Sm-Nd isotopic provinces of the Aldan Shield     

A. B. Kotov  E. B. Sal&#;nikova  V. A. Glebovitsky  V. P. Kovach  A. M. Larin  S. D. Velikoslavinsky  N. Yu. Zagornaya 《Doklady Earth Sciences》2006,410(7):1066-1069

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Paleoproterozoic accretion in the Northeast Siberian craton: Isotopic dating of the Anabar collision system   总被引：1，自引：0，他引：1  

O. M. Rosen  L. K. Levskii  D. Z. Zhuravlev  A. Ya. Rotman  Z. V. Spetsius  A. F. Makeev  N. N. Zinchuk  A. V. Manakov  V. P. Serenko 《Stratigraphy and Geological Correlation》2006,14(6):581-601

Geochronological database considered in the work and characterizing the Anabar collision system in the Northeast Siberian craton includes coordinated results of Sm-Nd and Rb-Sr dating of samples from crustal xenoliths in kimberlites, deep drill holes, and bedrock outcrops. As is inferred, collision developed in three stages dated at 2200–2100, 1940–1760, and 1710–1630 Ma. The age of 2000–1960 Ma is established for substratum of mafic rocks, which probably originated during the lower crust interaction with asthenosphere due to the local collapse of the collision prism. Comparison of Sm-Nd and Rb-Sr isochron dates shows that the system cooling from ≈700 to ≈300°C lasted approximately 300 m.y. with a substantial lag relative to collision metamorphism and granite formation. It is assumed that accretion of the Siberian craton resulted in formation of a giant collision mountainous structure of the Himalayan type that was eroded by 1.65 Ga ago, when accumulation of gently dipping Meso-to Neoproterozoic (Riphean) platform cover commenced.  相似文献   

New data on the structure of the Khabarovsk Terrane of the Jurassic accretionary prism (Sikhote-Alin)     

I. V. Kemkin  A. N. Filippov  A. I. Khanchuk 《Doklady Earth Sciences》2006,406(1):28-31

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Age of zircons from chromites in the residual ophiolitic rocks as a reflection of upper mantle magmatic events     

G. N. Savelieva  P. V. Suslov  A. N. Larionov  N. G. Berezhnaya 《Doklady Earth Sciences》2006,411(9):1401-1406

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Riphean riftogenic ophiolites and conjugated minerageny of the Southern Urals     

V. A. Koroteev  V. N. Ogorodnikov  V. N. Sazonov  Yu. A. Polenov 《Doklady Earth Sciences》2006,411(8):1195-1198

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A review of landsliding and coastal erosion damage to historic fortifications in South East England     

E. N. Bromhead  M.-L. Ibsen 《Landslides》2006,3(4):341-347

Coastal fortifications in South East England have been continuously built and rebuilt over the centuries according to the ebb and flow of politics in Europe. This paper covers an extensive historical period from the influx of the Romans to the present day, detailing how landslides and coastal erosion have affected the numerous constructions along this stretch of coastline. Principal landslide-prone strata form extensive sections of this part of the coast with the tendency to be weak and highly susceptible to marine attack and cliff retreat. Fortifications have been built out of necessity in strategic positions without full consideration of the ground upon which they have been constructed. The continual construction of fortifications along this section of coastline constitutes an unparalleled archaeological record, but it is one that is under continuous threat from coastal erosion and landsliding.  相似文献   

Mixing and differentiation in the Oruanui rhyolitic magma, Taupo, New Zealand: evidence from volatiles and trace elements in melt inclusions     

Yang Liu  Alfred T. Anderson  Colin J. N. Wilson  Andrew M. Davis  Ian M. Steele 《Contributions to Mineralogy and Petrology》2006,151(1):71-87

Large pyroclastic rhyolites are snapshots of evolving magma bodies, and preserved in their eruptive pyroclasts is a record of evolution up to the time of eruption. Here we focus on the conditions and processes in the Oruanui magma that erupted at 26.5 ka from Taupo Volcano, New Zealand. The 530 km³ (void-free) of material erupted in the Oruanui event is comparable in size to the Bishop Tuff in California, but differs in that rhyolitic pumice and glass compositions, although variable, did not change systematically with eruption order. We measured the concentrations of H₂O, CO₂ and major and trace elements in zoned phenocrysts and melt inclusions from individual pumice clasts covering the range from early to late erupted units. We also used cathodoluminescence imaging to infer growth histories of quartz phenocrysts. For quartz-hosted inclusions, we studied both fully enclosed melt inclusions and reentrants (connecting to host melt through a small opening). The textures and compositions of inclusions and phenocrysts reflect complex pre-eruptive processes of incomplete assimilation/partial melting, crystallization differentiation, magma mixing and gas saturation. ‘Restitic’ quartz occurs in seven of eight pumice clasts studied. Variations in dissolved H₂O and CO₂ in quartz-hosted melt inclusions reflect gas saturation in the Oruanui magma and crystallization depths of ∼3.5–7 km. Based on variations of dissolved H₂O and CO₂ in reentrants, the amount of exsolved gas at the beginning of eruption increased with depth, corresponding to decreasing density with depth. Pre-eruptive mixing of magma with varying gas content implies variations in magma bulk density that would have driven convective mixing. Electronic Supplementary Material Supplementary material is available for this article at and is accessible for authorized users.  相似文献   

Ammonium regeneration in intertidal sediments of the Yangtze estuary during air-exposure     

L.J. Hou  M. Liu  J.J. Lu  S.Y. Xu  D.N. Ou  Y. Yang  D.G. Zheng 《Environmental Geology》2006,49(7):937-945

The influences of exposure to the atmosphere on ammonium cycle in the intertidal surface sediments were in situ studied with a geochemical approach at a typical station in the Yangtze Estuary during three tidal cycles in September 2003. During an about 8-h emersion period of each diurnal tide, six high-resolution vertical profiles of adsorbed and dissolved ammonium were measured. It was observed that both adsorbed and dissolved ammonium generally had an increasing trend in sediment cores during the exposure. The rate of ammonium regeneration in sediments was estimated using the accumulation amount of ammonium including adsorbed and soluble fractions during the daytime emersion. The calculation result showed that there was relatively high ammonification rate (˜500 nmol N cm⁻³ day⁻¹), which reflected that organic nitrogen in sediments was quickly decomposed with a residence time of ˜52.7 days. Due to the dramatic temperature difference observed in sediment profiles, free convection was considered an important mechanism of regulating the efflux of produced ammonium into overlying waters. The total estimated amount of regenerated ammonium was ˜1.35×10⁵ t N year⁻¹ in the intertidal flat of the Yangtze Estuary, which occupied 7.6% of the total inorganic nitrogen annually transported to the estuarine ecosystem.  相似文献   

Petrogenesis and geotectonic setting of the PanAfrican basement rocks in Bamenda Massif, Obudu Plateau, southeastern Nigeria： Evidence from trace element geochemistry     

UKAEGBU V. U. EKWUEME B. N. 《中国地球化学学报》2006,25(2):122-131

1 IntroductionThe study area is part of the Obudu Plateau,which forms part of the Precambrian Pan-African tec-tonothermal belt, lying between the West African Cra-ton and the Gabon-Congo Craton ( Fig. 1). It isbounded by the Benue Trough, in the NE-SW axi…  相似文献   

Low-low satellite-to-satellite tracking: a comparison between analytical linear orbit perturbation theory and numerical integration   总被引：1，自引：0，他引：1  

P.N.A.M. Visser 《Journal of Geodesy》2005,79(1-3):160-166

Low-low satellite-to-satellite tracking (ll-SST) range-rate observations have been predicted by two methods: one based on a linear perturbation theory in combination with the Hill equations, and one based on solving the equations of motion of two low-flying satellites by numerical integration. The two methods produce almost equivalent Fourier spectra of the range-rate observations after properly taking into account a few resonant terms. For a typical GRACE-type configuration, where the two satellites trail each other at a distance of 300 km at an altitude of 460 km, and in the presence of the EGM96 gravity field model, complete to spherical harmonic degree and order 70, the agreement between the Fourier spectra is about 1 mm/s compared to a root-mean-square (RMS) value of more than 220 mm/s for the range-rate signal. The discrepancy of 1 mm/s can be reduced significantly when not taking into account perturbations caused by the J₂ term. Excluding the J₂ term, the agreement between the two methods improves to 0.4 mm/s compared to a RMS value of 6 mm/s for the range-rate signal. These values are 0.01 and 2.3 mm/s when ignoring the spectrum for frequencies below two cycles per orbital revolution, reducing the discrepancy even further to about 0.5% of the signal. The selected linear perturbation theory is thus capable of modeling gravity field induced range-rate observations with very high precision for a large part of the spectrum.  相似文献