京津唐地区地壳结构与强震的发生──Ⅱ．S波速度结构

利用１９８６－１９９３年发生在京津唐地区的２５１６个地震的２１９２７个Ｓ波到时进行层析成像，得出：（１）公元１０００年以来研究区强震震中在下地壳的投影大多分布在低速块体内或低速块体与高速块体相交地带偏低速块体的一侧；（２）唐山地震震源下方的物质，波速比Ｖｐ／Ｖｓ呈现高值，推测呈部分熔融状态，有热物质流从莫霍界面的下方沿通向震源下方的断裂入侵的迹象。（３）黄骅坳陷中心区的上地壳呈现低Ｖｐ／Ｖｓ值，推测那里为水－汽转变的地热系，这与在该地区所测量的高热流值一致。冀中坳陷区的高Ｖｐ／Ｖｓ值反映出其地下物质可能呈部分熔融状态。     

The Generation and Compaction of Partially Molten Rock

The equations governing the movement of the melt and the matrixof a partially molten material are obtained from the conservationof mass, momentum, and energy using expressions from the theoryof mixtures. The equations define a length scale _c called thecompaction length, which depends only on the material propertiesof the melt and matrix. A number of simple solutions to theequations show that, if the porosity is initially constant,matrix compaction only occurs within a distance _c of an impermeableboundary. Elsewhere the gravitational forces are supported bythe viscous stresses resulting from the movement of melt, andno compaction occurs. The velocity necessary to prevent compactionis known as the minimum fluidization velocity. In all casesthe compaction rate is controlled by the properties of the matrix.These results can only be applied to geological problems ifthe values of the permeability, bulk and shear viscosity ofthe matrix can be estimated. All three depend on the microscopicgeometry of the melt, which is in turn controlled by the dihedralangle. The likely equilibrium network provides some guidancein estimating the order of magnitude of these constants, butis no substitute for good measurements, which are yet to becarried out. Partial melting by release of pressure at constantentropy is then examined as a means of produced melt withinthe earth. The principal results of geological interest are that a meanmantle temperature of 1350?C is capable of producing the oceaniccrustal thickness by partial melting. Local hot jets with temperaturesof 1550?C can produce aseismic ridges with crustal thicknessesof about 20 km on ridge axes, and can generate enough melt toproduce the Hawaiian Ridge. Higher mantle temperatures in theArchaean can produce komatiites if these are the result of modestamounts of melting at depths of greater than 100 km, and notshallow melting of most of the rock. The compaction rate ofthe partially molten rock is likely to be rapid, and melt-saturatedporosities in excess of perhaps 3 per cent are unlikely to persistanywhere over geological times. The movement of melt througha matrix does not transport major and trace elements with themean velocity of the melt, but with a slower velocity whosemagnitude depends on the distribution coefficient. This effectis particularly important when the melt fraction is small, andmay both explain some geochemical observations and provide ameans of investigating the compaction process within the earth.     

The Generation of Kimberlites, Lamproites, and their Source Rocks

Measurements of rare earth element (REE) concentrations in SouthAfrican kimberlites and in the Argyle lamproite from WesternAustralia constrain the composition of the source rocks fromwhich these melts originate. To account for the concentrationsof Tm, Yb, and Lu in these magmas, their sources must firsthave been strongly depleted by 20% melting in the garnet stabilityfield, and then enriched by a metasomatic melt rich in lightREE and other incompatible elements. The calculated source compositionsclosely resemble those of coarse, low-temperature, depletedperidotite nodules that are the commonest nodules in kimberlites.Rarer nodule types have undergone either more or less depletionthan have the source regions of kimberlites and lamproites.The REE composition of the metasomatic melt calculated fromthe diopsides and garnets in the sheared nodules, from the diopsidemegacrysts, and from majorite garnet inclusions in diamonds,is in excellent agreement with that expected for a melt producedby melting 0.5% of the source region of ocean ridge basalts.The initial depletion event requires the extraction of 20% meltfrom a region in which garnet and chrome-spinel were stable.The melt distribution obtained from inversion of komatiite compositionssatisfies both these conditions. Kimberlite source rocks areshallower than the layer from which fertile nodules originate.Such nodules must therefore be transported by entrainment ofthe lower boundary of the layer that becomes unstable. Thisproposal can account for their strong fabric.     

2008年度大气科学领域项目评审与研究成果分析

12008年项目申请、送审与资助情况2008年地球科学五处共受理各类项目706项。其中:面上项目356项,青年科学基金210项,地区科学基金22项,上述三类项目共588项;“天气与气候系统变化过程与机制”优先发展领域重点项目23项(其中大气学科22项),“全球变化及其区域响应”优先发展领域     

Gravity studies of the Rockall and Exmouth Plateaux using SEASAT altimetry

Abstract SEASAT altimetric measurements are used to determine the gravity anomalies across two passive continental margins: the western margin of the Rockall Plateau, UK, and the Exmouth Plateau off north-west Australia. The small gravity anomalies observed over the starved western margin of the Rockall Plateau require the existence of a major density contrast within the crust, as well as the Moho, and show that the elastic thickness is less than 5 km at the time of rifting. The gravity anomaly over the Exmouth Plateau is compared with the gravity anomaly calculated from the sediment loading of a thin elastic plate, taking account of the variation in crustal thickness. This comparison shows that the Exmouth Plateau also has a small effective elastic thickness of 5 km, even for loads emplaced between 60 and 120 Myr after rifting. Elastic thicknesses of about 5 km have also been reported for other sedimentary basins, and are to be expected if the rheological properties of the crust and mantle depend on the ratio of the present temperature to the melting temperature. Flexural effects are therefore likely to be of minor importance in sedimentary basins.     

东疆中天山北缘大水锰矿带锰矿成因类型及找矿方向探讨

文章根据矿体产出地质部位、形态特征及与围岩的关系,把大水地区锰矿划分为4种成因类型:①近代风化堆积型锰矿,②受构造裂隙控制的风化淋滤型锰矿,③产于细碎屑岩中的沉积型锰矿,④产于地层与岩体接触带内的热接触-变质型锰矿。在对该区矿床成因及成矿条件进行对比分析的基础上,明确该区有望成为一处大型锰资源勘查-开发基地,深部找矿潜力巨大。提出今后找矿方向应以沉积型锰矿为主攻目标,以花坪锰矿为突破口,运用地质、物探相结合的方法在含锰岩系深部进行找矿,通过点上突破来带动整个锰矿带的找矿工作。     

黄岩海山链俯冲与吕宋岛斑岩铜金成矿

菲律宾吕宋岛上约5Ma以来的斑岩铜金矿床主要集中在北部的Baguio和Mankayan地区,它们在时空上与黄岩海山链密切相关。1907~2013年间的地震数据表明,在吕宋岛中部(16°N)附近存在地震稀疏带。吕宋岛上的斑岩铜金矿床分布在该地震稀疏带的两侧。收集到的相应时期埃达克岩的Sr/Y-(La/Yb)N、Sr/Y-Y和La/Yb-Yb图解表明,这些埃达克岩几乎都是洋壳部分熔融形成的。与吕宋岛北部侵入型埃达克岩相比,位于16°N附近的埃达克岩具有更高的Sr含量,这可能与南海古扩张脊俯冲撕裂形成的板片窗有关。斜长石是辉长岩的主要矿物之一,因此,撕裂的洋壳边缘的辉长岩层部分熔融,形成具有更高Sr含量的埃达克质岩浆。而位于吕宋岛南部Bataan弧中的埃达克质火山岩,可能是在南海古扩张脊俯冲之前形成的。根据已发表的斑岩铜金矿床数据,Mankayan地区的成矿年龄在约3.5~1.4Ma,Baguio地区的成矿年龄在约3.1~0.5Ma之间,有从北向南变年轻的趋势,这与黄岩海山链沿马尼拉海沟向南迁移一致。此外,吕宋岛北部Mt.Cagua到Baguio之间存在一个延伸了220km的第四纪火山活动的空隙,该区域大部分火山已经在中新世停止活动。这可能是黄岩海山链的俯冲使得俯冲倾角逐渐变缓、挤压加强而导致的。同时期的斑岩铜矿床正好分布在这一火山空隙中,是俯冲洋壳部分熔融的产物。     

钼的地球化学性质与成矿

钼在硅酸盐地球中的丰度很低,作为中度不相容元素,简单的岩浆形成、演化过程很难使之从地壳丰度直接富集到工业品位。我们研究结果显示钼的成矿主要通过两阶段富集过程来实现:一是与风化、沉积有关的表生过程;二是与板块俯冲或深埋熔融有关的岩浆过程。钼是变价元素,在寒武纪大气氧再次升高以后,钼在地表化学风化过程中容易被氧化为水溶性的Mo O42-,进入地表径流和海洋湖泊中,并且在还原条件下进入富含有机质的黑色页岩等沉积物(岩)中。富钼沉积物(岩)在随板块俯冲到地幔或深埋等条件下可以因升温变质,进而发生部分熔融,形成富钼的原始岩浆,在俯冲条件下往往形成斑岩铜(金)钼矿床,氧逸度低于斑岩铜矿,而斑岩钼矿的氧逸度更低。具有高化学风化速率、大的流域面积的封闭、半封闭型水域和河口地区是表生过程中钼富集的最佳区域,是大型钼矿形成的基础。     

橄榄岩蛇纹石化过程中氢气和烷烃的形成

蛇纹石化过程中形成氢气、烷烃和有机酸,为海底热液区生命活动提供物质和能量来源,可能对地球和其他行星早期生命起源和演化有重要影响。目前关于蛇纹石化过程中氢气和烷烃形成的研究大多以橄榄石为初始物,且温度和压力较低(≤300℃,500bar)。本研究通过一系列的水热实验,研究300~500℃、1~3kbar时橄榄石、斜方辉石、单斜辉石、橄榄岩、玄武岩以及玄武岩与橄榄岩混合物发生蛇纹石化反应后氢气和烷烃的生成。300℃、3kbar时,橄榄石蛇纹石化后产生的氢气远大于辉石蚀变后产生氢气的量。随着温度的增加,400~500℃、3kbar时,橄榄石蚀变程度极低,产生氢气的量低于斜方辉石。单斜辉石实验后没有发生蚀变,不产生氢气和烷烃。400~500℃、3kbar时,橄榄岩蛇纹石化后产生的氢气和烷烃远高于橄榄石、斜方辉石和单斜辉石。玄武岩蛇纹石化后生成氢气和甲烷的量低于橄榄岩,但与玄武岩和橄榄岩混合物相当。这是因为玄武岩的单斜辉石蚀变后形成富铁的透辉石(~8.1%FeO),透辉石的Fe以Fe2+为主,这降低了Fe3+和氢气的量。以上表明,橄榄岩的蛇纹石化不同于橄榄石和斜方辉石。不仅是海底热液蚀变产生氢气和甲烷,洋壳俯冲过程中地幔楔橄榄岩蛇纹石化也会生成氢气和甲烷,但由于洋壳玄武岩的加入,氢气和甲烷的量会远小于橄榄岩蚀变时的量。