对澳大利亚南极地带安德拜极地早前寒武系的地壳演化和地质年龄评论

安德拜(Enderby)极地的早期前寒武系克拉通(纳皮尔杂岩),如同其他太古宙克拉通一样,也被较年轻的活动带包围。但是它与众所熟知的花岗岩—绿岩克拉通被高级麻粒岩相片麻岩包围为特征的区域情况不同。安德拜极地克拉通的热力构造特征和复杂类型与编录良好的西格陵兰太古宙地层具有明显的相似性。在安德拜极地,发育良好的水平层理和平行强烈压扁及伸长的LS组构是称之为伏     

有关皮尔巴拉地区地层和变形史的花岗岩侵入体Rb/Sr年龄测定

本研究项目包括澳大利亚西北部皮尔巴拉太古宙地块的两处地方。一处为瓦拉武山峡(Warrawie Gap),在那里,库甘溪(Coongan Creek)切过出露于下瓦拉沃纳群的库甘同斜东侧。集块岩、一些酸性火山岩和一处保存完好的枕状熔岩块状部分均被钠质花岗岩—花岗闪长岩和粉红色长石石英二长岩等深成岩所侵入。这些岩体有在形成主要穹丘时(或以前)所生成的片理—褶皱幕F-_2。横切的细晶岩并未受F_2的影响。用λ~(87)Rb     

动态金幔柱模式──兼论金星上小型冠状构造的浅起源

热和组分密度异常共同驱动的动态金幔柱解析模式给出金幔柱在金幔中上升的历史．当金幔柱到达岩石层底时其头部的特征量是5个独立变量的函数：（1）金幔柱起源的深度;（2）金幔粘性系数;（3）源温度异常值;（4）源组分与热密度异常之比;（5）金幔柱的浮力通量．基于新的Mapellan数据,金星表面上有360多个冠状和类冠状构造已被发现,其中65％直径小于300km．这类小型冠状构造被认为是由具有下述特征的较小的金幔柱所形成：（1）最大直径小于300km;（2）当其头部到达岩石层底时,过剩温度足以产生部分熔融层,应高于150K;（3）被冠状构造下面的金幔柱带上来的总浮力有能力支撑冠状构造隆起的总质量．用这3个条件分析数值结果并约束金幔柱的源参数,根据本文的数值实验结果,金星上的小型冠状构造可能是起源于上金幔小于1000km深度的动态金幔柱形成的．     

白云鄂博REE-Nb-Fe矿床成因的氧、碳和锶同位素及微量元素地球化学证据

根据白云鄂博赋矿白云石大理岩的岩石学特征及地质产状将其分为两类：粗粒和细粒白云石大理岩．它们的氧、碳和锶同位素及微量元素地球化学特征显然有别于分布在宽沟背斜以北典型的沉积石灰岩和白云岩,而和幢源火成碳酸岩十分相似．与矿床进行对比研究说明,成矿流体和矿质主要起源于碳酸岩浆的分异作用,其放射性成因同位素和微量元素保持了地但指纹,而氧和碳同位素组成却向壳源方向漂移,证实碳酸岩浆侵位过程中受大陆地壳的混染作用非常微弱,但是由碳酸岩浆活动所引起的成矿热液体系中却有一定的地表水混人认为白云鄂博REE-Nb-Fe超大型矿床的成因应归属于火成碳酸岩型矿床．     

热带气象学——其经济意义及科学任务

载于《世界气象组织公报》1975年7月号。近年来,不管实用方面或科学方面都越来越着眼于热带气象的重要性.在实用方面,农业和水力资源的利用越来越需要热带气象观测资料以及几个月以上的长期天     

Regolith Geochemical Studies in Kimberlitic Terrain: A Case Study from Lattavaram Kimberlite Cluster, Eastern Dharwar Craton, Southern India

正Utility of geochemistry in mineral exploration is known since more than half-a-century.In reconnaissance diamond exploration,regolith geochemistry is a well known tool worldwide and helps in distinguishing bedrock     

西澳大利亚伊尔冈地块花岗岩—绿岩组合形式的成因

西澳大利亚的伊尔冈地块主要由太古宙椭圆形花岗质岩石区和围绕其边缘呈弧形分布的绿岩带组成。该地体典型部位的露头型式表明,它们起因于大型穹—盆褶皱干涉构造,而不是具有陡立边缘的岩基的底辟侵位。绿岩和下伏花岗质岩石最初是在近水平状态下一起变形的。结果,使花岗质岩石发生重结晶,并形成基本与绿岩层理平行的片麻状构造。近水平且巨厚的二长花岗岩岩席是后来侵入任绿岩系下部层位的,后期变形作用产生两组连续的并相互具高角度垂直轴而的褶皱,它们构成了直径从数匣米到50多公里的穹—盆褶皱干涉构造。     

Use of Surface Observations to Estimate Upper Air Humidity for the Objective Analysis of Relative Humidity over Indian Region

In the present study objective analyses of relative humidity (RH) at surface and at the levels of 850,700 and 500 hPa have been made using Gandin’s (1963) optimum interpolation scheme. As the horizontal resolution of the radiosonde stations is rather inadequate for upper air humidity analysis, a scheme has been developed, following Rasmussen (1982) to estimate the upper air RH from the surface observations like surface RH, present weather and cloud cover. The relative humidities at the levels 850, 700 and 500 hPa were related to the surface observations through three separate regression relations. The RH values at 850, 700 and 500 hPa levels were estimated from the surface RH, cloud coverage and present weather using the above regression relations and subsequently the objective analyses at 00 GMT for the period from 4 July to 8 July 1979, were made using these estimated data along with the observed radiosonde data. Objective analyses were also made for the same period using only the radiosonde data for comparison to study the impact of those estimated data. Root mean square errors were computed for all the five days by interpolating RH at the observing stations from the objectively analysed field and comparing them with the actually observed RH to examine how best the analyses (with and without estimated data) fitted the observations. Lastly they were compared with satellite cloud pictures. This study shows that the estimated upper air RH values have positive impact on the analysis of upper air RH and could be used over radiosonde date sparse region and even over oceanic regions.