Magnetic anisotropy produced by magma flow: theoretical model and experimental data from Ferrar dolerite sills (Antarctica)

Volcanic rocks forming sills, dykes or lava flows may display a magnetic anisotropy derived from the viscous flow during their emplacement. We model a sill as a steady-state flow of a Bingham fluid, driven by a pressure gradient in a horizontal conduit. The magma velocity as a function of depth is calculated from the motion and constitutive equations. Vorticity and strain rate are determined for a reference system moving with the fluid. The angular velocity and the orientation of an ellipsoidal magnetic grain immersed in the fluid are calculated as functions of time or strain. Magnetic susceptibility is then calculated for a large number of grains with a uniform distribution of initial orientations. It is shown that the magnetic lineation oscillates in the vertical plane through the magma flow direction, and that the magnetic foliation plane changes periodically from horizontal to vertical. The results are compared with the magnetic fabric of Ferrar dolerite sills (Victoria Land, East Antarctica) derived from low-field susceptibility measurements.     

Shorelines of the Uppsala Esker East-Central Sweden: Their Use as Indicators of Regional Differences in Shore Displacement

About 750 different shoremarks, mainly shore terraces, have been levelled along the Uppsala esker. Using various methods it has been possible to arrange the shoremarks to shorelines or rather shoremark zones containing more shoremarks than intervening parts. The material was divided into two major parts, i.e. shoremarks below c . 15 m above sea level and shoremarks above c . 15 m. It was found that shorelines on the whole were sloping towards the north. This was expected because of the faster shore displacement in the northern part of the area. However, the shorelines below c . 15 m a.s.l. indicated a slower increase in shore displacement than those of higher altitudes. A conclusion drawn from this might be that the increase towards the north is retarded in the area around Lake Mälar. This result is in reasonable agreement with recent isobase systems constructed from the evidence of mareograph records and repeated precise levellings. On the other hand, the shoreline studies give evidence of more pronounced regional differences in shore displacement in earlier Litorina times than those found today.     

煤中黄铁矿的成因研究

本文在系统地研究四川晚二叠世高硫煤中黄铁矿矿物学的基础上，运用微区电子探针、中子活化、Ｘ光电子能谱和硫同位素等多 种方法综合地研究煤中黄铁矿的结构、成分、价态及同位素等成因标型特征，对黄铁矿标型特征进行了成因探讨，有效地判别了成岩期形成的Ｉ型脉状黄铁矿及后生热液Ⅱ型脉状黄铁矿。同时提出直接沉淀系列（自形晶→集合→聚晶）和复杂成因（微粒、莓粒→圆球→结核→团块）等两大类成因演化模式。它不仅对不同类型     

香炉碗子金矿床稳定同位素研究及矿床成因探讨

香炉碗子金矿床产于脆一韧性剪切带内，控矿围岩为火山隐爆角砾岩体，通过硫，铅，氢，氧，碳，锶等同位素及稀土元素的研究可以看出，该矿床是一个中，低温有大气水参与火山热液型金矿床，其火山岩岩浆属太古宙结晶基底重熔再造，壳幔混合型。     

宁芜地区中生代岩浆岩的成因——岩石学与Nd,Sr,Pb同位素证据

宁芜中生代火山盆地产出火山岩与侵入岩，火山岩以玄武粗安岩，粗安岩和粗面岩为主，安山岩和响岩少量，火山岩以高钾富碱为特征，已确定为橄榄安粗岩系。侵入岩以辉长闪长玢岩－一辉长闪长岩为主，以高钠低硅为特征，并有辉长岩和花岗岩产生，据地质学和Ｎｄ，Ｓｒ，Ｐｂ同位素资料，侵入岩与火山岩属同一个岩浆系列，是碱性玄武岩浆在下地壳经过轻度ＡＦＣ混合后，侵入上地壳，在轻度混染的情况下，经过以结晶分离为主的岩浆分异形     

山东牟平邓格庄金矿的地球化学特征及成因

邓格庄大型石英脉型金矿，分布于燕山期昆嵛山花岗岩体内金牛山断裂带次级断裂中。成矿年龄１１８×１０６ａ，它比容矿岩体冷凝至３５０℃时还晚１２×１０６ａ。成矿深度小于１ｋｍ（约０．７５ｋｍ），而容矿岩体的定位深度大于１３ｋｍ，它们的定位深度差大于１２ｋｍ。成矿流体来自地壳深部，通过水－岩反应又从容矿岩体中萃取一部分金。故此金矿不是传统意义的岩浆期后热液矿床     

抚顺盆地超厚煤层的沉积条件分析

根据抚顺盆地早第三纪超厚煤层中异常丰富的成因标志，论证了一种与河流、风暴作用有关的陆相超厚煤层形成新机制－湖成异地－微异地混合堆积机制。在这一新机制中，由风暴上升流（也许还有地震）触发的水下重力流及风暴回流，既驱动湖滨泥炭沼泽和三角洲上的有机碎屑及无机碎屑进入湖泊中心区，又造成泥炭碎屑在较深水环境的再次堆积，从而使其中无机碎屑与泥炭碎屑有效地分离。     

湖北郧西六斗金矿床地质地球化学及矿床成因研究

郧西县六斗石英脉一破碎蚀变岩型金矿床，是鄂西北地区近年新发现的金矿床之一。通过对金矿床产出地质背景、控矿地质条件、围岩蚀变、矿石矿物、包体物理化学、同位素地球化学等的研究，阐述了六斗金矿床的形成机理和成矿物质来源。确定了该矿床成因类型为与韧性剪切变形变质作用有关的中一低温热液矿床。     

泌阳碱矿形成的地球化学模拟研究

泌阳碱矿过去一直被认为是原生沉积矿床。通过综合分析泌阳凹陷的地质、石油地质、碱矿地质和水文地质条件，从不同方面论证泌阳碱矿不太可能属于原生沉积矿床。利用地球化学模拟技术，从理论上模拟了泌阳碱矿的形成过程，提出了一种水－岩相互作用成矿模式，并用大量的事实支持了这种观点。     

岩浆活动对油气藏形成条件的影响

结合众多实例，总结了国内外含油地中岩浆活动对油气藏形成的影响。一方面，岩浆活动所携带的高热流可以提高古地温，加速生油岩的演化，亦将使与岩浆岩毗邻的生油岩达到高成熟或过成熟，