排序方式： 共有15条查询结果，搜索用时 30 毫秒
1.
1 Introduction The Gaojiacun intrusive complex is one of the numerous ultramafic-mafic intrusions in Sichuan Province of China. It was mapped during the 1970s and studied mainly by Chinese scientists (e.g. Geological Team 106, 1975; Shen et al., 1986, 1989; CGGJC, 1986; Yang et al., 1993; Li et al., 1995; Shen et al., 2003; Zhu et al., 2004a). Since the year 2000, China has become one of the largest PGE consumers. While the country can produce only less than 1 ton PGE/year, the Chin… 相似文献
2.
Alvaro P. CRÓSTA César KAZZUO‐VIEIRA Lidia PITARELLO Christian KOEBERL Thomas KENKMANN 《Meteoritics & planetary science》2012,47(1):51-71
Abstract– Vargeão Dome (southern Brazil) is a circular feature formed in lava flows of the Lower Cretaceous Serra Geral Formation and in sandstones of the Paraná Basin. Even though its impact origin was already proposed in the 1980s, little information about its geological and impact features is available in the literature. The structure has a rim‐rim diameter of approximately 12 km and comprises several ring‐like concentric features with multiple concentric lineaments. The presence of a central uplift is suggested by the occurrence of deformed sandstone strata of the Botucatu and Pirambóia formations. We present the morphological/structural characteristics of Vargeão Dome, characterize the different rock types that occur in its interior, mainly brecciated volcanic rocks (BVR) of the Serra Geral Formation, and discuss the deformation and shock features in the volcanic rocks and in sandstones. These features comprise shatter cones in sandstone and basalt, as well as planar microstructures in quartz. A geochemical comparison of the target rock equivalents from outside the structure with the shocked rocks from its interior shows that both the BVRs and the brecciated sandstone have a composition largely similar to that of the corresponding unshocked lithologies. No traces of meteoritic material have been found so far. The results confirm the impact origin of Vargeão Dome, making it one of the largest among the rare impact craters in basaltic targets known on Earth. 相似文献
3.
Abstract: The Balfour Formation has a pronounced lithological variation that is characterized by alternating sandstone- and mudstone-dominated members. The sandstone-dominated Oudeberg and Barberskrans Members are composed of lithofacies that range from intraformational conglomerates to fine-grained sediments, whereas the mudstone-dominated members (Daggaboersnek, Elandsberg, and Palingkloof) are dominated by the facies Fm and Fl. Petrography, geochemistry, and a paleocurrent analysis indicated that the source rock of the Balfour Formation was to south east and the rocks had a transitional/dissected magmatic arc signature. The sandstones-rich members were deposited by seasonal and ephemeral high-energy, low-sinuous streams, and the fine-grained-rich members were formed by ephemeral meandering streams. The paleoclimates have been equated to present temperate climates; they were semiarid becoming arid towards the top of the Balfour Formation. This has been determined by reconstructing the paleolatitude of the Karoo Basin, geochemistry, paleontology, sedimentary structures, and other rock properties, like color. 相似文献
4.
CR Weir 《African Journal of Marine Science》2016,38(3):385-394
During October and November 2015, the first systematic survey of Sousa teuszii was carried out in the Saloum Delta (Senegal, West Africa), comprising 1 617.5 km of boat-based survey coverage. Thirty sightings were recorded in the Saloum and Diomboss rivers, and along the southern coastline. Dolphins were also observed entering the Bandiala and Djinack channels, and travelling across the border into Gambia. The initial sighting locations were 0.043–1.192 km from shore, and tracked dolphins did not move more than 2.082 km from shore. Groups comprised 1–29 animals (mean 9.3 animals), and at least three neonate calves were observed during November. The overall relative abundance was 0.018 sight. km?1 and 0.175 ind. km?1. Sightings were concentrated in the Diomboss where relative abundance reached 0.037 sight. km?1 and 0.331 ind. km?1. Non-intensive photo-identification produced a minimum population size of 103 animals, the highest recorded for S. teuszii anywhere in its range. Photo-identification also confirmed a movement of individuals between different parts of the Saloum Delta. Combined travel–forage dominated the behaviour. Dolphins were photographed capturing mullet (Mugil sp.) on three occasions. The distribution, population size and movements of S. teuszii are discussed in relation to management. 相似文献
5.
北秦岭西段冥古宙锆石(4.1～3.9Ga)年代学新进展 总被引：15，自引：13，他引：2
2007年王洪亮等报道在北秦岭西段火山岩中获得一粒年龄为4079±5Ma的冥古宙捕虏锆石。之后,对这一发现开展了深入的调查研究,我们除利用SHIMP技术方法对原4079Ma的锆石进行验证外,新获得了两粒~(207)Pb/~(206)Pb年龄为4007±29Ma和3908±45Ma捕获的变质成因锆石,表明早在4.0Ga已经有变质作用的发生,这或许说明在冥古宙时期地球已经具有相当规模和厚度的地壳。同时开展的岩石学研究表明,蕴含古老锆石的母岩属于火山碎屑熔岩类而不是火山熔岩。 相似文献
6.
A number of cyclic triaxial tests were carried out on mine tailings and natural sediment samples under undrained conditions
to investigate their resistance to cyclic loading. The tests were performed on more than 100 samples with a cyclic shear stress
ratio ranging from 0.10 to 0.40 under varying void ratio and the same confining pressure. It was observed that the axial strain
and excess pore water pressure increased with the number of loading cycles while the effective stress decreased with increasing
number of loading cycles. The liquefaction resistance of the tailings was also observed to be higher than that of natural
soils with similar particle size distribution, void ratio and plasticity index. It was observed that the influence of specific
gravity on the cyclic strength of mine tailings is significant. The results showed that the cyclic resistance of the tailings
was not strongly influenced by plasticity index for low plasticity tailings. A boundary relationship between void ratio and
normalized cyclic resistance ratio was established based on the results. 相似文献
7.
Bernardi Mara S. Africa Pasquale C. de Falco Carlo Formaggia Luca Menafoglio Alessandra Vantini Simone 《Mathematical Geosciences》2021,53(8):1781-1812
Mathematical Geosciences - Recent advances in satellite technologies, statistical and mathematical models, and computational resources have paved the way for operational use of satellite data in... 相似文献
8.
9.
M. A. R. VASCONCELOS K. WÜNNEMANN A. P. CRÓSTA E. C. MOLINA W. U. REIMOLD E. YOKOYAMA 《Meteoritics & planetary science》2012,47(10):1659-1670
Forward modeling is commonly applied to gravity field data of impact structures to determine the main gravity anomaly sources. In this context, we have developed 2.5‐D gravity models of the Serra da Cangalha impact structure for the purpose of investigating geological bodies/structures underneath the crater. Interpretation of the models was supported by ground magnetic data acquired along profiles, as well as by high resolution aeromagnetic data. Ground magnetic data reveal the presence of short‐wavelength anomalies probably related to shallow magnetic sources that could have been emplaced during the cratering process. Aeromagnetic data show that the basement underneath the crater occurs at an average depth of about 1.9 km, whereas in the region beneath the central uplift it is raised to 0.5–1 km below the current surface. These depths are also supported by 2.5‐D gravity models showing a gentle relief for the basement beneath the central uplift area. Geophysical data were used to provide further constraints for numeral modeling of crater formation that provided important information on the structural modification that affected the rocks underneath the crater, as well as on shock‐induced modifications of target rocks. The results showed that the morphology is consistent with the current observations of the crater and that Serra da Cangalha was formed by a meteorite of approximately 1.4 km diameter striking at 12 km s?1. 相似文献
10.
On the basis of a 2008 survey conducted in the Msunduzi municipality in the KwaZulu-Natal province, the paper begins an exploration of the character of popular politics and citizenship in South Africa. Embracing a ‘citizen-centred’ methodology informed by participation literatures, and sensibilities to the ‘work in progress’ character of African cities from urban studies debates, the paper interrogates the mainstream liberal-participatory model of citizenship in South Africa, and the critiques of current South African politics informed by these notions, specifically the ‘racial census’ and ‘dominant party syndrome’ analyses. Taken together these views can be read as characterising South African politics as a game for individual citizens governed by liberal rules, but played by racial and/or partisan groups in exclusionary ways, thus distorting liberal democratic mechanisms of representation and accountability. The paper also examines evidence for an alternative class-based analysis of one aspect of citizenship, namely, protest against poor local governance.The paper looks to unpack this ‘liberal model versus racialised communitarian practice’ imaginary by, on the one hand, demonstrating the ways in which citizenship is not racialised, or is asymmetrically racialised. Indeed, other than party allegiances and trust in key offices, very little by way of what citizens do, believe or think of themselves follows discrete racial lines. Similar points hold for partisanship too. On the other hand, the paper does not redeem the liberal-democratic model as there is also evidence of trust in government when it is not deserved based on performance, but more importantly, evidence that citizens embrace ‘informal’ means to secure their rights. A good example of this is protestors who are also more likely to vote than non-protestors. Taken together, these findings affirm both the way in which the racial and partisan legacy of the past is being undone by new institutions and practices, and suggest the complex intersection of these with networks of personal relations which characterise the local politics of most African cities. 相似文献