩中的蛇纹岩Fe和Zn同位素的分馏与其变质程度密切相关。蛇纹岩在进变质过程中δ 56Fe值与Fe 3+/∑Fe值呈负相关，而Zn含量和δ 66Zn值则呈现正相关，表明蛇纹岩变质脱水能够释放氧化性流体；② 与橄榄岩相比，蛇纹岩具有明显低的δ 65Cu值，表明橄榄岩蛇纹石化过程中存在氧化性流体的加入。蛇纹岩Fe、Zn、Cu同位素在示踪流体性质和氧化还原状态方面有很大潜力，对壳幔系统的化学循环具有重要意义。     

近海核电厂核素地下水释放通量的模型计算方法

为了定量计算陵区近海核电站排水管线泄漏情景下核素通过地下水途径向海洋环境的释放通量，以某近海核电站为例进行研究。首先，应用GOCAD软件建立三维地形地质模型，刻画地层的分布、剥蚀以及倾向等特点；然后，运用地下水数值模拟软件FEFLOW精细刻画丘陵区地下水系统的补给、径流和排泄特征；最后，以不被吸附滞留的核素³H和被吸附滞留的核素⁹⁰Sr、¹³⁷Cs为对象，通过实验测定了⁹⁰Sr、¹³⁷Cs在不同岩土介质中的分配系数，模拟计算了排水管线连续渗漏60 a后³H、⁹⁰Sr、¹³⁷Cs在地下水中的放射性分布及释放。结果表明：³H迁移速度基本与地下水流速一致，地下水中的最大放射性浓度为0.285 0 Bq/L，第20 000天时向收纳水域的释放通量达到最大值，约526 Bq/d；⁹⁰Sr吸附性能相对较弱，最大迁移距离约80 m，地下水中的最大放射性浓度为0.032 1 Bq/L；¹³⁷Cs吸附能力较强，相当长的时间内被滞留在管线附近，地下水中最大放射性浓度分别为6.840×10^-3 Bq/L，释放通量为0 Bq/d。由弥散度的不确定分析可知，弥散度越大，地下水中³H的最大放射性浓度越小，向海洋环境的释放通量越多。     

The effect of an optically thin region on stability of an accretion disk around a supermassive black hole

We analyse conditions of the innermost portion of an accretion disk and establish a set of equations for this region. A stable innermost region may exist, which can probably explain the observed UV and X-ray spectra, avoiding the unstable emission. We then discuss the detailed radial structure of a disk around a black hole for typical AGN parameters and obtain different kinds of- relationships for different regions of a disk. On the basis of this, we discuss the stability. A new type of cycle is present, which we call a double S shaped cycle. In this cycle, the extent of accretion rate variability is much larger than that in dwarf nova cycles. This probably solves the problem of violent variability of AGN. In the meantime, the very high accretion rate at the hottest state in limit cycles in the unstable region may provide continuous injection of matter to the jet and power the relativistic motion of the jet.