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  • 1
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Earth and Planetary Science Letters 126 (1994), S. 15-22 
    ISSN: 0012-821X
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Geosciences , Physics
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Mineralogy and petrology 53 (1995), S. 1-26 
    ISSN: 1438-1168
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Description / Table of Contents: Zusammenfassung Al-reiche Spinelle (100Cr/(Cr + Al) 〈 5, Al2O3 〉 50 Gew.%) sind in alpinen Peridotiten, in terrestrischen und lunaren mafischen und ultramafischen Kumulaten und in manchen metamorphen Gesteinen weit verbreitet, aber sie scheinen in terrestrischen, vulkanischen Gesteinen selten zu sein. Wir beschreiben hier das Vorkommen von Al-reichen Spinell-Inklusionen in Olivinkristallen von Inselbogen-Vulkaniten von 5 neuen Lokalitäten: Bukit Mapas (Sumatra) und Ost-Bali im Sunda-Bogen und die Inseln Epi, Merelava und Ambrym im Vanuatu-Bogen. Relativ Cr-reiche Spinelle kommen häufiger auch als Einschlüsse in denselben Olivin-Kristallen vor, und es scheint, daß Chrom-arme Aluminiumspinelle im Ungleichgewicht mit ihren basaltischen Mutterschmelzen stehen. In den untersuchten Gesteinen kommen Al-reiche Spinelle zusammen mit Silikatgläsern und Aluminium-reichen Klinopyroxenen in Schmelzeinschlüssen in Olivinen vor. Diese Assoziation weist auf einen Ursprung hin, der Kontamination durch lokalisierte Al-reiche “pockets” von Schmelze involviert; dies steht im Gegensatz zu einem Ursprung als Xenokristalle. Wir schlagen zwei Mechanismen vor, die diese Aluminium-reiche Schmelze in basaltischen Magmakammern erzeugen können: (1) lokalisierte Produktion von Aluminium-reicher Schmelze durch vollkommene Auflösung von assimilierten gabbroischen Gesteinen aus der unteren Kruste. In diesem Modell kann die Aluminium-reiche Schmelze Al-reiche Spinelle kristallisieren, die dann anschließend als feste Einschlüsse von Phenokristallen in der basaltischen Mutterschmelze eingefangen werden oder als Schmelzeinschlüsse, in denen Al-reiche Spinelle und Al-reiche Klinopyroxene als Tochterphasen kristallisieren. (2) Inkongruenter Zerfall von Amphibol in Amphibol-reichen Kumulaten in Magmakammern unter Inselbögen oder unter OIB-Vulkanen. Die letztgenannte Reaktion erzeugt eine Schmelze mit ungefähr 20–22% Al2O3, Aluminium-haltigen Klinopyroxen, Al-reichen Spinell und Olivin. Mischung zwischen diesen Produkten des Zerfalls von Amphibol und basaltischer Mutterschmelze kann während der ganzen Evolution eines magmatischen Systems stattfinden, aber besonders während der Zufuhr neuer heißer Magnesium-reicher Basalte. Aluminium-haltige Spinelle und Klinopyroxene, die während des Zerfalls von Amphibol entstanden sind oder vielleicht aus einer Aluminium-haltigen Schmelze in derselben Reaktion produziert wurden, werden während der Neuzufuhr in das Magma inkorporiert und im Anschluß daran, zusammen mit den koexistierenden Cr-Spinellen, von kristallisierendem Olivin und Klinopyroxen eingefangen.
    Notes: Summary Al-rich spinels (100Cr/(Cr + Al) 〈 5, Al2O3 〉 50 wt%) are common in alpine peridotites, both terrestrial and lunar mafic and ultramafic cumulates, and in certain metamorphic rocks, but they are apparently rare in terrestrial volcanic rocks. Here we describe the occurrence of Al-rich spinel inclusions in olivine phenocrysts in island arc volcanic rocks from five new localities: Bukit Mapas (Sumatra) and eastern Bali in the Sunda arc, and Epi, Merelava, and Ambrym islands in the Vanuatu arc. More commonly, relatively Cr-rich spinels also occur as inclusions in the saine olivine phenocrysts, and it appears that the Cr-poor aluminous spinels must be in disequilibrium with the host basaltic melts. In the rocks studied, Al-rich spinels also coexist with trapped silicate glasses and highly aluminous clinopyroxene in melt inclusions in olivine. This paragenesis suggests an origin involving contamination by localized Al-rich melt pockets as opposed to a xenocrystic origin. Two mechanisms to produce this high-Al melt in basaltic magma chambers are suggested: (1) localized high-Al melt production by complete breakdown of assimilated lower crustal gabbroic rocks. In this model the high-Al melt may crystallise Al-rich spinels which are subsequently trapped as solid inclusions by phenocryst phases of the host basaltic melt or may be trapped as melt inclusions in which Al-rich spinels and Al-rich clinopyroxene crystallise as daughter phases, and (2) in congruent breakdown of amphibole in amphibole-rich cumulates in sub-arc, or sub-OIB volcano magma chambers. The latter reaction produces a melt with ∼ 20–22% of Al2O3, aluminous clinopyroxene, Al-rich spinel and olivine. Mixing between these amphibole breakdown products and host basaltic melt may occur throughout the evolution of a magmatic system, but particularly during recharge with hot magnesian basalt batches. Aluminous spinels and aluminous clinopyroxene produced during amphibole breakdown, or perhaps crystallised from aluminous melt produced in the saine reaction, are incorporated into the magma during recharge, and subsequently trapped, together with the coexisting Cr-spinels, by crystallising olivine and clinopyroxene.
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Environmental geology 39 (2000), S. 963-976 
    ISSN: 1432-0495
    Keywords: Key words Larsemann Hills ; Antarctica ; Trace metals ; Water geochemistry ; Anthropogenic contamination
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Notes: Abstract Fresh water lakes are found in basement rock basins in the Larsemann Hills, East Antarctica, during the summer months. These lakes constitute a relatively simple natural laboratory to investigate the effects of recent and well-documented anthropogenic impact on a “pristine” environment. Larsemann Hills freshwaters have extremely low salinity (typically 〈1‰), and contain very low concentrations of trace elements of environmental significance such as Pb, U, and Zn. Typical Pb concentrations range from less than 5 ppt to 250 ppt. Although trace metal concentrations appear to be higher in lakes situated in the vicinity of stations, they are consistently lower (by several orders of magnitude, for some elements) than Standard International Drinking Water Guidelines. The chemistry of the lake waters is dominated by sea-spray input. Consequently, it is primarily a function of geographical factors, such as distance from the shore and exposure to winds. Shallow-level groundwater and surface water also contribute to the lake chemistry. No evidence was found for contamination from global air circulation. Although contamination resulting from activities at the research stations is generally near or below detection levels, very low levels of trace metal anthropogenic contamination were found in the vicinity of some research stations.
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  • 4
    Electronic Resource
    Electronic Resource
    Springer
    Mineralogy and petrology 64 (1998), S. 89-117 
    ISSN: 1438-1168
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Description / Table of Contents: Zusammenfassung Neue geochemische und Sr-, Nd-, und Pb-Isotopenanalysen von quartären und kretazischen Sedimenten des nordöstlichen Indischen Ozeans werden dazu herangezogen, um die Zusammensetzung des entlang des Sunda-Tiefseegrabens subduzierten Sedimentmaterials und die Effekte von Krustenassimilation versus Subduktionsbedingtem Sedimenteintrag in die quartären Vulkanite des westlichen Sundabogens zu evaluieren. Zwei sedimentäre Endglieder wurden identifiziert: eine silikatischklastische (SS) und eine karbonatisch-organische (CS) Komponente, letztere kann als durch organisches Material, insbesondere durch CaCO3. stark verdünnte SS-Komponenete betrachtet werden. Silikatisch-klastische Sedimente sind durch eine Komponente charakterisiert, die isotopisch und geochemisch ähnlich der „typischen” durchschnittlichen Oberkruste ist. Daher erlauben LILE und LREE Konzentrationen, LILE/LILE und LILE/LREE Werte, sowie Sr-, Nd-, und Pb-Isotopenverhältnisse von Vulkaniten des West-Sundabogens keine einfache Unterscheidung zwischen Assimilation von Krustenmaterial durch aufsteigende Magmen und Kontamination ihrer Mantelquelle durch Sedimente. Post-miozäne silikatisch-klastische Sedimentproben, die in der Nähe des Sunda-Bogens genommen wurden, stammen großteils selbst vom Inselbogen und sollten daher nicht für eine Abschätzung des Ausmasses der Sedimentkontamination im indonesischen Vulkanbogens verwendet werden. Ferner gibt es geophysikalische Evidenz, die eher für Akkretion als Subduktion dieser Sedimente spricht und auch die10Be Isotopendaten zeigen, daß post-miozäne Sedimente nicht vom derzeitigen Vulkanismus rezykliert werden. Da die am geringsten kontaminierten Vulkanite im Ostabschnitt des Sunda-Bogens, von wo der höchste Sediment-Flux berechnet worden ist, zu finden sind, scheint die Subduktion prämiozäner Sedimente des nordöstlichen Indischen Ozeans oder die Beteiligung von aus diesen in die Quelle der Vulkanite Westsundas freigesetzten Fluiden, nicht auszureichen, um den Streubereich und die räumliche Verteilung von Sr-, Nd-, und Pb-Isotopenwerten in den Vulkaniten zu reproduzieren. Im Gegensatz dazu scheint Assimilation von Krustenmaterial - bis zu 10% für die am stärksten kontaminierten Vulkanite — durch aufsteigende Schmelzen, die aus dem „Indischen Ozean-Typ” Mantelkeil stammen, die Sr-, Nd- und Pb-Isotopensystematik der Vulkanite besser zu erklären. Sie ist auch konsistent mit der Variation der Krustendicke und Zusammensetzung entlang des Vulkanbogens und mit der räumlichen Verteilung der Sr-, Nd-, und Pb-Werte in den mafischen Vulkaniten. Diese Schlußfolgerungen werden durch die niedrigen10Be, gekoppelt mit hohen B/Be Werten und durch die positive B/Be-SiO2 und B/Be-87Sr/86Sr Korrelationen in den kalk-alkalischen Sunda-Vulkaniten, untermauert.
    Notes: Summary New geochemical and Sr, Nd, and Pb isotopic analyses of Quaternary to Cretaceous sediments from the northeastern Indian Ocean are used to estimate the composition of the sedimentary material subducted along the Sunda Trench, and to evaluate the effects of crustal contamination versus subducted sediment input in the Quaternary volcanics of the west Sunda arc. Two sediment endmember components are identified: siliceousclastic (SS) and calcareous-organogenic (CS); the latter can be regarded as SS strongly diluted by organogenic material, mainly CaCO3. Siliceous-clastic sediments are characterised by a component isotopically and geochemically similar to “typical” average upper crust. Consequently, LILE and LREE concentrations, LILE/LILE and LILE/LREE values, and Sr, Nd, and Pb isotopic ratios in West Sunda arc volcanics cannot easily distinguish between assimilation of crustal material by uprising magmas and contamination of their mantle source by bulk sediments. Post-Miocene siliceousclastic sediments sampled in the vicinity of the Sunda arc are largely derived from the arc itself, and therefore should not be used to evaluate the extent of sediment contamination of Indonesian arc volcanics. In addition, geophysical evidence suggests that post-Miocene sediments are largely accreted rather than subducted, and existing10Be isotopic data imply that post-Miocene sediments are not recycled by present-day volcanism. As the least contaminated arc volcanics occur in the eastern section of the west Sunda arc, where the highest sediment fluxes have been calculated, subduction of pre-Miocene northeastern Indian Ocean sediments or incorporation of fluids released from them into the sources of west Sunda are volcanics seem unable to reproduce the range and spatial distribution of Sr, Nd, and Pb isotopic values in the arc volcanics. By contrast, assimilation of crustal material by uprising melts derived from Indian Ocean-type mantle wedge, up to a maximum of approximately 10% for the most contaminated arc volcanics, seems better able to account for the Sr, Nd, and Pb isotope systematics of the arc volcanics, and is consistent with the variations in crustal thickness and composition along the arc, and with the spatial distribution of Sr, Nd, and Ph isotope values in mafic arc volcanics. These conclusions are also supported by the low10Be coupled with high B/Be values, and by the positive B/Be-SiO2 and B/Be-87Sr/86Sr correlations in calc-alkaline Sunda arc volcanics.
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  • 5
    Publication Date: 2000-07-14
    Print ISSN: 0943-0105
    Electronic ISSN: 1432-0495
    Topics: Geosciences
    Published by Springer
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  • 6
    Publication Date: 2020-02-18
    Print ISSN: 1735-1472
    Electronic ISSN: 1735-2630
    Topics: Energy, Environment Protection, Nuclear Power Engineering
    Published by Springer
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  • 7
    Publication Date: 2012-10-11
    Print ISSN: 0722-4028
    Electronic ISSN: 1432-0975
    Topics: Biology , Geosciences
    Published by Springer
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  • 8
  • 9
    Publication Date: 2012-05-17
    Description: Antarctic snow samples collected from the Wilkins Runway, c. 50 km inland from the Windmill Islands, East Antarctica, contain aeolian-derived diatoms. The diatom assemblage preserved is exclusively of marine origin. As diatoms are excellent indicators of source conditions, we are able to confirm that an unusual weather event, with anomalous north-westerly winds blowing at around 10 m s-1, resulted in the deposition of coastal marine species at the Wilkins Runway. The composition of the floral assemblage collected indicate that the parent water mass was from a coastal marine region undergoing typical Antarctic summer conditions with periods of both consolidated sea ice and open water. On inspection of available satellite imagery, these conditions were found upwind of the deposition site. This study provides a methodology for diatoms found within ice cores to be identified and the source region to be determined. It also provides evidence for a large-scale aeolian deposition of marine diatoms to an ice sheet, which may have implications for the interpretation of controversial marine diatoms found in sediments that have been used as evidence for the retreat of the East Antarctic Ice Sheet.
    Print ISSN: 0954-1020
    Electronic ISSN: 1365-2079
    Topics: Biology , Geography , Geosciences
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  • 10
    Publication Date: 2014-06-01
    Print ISSN: 0009-2541
    Electronic ISSN: 1872-6836
    Topics: Chemistry and Pharmacology , Geosciences
    Published by Elsevier
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