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981.
地壳升降对渤、黄、东海潮波系统的影响 总被引:1,自引:1,他引:0
利用海平面变化预测模型,预测了渤黄东海未来海平面的上升值。该模型考虑了温室效应和地壳升降。根据潮波运动基本方程和海平面上升的预测值,数值模拟了渤黄东海潮波系统的变化。结果显示,半日分潮(M2,S2)的振幅变化ΔH(或位相变化Δg)有相似的正负分布模式,全日分潮(K1,Q1)的也是如此。考虑和不考虑地壳升降情况下得到的正负分布模式,在黄海存在着较明显的差别,那是由于在黄海存在一个范围很广的海平面变化年速率为负的区域所致。在我国沿岸主要站点,考虑地壳升降情况下获得的主要分潮振幅与不考虑的相比,其中M2分潮的差别最大,其差值范围为-1.8~3.3 cm。在主要站点,利用考虑地壳升降情况下获得的调和常数计算所得的海图深度基准面、最高和最低天文潮位,与利用原调和常数计算所得的相比,海图深度基准面的变化范围为-12.4~14.6 cm,最高天文潮位的变化范围为-11.7~13.0 cm,最低天文潮位的变化范围为-11.9~10.5 cm。 相似文献
982.
土壤结皮深刻影响绿洲边缘固沙植被区的土壤水文过程。土壤结皮斥水性是量化上述影响的潜在指标。采用滴水穿透时间(WDPT)法,研究了河西走廊荒漠边缘不同建植年限梭梭植被区固定沙丘土壤结皮斥水性的时间演变规律及影响因素。结果表明:建植20 a后,丘顶与丘间地土壤结皮出现显著斥水性(WDPT>5 s),而丘坡土壤结皮无斥水性(WDPT<5 s)。丘顶土壤结皮斥水性与总有机碳、微生物量碳、有机碳C-H组分以及电导率显著相关(P<0.01);而丘间地土壤结皮斥水性与黏、粉粒含量显著相关(P<0.01)。植被形成的“碳岛”及“盐岛”效应是丘顶土壤结皮斥水性形成的主要原因,而黏、粉粒在土壤表层的积聚是丘间地土壤结皮斥水性形成的主要原因。 相似文献
983.
The exhumation mechanism of high‐pressure (HP) and ultrahigh‐pressure (UHP) eclogites formed by the subduction of oceanic crust (hereafter referred to as oceanic eclogites) is one of the primary uncertainties associated with the subduction factory. The phase relations and densities of eclogites with MORB compositions are modelled using thermodynamic calculations over a P–T range of 1–4 GPa and 400–800 °C, respectively, in the NCKFMASHTO (Na2O–CaO–K2O–FeO–MgO–Al2O3–SiO2–H2O–TiO2–Fe2O3) system. Our modelling suggests that the mineral assemblages, mineral proportions and density of oceanic crust subducted along a cold P–T path are quite different from those of crust subducted along a warm P–T path, and that the density of oceanic eclogites is largely controlled by the stability of low‐density hydrous minerals, such as lawsonite, chlorite, glaucophane and talc. Along a cold subduction P–T path with a geotherm of ~6 °C km?1, lawsonite is always present at 1.1 to >4.0 GPa, and chlorite, glaucophane and talc can be stable at pressures of up to 2.3, 2.6 and 3.6 GPa respectively. Along such a P–T path, the density of subducted oceanic crust is always lower than that of the surrounding mantle at depths shallower than 110–120 km (< 3.3–3.6 GPa). However, along a warm subduction P–T path with a geotherm of ~10 °C km?1, the P–T path is outside the stability field of lawsonite, and the hydrous minerals of chlorite, epidote and amphibole break down completely into dry dense minerals at relatively lower pressures of 1.5, 1.85 and 1.9 GPa respectively. Along such a warm subduction P–T path, the subducted oceanic crust becomes denser than the surrounding mantle at depths >60 km (>1.8 GPa). Oceanic eclogites with high H2O content, oxygen fugacity, bulk‐rock XMg [ = MgO/(MgO + FeO)], XAl [ = Al2O3/(Al2O3 + MgO + FeO)] and low XCa [ = CaO/(CaO + MgO + FeO + Na2O)] are likely suitable for exhumation, which is consistent with the bulk‐rock compositions of the natural oceanic eclogites on the Earth's surface. On the basis of natural observations and our calculations, it is suggested that beyond depths around 110–120 km oceanic eclogites are not light enough and/or there are no blueschists to compensate the negative buoyancy of the oceanic crust, therefore explaining the lack of oceanic eclogites returned from ultradeep mantle (>120 km) to the Earth's surface. The exhumed light–cold–hydrous oceanic eclogites may have decoupled from the top part of the sinking slab at shallow depths in the forearc region and are exhumed inside the serpentinized subduction channel, whereas the dense–hot–dry eclogites may be retained in the sinking slab and recycled into deeper mantle. 相似文献
984.
985.
M. SANDIFORD 《Journal of Metamorphic Geology》2010,28(6):569-577
Variations in gravitational potential energy contribute to the intraplate stress field thereby providing the means by which lithospheric density structure is communicated at the plate scale. In this light, the near equivalence in the gravitational potential energy of typical continental lithosphere with the mid‐ocean ridges is particularly intriguing. Assuming this equivalence is not simply a chance outcome of continental growth, it then probably involves long‐term modulation of the density configuration of the continents via stress regimes that are able to induce significant strains over geological time. Following this notion, this work explores the possibility that the emergence of a chemically, thermally and mechanically structured continental lithosphere reflects a set of thermally sensitive feedback mechanisms in response to Wilson cycle oscillatory forcing about an ambient stress state set by the mid‐ocean ridge system. Such a hypothesis requires the continents are weak enough to sustain long‐term (108 years) strain rates of the order of ~10?17 s?1 as suggested by observations that continental lithosphere is almost everywhere critically stressed, by estimates of seismogenic strain rates in stable continental interiors such as Australia and by the low‐temperature thermochronological record of the continents that requires significant relief generation on the 108 year time‐scale. Furthermore, this notion provides a mechanism that helps explain interpretations of recently published heat flow data that imply the distribution of heat‐producing elements within the continents may be tuned to produce a characteristic thermal regime at Moho depths. 相似文献
986.
南海西北次海扩张时代和洋壳性质:沉积地层及重磁依据 总被引:1,自引:0,他引:1
利用沉积地层被动超覆和基底重磁异常特征对南海西北次海形成时代和洋壳性质进行了探讨。推断南海西北次海初始扩张时间为早渐新世,结束扩张时间为晚渐新世早期。地层变形、被动超覆特征、洋壳基底形态及对称性特点反映出两期洋壳扩张事件。第一期发生在早渐新世。由于洋壳扩张,上始新统被拉断,在洋壳边界处上始新统突然终止现象明显。受洋壳横向扩张推挤和纵向沉降作用影响,上始新统明显变形,并向扩张中心倾覆。第二期洋壳扩张发生在晚渐新世早期。该期洋壳扩张持续时间短,扩张幅度小,下渐新统被拉开的距离有限。由于南海西北次海形成期间不同部位地壳伸展减薄程度不同,南海西北次海洋壳基底呈北东部较宽,向南西方向变窄,并逐渐尖灭的不规则三角形。根据盆地边缘上始新统向海盆中心方向的断点/线和重磁异常资料,推测西北次海南西侧洋壳边界位于海盆基底坡角处附近,洋壳较窄;而北东侧洋壳边界位于海底坡角处附近,洋壳相对较宽。另外,重磁异常表明,在洋壳基底中有陆壳残留块体存在。上述这些现象说明南海西北次海在洋壳萌芽阶段就先天夭折,停止发育。 相似文献
987.
《International Geology Review》2012,54(8):1020-1038
ABSTRACTThe La Tinta mélange is a small but singular ultramafic mélange sheet that crops out in eastern Cuba. It is composed of dolerite-derived amphibolite blocks embedded in a serpentinite matrix. The amphibolite blocks have mid-ocean ridge basalt (MORB)-like composition showing little if any imprint of subduction zone component, similar to most forearc and MOR basalts worldwide. Relict Cr-spinel and olivine mineral chemistry of the serpentinized ultramafic matrix suggest a forearc position for these rocks. These characteristics, together with a hornblende 40Ar/39Ar age of 123.2 ± 2.2 Ma from one of the amphibolite blocks, suggest that the protoliths of the amphibolite blocks correspond to forearc basalt (FAB)-related rocks that formed during the earlier stage of subduction initiation of the Early Cretaceous Caribbean arc. We propose that the La Tinta amphibolites correspond to fragments of sills and dikes of hypoabyssal rocks formed in the earlier stages of a subduction initiation scenario in the Pacific realm (ca. 136 Ma). The forearc dolerite-derived amphibolites formed by partial melting of upwelling fertile asthenosphere at the beginning of subduction of the Proto-Caribbean (Atlantic) slab, with no interaction with slab-derived fluids/melts. This magmatic episode probably correlates with Early Cretaceous basic rocks described in Hispaniola (Gaspar Hernandez serpentinized peridotite-tectonite). The dikes and sills cooled and metamorphosed due to hydration at low pressure (ca. 3.8 kbar) and medium to high temperature (up to 720ºC) and reached ca. 500ºC at ca. 123 Ma. At this cooling stage, serpentinite formed after hydration of the ultramafic upper mantle. This process might have been favoured by faulting during extension of the forearc, indicating an early stage of dike and sill fragmentation and serpentinite mélanges formation; however, full development of the mélange likely took place during tectonic emplacement (obduction) onto the thrust belt of eastern Cuba during the latest Cretaceous. 相似文献
988.
华北克拉通北缘尚义地区新太古代TTG成因分析:洋壳玄武岩不同深度下熔融的产物 总被引:2,自引:1,他引:1
尚义玄武岩为尚义-赤城新太古代洋壳残片的组成端元,地球化学性质指示其源于富集地幔。根据稀土元素分配特征,尚义玄武岩可被分为TH1型(稀土元素平坦型)和TH2型(稀土元素分异型)。尚义TTG属于中钾偏铝质钙碱性岩类,其Al2O3含量与低铝型TTG相近,同时微量元素Rb、Sr、Y和REE表现出俯冲板片熔融成因的埃达克岩的性质。根据主量元素SiO2、K2O、Na2O、Al2O3和微量元素Rb、Sr、Y、REE等指标判别和微量元素平衡熔融模式计算得出,尚义TTG形成压力遍及低压—高压范围,是洋壳玄武岩(TH1型)在深度压力变化的条件下部分熔融形成的,其中的低铝型TTG形成于低压熔融。 相似文献
989.
大陆下地壳和岩石圈地幔含水性的差异——山东莒南玄武岩中深源包体的初步观察 总被引:1,自引:0,他引:1
对产于莒南晚中生代玄武岩中的镁铁质麻粒岩和橄榄岩包体矿物进行了傅里叶变换红外光谱(FTIR)分析.结果显示,麻粒岩矿物和全岩中水含量分别为:单斜辉石300×10-6~1 180×10-6,斜方辉石80×10-6~169×10-6,斜长石717×10-6~1 239×10-6,全岩525×10-6~855×10-6;橄榄岩矿物和全岩中水含量分别为:单斜辉石466×10- 6~746×10-6,斜方辉石187×10-6~304×10-6,橄榄石6×10-6~15×10-6,全岩81×10-6~245×10-6.从单矿物看,麻粒岩和橄榄岩之间水含量的差距不是很明显,但麻粒岩的全岩水含量明显高于橄榄岩,表明大陆深部岩石圈的水含量在垂向上具有不均一性. 相似文献
990.
下地壳含水性的演化 ——来自不同时代麻粒岩中长石水含量的证据 总被引:1,自引:1,他引:0
利用傅里叶变换红外光谱(FTIR)和电子探针(EMP)分析了早古生代的松树沟麻粒岩和桐柏麻粒岩地体以及古元古代的莒南麻粒岩包体(其寄主岩石为新生代玄武岩)中长石的水含量和化学成分。结果显示,麻粒岩中的长石均含有以OH和H2O形式存在的结构水;3个地点的长石水含量分别为465×10-6~733×10-6、210×10-6~993×10-6和717×10-6~1 239×10-6。对比前人报道的中生代(道县和汉诺坝包体)和古元古代(女山包体、汉诺坝地体)的麻粒岩研究结果,发现早古生代样品和古元古代样品中长石的水含量都比中生代样品明显的高,而早古生代和古元古代样品之间却没有差别,指示了中国东部下地壳在中生代之前更加富水。 相似文献