庐山星子群变质岩的变质作用P-T条件研究

对分布于扬子块体南缘古元古代星子群变质宏的变质作用研究表明，它们普遍经历了角闪岩相的变质，其变质温度为480℃-580℃，压力在300MPa-500MPa之间。这与扬子块体南缘其他元古代地层仅经历了轻微变质的事实截然不同，表明星子群变质岩具有独特的构造演化历史。越来越多的研究发现，星子群变质岩是由地壳伸展作用引发的、来源于下地壳的前寒武纪变质基底，它并不是来源于华夏块体的“飞来峰”。     

天然焦型煤层气储存特征

天然焦具有良好的物性条件，含有大量的瓦斯气体，是一个理想的储气层。但在煤矿生产中却经常是遇到天然焦因瓦斯增大而中止生产的现象时有发生。本文根据天然焦的物性条件，结合阜新矿区井下实践，论述了煤层气在天然焦内的储存特征，并指出了在煤层气开发利用方面应予以重视的问题。     

吉林延边开山屯地区蓝片岩相变质作用——来自硬绿泥石＋纤锰柱石＋多硅白云母组合的证据

吉林延边开山屯低级变质作用发育于兴凯地块西南晚古生代活动大陆边缘，这里产出二叠纪末的消减增生杂岩。低级变质作用矿物除冻蓝闪石、阳起石、玉髓、黝帘石、多硅白云母、绿泥石、钠长石外，还在灰黑色变泥质岩中发现硬绿泥石 纤锰柱石 多硅白云母组合。这是国内首次报道的以泥质岩为原岩并具有硬绿泥石 纤锰柱石标志矿物组合的蓝片岩相岩石。研究表明，该组合的形成温度290．14(或370．8)℃，具明显的低温特征。     

地质基础理念之我见

任-侵位的岩浆体，在结晶分异、固化成岩过程中，一般都可分为：已结晶的固相岩体、正(半)结晶的可塑相岩体及未结晶的熔融相岩浆3部分．此时，若发生了地壳运动，地壳运动的构造作用力。使正(半)结晶的可塑相岩体发生可塑相变形，形成片麻化岩体；地壳运动(包括地震)时的构造作用力为脉动性质的挤压作用力；岩体发生片麻化的地壳运动，又使已结晶的固相岩体和围岩发生断裂活动，形成了断裂带控矿、容矿构造；未结晶的熔融相岩浆再度上升侵位，便形成了小侵入岩体控矿构造．残浆的形成与排出，控矿构造的发生、发展与控矿过程，都是在这次地壳运动过程中完成的．因此，对这次地壳运动可称成矿作用．     

北大别燕子河片麻岩的锆石U-Pb年龄：印支期变质事件的确定

本文对北大别燕子河地区英云闪长质片麻岩中的锆石进行了单颗粒U-Pb年龄测定。该片麻岩中存在两种类型的锆石,一种是片麻岩原岩中的岩浆锆石,在后期的变质事件中经历了不同程度的Pb丢失;另一种是变质作用过程中的新生锆石。5个分析点拟合出一条很好的不一致线,得到上下交点的年龄分别为880±110Na和228±13Ma(MSWD=1.1),其中上交点的年龄代表了片麻岩原岩的形成时代,下交点的年龄代表了变质作用发生的时间。变质锆石给出了238Ma的一致年龄,与不一致线给出的下交点年龄在误差范围内相同。这一结果表明北大别片麻岩也经历了印支期变质作用。北大别地体为扬子板块的北缘,华北与扬子板块的缝合线应位于北大别以北。     

高压下玄武岩浆的不混溶及其对双峰式火山岩的成因意义

我们在温度850～1300℃,压力1.0～3.0GPa和含约2%水的条件下的碱性玄武岩熔融实验产物中发现在高于2.0GPa压力下玄武岩熔融后的淬火产物中存在着两种不同成分的玻璃,其中一种呈褐色,另一种为浅色或无色.玻璃的电子探针分析结果表明,褐色玻璃具有相对高的MgO、FeO和相对低的SiO2、K2O、Na2O含量及Na2O＞K2O的特征.熔体的不混溶间隙与温度无明显关系,但与压力关系密切,即在大于2.0GPa的压力条件下两种玻璃的不混溶间隙突然增大.因此,由不混溶作用形成的双峰式火山岩应来自大于2.0GPa的上地幔,且是能够提供酸性端员物质以及快速上升的构造环境.这与双峰火山岩可以产生于大陆裂谷环境或主要产于俯冲带的弧后拉张环境而不是岛弧前缘一致.     

地球深部物质的某些物性测量方法研究

文中介绍了地球深部物质实验室近 2 0年来开展高温高压下地球深部物质物性实验研究过程中 ,在测量方法方面的进步和应用情况。这些测量方法包括了高温、高压下弹性的超声测量方法、高温高压下电性的测量方法、高压差热分析法和高压下热学Gr櫣ｎｅｉｓｅｎ参数的测量方法诟呶赂哐瓜卵沂涂笪锏牡猿饬恐?,我们由超声脉冲透射方法改进为超声脉冲透射反射法 ,克服了样品室中压力和温度梯度对样品的影响。在高温高压下岩石和矿物的电学性质测量中 ,我们由直流法发展为阻抗谱法 ,不仅克服了样品极化对测量结果的影响 ,还可以获得离子在溶液中的多种物理化学参数 ,以及监测含水矿物在高温高压下的脱水动力学特征。在固体传压介质中建立的高压热学Gr櫣ｎｅｉｓｅｎ参数的测量方法 ,由于升压速率比较小且叶蜡石在高压下的热导系数增大 ,其测量结果需要进行校正 ,其测量方法有待进一步改进。     

中国东部苏鲁榴辉岩超基性岩褶皱带的演化及其与大别(中国)和柯切塔夫(哈萨克斯坦)杂岩的对比(英文)

苏鲁褶皱带形成于元古宙 (2 2 33～ 185 5Ma)典型优地槽构造环境 ,主要由石榴橄榄岩、石榴辉石岩、榴辉岩等侵入岩 (柯石英深度相地幔岩浆房中形成 )和它们的火山沉积建造围岩一起经褶皱、变质而形成。变质作用经历了先蓝片岩相 (前花岗岩 )后片麻岩混合岩相过程。由于变质作用的不规律性 ,苏鲁褶皱带可分为 2个构造带 :(1)东部构造带 (蓝片岩 )和 (2 )西部构造带 (片麻岩混合岩 )。根据A·都城秋穗所识别的变质带系统 ,可将其作为一个双变质带。东部构造带以出现许多块状、条带状榴辉岩辉石岩橄榄岩组合的残余岩块为特征 ,其中还残留着高压的矿物 (石榴石、绿辉石、柯石英 ) ,而且有被混合岩和各种交代岩替代的显著标志。在中生代 ,苏鲁元古褶皱带受造山作用的影响活化 ,导致许多花岗岩体的侵入 ,使交代岩广泛发育。     

A comparison of the evolution of diamondiferous quartz-rich rocks from the Saxonian Erzgebirge and the Kokchetav Massif: are so-called diamondiferous gneisses magmatic rocks?

The petrography and chemical composition of minerals of quartz-rich diamondiferous rocks from the Kokchetav Massif, especially the zonation of garnet, were studied and compared with diamondiferous quartzofeldspathic rocks from the Saxonian Erzgebirge. Many compositional and textural features were found to be similar. For instance, microdiamonds are enclosed systematically in a specific intermediate growth zone of garnet in these rocks. On the basis of experimental data, a magmatic scenario was constructed to check if the quartz-rich diamondiferous rocks are of magmatic origin. By this, the P-T paths, derived here for the Kokchetav rocks, and the textural observations it is concluded that the minerals of the diamondiferous rocks have crystallized from silicate melts. These melts originated by anatexis of deeply submerged metasediments (Erzgebirge: at T as high as 1200°C, Kokchetav Massif: at 50-100°C lower T) and ascended from at least 200 km depth. Relics of the pre-anatectic evolution are still present, for instance, as garnet cores. After ascent and emplacement of the magma in deep portions of thickened continental crust (Kokchetav Massif: 45-50 km close to 800°C, Erzgebirge: 55-60 km at 30-50°C lower T) considerable quantities of (white and/or dark) micas formed by peritectic reactions from melt. For instance, garnets could be resorbed at this stage and biotite grew instead. After the magmatic stage, retrogression took place much stronger in the Kokchetav Massif. This was accompanied by deformation transforming broadly the magmatic texture of quartz-rich diamondiferous rocks from the Kokchetav Massif to a gneissic texture.     

Characterisation of the 1997 Vulcanian explosions of Soufrière Hills Volcano,Montserrat, by video analysis

The activity of Convention at Montserrat Soufrière Hills Volcano, Montserrat, during the period 1995–1999 included numerous violent explosions. Two major cycles of Vulcanian explosions occurred in 1997: a first of 13 explosions between 4 and 12 August and a second of 75 between 22 September and 21 October. The explosions were short-lived events lasting a few tens of seconds during which partial fountain collapse generated pyroclastic surges and pyroclastic flows, and buoyant plumes ascended 3–15 km into the atmosphere. Each explosion discharged on average 3×10⁵ m³ (dense-rock equivalent, DRE) of magma, draining the conduit to depths of 1–2 km. The paper focuses on the first few seconds of three explosions of the 75 that occurred in September/October 1997: 6 October 1997 at 17:50, 7 October 1997 at 16:02 and 9 October 1997 at 12:32. Physical parameters such as exit velocities, magmatic water contents and magma pressures at fragmentation are estimated by following and modelling the ascent of individual momentum-dominated finger jets visible on videos during the initial stages of each explosion. The model treats each finger jet as an incompressible flow sustained by a steady flux of gas and particles during the few seconds of ascent, and produces results that compare favourably with those using a multiphase compressible code run using similar eruptive parameters. Each explosion reveals a progressive increase in eruptive intensity with time, jet exit velocities increasing from 40 m s^–1 at the beginning of the explosion up to 140 m s^–1 after a few seconds. Modelling suggests that the first magma to exit was largely degassed, whereas that discharged after a few seconds contained up to 2 wt% water. Magma overpressures up to ~10 MPa are estimated to have existed in the conduit immediately prior to each explosion. Progressive increases in jet exit velocity with time over the first few seconds of each explosion provide direct evidence for strong pre-eruptive gradients in water content and magma pressure in the upper reaches (probably 100–500 m) of the conduit. Fountain collapse occurred during the first 10–20 s of each explosion because the discharging jets had bulk densities up to 100 times that of the atmosphere and were unable to entrain enough air to become buoyant. Such high eruptive densities were due to the presence of partially degassed magma in the conduit.Editorial responsibility: A. Woods