Jurassic to Palaeogene tectono‐magmatic evolution of northern Chile and adjacent Bolivia from detrital zircon U‐Pb geochronology and heavy mineral provenance     

Jörn F. Wotzlaw  Audrey Decou  Hilmar von Eynatten  Gerhard Wörner  Dirk Frei 《地学学报》2011,23(6):399-406

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Erratum to: The thermal stability of radiation-induced defects in illite     

T. Riegler  T. Allard  D. Beaufort  J.-L. Cantin  H. J. von Bardeleben 《Physics and Chemistry of Minerals》2016,43(1):31-31

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Geochronological and isotopic records of crustal storage and assimilation in the Wolverine Creek–Conant Creek system,Heise eruptive centre,Snake River Plain     

D. Szymanowski  B. S. Ellis  J. F. Wotzlaw  Y. Buret  A. von Quadt  I. Peytcheva  I. N. Bindeman  O. Bachmann 《Contributions to Mineralogy and Petrology》2016,171(12):106

Understanding the processes of differentiation of the Yellowstone–Snake River Plain (YSRP) rhyolites is typically impeded by the apparent lack of erupted intermediate compositions as well as the complex nature of their shallow interaction with the surrounding crust responsible for their typically low O isotopic ratios. A pair of normal-δ¹⁸O rhyolitic eruptions from the Heise eruptive centre in eastern Idaho, the Wolverine Creek Tuff and the Conant Creek Tuff, represent unique magmatic products of the Yellowstone hotspot preserving abundant vestiges of the intermediate differentiation steps leading to rhyolite generation. We address both shallow and deep processes of magma generation and storage in the two units by combining high-precision ID–TIMS U–Pb zircon geochronology, trace element, O and Hf isotopic studies of zircon, and Sr isotopic analyses of individual high-Mg# pyroxenes inherited from lower- to mid-crustal differentiation stages. The zircon geochronology confirms the derivation of both tuffs from the same rhyolitic magma reservoir erupted at 5.5941 ± 0.0097 Ma, preceded by at least 92 ± 14 ky of continuous or intermittent zircon saturation approximating the length of pre-eruptive magma accumulation in the upper crust. Some low-Mg# pyroxenes enclosing zircons predate the eruption by at least 45 ± 27 ky, illustrating the co-crystallisation of major and accessory phases in the near-liquidus rhyolitic melts of the YSRP over a significant period of time. Coeval zircon crystals are isotopically heterogeneous (two populations at εHf ~?5 and ?13), requiring the assembly of isotopically distinct melt pockets directly prior to, or during, the eruption. The primitive Mg# 60–90 pyroxenes are out of isotopic equilibrium with the host rhyolitic melt (⁸⁷Sr/⁸⁶Sr_i = 0.70889), covering a range of ⁸⁷Sr/⁸⁶Sr_i = 0.70705–0.70883 corresponding to ratios typical of the most radiogenic YSRP basalts to the least radiogenic YSRP rhyolites. Together with the low εHf in zircon, the Sr isotopic ratios illustrate limited assimilation dominated by radiogenic Archean crustal source materials incorporated into variably evolved YSRP melts as they progress towards rhyolitic compositions by assimilation–fractional crystallisation.  相似文献   

Alpine thermal events in the central Serbo-Macedonian Massif (southeastern Serbia)     

Milorad D. Antić  Alexandre Kounov  Branislav Trivić  Andreas Wetzel  Irena Peytcheva  Albrecht von Quadt 《International Journal of Earth Sciences》2016,105(5):1485-1505

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Limno-ecological characteristics and distribution patterns of spring habitats and invertebrates from the Lowlands to the Alps     

Martin Reiss  Peter Martin  Reinhard Gerecke  Stefanie von Fumetti 《Environmental Earth Sciences》2016,75(12):1033

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Tectonic significance of Triassic mafic rocks in the June Complex,Sanandaj–Sirjan zone,Iran     

Farzaneh Shakerardakani  Franz Neubauer  Xiaoming Liu  Manfred Bernroider  Behzad Monfaredi  Albrecht von Quadt 《Swiss Journal of Geoscience》2018,111(1-2):13-33

This study concentrates on the petrological and geochemical investigation of mafic rocks embedded within the voluminous Triassic June Complex of the central Sanandaj–Sirjan zone (Iran), which are crucial to reconstruct the geodynamics of the Neotethyan passive margin. The Triassic mafic rocks are alkaline to sub-alkaline basalts, containing 43.36–49.09 wt% SiO₂, 5.19–20.61 wt% MgO and 0.66–4.59 wt% total alkalis. Based on MgO concentrations, the mafic rocks fall into two groups: cumulates (Mg# = 51.61–58.94) and isotropic basaltic liquids (Mg# = 24.54–42.66). In all samples, the chondrite-normalized REE patterns show enrichment of light REEs with variable (La/Yb)_N ratios ranging from 2.48 to 9.00, which confirm their amalgamated OIB-like and E-MORB-like signatures. Enrichment in large-ion lithophile elements and depletion in high field strength elements (HFSE) relative to the primitive mantle further support this interpretation. No samples point to crustal contamination, all having undergone fractionation of olivine + clinopyroxene + plagioclase. Nevertheless, elemental data suggest that the substantial variations in (La/Sm)_PM and Zr/Nb ratios can be explained by variable degrees of partial melting rather than fractional crystallization from a common parental magma. The high (Nb/Yb)_PM ratio in the alkaline mafic rocks points to the mixing of magmas from enriched and depleted mantle sources. Abundant OIB alkaline basalts and rare E-MORB appear to be linked to the drifting stage on the northern passive margin of the Neotethys Ocean.  相似文献   

Evaluating igneous sources of the Taveyannaz formation in the Central Alps by detrital zircon U–Pb age dating and geochemistry     

Gang Lu  Wilfried Winkler  Meinert Rahn  Albrecht von Quadt  Sean D. Willett 《Swiss Journal of Geoscience》2018,111(3):399-416

Late Palaeogene syn-tectonic volcanic products have been found in the Northern Alpine foreland basin and in the South Alpine hemipelagic basin. The source of abundant volcanic fragments is still in debate. We analyzed the geochronology and geochemistry of detrital zircons, and evaluated their temporal and genetic relationships with potential volcanic sources. The study shows that the detrital zircon U–Pb age patterns have two major age groups: a dominance (ca. 90%) of pre-Alpine zircons was found, as commonly observed in other Alpine flysch formations. These zircons apparently derived from erosion of the early Alpine nappe stack in South Alpine and Austroalpine units. Furthermore, a few Neo-Alpine zircons (ca. 10%) have ages ranging from Late Eocene to Early Oligocene (~ 41–29 Ma). Both source materials were mixed during long riverine transport to the basin margins before being re-deposited by gravity flows. These Palaeogene ages match with the activity of Peri-Adriatic magmatism, including the Biella volcanic suite as well as the Northern Adamello and Bergell intrusions. The values of REE and ¹⁷⁶Hf/¹⁷⁷Hf_(t) ratios of the Alpine detrital zircons are in line with the magmatic signatures. We observe an in time and space variable supply of syn-sedimentary zircons. From late Middle Eocene to Late Eocene, basin influx into the South Alpine and Glarus (A) basins from the Northern Adamello source is documented. At about 34 Ma, a complete reorganisation is recorded by (1) input of Bergell sources into the later Glarus (B) basin, and (2) the coeval volcaniclastic supply of the Haute-Savoie basin from the Biella magmatic system. The Adamello source vanished in the foreland basin. The marked modification of the basin sources at ~ 34 Ma is interpreted to be initiated by a northwestern shift of the early Alpine drainage divide into the position of the modern Insubric Line.  相似文献   

An experimental study of Fe–Ni exchange between sulfide melt and olivine at upper mantle conditions: implications for mantle sulfide compositions and phase equilibria     

Zhou?ZhangEmail authorView author&#;s OrcID profile  Anette?von der Handt  Marc?M.?Hirschmann 《Contributions to Mineralogy and Petrology》2018,173(3):19

The behavior of nickel in the Earth’s mantle is controlled by sulfide melt–olivine reaction. Prior to this study, experiments were carried out at low pressures with narrow range of Ni/Fe in sulfide melt. As the mantle becomes more reduced with depth, experiments at comparable conditions provide an assessment of the effect of pressure at low-oxygen fugacity conditions. In this study, we constrain the Fe–Ni composition of molten sulfide in the Earth’s upper mantle via sulfide melt–olivine reaction experiments at 2 GPa, 1200 and 1400 °C, with sulfide melt \(X_{{{\text{Ni}}}}^{{{\text{Sulfide}}}}=\frac{{{\text{Ni}}}}{{{\text{Ni}}+{\text{Fe}}}}\) (atomic ratio) ranging from 0 to 0.94. To verify the approach to equilibrium and to explore the effect of \({f_{{{\text{O}}_{\text{2}}}}}\) on Fe–Ni exchange between phases, four different suites of experiments were conducted, varying in their experimental geometry and initial composition. Effects of Ni secondary fluorescence on olivine analyses were corrected using the PENELOPE algorithm (Baró et al., Nucl Instrum Methods Phys Res B 100:31–46, 1995), “zero time” experiments, and measurements before and after dissolution of surrounding sulfides. Oxygen fugacities in the experiments, estimated from the measured O contents of sulfide melts and from the compositions of coexisting olivines, were 3.0?±?1.0 log units more reduced than the fayalite–magnetite-quartz (FMQ) buffer (suite 1, 2 and 3), and FMQ ??1 or more oxidized (suite 4). For the reduced (suites 1–3) experiments, Fe–Ni distribution coefficients \(K_{{\text{D}}}^{{}}=\frac{{(X_{{{\text{Ni}}}}^{{{\text{sulfide}}}}/X_{{{\text{Fe}}}}^{{{\text{sulfide}}}})}}{{(X_{{{\text{Ni}}}}^{{{\text{olivine}}}}/X_{{{\text{Fe}}}}^{{{\text{olivine}}}})}}\) are small, averaging 10.0?±?5.7, with little variation as a function of total Ni content. More oxidized experiments (suite 4) give larger values of K_D (21.1–25.2). Compared to previous determinations at 100 kPa, values of K_D from this study are chiefly lower, in large part owing to the more reduced conditions of the experiments. The observed difference does not seem attributable to differences in temperature and pressure between experimental studies. It may be related in part to the effects of metal/sulfur ratio in sulfide melt. Application of these results to the composition of molten sulfide in peridotite indicates that compositions are intermediate in composition (\(X_{{{\text{Ni}}}}^{{{\text{sulfide}}}}\)?~?0.4–0.6) in the shallow mantle at 50 km, becomes more Ni rich with depth as the O content of the melt diminishes, reaching a maximum (0.6–0.7) at depths near 80–120 km, and then becomes more Fe rich in the deeper mantle where conditions are more reduced, approaching (\(X_{{{\text{Ni}}}}^{{{\text{sulfide}}}}\)?~?0.28)?>?140 km depth. Because Ni-rich sulfide in the shallow upper mantle melts at lower temperature than more Fe-rich compositions, mantle sulfide is likely molten in much of the deep continental lithosphere, including regions of diamond formation.  相似文献   

Biogenic and lithogenic magnetic minerals in Atlantic and Pacific deep sea sediments and their paleomagnetic significance     

H. Vali  T. von Dobeneck  G. Amarantidis  O. Förster  G. Morteani  L. Bachmann  N. Petersen 《International Journal of Earth Sciences》1989,78(3):753-764

The carrier of the natural magnetization of deep sea sediments was characterized by mineralogical, electron microscopic, and rock magnetic investigations. Magnetic single domain (SD) and pseudo single domain (PSD) particles which are most important for the stable remanent magnetization were separated from the magnetic »coarse fraction« and concentrated as magnetic »fine fraction«. The magnetic coarse fraction consists of lithogenic magnetite and titanomagnetite, which often contains exsolution-lamellae of ilmenite. Both minerals are partially maghematized and occur isolated in the sediment or embedded in rock particles, in regionally different concentrations. The magnetic fine fraction consists of lithogenic magnetite and titanomagnetite and biogenic magnetite (magnetofossils = fossil bacterial magnetosomes), the latter generally maghematized.A graphical method is described which allows the classification and characterization of the magnetic fine fraction by demagnetization of the anhysteretic remanent magnetization (ARM) of whole sediment samples. Three groups with different magnetic properties can be distinguished, characterized by three ARM type-curves: Type A curves are associated with sediments from abyssal plaines. They show nearly identical ARM properties and are typical for magnetofossils.Type B curves are produced by sediments from the vicinity of volcanic regions. Their shapes are variable to a certain degree and indicate two lithogenic magnetic phases.Type C curves are found for sediments from submarine ridges and regions with input of terrigenous detritus. These curves have the largest deviations among each other indicating a magnetic multi-phase assemblage including magnetofossils.

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Zusammenfassung Die Träger der Magnetisierung von Tiefseesedimenten wurden mineralogisch, elektronenmikroskopisch und gesteinsmagnetisch untersucht. Magnetische Eindomänen (SD) und Pseudo-Eindomänen (PSD) Partikel, die für eine stabile remanente Magnetisierung wichtig sind, wurden als magnetische »Feinfraktion« von der magnetischen »Grobfraktion« abgetrennt. Die magnetische Grobfraktion besteht aus lithogenem Titanomagnetit und Magnetit die teilweise maghemitisiert sind und teilweise auch Ilmenit-Entmischungslamellen aufweisen. In regional unterschiedlichen Konzentrationen liegen sie frei im Sediment oder in silikatischer Matrix eingebettet vor. Die magnetische Feinfraktion besteht sowohl aus lithogenem Titanomagnetit und Magnetit, als auch aus biogenem Magnetit (Magnetofossilien = fossile bakterielle Magnetosomen); letzterer ist größtenteils maghemitisiert.Es wird eine grafische Darstellungsmethode beschrieben, die anhand von Untersuchungen der anhysteretischen remanenten Magnetisierung (ARM) von Sedimentproben eine Charakterisierung der magnetischen Feinfraktion erlaubt. Es lassen sich dadurch drei Gruppen mit unterschiedlichen magnetischen Eigenschaften unterscheiden, die durch drei Gruppen von ARM-Kurventypen charakterisiert sind.Kurventyp A wird bei Sedimenten aus Tiefsee-Ebenen beobachtet. Die ARM-Daten sind nahezu identisch und zeigen ein Verhalten, wie es für Magnetofossilien typisch ist. Kurventyp B tritt bei Sedimenten aus dem Einzugsbereich vulkanischer Gebiete auf. Er zeigt eine größere Variation und die Form der Kurven spricht für ein System aus zwei lithogenen magnetischen Komponenten.Kurventyp C gehört zu Sedimenten aus submarinen Rücken und dem Einzugsgebiet terrigener Schüttungen. Die Kurvenverläufe sind uneinheitlich und sprechen für ein magnetisches Mehrkomponenten-System mit Beteiligung von Magnetofossilien.

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Résumé Les minéraux porteurs du magnétisme dans les sédiments de mer profonde ont été explorés par les méthodes de la minéralogie, de la microscopie électronique et du magnétisme des roches. Les particules qui correspondent à un domaine magnétique unique (SD) et pseudo-unique (PSD), significatives pour un magnétisme rénanent stable, ont été concentrées comme «fraction magnétique fine» après séparation de la «fraction magnétique grossière». Cette dernière consiste en magnétite et titanomagnétite lithogéniques, qui renferment souvent des lamelles d'exsolution d'ilménite. Ces deux minéraux sont partiellement maghémitisés; ils se présentent isolés ou inclus dans des fragments de roches, avec des concentrations régionales diverses. La fraction magnétique fine consiste en magnétite et titanomagnétite lithogéniques, ainsi qu'en magnétite biogénique (magnétofossile = magnétosome fossile bactérien), cette dernière ordinairement maghemitisée.Les auteurs présentent une méthode graphique qui permet de caractériser la fraction magnétique fine à partir de l'examen du magnétisme rémanent anhystérique (ARM) de l'échantillon de sédiment. Cette méthode permet de distinguer trois groupes de propriétés magnétiques différentes, caractérisés par trois types de courbes ARM. Les courbes de type A caractérisent les sédiments de plaines abyssales; elles montrent des propriétés ARM presque identiques et sont typiques pour les magnétofossiles. Les courbes de types B sont fournies par les sédiments voisins des régions volcaniques; leurs formes varient dans une certaine mesure et indiquent un système à deux composants magnétiques lithogéniques. Les courbes de type C correspondent aux sédiments des crêtes sous-marines et des régions à apports terrigènes; ces courbes présentent entre elles des différences plus marquées, ce qui indique un système magnétique à composants multiples, comportant des magnétofossiles.

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Dynamic response of 2D and 3D block foundations on a halfspace with inclusions     

H. Antes  O. von Estorff 《Soil Dynamics and Earthquake Engineering》1994,13(5)

The present study aims to demonstrate how the dynamic behaviour of structures is affected by local inhomogeneities inside the soil. Particularly, the influence of block-shaped elastic inclusions directly beneath a vertically vibrating block foundation is considered. Comparisons between a 2D and a 3D modelling of the soil—structure system are made. It can be observed that, depending on the stiffness of the inclusion and especially on the excitation frequency, the dynamic response of the foundation may either increase or decrease.  相似文献