超临界流体热力学函数的理论计算

Ｄｕａｎ等（１９９２。１９９６）基于分子间相互作用势能模型,建立了一个适合于超临界流体的状态方程,此方程能反演出世界上几十个实验室测定的成千上万个纯组分及混合物的ＰＶＴ（压力、体积、温度）数据（温压范围：Ｐ〈２ＧＰａ,Ｔｃ〈Ｔ〈２０００Ｋ）。最近的研究发现,此方程能准确预测Ｈ２Ｏ、ＣＯ２、ＣＨ４、Ｎ２及它们的混合物在Ｔ＝１．３Ｔｃ,Ｐ＝０到Ｔ＝２０００Ｋ,Ｐ＝１０ＧＰａ这一温压范围内的压力、体积、     

使用流体压差法建立根缘油气藏动态平衡

根缘油气藏(深盆油气藏) 是紧临源岩存在的烃类聚集, 是在高勘探程度下所发现的油气藏类型.由于它在成藏机理及存在方式上的特殊性, 常规意义上所采用的动力平衡方程不再适合于对其成藏平衡作用过程的分析.结合根缘油气藏地质特征及其演化特点, 采用对连续油气柱上升力的分解分析方法, 讨论了流体压差的平衡问题, 建立了位于源岩上部的根缘油气藏的动力平衡方程.      

我国火山地热流体地球化学研究新进展

本文综述了最近几年来中国研究者在地热流体地球化学研究领域取得的主要进展。在国际上关于地球内部流体及其作用研究取得重要进展的大背景下,我国学者在地热流体地球化学研究上也取得了一些重要成果,主要表现在火山地热区和非火山地热区两大方面,在火山学、地热学、环境学、大地构造学、地震学等五个学科领域都取得了一些重要进展。     

右江盆地含油气成矿流体性质及其成藏-成矿作用

右江盆地含油气成矿流体是一种多组分、多相态的不混溶体系,成藏流体具低温(多为90～160℃)和低盐度(多小于6wt%NaCl)的特征,其主要组分是有机质、CO2和H2O;金矿成矿流体以中低温(多集中于150～250℃)和低盐度(0.4～6.7wt%NaCl)为特征,其主要组分为H2O和CO2,次为烃类有机组分。盆地内古油藏与金矿床在空间上密切共存,在成藏和成矿流体活动时限上基本一致,在成因上一脉相承,表明两者均为盆地有机成矿流体演化的产物。加里东晚期至印支中期,"盆-台相间"的沉积构造格局为成矿和成藏奠定了物质基础,盆地有机成矿流体的活动使油气和金属分别聚集形成油气藏和金属矿床。印支晚期至燕山早期,伴随褶皱造山作用的盆地流体活动使油气的原始分布格局发生改变,并造成了油气和金属矿床的空间分带。燕山中晚期强烈的构造抬升剥蚀,使油气藏和金属矿床遭受强烈的破坏与改造。     

固体地球观向流体地球观的概念更新

长时间内人们把地球看成为一个固体星球,忽视流体在地球动力学中非常重要的作用.在本文中我们将列举一系列的资料来证明它.此流体由H\|A\|C\|O\|N\|S组成.H (氢, 卤素和热), A (碱金属, 例如 Na, K等.), C (碳), O (氧), N (氮), S (硫族).此流体从深部外地核H, H2流向上进入地幔演化为H\|HACONS, 向上到上地幔演化为A\|HACONS, 向上进入地壳后演化为O\|HACONS. 此流体可以使固体地幔,地壳发生弱化,变软,熔融和排气,结果造成地球动力学及大地构造运动和众多自然灾害.     

埋藏有机酸性流体对四川盆地东北部飞仙关组储层的溶蚀改造作用：溶解动力学实验研究

通过白云岩化鲕粒灰岩与0.1 mol/L乙酸的旋转盘溶解动力学实验,研究了深埋藏中有机质热演化过程中伴生的有机酸对鲕粒灰岩储层的改造作用机理.结果显示,白云岩化鲕粒灰岩溶解反应的速率在3.26×10-7～6.66×10-7 mol/(cm2·s)之间,并且溶蚀速率随温度和转速的增加而增大.反应前后样品表面的扫描电子显微...     

The origin of magnetization and geochemical alteration in a fault zone,Kilve, England

The origin of an apparently syndeformational chemical remanent magnetization (CRM) and geochemical alteration in a fault zone in the Bristol Channel Basin, southwest England, was investigated. Deformation in the fault zone occurs in Jurassic aged, organic-rich limestones and consists of numerous normal and oblique-slip faults and associated folds. Migration of basinal, radiogenic fluids is indicated by elevated ⁸⁷Sr/⁸⁶Sr values for calcite veins that occur throughout the fault zone. Some of the calcite veins contain hydrocarbons sourced from deeper strata. Elevated ⁸⁷Sr/⁸⁶Sr values in the host Jurassic limestones indicate that they were also extensively altered by radiogenic fluids that migrated through microfractures in addition to major fault and fracture planes. Folded and tilted host limestones contain a pervasive secondary CRM residing in magnetite that was acquired during deformation in the Tertiary. The association between this pervasive CRM and the pervasive geochemical alteration is consistent with a genetic connection between the orogenic fluids and the CRM although the timing of CRM acquisition (Tertiary) is not consistent with structural interpretations for the timing of most veining. An alternative remagnetization mechanism which is not triggered by externally derived fluids, such as diagenesis of hydrocarbons, might account for the CRM. Hydrocarbon-bearing veins also contain a CRM that resides in magnetite, although the time for remanence acquisition is not well constrained by field tests. © 1998 John Wiley & Sons, Ltd.     

Nonlinear pulsations of horizontal jets

A shallow-water model with horizontally nonuniform density is used to study the dynamics of jet flows that arise under the influence of buoyancy and the Coriolis force. Within this approach, the jet is described by a self-similar compactly-localized solution and interpreted as a band of shear flow having a temperature contrast with the ambient fluid. In addition to stationary states, the dynamics of such jets admit cyclonic rotation with a constant angular velocity and transverse nonlinear pulsations. The phase portrait corresponding to this model shows that regimes with pulsating jets develop along closed trajectories bounded by the separatrix loop. The theory predicts that the period for warm jet pulsations is longer than the inertial oscillation period caused by the Earth’s rotation, while for cold jet pulsations, it is shorter. Thus, only warm jets can have a noticeable effect on the atmospheric dynamics in the synoptic range. In particular, they may well be responsible for additional spectral peaks that appear in this range of wind speed fluctuations.