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1.
本文以成矿地质模型为依据,对观驾山—黑山岛一带的化探、物探、遥感及地质等信息变量进行了详细的分析,选取了10个信息变量24个标志状态;在此基础上,运用信息量法对研究区内458个单元的信息量值进行计算,并由此确定了研究范围内的成矿远景区。事实表明,研究区信息量成矿预测是非常有效的  相似文献   
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辽南庄河地区辽河群变形型式独特。由于群内分层剪切作用,岩层构造置换强烈,伸展构造形迹发育,变形特征清楚,属正向韧脆性滑脱构造系统的上盘组成部分。其运动方向由北东而南西,形成时间早于中生代。不同级别的滑脱面构造,由于晚期构造作用影响,在早期韧脆性变形的基础上叠加了脆性变形,形成构造角砾岩带。沿角砾岩带蚀变普遍,金元素及其伴生元素含量明显高于两侧围岩,个别地段可达工业品位,构成矿体。因而,在辽河群出露区域鉴别同类型构造,沿滑脱面寻找受破碎带控制的蚀变构造岩型金矿,具有重要的找矿意义。  相似文献   
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Non-steady state timescales are complicated and their application to specific geophysical systems requires a common theoretical foundation. We first extend reservoir theory by quantifying the difference between turnover time and transit time (or residence time) for time-dependent systems under any mixing conditions. We explicitly demonstrate the errors which result from assuming these timescales are equal, which is only true at steady state. We also derive a new response function which allows the calculation of age distributions and timescales for well-mixed reservoirs away from steady state, and differentiate between timescales based on gross and net fluxes. These theoretical results are particularly important to tracer-calibrated "box models" currently used to study the carbon cycle, which usually approximate reservoirs as well-mixed. We then apply the results to the important case of anthropogenic CO2 in the atmosphere, since timescales describing its behavior are commonly used but ambiguously defined. All relevant timescales, including lifetime, transit time, and adjustment time, are precisely defined and calculated from data and models. Apparent discrepancies between the current, empirically determined turnover time of 30-60 years and longer model-derived estimates of expected lifetime and adjustment time are explained within this theoretical framework. We also discuss the results in light of policy issues related to global warming, in particular since any comparisons of the "lifetimes" of different greenhouse gases (CO2, CH4, N2O, CFC's etc.) must use a consistent definition to be meaningful.  相似文献   
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The concentrations of Ni, Cu, Zn, Ga, Ge, and Se in five, fine-grained chondrule rims in the highly unequilibrated CO3 chondrite ALH A77307 (3.0) have been determined for the first time by synchrotron X-ray fluorescence (SXRF) microprobe at Brookhaven National Laboratory. These elements are especially useful for tracing the role of condensation and evaporation processes which occurred at moderate temperatures in the solar nebula. Understanding the distribution of moderately volatile elements between matrix and chondrules is extremely important for evaluating the different models for the volatile depletions in chondritic meteorites. The data show that the trace element chemistry of rims on different chondrules is remarkably similar, consistent with data obtained for the major and minor elements by electron microprobe. These results support the idea that rims are not genetically related to individual chondrules, but all sampled the same reservoir of homogeneously mixed dust. Of the trace elements analyzed, Zn and Ga show depletions relative to CI chondrite values, but in comparison with bulk CO chondrites all the elements are enriched by approximately 1.5 to 3.5 x CO. The abundance patterns for moderately volatile elements in ALH A77307 chondrule rims closely mimic those observed in the bulk chondrite, indicating that matrix is the major reservoir for these elements. The close matching of the patterns for the volatile depleted bulk chondrite and enriched matrix is especially striking for Na, which is anomalously depleted in ALH A77307 in comparison with average CO chondrite abundances. The depletion in Na is probably attributable to the effects of leaching in Antarctica. With the exception of Na, the volatile elements show a relatively smooth decrease in abundance as a function of condensation temperature, indicating that their behavior is largely controlled by their volatility.  相似文献   
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以前有关深成岩体的侵位研究都试图解释岩体侵位空间如何形成。事实上,幔源岩浆侵位期间在地壳中“制造空间”的途径不外乎;(1)莫霍面降低;(2)地球表面外移。其它的“岩体侵位机制”均是不增加地壳体积的物质迁移作用(MTPs)。得到广泛引用的“同心带状气球膨胀岩体”侵位时的MTPs是岩体附近围岩的韧性流动。这类深成岩体附近可能形成的构造和总应变与岩体的三维形态、接触变质带的宽度以及岩体是否为刺穿底辟有关  相似文献   
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