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21.
中国大陆科学钻探终孔及研究进展   总被引:24,自引:4,他引:24       下载免费PDF全文
中国大陆科学钻探工程经过1309天的努力奋斗,于2005年1月23日,钻井终孔深度达到5118.20m。成为中国钻探技术发展的新里程碑。全面研究正在开展,在巨量物质深俯冲、超高压深俯冲与折返的精确定年、超高压岩石的原岩形成背景、上地幔流变学、地幔特殊新矿物发现、地下流体异常及地下微生物发现等方面已取得重要进展。  相似文献   
22.
中国大陆科学钻探工程主孔榴辉岩的岩石学研究   总被引:19,自引:0,他引:19       下载免费PDF全文
中国大陆科学钻探工程5000m主孔位于苏鲁超高压变质带南部。该钻孔0~2000m主要由榴辉岩、片麻岩、石榴石橄榄岩和少量片岩和石英岩组成。累积厚度达1000多米的榴辉岩具有不同的矿物组成、不同的矿物含量和不同的全岩化学成分,可划分成富Si的石英榴辉岩、富Ti的金红石榴辉岩、富Al的多硅白云母和蓝晶石榴辉岩、富Mg的双矿物榴辉岩和具有正常玄武岩成分的普通榴辉岩。榴辉岩的原岩包括基性层状侵入岩和变质表壳岩。榴辉岩全岩成分对石榴石和绿辉石中某些化学组分的含量有明显控制,而且直接影响到变质条件估算的准确性。扩散成分环带的广泛发育表明超高压矿物在早期退变质过程中发生了成分再平衡。这一事实以及具有成分生长环带石榴石变斑晶的存在,为榴辉岩形成在更高温度(>940℃)和更高压力(>4.5GPa)条件下提供了有力的证据。  相似文献   
23.
地球内部放射性产热元素U、Th及K(HPE)含量如何随深度的变化而变化是固体地球科学中的一个重要参数,在限定地壳的热和流变学结构、地球化学、岩石和构造模型中起关键性的作用。对HPE深部分布的认识主要来自于对大型花岗岩岩基的研究及对地表热流值和产热率之间关系的模拟,对高压-超高压变质地体的HPE随深度的分布缺乏认识。在苏鲁超高压变质带中实施的中国大陆科学钻探工程届时将提供超过5km的岩心,为确定苏鲁超高压带的HPE结构提供了最好的机会。对CCSD的100~2000m岩心的732块样品详细的放射性产热元素含量的测试及现今产热率计算的初步结果表明:(1)花岗质片麻岩具有最高的产热率,平均为1665×10-11W/kg;(2)副片麻岩(变沉积岩)具有中等的产热率,为994×10-11W/kg;(3)金红石榴辉岩及石榴石橄榄岩具有最低的产热率,为17×10-11~20×10-11W/kg;(4)放射性产热元素的浓度及相应的产热率随岩性的变化而变化,呈现阶梯状的分布特征。产热率随深度的变化特征表明CCSD主孔中的HPE三明治结构。该结构可能代表着高压-超高压变质地体中的典型HPE结构,比大型花岗岩岩基的HPE结构更复杂,与传统的HPE指数衰减分布模式不吻合。CCSD主孔中所揭示的三明治式HPE结构是大陆被动陆缘中的基性及超基性岩、沉积岩及花岗岩在深  相似文献   
24.
对中国大陆科学钻探主孔的岩心进行了声发射测量,确定了301~1531m深度的最大主应力。并与钻孔崩落法(深度1269~1655m)测量结果进行了对比,结果表明,声发射测量所得测值基本上落在钻孔崩落法测值的趋势线上,两种方法所得结果一致,说明测量结果可信。测量结果表明科学钻探主孔地应力大小随深度增加,在浅部301m最大主应力为13.4MPa,在深部1655m为55.2MPa。随深度的增加率为0.0279MPa/m。最大主应力方向为N54°±3.3°E,且方向不随深度变化。  相似文献   
25.
班公湖—怒江构造带西段三叠纪—侏罗纪构造—沉积演化   总被引:20,自引:2,他引:20  
王冠民  钟建华 《地质论评》2002,48(3):297-303
班公湖-怒江构造带西段在大地构造位置上处于特提斯构造域东端,横跨班公湖-怒江断裂带。三叠纪-株罗纪期间,其构造-沉积演化经历了大陆初始裂谷(T)、原洋裂谷(J1)、残余弧后盆地(J2-J3)阶段。初始裂谷阶段的拉张是呈南断北超的半地堑式由东向西进行的,逐渐形成地堑式原洋裂谷盆地。中晚侏罗世,南部新特提斯洋壳开始北各俯冲,产生的区域挤压应力使原洋裂谷逐渐封闭,裂谷盆地的小洋壳表现出以南向俯冲为主的双向式腑冲,同时伴生区域热沉降,盆地具残余弧后盆地的性质。该阶段,羌南地区发育碳酸盐岩为主的稳定陆缘沉积,冈度斯-念青唐古拉板片北部则形成广泛南超的近源碎屑沉积。  相似文献   
26.
在简述盆地地质环境和含水系统、水文地质期与水压系统类型定位的基础上,通过建立数学模型,采用反演、比拟和地静压力等方法,模拟计算了各研究层在各研究时期泥岩压出水水头值(m),Es^2层的依次为2-28,2-26,2-6,2-16,0.5-3.5;Es^1层的依次为2-42,2-26,2-6,10-54,1-14;Ed层的依次为2-22,2-54,2-12;Ng层的依次为10-24,1-5;Nm层的为12-24。各研究层在各研究时期的压挤式水交替强度均小于1,累加值Es^2,Es^1,Ed层的均大于1,Ng,Nm层的小于1;Ed层渗入水交替强度为0.44。各研究层在各研究时期渗流场的高水压带位置和流动态具有相似性,并均以离心型流动型为主要特征。  相似文献   
27.
Multichannel seismic reflection data acquired by Marine Arctic Geological Expedition (MAGE) of Murmansk, Russia in 1990 provide the first view of the geological structure of the Arctic region between 77–80°N and 115–133°E, where the Eurasia Basin of the Arctic Ocean adjoins the passive-transform continental margin of the Laptev Sea. South of 80°N, the oceanic basement of the Eurasia Basin and continental basement of the Laptev Sea outer margin are covered by 1.5 to 8 km of sediments. Two structural sequences are distinguished in the sedimentary cover within the Laptev Sea outer margin and at the continent/ocean crust transition: the lower rift sequence, including mostly Upper Cretaceous to Lower Paleocene deposits, and the upper post-rift sequence, consisting of Cenozoic sediments. In the adjoining Eurasia Basin of the Arctic Ocean, the Cenozoic post-rift sequence consists of a few sedimentary successions deposited by several submarine fans. Based on the multichannel seismic reflection data, the structural pattern was determined and an isopach map of the sedimentary cover and tectonic zoning map were constructed. A location of the continent/ocean crust transition is tentatively defined. A buried continuation of the mid-ocean Gakkel Ridge is also detected. This study suggests that south of 78.5°N there was the cessation in the tectonic activity of the Gakkel Ridge Rift from 33–30 until 3–1 Ma and there was no sea-floor spreading in the southernmost part of the Eurasia Basin during the last 30–33 m.y. South of 78.5°N all oceanic crust of the Eurasia Basin near the continental margin of the Laptev Sea was formed from 56 to 33–30 Ma.  相似文献   
28.
The origin of the Baikal rift zone (BRZ) has been debated between the advocates of passive and active rifting since the 1970s. A re-assessment of the relevant geological and geophysical data from Russian and international literature questions the concept of broad asthenospheric upwelling beneath the rift zone that has been the cornerstone of many “active rifting” models. Results of a large number of early and recent studies favour the role of far-field forces in the opening and development of the BRZ. This study emphasises the data obtained through studies of peridotite and pyroxenite xenoliths brought to the surface by alkali basaltic magmas in southern Siberia and central Mongolia. These xenoliths are direct samples of the upper mantle in the vicinity of the BRZ. Of particular importance are suites of garnet-bearing xenoliths that have been used to construct PT- composition lithospheric cross-sections in the region for the depth range of 35–80 km.Xenolith studies have shown fundamental differences in the composition and thermal regime between the lithospheric mantle beneath the ancient Siberian platform (sampled by kimberlites) and beneath younger mobile belts south of the platform. The uppermost mantle in southern Siberia and central Mongolia is much hotter at similar levels than the mantle in the Siberian craton and also has significantly higher contents of ‘basaltic’ major elements (Ca, Al, Na) and iron, higher Fe/Si and Fe/Mg. The combination of the moderately high geothermal gradient and the fertile compositions in the off-cratonic mantle appears to be a determining factor controlling differences in sub-Moho seismic velocities relative to the Siberian craton. Chemical and isotopic compositions of the off-cratonic xenoliths indicate small-scale and regional mantle heterogeneities attributed to various partial melting and enrichment events, consistent with long-term evolution in the lithospheric mantle. Age estimates of mantle events based on Os–Sr–Nd isotopic data can be correlated with major regional stages of crustal formation and may indicate long-term crust–mantle coupling. The ratios of 143/144Nd in many LREE-depleted xenoliths are higher than those in MORB or OIB source regions and are not consistent with a recent origin from asthenospheric mantle.Mantle xenoliths nearest to the rift basins (30–50 km south of southern Lake Baikal) show no unequivocal evidence for strong heating, unusual stress and deformation, solid state flow, magmatic activity or partial melting that could be indicative of an asthenospheric intrusion right below the Moho. Comparisons between xenoliths from older and younger volcanic rocks east of Lake Baikal, together with observations on phase transformations and mineral zoning in individual xenoliths, have indicated recent heating in portions of the lithospheric mantle that may be related to localised magmatic activity or small-scale ascent of deep mantle material. Overall, the petrographic, PT, chemical and isotopic constraints from mantle xenoliths appear to be consistent with recent geophysical studies, which found no evidence for a large-scale asthenospheric upwarp beneath the rift, and lend support to passive rifting mechanism for the BRZ.  相似文献   
29.
Thermal and rheological structures of the Xisha Trough, South China Sea   总被引:8,自引:0,他引:8  
The Xisha Trough, located in the northwest of the South China Sea (SCS) mainly rifted 30 Ma ago, has been a failed rift since the cessation of the seafloor spreading of the NW subbasin. Based on the velocity–depth model along Profile OBH-4 across the Xisha Trough, a seven-layer density–depth model is used to estimate density structure for the profile. The relationship between seismic velocity and radiogenic heat production is used to estimate the vertical distribution of heat sources in the lower crust. The 2-D temperature field is calculated by applying a 2-D numerical solution of the heat conduction equation and the thermal lithosphere thickness is obtained from the basalt dry solidus (BDS). The rheology of the profile is estimated on the basis of frictional failure in the brittle regime and power-law steady-state creep in the ductile regime. Rheological model is constructed for a three-layer model involving a granitic upper crust, a quartz diorite lower crust and an olivine upper mantle. Gravity modeling supports basically the velocity–depth model. The Moho along Profile OBH-4 is of relatively high heat flow ranging from 46 to 60 mW/m2 and the Moho heat flow is higher in the trough than on the flanks. The depth of the “thermal” lithospheric lower boundary is about 54 km in the center, deepens toward two sides, and is about 75 km at the northern slope area and about 70 km at the southern Xisha–Zhongsha Block. Rheological calculation indicates that the two thinnest ductile layers in the crust and the thickest brittle layer in the uppermost mantle lie in the central region, showing that the Xisha Trough has been rheologically strengthened, which are mainly due to later thermal relaxation. In addition, the strengthening in rheology during rifting was not the main factor in hampering the breakup of the Xisha Trough.  相似文献   
30.
The nature and origin of the sediments and crust of the Murray Ridge System and northern Indus Fan are discussed. The uppermost unit consists of Middle Miocene to recent channel–levee complexes typical of submarine fans. This unit is underlain by a second unit composed of hemipelagic to pelagic sediments deposited during the drift phase after the break-up of India–Seychelles–Africa. A predrift sequence of assumed Mesozoic age occurring only as observed above basement ridges is composed of highly consolidated rocks. Different types of the acoustic basement were detected, which reflection seismic pattern, magnetic anomalies and gravity field modeling indicate to be of continental character. The continental crust is extremely thinned in the northern Indus Fan, lacking a typical block-faulted structure. The Indian continent–ocean transition is marked on single MCS profiles by sequences of seaward-dipping reflectors (SDR). In the northwestern Arabian Sea, the Indian plate margin is characterized by several phases of volcanism and deformation revealed from interpretation of multichannel seismic profiles and magnetic anomalies. From this study, thinned continental crust spreads between the northern Murray Ridge System and India underneath the northern Indus Fan.  相似文献   
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