新疆西南天山哈布腾苏一带榴辉岩的岩石学特征及变质作用P-T轨迹

西南天山哈布腾苏河沿岸的含石墨的石榴石多硅白云母石英片岩中出露一套若干大小不等的布丁状变基性岩块,产状与区域面理一致。本文对其中保存完好的榴辉岩体进行了较为细致的岩石学研究和温压演化条件计算。根据主要矿物的含量,将该套榴辉岩大致分为两类—角闪榴辉岩和钠云母榴辉岩,二者的主要矿物均为 Grt Omp Na-Ca-Amp Pg Dol/Cal Rt±Qtz。石榴石变斑晶两阶段生长明显,从核部到边部 X_(Mn)和X_(Fe)降低,X_(Mg)和 X_(Ca)升高,指示了升温降压的变质过程。根据石榴石核部和边部的包体组合特征,确立了两期榴辉岩相变质作用:前一阶段经历了高压但较低温的硬柱石-硬绿泥石(仅见假象)榴辉岩相,变质温度为400～500℃,压力不低于1.8～1.9GPa,表明早期经历了快速俯冲过程;后一阶段的变质温度为570±30℃,压力为2.0～2.5GPa。在退变质绿帘角闪岩相阶段,形成低压脉体(矿物组合为 Ab Di Na-Ca-Amp Ep/Czo Cal)和一系列退变质反应结构,如 Dol 的 Cal 增生边,Omp 的 Di Ab 后成合晶结构。利用 Dol-Cal 分溶温度计和 Di的 Jd 分子含量得到该阶段的温度约500～530℃,压力小于0.9～1.1GPa,表明其退变质经历的是降温降压过程。这与利用Thermocalc 3.1在 NCFMASH 体系下计算的 PT 视剖面图是一致的。     

榍石：U－Pb定年及变质P－T－t轨迹的建立

榍石在各类岩石中普遍存在，其稳定性受全岩成分、氧逸度和水活度以及温度和压力等因素影响。它在岩浆岩中主要存在于高Ca/Al比值的岩石中，在变质岩中常见于绿片岩相、蓝片岩相和角闪岩相岩石，在钙质变质岩中其稳定范围可达榴辉岩相或高压麻粒岩相。一般榍石结构中U含量较高，且具有高达高角闪岩相上限的U Pb同位素体系封闭温度，是理想的U-Pb定年矿物。由于榍石的组成元素均为岩石中的主要元素，很容易与其它矿物、熔体及流体发生反应，所以榍石的U-Pb年龄记录的更可能是结晶年龄，而不是简单的扩散重置年龄；也因为它容易反应，变质榍石复杂的U Pb体系可能记录了岩石的整个变质历史信息。通过与榍石平衡共生的矿物组合或利用榍石Zr温压计可确定岩石的P T条件，结合相关的榍石年龄信息即可建立变质过程的P T t轨迹。利用SHRIMP、LA MC ICP MS以及LA ICP MS方法可对不均一榍石颗粒内部进行原位微区分析得到有意义的U Pb年龄；利用榍石中Zr含量对温度，尤其是对压力比较敏感，可建立榍石Zr含量温压计。     

一次暴雨过程的EOF分析

在用21层η坐标细网格模式对1998年7月21～22日发生在武汉地区的一次持续性特大暴雨过程数值模拟的基础上， 利用较高时空分辨的模式输出结果对暴雨过程做经验正交函数分解（EOF分析）尝试。结果表明:EOF第1主分量的空间分布代表典型的暴雨环境背景场的低值系统；EOF第2主分量的空间分布与人字形切变线（西部为冷式切变，东部为暖式切变）相联系，是影响这次暴雨的重要形势场；利用相轨线分析方法发现，暴雨过程中EOF第1主分量和EOF第2主分量的时间系数在暴雨临近阶段，两者正相关，激发暴雨，在暴雨后期两者负相关，促使这次暴雨趋于减弱结束。     

2005年登陆我国热带气旋特征分析

热带气旋是影响我国沿海的主要灾害性天气系统之一, 它产生的狂风、暴雨、巨浪和风暴潮, 给沿岸地区人民生命和国家财产安全带来严重威胁。而严重的台风灾害, 往往是台风登陆引起的。为进一步研究登陆热带气旋的活动规律, 总结了2005年登陆我国热带气旋的特点, 结果表明:2005年登陆我国热带气旋具有登陆季节短、登陆地点分布异常、台风比例异常偏高、灾害损失极为严重的特点。同时, 还讨论了2005年登陆我国热带气旋异常的气候原因, 并指出未来几年登陆热带气旋和台风的年频数处在上升趋势中。     

双轴压缩条件下绿片岩的蠕变规律研究

在锦屏二级水电站辅助洞绿片岩的双轴压缩蠕变试验结果的基础上,研究了应力路径对双轴压缩蠕变变形的影响。结果表明:当侧向应力相同时,随着轴向应力的增加,轴向稳态蠕变阶段的变形速率逐渐增加;当轴向应力相同时,随着侧向应力的增加,轴向稳态蠕变阶段的变形速率逐渐减小。     

Calculating phase diagrams involving solid solutions via non-linear equations, with examples using THERMOCALC

Phase diagrams involving solid solutions are calculated by solving sets of non-linear equations. In calculating P–T  projections and compatibility diagrams, the equations used for each equilibrium are the equilibrium relationships for an independent set of reactions between the end-members of the phases in the equilibrium. Invariant points and univariant lines in P–T  projections can be calculated directly, as can coordinates in compatibility diagrams. In calculating P–T  and T–x / P–x pseudosections – diagrams drawn for particular bulk compositions – the equilibrium relationship equations are augmented by mass balance equations. Lines in pseudosections, where the mode of one phase in the lower variance equilibrium is zero, and points, where the modes of two phases are zero, can then be calculated directly. The software, THERMOCALC, allows the calculation of these and a range of other types of phase diagram. Examples of phase diagrams and phase diagram movies, with instructions for their production, along with the THERMOCALC input and output files, and the Mathematica^TM functions for assembling them, are presented in this paper, partly in hard copy and partly on the JMG web sites (http://www.gly.bris.ac.uk/www/jmg/jmg.html, or equivalent Australian or USA sites).
     

通化集安群石榴子石和黑云母微区化学成分特征及其对变质作用p-T-t轨迹的指示意义

集安群片麻岩中石榴子石和黑云母接触带两侧边缘广泛发育Fe－Mg交换反应所形成的扩散环带,但晶体内部各自保持变质峰期的成分,中温带石榴子石可保留生长环带。经微区化学成分详细研究后,正确运用Grt－Bt温度计获得进变质阶段,变质高峰期和修期后Fe－Mg交换反应停止时的温度条件。按石榴子石和斜长石的微区钙含量变化确定了峰期和退变质阶段压力。据此建立起逆时针形式的变质作用p－T－t轨迹,反映该区早元古代陆壳内裂陷带的闭合过程。     

四川石棉草科穹状岩浆核杂岩构造特征

位于扬子陆块西缘的石棉草科穹状变形变质体,据近年来的研究表明,该穹隆体经历了三次变形变质时期：早期为收缩滑脱变形的区域动力变质、中期热隆伸展动热变质和后期岩浆热接触变质。对主期变质划分出黑云母带、石榴石带、红柱石－十字石带和矽线石带,确定为低压相系,利用变质反应、矿物地质温压计及相关的同位素年龄资料,建立了草科穹状变形变质体演化的ｐ－Ｔ－ｔ－Ｄ轨迹。轨迹图呈顺时针形式,具碰撞造山带环境的特点,变形变质过程受变质体前缘西油房韧性剪切带逆冲－推覆作用和后缘碰撞晚期岩浆大规模上侵的双重制约,为深源岩浆热动力变质成因,属穹状岩浆核杂岩构造。     

胶东早元古代荆山群变质作用演化样式及其构造环境探讨

胶东地区发育大面积的早无古代变质地层──荆山群。该套岩系经历了三期五个阶段的变质作用,峰期温压条件为T＝700～750℃,p＝0．50～0．60GPa,达角闪麻拉岩相。变质作用pTt轨迹为逆时针形式,反映早元古代陆缘壳内裂陷带的闭合过程。     

The Narryer Gneiss Complex of the Yilgarn Block, Western Australia: a segment of Archaean lower crust uplifted during Proterozoic orogeny

The Narryer Gneiss Complex of the Yilgarn Block is a key segment of the Western Australian Precambrian Shield. It is a regional granulite facies terrain comprised of predominantly quartzo-feldspathic gneisses derived from granitic intrusions c. 3.6–3.4 Ga old. Granulite facies metamorphism occurred c. 3.3 Ga ago, and conditions of 750–850°C and 7–10 kbar are estimated for the Mukalo Creek Area (MCA) near Errabiddy in the north. The P–T path of the MCA has been derived from metamorphic assemblages in younger rocks that intruded the gneisses during at least three subsequent events, and this path is supported by reaction coronas in the older gneisses. There is no evidence for uplift immediately following peak metamorphism of the MCA, and a period of isobaric cooling is inferred from the pressures recorded in younger rocks. Pressures and temperatures estimated from metadolerites, which intruded the older gneisses during ‘granite–greenstone’tectonism at about 2.6 Ga and during early Proterozoic thrusting show that the Errabiddy area remained in the lower crust, although it was probably reheated during the younger events. Isothermal uplift to upper crustal levels occurred at c. 1.6 Ga ago, and was followed by further deformation and patchy retrogression of high-grade assemblages. The effects of younger deformation, cooling and reheating can be discerned in the older gneisses, but as there has been no pervasive deformation or rehydration, the minerals and microstructures formed during early Archaean granulite facies metamorphism for the most part are retained. The MCA remained in the lower crust for about 1700 Ma following peak metamorphism and some event unrelated to the original metamorphism was required to exhume it. Uplift occurred during development of the Capricorn Orogen, when some 30–35 km were added to the crust beneath the Errabiddy area. The recognition of early Proterozoic thrusting, plus crustal thickening, suggests that the Capricorn Orogen is a belt of regional compression which resulted from convergence of the Yilgarn and Pilbara Cratons.