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111.
庐山地区星子群碎屑锆石SIMS U-Pb年龄及其地质意义   总被引:1,自引:0,他引:1  
江西庐山地区出露的星子群为一套遭受角闪岩相变质的中深变质岩系,前人将其划分为古元古代地层,并将其与华南早期地壳的形成与演化和中生代变质核杂岩构造相联系。本文通过对星子群浅粒岩中碎屑锆石U-Pb SIMS年代学研究,获得了(834±4)Ma碎屑锆石年龄,代表了该套地层沉积时代的下限;再结合其上覆筲箕洼组(830±5)Ma的火山岩年龄,将星子群的地层时代限定于新元古代。这一研究结果表明庐山地区并未出露古元古代的变质基底;而且野外也并未找到典型大规模拆离断层的存在,因此前人厘定的中生代变质核杂岩构造也值得商榷。根据碎屑锆石U-Pb不一致线下交点年龄为(133±20)Ma,推断星子群的变质作用发生在中生代。另外,由星子群单一的碎屑锆石年龄、锆石形态特征及矿物组成特征推断,星子群是源区花岗质岩石快速抬升、风化剥蚀和搬运沉积的产物,暗示着强烈的地壳运动过程,可能与Rodinia超大陆的裂解有关。  相似文献   
112.
通过对滇东北东川下田坝地区黑云母二长花岗岩和似斑状钾长花岗岩2种岩体的地球化学分析及对黑云母二长花岗岩的U-Pb同位素测试,得到如下认识:黑云母二长花岗岩和似斑状钾长花岗岩总体地球化学特征相似,主量元素表现出高SiO2(平均71.7%)、过铝质(A/CNK指数在1.03~1.52)的特征,过碱指数在0.95~1.37之间,总体属于钙碱系列;稀土元素总量较高(ΣREE平均313×10-6),(Ce/Yb)N均值为8.85,(La/Yb)N均值为9.54,呈现轻稀土元素(LREE)富集,仅Eu亏损(δEu均值0.31)的海鸥型右倾模式;大离子亲石元素Rb、Th、U、K等相对富集,高场强元素Nb、Ta、Sr、Ti等呈明显负异常,说明岩浆源岩以陆壳成分为主;Ga/Al均值为2.69,(Zr+Nb+Ce+Y)均值为383;微量元素Sr、Eu低,富集Nb、Zr等元素,反映其源区存在斜长石的残留;锆石饱和温度为724~786℃,表明初始岩浆温度较高。上述特征说明,下田坝花岗岩为典型的A型花岗岩,形成于中上地壳的板内伸展背景。黑云母二长花岗岩LA-ICP-MS锆石U-Pb年龄为801.1±6.6Ma,同时受到762.1±6.2Ma热事件的影响,与新元古代Rodinia超大陆裂解事件在时间上一致,亦与东川铜矿成矿时代相符,说明新元古代裂谷环境的岩浆事件范围可扩大至滇东北东川,并可能引发热液成矿作用。  相似文献   
113.
藏北羌塘奥陶纪平行不整合面的厘定及其构造意义   总被引:7,自引:5,他引:2  
杨耀  赵中宝  苑婷媛  刘焰  李聪颖 《岩石学报》2014,30(8):2381-2392
西藏羌塘块体有无变质基底、其前新生代构造属性与演化过程是长期争论的议题。本文报道南羌塘块体北部,中、上奥陶统塔石山组底砾岩平行不整合于浅变质中厚层石英砂岩夹薄层泥灰岩之上。近600粒碎屑锆石测年结果表明浅变质石英砂岩的最大沉积年龄为527±7Ma,300余粒碎屑锆石测年结果表明塔石山组底部石英砂岩的最大沉积年龄为471±6Ma。不整合面上、下石英砂岩最大沉积年龄之差达56Myr,表明这两套石英砂岩之间存在明显的沉积间断,证实了该平行不整合面的时代为奥陶纪早期。另一独立的证据是在邻区发现了早奥陶世花岗岩类岩石(471~477Ma)侵位于该浅变质石英岩,因此将不整合面之下的浅变质石英岩暂命名为荣玛组,归入寒武系地层。阴极发光与年代学研究进一步表明不整合面之上的碎屑锆石主要来源于在"泛非"运动晚期形成的结晶岩,为近源锆石,表明"泛非运动"晚期所形成的结晶岩在奥陶纪早期就已隆升,遭受剥蚀,为区内中上奥陶统沉积岩的形成提供物质来源。该奥陶纪平行不整合面的发现,表明南羌塘块体与喜马拉雅、拉萨等块体相似,同属冈瓦纳大陆体系。南、北羌塘早古生代地层系统之间的显著差异表明在寒武-奥陶纪之交,南、北羌塘块体就已被古大洋盆分隔开,开始各自独立演化。  相似文献   
114.
Within the Albany–Fraser Orogen of southwestern Australia, the Coramup Gneiss is a NE–SW trending zone of high‐strain rocks that preserves a detailed record of orogenesis related to Mesoproterozoic convergence of the West Australian and Mawson cratons. New structural, metamorphic and U–Pb SHRIMP zircon age data establish that the Coramup Gneiss underwent high‐grade tectonism during both Stage I (c. 1290 Ma) and Stage II (c. 1170 Ma) of the Albany–Fraser Orogeny. Stage I commenced with c. 1300 Ma high‐T, low‐P M1a metamorphism during extension, and the formation of small‐scale ptygmatic folds within a subhorizontal S1a gneissosity. High‐P M1b metamorphism at c. 1290 Ma was accompanied by the transposition and shearing of S1a into a composite, shallow SE‐dipping S1b foliation, and the development of tight recumbent F1b folds with S1‐parallel axial surfaces and asymmetries indicating NW‐directed thrusting. The preservation of a similar PT–time record in the Fraser Complex (NE of the Coramup Gneiss) is consistent with large‐scale, NW‐directed Stage I thrusting of the Mawson Craton margin over the south‐eastern edge of the West Australian Craton. Stage II tectonism in the western Coramup Gneiss involved high‐T, low‐P M2a metamorphism and the formation of subvertical SE‐dipping D2 shear zones, shallow SW‐plunging L2 mineral stretching lineations, and NW‐verging F2 folds with S2‐parallel axial surfaces. A synkinematic pegmatite dyke emplaced into a D2 shear zone yielded a U–Pb SHRIMP zircon age of 1168 ± 12 Ma. Kinematic indicators suggest a combination of pure shear flattening perpendicular to S2, and dextral simple shear. However, contemporaneous structures elsewhere in the Albany–Fraser Orogen are consistent with continued NW–SE convergence at craton‐scale during Stage II, and oblique compression in the Coramup Gneiss is attributed to the arcuate geometry of the orogen‐scale deformation front.  相似文献   
115.
大气中的沙尘通过对太阳光的吸收和散射对地表温度产生影响,进而对大气环流和降水等也产生影响,但是在地球的不同历史时期尤其是深时地球大气中的沙尘量如何变化以及如何影响气候还有很多不清楚的地方。本文通过模式模拟对地球上4个不同时期的沙尘变化及其气候影响进行了研究,这4个时期分别是陆地植被还没有出现的前寒武时期、有植被且全球气温较高的盘古超大陆时期、大陆分布接近现代但气候较寒冷的末次盛冰期和气候较温暖的中全新世。在前寒武时期,由于陆地起沙面积大,大气中的沙尘含量可以达到现代地球的近10倍,使得全球地表温度下降也有近10 ℃。在盘古超大陆时期,由于在副热带的陆地面积比现代稍大,因此大气沙尘量也比现代稍大,对全球平均温度的影响很小。在末次盛冰期,由于寒冷干燥,沙尘量是现代的约两倍,但是它对全球有强烈的增温作用,如果没有沙尘,全球温度可能降低约2.5 ℃。在中全新世,观测显示全球沙尘量比现代少很多,模拟显示,采用现代沙尘和把沙尘全部去掉对全球平均温度的影响可以忽略,但是大西洋经向翻转流有显著变化。  相似文献   
116.
Diverse models have been proposed for the role of the Tarim Craton within the Paleoproterozoic Columbia supercontinent assembly. Here we report a suite of-1.71 Ga Nb-enriched meta-gabbro lenses in the eastern Quanji Massif, within the Tarim Craton in NW China. The meta-gabbroic rocks have Nb contents of 11.5-16.4 ppm with Nb/La ratios varying from 0.84 to 1.02((Nb/La)_N = 0.81-0.98) and Nb/U ratios from 38.0 to 47.2. They show low SiO_2(45.1-48.5 wt.%) and MgO(5.96-6.81 wt.%) and Mg#(Mg# = Mg/(Mg + Fe) = 43.5-47.7), high FeO~t(13.0-15.7 wt.%) and moderate Ti02(1.70-2.51 wt.%).with tholeiitic affinities. These rocks possess low fractionated REE patterns without obvious Eu anomalies(Eu/Eu~* = 0.87-1.02). Their primitive mantle-normalized elements patterns display significant Zr-Hf troughs, positive Nb anomalies, weak negative Ti and P anomalies, and high contents of Rb and Ba,resembling Nb-enriched basalts generated in arc-related tectonic settings. Their arc-like geochemical signatures together with whole rock εNd(t) values of 0.4-2.1 and corresponding old T_(DM)(2.22-2.37 Ga)as well as(~(143)Nd/~(144)Nd)_t and(~(87)Sr/~(86)Sr)t(t = 1712 Ma) values of 0.5104-0.5105 and 0.7030-0.7058,respectively, suggest that their precursor magma originated from mantle wedge peridotite metasomatised by subduction-derived melts. The results from our study reveal subduction along the eastern periphery of the Tarim Craton and marginal outgrowth continuing to ~1.7 Ga within the Columbia supercontinent.  相似文献   
117.
出露于阿中地块库木塔什萨依一带的亚干布阳片麻岩主要岩性为黑云斜长片麻岩、黑云二长片麻岩。利用LA-ICPMS方法进行锆石微区U-Pb同位素定年,得到206Pb/238U年龄加权平均值为900.2±2.9Ma,表明亚干布阳片麻岩原岩形成于新元古代早期青白口纪;地球化学结果显示,主量元素具有高SiO_2、Al_2O_3、K_2O+Na_2O含量,低Na_2O、MgO、CaO和TiO_2含量的特征,A/CNK值介于0.95~1.22之间,属于高钾钙碱性系列的过铝质花岗岩。岩石富集Rb、Th、K等大离子亲石元素,亏损Nb、Sr、P、Hf、Ti等高场强元素;岩石轻稀土元素分馏较强而重稀土元素分馏较弱,具有明显的负Eu异常,总体呈右倾的"V"字形稀土元素配分模式,显示典型的地壳重熔型花岗岩特征。亚干布阳片麻岩的源岩主要为地壳中沉积岩类的部分熔融,形成于俯冲-同碰撞构造环境。综上说明亚干布阳片麻岩是新元古代早期俯冲碰撞热事件的产物,反映阿中地块和柴达木地块青白口纪处于汇聚碰撞阶段,构造岩浆活动强烈,与Rodinia超大陆汇聚事件具有一致性。  相似文献   
118.
The bulk of the Atlantic shield basement in the eastern South American platform is made of Rhyacian calc-alkaline magmatic rocks (∼2.2–2.15 Ga) affected by granulite-facies metamorphism at around 2.06 Ga, as part of a Paleoproterozoic orogenic system which joined Archean crustal fragments together. Orosirian (2050–1800 Ma) rocks, on the other hand, are scarce in all four major provinces of eastern South America (the Borborema, São Francisco, Tocantins and Mantiqueira provinces). Recently, however, sparse occurrences of Orosirian-aged rocks have been described, particularly in the northern São Francisco Craton margin and adjoining fold belts that compose the Borborema Province further north. In this paper, we present new geochemical, geochronological and isotopic data of amphibolites which compose the basement of the Rio Preto fold belt, in the northwestern São Francisco Craton margin. Geochemical data suggest tholeiitic gabbro protoliths intruded in a subduction-related setting, as suggested by tectonic discrimination diagrams and differentiation trends. U–Pb analyses of magmatic zircon crystals yielded a 1958.3 ± 16 Ma Concordia age. Slightly negative to positive εNd(1.96) = (−0.3 to +1.0) and εHf(1.96) from −0.76 to −4.55 suggest variable mixing of a depleted mantle source and older continental crust. We interpret the amphibolite body as a remnant of a subduction-related crustal fragment developed in the Orosirian, around 1.96 Ga ago, possibly in a continental back-arc setting. This crustal fragment was further reworked as part of the basement of the Rio Preto fold belt during the Brasiliano Orogeny (∼600–550 Ma). The Cristalândia do Piauí Complex gneisses further north might represent fragments of a coeval continental magmatic arc. These rocks could be the first well documented representatives of an Orosirian tectono-magmatic event which has been, up to now, broadly ignored within this portion of West Gondwana, and thus present major implications for the Proterozoic crustal evolution of South America and for Paleoproterozic supercontinent reconstructions in general.  相似文献   
119.
120.
The Albany–Fraser Orogen in southwestern Australia preserves an important thermo‐tectonic record of Australo‐Antarctic cratonic assembly during the Mesoproterozoic. New petrologic and thermobarometric data from the Coramup Gneiss (a 10 km wide zone of high strain rocks within the NE‐trending eastern Albany–Fraser Orogen) indicate at least two high‐grade metamorphic events during 1345–1140 Ma convergence and amalgamation of the West Australian and Mawson cratons. The first event (M1) involved c. 1300 Ma granulite facies metamorphism of the Coramup Gneiss (M1a: 800–850 °C, 5–7 kbar), followed by burial and recrystallization under high‐P conditions (M1b: 800–850 °C, c. 10 kbar) prior to high‐T decompression (M1c: 700–800 °C, 7–8 kbar) and the 1290–1280 Ma emplacement of Recherche Granite sills. The second event (M2) entailed high‐T, low‐P metamorphism within dextral D2 shear zones (M2a: 750–800 °C, 5–6 kbar), followed by fluid‐present amphibolite facies M2b retrogression. Subsequent sinistral D3 mylonites and pseudotachylites are considered contemporaneous with similar structures in the adjacent Nornalup Complex that postdate the c. 1140 Ma Esperance Granite. Our petrological and thermobarometric data permit two end‐member PT‐time relationships between M1 and M2: (1) a single post‐M1b event involving continuous M1b–M1c–M2a–M2b cooling and decompression, and (2) a two‐stage post‐M1b evolution involving M1c metamorphism during the waning stages of an event unrelated causally or temporally to subsequent M2a metamorphism and D2 deformation. In a companion paper, new structural and U–Pb SHRIMP zircon data are presented to support a two‐stage PT evolution for the Coramup Gneiss, with M1 and M2, respectively, reflecting thermo‐tectonic activity during Stage I (1345–1260 Ma) and Stage II (1215–1140 Ma) of the Albany–Fraser Orogeny.  相似文献   
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