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171.
固体颗粒破碎强度的尺寸效应是一种普遍存在的现象,冰块、岩石颗粒、陶瓷和混凝土块等的破碎强度都表现出随颗粒直径增加而减小的现象,分形模型为解释固体颗粒破碎强度的尺寸效应提供了可行的方法。本文采用Steacy和Sammis分形模型模拟了岩石颗粒压碎特征,分析岩石颗粒破碎后的颗粒分布规律,给出颗粒破碎分维的确定方法,建立颗粒压碎强度与粒径的理论关系,颗粒破碎强度与颗粒粒径的关系用分维D表示为fdD-3。已有的颗粒破碎分布的数据表明,岩石颗粒破碎的分维大约为2.50~2.60,颗粒破碎强度符合用分维表示的尺寸效应。 相似文献
172.
173.
通过对漕河崖矿段进行勘探工作,发现该区岩盐矿层赋存较多,矿层厚度在0.40~14.72 m,NaCl 平均品位86.39%,属厚度较稳定,品位均匀矿层;岩盐矿层不仅局限在 F2,F3,F43个断层的切割范围内,在 F3断层北部尚有岩盐层赋存。 相似文献
174.
The organic geochemical methods of hydrocarbon prospecting involve the characterization of sedimentary organic matter in terms of its abundance, source and thermal maturity, which are essential prerequisites for a hydrocarbon source rock. In the present study, evaluation of organic matter in the outcrop shale samples from the Semri and Kaimur Groups of Vindhyan basin was carried out using Rock Eval pyrolysis. Also, the adsorbed low molecular weight hydrocarbons, methane, ethane, propane and butane, were investigated in the near surface soils to infer the generation of hydrocarbons in the Vindhyan basin. The Total Organic Carbon (TOC) content in shales ranges between 0.04% and 1.43%. The S1 (thermally liberated free hydrocarbons) values range between 0.01–0.09 mgHC/gRock (milligram hydrocarbon per gram of rock sample), whereas the S2 (hydrocarbons from cracking of kerogen) show the values between 0.01 and 0.14 mgHC/gRock. Based on the Tmax (temperature at highest yield of S2) and the hydrogen index (HI) correlations, the organic matter is characterized by Type III kerogen. The adsorbed soil gas, CH4 (C1), C2H6 (C2), C3H8 (C3) and nC4H10, (nC4), concentrations measured in the soil samples from the eastern part of Vindhyan basin (Son Valley) vary from 0 to 186 ppb, 0 to 4 ppb, 0 to 5 ppb, and 0 to 1 ppb, respectively. The stable carbon isotope values for the desorbed methane (δ13C1) and ethane (δ13C2) range between −45.7‰ to −25.2‰ and −35.3‰ to −20.19‰ (VPDB), respectively suggesting a thermogenic source for these hydrocarbons. High concentrations of thermogenic hydrocarbons are characteristic of areas around Sagar, Narsinghpur, Katni and Satna in the Son Valley. The light hydrocarbon concentrations (C1–C4) in near surface soils of the western Vindhyan basin around Chambal Valley have been reported to vary between 1–2547 ppb, 1–558 ppb, 1–181 ppb, 1–37 ppb and 1–32 ppb, respectively with high concentrations around Baran-Jhalawar-Bhanpur-Garot regions (Kumar et al., 2006). The light gaseous hydrocarbon anomalies are coincident with the wrench faults (Kota – Dholpur, Ratlam – Shivpuri, Kannod – Damoh, Son Banspur – Rewa wrench) in the Vindhyan basin, which may provide conducive pathways for the migration of the hydrocarbons towards the near surface soils. 相似文献
175.
Mashallah Khamehchiyan Morteza Rahimi Dizadji Majid Esmaeili 《Geomechanics and Geoengineering》2014,9(1):63-71
Earthwork and surface excavation activities play an important role in construction projects. Selecting the best technique to loosen the overburden material within the surface excavation in open mining and geotechnical projects is of great importance from economical and technical viewpoints. Surface excavation includes direct digging, ripping and blasting. To select the most effective method and plan for excavation, geotechnical investigation is very important. It is also a big help in avoiding conflict between contractors and clients when they do not reach mutual agreement regarding the price of rock and soil excavation. There are many engineering classification systems used to assess rock masses for excavation purposes. All of these systems consider several geotechnical parameters to assess the earth masses. This study reviews these systems and then offers a new categorization based on the Rock Mass index (RMi) classification system and block volume to assess excavation in rock masses. The original dataset was obtained from the literature review as well as the surface excavation in Upper Gotvand dam and Hydro Power Plant (HPP). The offered system was also validated through the data extracted from the surface excavation in Sardasht dam and HPP in Iran. 相似文献
176.
Márton Veress Zoltán Zentai Kálmán Péntek Ljubov Döbröntei Ljubov Danilovna Kiprijanova 《Proceedings of the Geologists' Association. Geologists' Association》2014
The study deals with the Lena Pillars (Sakha Republic, Russia, Siberia). The Lena Pillars are pinnacle features which are characteristic on karsts. The importance of these features is that they are extremely large and occur on very large areas. Their occurrence is interesting because they do not appear on tundra karst. We investigated the veneers of cliffs, the fracture density of the building rock, the distribution and dispersion of the fracture directions, direction distribution and dispersion of the giant grikes between the pillars, the layer thickness of the building rock, the size and dispersion of debris. We distinguished pillar types, and then we classified the features on the area of the pillars from a morphogenetical point of view. According to investigations and morphological analyses, the pillars developed from palaeokarsts. During the former karstification grikes and caverns developed close to the surface. These features coalesced into each other. The giant grikes of great size became filled and the pillars were covered. After the cut of the Lena River these features were revealed and became exhumed. Now the pillars are destroyed and continue developing by frost weathering. 相似文献
177.
胶北地体地壳演化:玲珑黑云母花岗岩继承锆石U-Pb年龄、微量元素和Hf同位素证据 总被引:6,自引:5,他引:1
胶北地体晚侏罗世下地壳重熔的玲珑黑云母花岗岩大面积出露,其中残留有大量继承锆石,记录了多期热事件,为复杂的地壳演化过程提供了重要线索。论文通过分析玲珑黑云母花岗岩中继承锆石的U-Pb年龄、微量元素和Hf同位素组成,探讨了胶北地体的地壳演化历史。结果显示胶北地体前寒武纪经历了~2.9Ga和~2.7Ga两期主要的地壳生长事件,~2.5Ga和2.2~1.8Ga两期地壳重熔改造事件,~2.5Ga和1.95~1.8Ga两期变质事件。~2.9Ga的岩浆作用形成于岛弧环境,~2.7Ga岩浆活动与下地壳基性物质的部分熔融有关,~2.5Ga发生的岩浆和变质事件与地幔柱底侵作用有关,并有同时期的表壳岩组合-胶东岩群形成。~2.1Ga地壳处于拉张状态,伴有与裂谷活动有关的双峰式岩浆作用,荆山群和粉子山群开始沉积,而后1.95~1.8Ga发生碰撞造山运动,胶北所有早前寒武纪岩石单元卷入此次事件,并发生变质作用。自此之后,直至二叠纪末,胶北处于岩浆活动的沉寂期,但于~1.7Ga和~1.0Ga发生沉积作用,形成芝罘群和蓬莱群。二叠纪末扬子板块向北俯冲于华北克拉通之下,并于三叠纪与华北克拉通发生陆陆碰撞作用,致使扬子板块北缘新元古代花岗岩发生超高压变质,形成苏鲁超高压变质带,之后超高压变质岩发生折返。玲珑黑云母花岗岩复杂的继承锆石组成可能表征了前寒武纪岩石卷入陆-陆碰撞事件而发生再循环作用。 相似文献
178.
通过对辽宁区域岩石41种元素的区域分布研究,作者提出了辽宁岩石元素地球化学分区系统。依次划出1个地球化学省、2个地球化学区、12个地球化学分区及若干地球化学小区。以地球化学分区为基本单位,讨论了各分区岩石元素的浓集状况,指出了不同地球化学分区岩石元素分布的差异,分析了某些元素的富集趋势与成矿的联系。对探讨不同分区的地球化学演化历程,确定找矿方向,具有一定意义。 相似文献
179.
The extensive hematite deposit in Meridiani Planum was selected as the landing site for the Mars Exploration Rover Opportunity because the site may have been favorable to the preservation of evidence of possible prebiotic or biotic processes. One of the proposed mechanisms for formation of this deposit involves surface weathering and coatings, exemplified on Earth by rock varnish. Microbial life, including microcolonial fungi and bacteria, is documented in rock varnish matrices from the southwestern United States and Australia. Limited evidence of this life is preserved as cells and cell molds mineralized by iron oxides and hydroxides, as well as by manganese oxides. Such mineralization of microbial cells has previously been demonstrated experimentally and documented in banded iron formations, hot spring deposits, and ferricrete soils. These types of deposits are examples of the four “water-rock interaction” scenarios proposed for formation of the hematite deposit on Mars. The instrument suite on Opportunity has the capability to distinguish among these proposed formation scenarios and, possibly, to detect traces that are suggestive of preserved martian microbiota. However, the confirmation of microfossils or preserved biosignatures will likely require the return of samples to terrestrial laboratories. 相似文献
180.
Vladimir V. Svetsov 《Planetary and Space Science》2005,53(12):1205-1220
Vertical impacts on the Earth of asteroids 500-3000 km in diameter at 15 km/s have been numerically modelled using the hydrodynamic SOVA code. This code has been modified for the spherical system of coordinates well suited for simulations of very large impacts when the entire Earth is involved in motion. The simulations include cratering process, upward motion of deep mantle layers, fall of ejecta on the Earth, escape of matter to space, and formation of rock vapour atmospheres. The calculations were made for the period preceding disappearance of rock vapour atmospheres caused by radiation several years after the largest impacts. For very large vertical impacts at 15 km/s, escaping masses proved to be negligibly small. Quantities of kinetic, internal, potential, and radiated away energies are obtained as functions of time and space. After the impacts, a global layer of condensed ejecta covers the whole of the Earth's surface and the ejecta energy is sufficient to vaporise an ocean 3 km deep. The mass of rock vapour atmosphere is 10-23% of the impactor mass. This atmosphere has a greater mass than the water atmosphere if impactor is 2000 km in diameter or larger. 相似文献