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111.
本文主要讨论了岩浆不混溶的内在因素和物化条件。研究提出阳原杂岩大于零的过剩自由能是出现不混溶的内在原因。岩浆中高P_2O_5、TiO_2、Zr、Hf、Ta、REE是岩浆不混溶的诱导因素。化学位计算揭示了球状黑云辉石正长岩之球体、基质两相及正长质和辉石质岩浆单元在液态时曾处于平衡状态。岩浆不混溶可能是在温度约1200℃、上地壳深度范围内发生的。阳原母岩浆不混溶的两液相可以分离聚集成两大岩浆单元,岩浆分溶不充分,便产生中间成分的黑云辉石正长岩。 相似文献
112.
Samples are available from 37 stony meteorites falling in China. Twenty-two chondrites are examined in terms of chemical and mineral compositions, cosmogenic nuclides, formation and exposure ages, impact effect and chondrule textures. On the basis of chemical-petrologic features these chondrites are classified asE 4 (Qingzhen),H 5 (Jilin, Changde, Shuangyang, Anlong, Xinyi and Yangjang),L 6 (Renqiu, Junan, Heze, Rugao and Nei Monggol) andLL 6 (Dongtai). E 4 is characterized by high iron and sulfur, with the former occurring mainly as Feo and FeS. FromH 5 throughH 6 toLL 6, iron and nickel decrease gradually while FeO and the ratio of Fe silicate to total iron increase gradually. indicating a general increase in the orderE-H-L-LL in the degree of oxidation at the time of formation. E 4 consists mainly of enstatite and, to much less extent, free SiO2 but olivine is hardly to be found. The olivine proportions amount to 29.07, 41.98 and 51.36 percent inH 5,L 6 andLL 6 respectively, with Fa increasing from 17 to 27 percent. Recrystallization has been noticed to different degrees inH 4,H 5,L 6 andLL 6 chondrites. The extent to which the original structure disappears and the boundaries of chondrules become indistinct decreases from type 6 through type 5 to type 4, reflecting different degrees of thermal metamorphism. Major minerals in the meteorites all exhibit signs of low to medium shock metamorphism. Specific activity, depth effect and orbit effect are also measured on some chondrites that have fallen in recent years and some new information has been obtained with respect to the orbit and source region for meteorite parent bodies in space. This results show that the environment of formation ofE group may be nearer to Mars than that ofO group. Each chemical group of chondrites has its own evolutionary history, and chondritets of different chemical groups may have originated from parent bodies of different compositions. Or owing to the differentiation caused by thermal melamorphism, various kinds of meteorites may be derived from a common parent body. From this argument it is suggested that five stages may be recognized during the formation process of chondrites. 相似文献
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James Glimm Shuling Hou Hongjoong Kim Yoon-ha Lee David H. Sharp Kenny Ye Qisu Zou 《Computational Geosciences》2001,5(3):173-197
We consider numerical solutions of the Darcy and Buckley–Leverett equations for flow in porous media. These solutions depend on a realization of a random field that describes the reservoir permeability. The main content of this paper is to formulate and analyze a probability model for the numerical coarse grid solution error. We explore the extent to which the coarse grid oil production rate is sufficient to predict future oil production rates. We find that very early oil production data is sufficient to reduce the prediction error in oil production by about 30%, relative to the prior probability prediction. 相似文献
117.
跨断裂水准剖面观测在地震监测中的应用 总被引:3,自引:0,他引:3
由于活动地块的相对运动和变形,其边界带往往构造活动强烈,是反映地壳运动的敏感部位。基于上述思路,昆仑山口西8.1级大震发生后,通过大范围监测布设在青藏块体北部地区及周边主要构造带上的水准剖面,在短期内快速获取了大范围的断裂活动信息和不同断裂带对大区域构造应力场变化的响应特征。实践证明,这种监测方式灵活、作业周期短、资料处理快,能及时对震情趋势做出估计,不失为当前区域形变监测工作的一种新的探索。 相似文献
118.
Wang Yong Hou Zengqian Mo Xuanxue Dong Fangliu Bi Xianmei Zeng Pusheng 《Frontiers of Earth Science》2007,1(3):322-332
More than 140 middle-small sized deposits or minerals are present in the Weishan-Yongping ore concentration area which is
located in the southern part of a typical Lanping strike-slip and pull-apart basin. It has plenty of mineral resources derived
from the collision between the Indian and Asian plates. The ore-forming fluid system in the Weishan-Yongping ore concentration
area can be divided into two subsystems, namely, the Zijinshan subsystem and Gonglang arc subsystem. The ore-forming fluids
of Cu, Co deposits in the Gonglang arc fluid subsystem have δD values between −83.8‰ and −69‰, δ18O values between 4.17‰ and 10.45‰, and δ13C values between −13.6‰ and 3.7‰, suggesting that the ore-forming fluids of Cu, Co deposits were derived mainly from magmatic
water and partly from formation water. The ore-forming fluids of Au, Pb, Zn, Fe deposits in the Zijinshan subsystem have δD
values between −117.4‰ and −76‰, δ18O values between 5.32‰ and 9.56‰, and Δ13C values between −10.07‰ and −1.5‰. The ore-forming fluids of Sb deposits have δD values between −95‰ and −78‰, δ18O values between 4.5‰ and 32.3‰, and Δ13C values between −26.4‰ and −1.9‰. Hence, the ore-forming fluids of the Zijinshan subsystem must have been derived mainly
from formation water and partly from magmatic water. Affected by the collision between the Indian and Asian plates, ore-forming
fluids in Weishan-Yongping basin migrated considerably from southwest to northeast. At first, the Gonglang arc subsystem with
high temperature and high salinity was formed. With the development of the ore-forming fluids, the Zijinshan subsystem with
lower temperature and lower salinity was subsequently formed.
Translated from Mineral Deposits, 2006, 25(1): 60–70 [译自: 矿床地质] 相似文献
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