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201.
大青山造山带中基底再造杂岩的特征及其指示意义 总被引:4,自引:0,他引:4
大青山造山带中基底再造杂岩主要由高温韧性剪切变形变质作用的糜棱片麻岩类、部分重烙作用形成的混合岩化糜棱片麻岩类及太古宙地壳残块三部分组成。进一步研究表明该基底再造条岩不仅可以作为一个特定的构造岩性单元,属于造山带根部地壳的一部分,而且其中前两部分既不属于太古富变质上壳岩和侵入岩系,也不属于早元古代变质上亮岩,而是早元古代造山带演化过程中,变形变质作用和部分重熔作用对太古宙基底综合改造作用的产物。基底再造杂岩的研究为进一步探讨前寒武纪克拉通内硅铝壳造山作用的性质、规模和成因机制提供了极为重要的地质证据和信息。 相似文献
202.
湖北宜昌石板溪金矿区断层空间结构及其控矿规律研究 总被引:1,自引:0,他引:1
断层空间结构包括变形结构和几何结构两部分。本文在解析石板溪金矿区主要断层变形结构和几何结构的基础上,探讨了其空间结构模式和控矿规律。 相似文献
203.
204.
长城系团山子组火山岩颗粒锆石U-Pb年龄及其地质意义 总被引:46,自引:1,他引:46
蓟县中-上元古界典型剖面之邻区平谷县境内,长城系团山子组连续发育两层厚度各为1m左右的富钾粗面安山岩,发育气孔构造和绳状构造。其中存在三种不同成因类型锆石,应用颗粒锆石U-Pb测定年龄技术,得到:(1)自生锆石,其U-Pb不一致上交点年龄为1683±67Ma,代表该火山岩形成年龄;(2)捕获锆石,多为原碎屑锆石,较年轻的一种捕获锆石的207Pb/206Pb表面年龄为1823±68Ma,这限定了长城系底界年龄应新于1823Ma;(3)后生热液锆石,其U-Pb年龄为460Ma左右,反映后期热液事件发生的时代。 相似文献
205.
内蒙古东五分子地区韧性剪切变质作用的特征 总被引:6,自引:0,他引:6
东五分子地区花岗-绿岩地体经受了三种类型变质作用的改造。韧性剪切带不仅控制了区域变质岩组合的分布,而且也导致其变质作用的强度出现了逆转序列。根据岩石的结构、碎斑含量及矿物成分,韧性剪切变质岩划分为三类,其共同特点是具有碎斑结构。其变形结构分为单矿物型及组合型。同一块韧性剪切变质岩由处在单变平衡的一组矿物组成。根据岩石变形及重结晶的特点,结合其产状,确定出两种不同类型韧性剪切变质带。共生矿物对的研究证明它们形成于地壳不同深度及温度、压力条件。本区的金矿化、运移、沉淀与韧性剪切变质带紧密相关。 相似文献
206.
207.
Jan Pleuger Sybille Roller Jens M. Walter Ekkehard Jansen Nikolaus Froitzheim 《International Journal of Earth Sciences》2007,96(2):229-252
The boundary zone between two Penninic nappes, the eclogite-facies to ultrahigh-pressure Zermatt-Saas zone in the footwall
and the blueschist-facies Combin zone in the hanging wall, has been interpreted previously as a major normal fault reflecting
synorogenic crustal extension. Quartz textures of mylonites from this fault were measured using neutron diffraction. Together
with structural field observations, the data allow a refined reconstruction of the kinematic evolution of the Pennine nappes.
The main results are: (1) the contact is not a normal fault but a major thrust towards northwest which was only later overprinted
by southeast-directed normal faulting; (2) exhumation of the footwall rocks did not occur during crustal extension but during
crustal shortening; (3) the Sesia-Dent Blanche nappe system originated from a continental fragment (Cervinia) in the Alpine
Tethys ocean, and the Combin zone ophiolites from the ocean basin southeast of Cervinia; (4) out-of-sequence thrusting played
a major role in the tectonic evolution of the Penninic nappes.
An erratum to this article can be found at 相似文献
208.
Qu JianJun Zhang KeCun Sun Bo Jiang ShengXiang Dong GuangRong Zu RuiPing Fang HaiYan 《中国科学D辑(英文版)》2007,50(9):1351-1358
The sound-producing mechanism of booming sand has long been a pending problem in the blown sand physics. Based on the earlier researches, the authors collected some silent sand samples from Teng- ger Desert, Australian Desert, Kuwait Desert, beaches of Hainan Island and Japanese coast as well as the soundless booming sand samples from the Mingsha Mountain in Dunhuang to make washing ex- periments. In the meantime the chemical corrosion experiment of glass micro-spheres, surface coating experiment and SEM examination were also conducted. The experimental results show that the sound production of booming sand seems to have nothing to do with the presence of SiO2 gel on the surface of sand grains and unrelated to the surface chemical composition of sand grains but is related to the resonance cavities formed by porous (pit-like) physical structure resulting from a number of factors such as wind erosion, water erosion, chemical corrosion and SiO2 gel deposition, etc. Its resonance mechanism is similar to that of Hemholz resonance cavity. Under the action of external forces, nu- merous spherical and sand grains with smooth surface and porous surface are set in motion and rub with each other to produce extremely weak vibration sound and then become audible sound by human ears through the magnification of surface cavity resonance. However the booming sands may lose their resonance mechanism and become silent sand due to the damping action caused by the invasion of finer particles such as dust and clay into surface holes of sand grains. Therefore, clearing away fine pollutants on the quartz grain surface is an effective way to make silent sand emit audible sound. 相似文献
209.
This paper examines the limitations and deficiencies of the current British archaeomagnetic calibration curve and applies several mathematical approaches in an attempt to produce an improved secular variation curve for the UK for use in archaeomagnetic dating. The dataset compiled is the most complete available in the UK, incorporating published results, PhD theses and unpublished laboratory reports. It comprises 620 archaeomagnetic (directional) data and 238 direct observations of the geomagnetic field, and includes all relevant information available about the site, the archaeomagnetic direction and the archaeological age. A thorough examination of the data was performed to assess their quality and reliability. Various techniques were employed in order to use the data to construct a secular variation (SV) record: moving window with averaging and median, as well as Bayesian statistical modelling. The SV reference curve obtained for the past 4000 years is very similar to that from France, most differences occurring during the early medieval period (or Dark Ages). Two examples of dating of archaeological structures, medieval and pre-Roman, are presented based on the new SV curve for the UK and the implications for archaeomagnetic dating are discussed. 相似文献
210.
A Least-squares Window Curves Method for Interpretation of Magnetic Anomalies Caused by Dipping Dikes 总被引:1,自引:0,他引:1
E. M. Abdelrahman E. R. Abo-Ezz K. S. Soliman T. M. El-Araby K. S. Essa 《Pure and Applied Geophysics》2007,164(5):1027-1044
We have developed a least-squares method to determine simultaneously the depth and the width of a buried thick dipping dike
from residualized magnetic data using filters of successive window lengths. The method involves using a relationship between
the depth and the half-width of the source and a combination of windowed observations. The relationship represents a family
of curves (window curves). For a fixed window length, the depth is determined for each half-width value by solving one nonlinear
equation of the form f (z) = 0 using the least-squares method. The computed depths are plotted against the width values representing a continuous curve.
The solution for the depth and the width of the buried dike is read at the common intersection of the window curves. The method
involves using a dike model convolved with the same moving average filter as applied to the observed data. As a result, this
method can be applied to residuals as well as to measured magnetic data. Procedures are also formulated to estimate the amplitude
coefficient and the index parameter. The method is applied to theoretical data with and without random errors. The validity
of the method is tested on airborne magnetic data from Canada and on a vertical component magnetic anomaly from Turkey. In
all cases examined, the model parameters obtained are in good agreement with the actual ones and with those given in the published
literature. 相似文献