966 resultados para ams facility


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IEECAS SKLLQG

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High-amplitude, rapid climate fluctuations are common features of glacial times. The prominent changes in air temperature recorded in the Greenland ice cores (Dansgaard et al., 1993, doi:10.1038/339532a0; Grootes et al., 1993 doi:10.1038/366552a0) are coherent with shifts in the magnitude of the northward heat flux carried by the North Atlantic surface ocean (Bond et al., 1993, doi:10.1038/365143a0; Bond and Lotti, 1995, doi:10.1126/science.267.5200.1005); changes in the ocean's thermohaline circulation are a key component in many explanations of this climate flickering (Broecker, 1997, doi:10.1126/science.278.5343.1582). Here we use stable-isotope and other sedimentological data to reveal specific oceanic reorganizations during these rapid climate-change events. Deep water was generated more or less continuously in the Nordic Seas during the latter part of the last glacial period (60 to 10 thousand years ago), but by two different mechanisms. The deep-water formation occurred by convection in the open ocean during warmer periods (interstadials). But during colder phases (stadials), a freshening of the surface ocean reduced or stopped open-ocean convection, and deep-water formation was instead driven by brine-release during sea-ice freezing. These shifting magnitudes and modes nested within the overall continuity of deep-water formation were probably important for the structuring and rapidity of the prevailing climate changes.

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Stable isotope data on benthic foraminifera from more than 30 cores on the northern Emperor Seamounts and in the Okhotsk Sea are synthesized in paleohydrographic profiles spanning the depth range 1000-4000 m. Holocene (core-top) benthic foraminiferal d18O and d13C data are calibrated to modern hydrographic properties through measurements of d13C of SumCO2 and d18O of seawater. Cibicidoides stable isotope ratios are close to the d13C and equilibrium d18O of seawater, whereas Uvigerina d18O and d13C are variably offset from Cibicidoides. Glacial maximum d13C of Cibicidoides displays a different vertical profile than that of the Holocene. When results are adjusted by +0.32 per mil to account for the secular change in d13C during the last glacial maximum, the data coincide with the modern seawater and foraminiferal curves deeper than ~2 km. However, at shallower depths d13C gradually increases by as much as 1 per mil above the modern value. Furthermore, above 2 km the benthic d18O decreases by ~0.5 per mil. These results are consistent with a benthic front at ~2 km in the North Pacific (see Herguera et al., 1992), but they differ from interpretations based on trace metal data which indicate a source of nutrient-depleted deep water during glaciation. The isotopic data suggest that during glaciation there was a better ventilated watermass at intermediate depths in the far northwestern Pacific, it was relatively fresher than deep waters there, and deep waters were as nutrient-rich as today.

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Cold-water corals are common along the Moroccan continental margin off Melilla in the Alboran Sea (western Mediterranean Sea), where they colonise and largely cover mound and ridge structures. Radiocarbon ages of the reef-forming coral species Lophelia pertusa and Madrepora oculata sampled from those structures, reveal that they were prolific in this area during the last glacial-interglacial transition with pronounced growth periods covering the Bølling-Allerød interstadial (13.5-12.8 ka BP) and the Early Holocene (11.3-9.8 ka BP). Their proliferation during these periods is expressed in vertical accumulation rates for an individual coral ridge of 266-419 cm ka**-1 that consists of coral fragments embedded in a hemipelagic sediment matrix. Following a period of coral absence, as noted in the records, cold-water corals re-colonised the area during the Mid-Holocene (5.4 ka BP) and underwater photographs indicate that corals currently thrive there. It appears that periods of sustained cold-water coral growth in the Melilla Coral Province were closely linked to phases of high marine productivity. The increased productivity was related to the deglacial formation of the most recent organic rich layer in the western Mediterranean Sea and to the development of modern circulation patterns in the Alboran Sea.

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An Accelerator Mass Spectrometry (AMS) 14C dated multiparameter event stratigraphy is developed for the Aegean Sea on the basis of highly resolved (centimeter to subcentimeter) multiproxy data collected from four late glacial to Holocene sediment cores. We quantify the degree of proportionality and synchroneity of sediment accumulation in these cores and use this framework to optimize the confidence levels in regional marine, radiocarbon-based chronostratigraphies. The applicability of the framework to published, lower-resolution records from the Aegean Sea is assessed. Next this is extended into the wider eastern Mediterranean, using new and previously published high-resolution data from the northern Levantine and Adriatic cores. We determine that the magnitude of uncertainties in the intercore comparison of AMS 14C datings based on planktonic foraminifera in the eastern Mediterranean is of the order of ±240 years (2 SE). These uncertainties are attributed to synsedimentary and postsedimentary processes that affect the materials dated. This study also offers a background age control that allows for vital refinements to radiocarbon-based chronostratigraphy in the eastern Mediterranean, with the potential for similar frameworks to be developed for any other well-studied region.

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As part of a wider paleoclimate and paleoceanographic study of Holocene-upper Pleistocene laminated sediments from the eastern equatorial Pacific and Peru continental margin, we completed 32 accelerator mass spectrometry (AMS) 14C dates from cores recovered during Ocean Drilling Program (ODP) Leg 201. Sample preparation and measurement were carried out at the ANTARES AMS facility, Australian Nuclear Science and Technology Organisation (ANSTO), in Sydney, Australia (Lawson et al., 2000, doi:10.1016/S0168-583X(00)00276-7; Fink et al., 2004, doi:10.1016/j.nimb.2004.04.025). Although the sediments are predominantly diatomaceous oozes (D'Hondt, Jørgensen, Miller, et al., 2003, doi:10.2973/odp.proc.ir.201.2003), they contain sufficient inorganic (e.g., foraminifer tests and nannofossil plates) and organic (Meister et al., 2005, doi:10.2973/odp.proc.sr.201.105.2005) carbon to allow 14C dating. These dates permitted us to reconstruct a history of sediment accumulation over the past 20 k.y., particularly on the Peru continental margin. In this report we present 14C AMS dates and other pertinent data from cores from Sites 1227, 1228, and 1229 collected during Leg 201 at the Peru continental margin.

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To determine the influence of fire and thermokarst in a boreal landscape, we investigated peat cores within and adjacent to a permafrost collapse feature on the Tanana River Floodplain of Interior Alaska. Radioisotope dating, diatom assemblages, plant macrofossils, charcoal fragments, and carbon and nitrogen content of the peat profile indicate ~600 years of vegetation succession with a transition from a terrestrial forest to a sedge-dominated wetland over 100 years ago, and to a Sphagnum-dominated peatland in approximately 1970. The shift from sedge to Sphagnum, and a decrease in the detrended tree-ring width index of black spruce trees adjacent to the collapse coincided with an increase in the growing season temperature record from Fairbanks. This concurrent wetland succession and reduced growth of black spruce trees indicates a step-wise ecosystem-level response to a change in regional climate. In 2001, fire was observed coincident with permafrost collapse and resulted in lateral expansion of the peatland. These observations and the peat profile suggest that future warming and/or increased fire disturbance could promote permafrost degradation, peatland expansion, and increase carbon storage across this landscape; however, the development of drought conditions could reduce the success of both black spruce and Sphagnum, and potentially decrease the long-term ecosystem carbon storage.

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Based on a radiocarbon and paleomagnetically dated sediment record from the northern Red Sea and the exceptional sensitivity of the regional changes in the oxygen isotope composition of sea water to the sea-level-dependent water exchange with the Indian Ocean, we provide a new global sea-level reconstruction spanning the last glacial period. The sea-level record has been extracted from the temperature-corrected benthic stable oxygen isotopes using coral-based sea-level data as constraints for the sea-level/oxygen isotope relationship. Although, the general features of this millennial-scale sea-level records have strong similarities to the rather symmetric and gradual Southern Hemisphere climate patterns, we observe, in constrast to previous findings, pronounced sea level rises of up to 25 m to generally correspond with Northern Hemisphere warmings as recorded in Greenland ice-core interstadial intervals whereas sea-level lowstands mostly occur during cold phases. Corroborated by CLIMBER-2 model results, the close connection of millennial-scale sea-level changes to Northern Hemisphere temperature variations indicates a primary climatic control on the mass balance of the major Northern Hemisphere ice sheets and does not require a considerable Antarctic contribution.

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The contamination of Japan after the Fukushima accident has been investigated mainly for volatile fission products, but only sparsely for actinides such as plutonium. Only small releases of actinides were estimated in Fukushima. Plutonium is still omnipresent in the environment from previous atmospheric nuclear weapons tests. We investigated soil and plants sampled at different hot spots in Japan, searching for reactor-borne plutonium using its isotopic ratio Pu-240/Pu-239. By using accelerator mass spectrometry, we clearly demonstrated the release of Pu from the Fukushima Daiichi power plant: While most samples contained only the radionuclide signature of fallout plutonium, there is at least one vegetation sample whose isotope ratio (0.381 +/- 0.046) evidences that the Pu originates from a nuclear reactor (Pu239+240 activity concentration 0.49 Bq/kg). Plutonium content and isotope ratios differ considerably even for very close sampling locations, e.g. the soil and the plants growing on it. This strong localization indicates a particulate Pu release, which is of high radiological risk if incorporated.

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Atmosphärische Aerosolpartikel haben einen Einfluss sowohl auf das Klima als auch auf die menschliche Gesundheit, wobei sowohl die Größe, als auch die chemische Zusammensetzung der Partikel maßgeblich sind. Um insbesondere die chemische Zusammensetzung der Partikel in Abhängigkeit ihrer Quellen besser zu verstehen, wurden im Rahmen dieser Arbeit massenspektrometrische Untersuchungen thermisch verdampfbarer Partikel im Submikrometerbereich durchgeführt. Hierzu wurden sowohl die Massenspektren einzelner Partikel, als auch die von Ensembles von Partikeln mit dem Aerodyne Aerosolmassenspektrometer (AMS) in mehreren Feldmesskampagnen untersucht. Für die Messung von Einzelpartikelmassenspektren wurde das AMS zunächst durch den Einbau eines optischen Partikeldetektors (light scattering probe) modifiziert und anschließend eingehend charakterisiert. Dabei wurde festgestellt, dass mit dem Gerät im Partikelgrößenbereich von etwa 400-750 nm (untere Grenze bedingt durch die Detektionseffizienz des optischen Detektors, obere Grenze durch die Transmissionseffizienz des Aerosoleinlasssystems) quantitative Einzelpartikelmessungen möglich sind. Zudem wurde die Analyse der erhaltenen Messdaten systematisiert, und durch Einsatz von Standardspektren ein Sortieralgorithmus für die Einzelpartikelmassenspektren entwickelt, der erfolgreich auf Daten von Feldmesskampagnen angewandt werden konnte. Mit diesem Sortieralgorithmus sind zudem quantitative Aussagen über die verschiedenen Partikelbestandteile möglich. Im Sommer 2009 und im Winter 2010 fanden im Großraum Paris zwei einmonatige Feldmesskampagnen statt, bei denen unter anderem der Einfluss der Abluftfahne der Megastadt auf seine Vororte untersucht wurde. Erhöhte Konzentrationen sekundär gebildeter Aerosolkomponenten (Nitrat, Sulfat, oxidiertes organisches Aerosol (OOA)) waren insbesondere beim Herantransport kontinentaler Luftmassen zu beobachten. Im Gegensatz dazu waren die beobachteten Konzentrationen der Tracer primärer Emissionen NOx, BC (black carbon) und HOA (hydrocarbonlike organic aerosol) neben der lokalen Quellstärke insbesondere durch die herrschende Windgeschwindigkeit beeinflusst. Aus dem Vergleich der Messungen an drei Stationen konnte der Einfluss der Megastadt Paris auf seine Vororte (unter Annahme gleicher lokaler Emissionen an den zwei Vorort-Stationen) zu 0,1-0,7 µg m-3 BC, 0,3-1,1 µg m-3 HOA, und 3-5 ppb NOx abgeschätzt werden. Zudem konnten für zwei Stationen aus den Ensemble- bzw. den Einzelpartikelmessungen unabhängig voneinander zwei verschiedene HOA-Typen unterschieden werden, die den Quellen „Kochen“ und „Autoabgase“ zugeordnet wurden. Der Anteil der Partikel aus den Quellen „Kochen“ bzw. „Autoabgase“ am Gesamt-HOA betrug 65,5 % und 34,5 % für die Ensemblemessungen in der Innenstadt (nahe vieler Restaurants), und für die Einzelpartikelmessungen in einem Vorort 59 % bzw. 41 % (bezogen auf die Partikelanzahl, welche hier der Masse etwa proportional ist). Die Analyse der Einzelpartikelmassenspektren erbrachte zudem neue Erkenntnisse über den Mischungszustand der Einzelpartikel. So konnte belegt werden, dass Nitrat, Sulfat und OOA intern gemischt sind, HOA-Partikel aber als externe Mischung mit diesen vorliegen. Zudem konnte anhand der Tagesgänge der Masse pro Partikel von OOA, Nitrat und Sulfat und der Anzahl der diese Substanzen enthaltenden Partikel gezeigt werden, dass der im Ensemblemodus beobachtete fehlende Tagesgang der Sulfat-Massenkonzentration wahrscheinlich durch die gegensätzlichen Effekte der Modulation der Partikelanzahlkonzentration durch die sich verändernde Mischungsschichthöhe und der variierenden Masse an Sulfat pro Partikel (mittägliche photochemische Neuproduktion und Kondensation auf existierende Partikel) erklärt werden kann. Für OOA ist eine ähnliche Erklärung des Ensemblemodus-Tagesganges jedoch nur teilweise möglich; weitere Arbeit ist daher nötig, um auch für diese Substanzklasse belastbare Aussagen aus dem Vergleich der Ensemble- und Einzelpartikelmessungen zu erhalten. Im Rahmen einer Labormesskampagne an der AIDA-Kammer in Karlsruhe wurden Ensemble- und Einzelpartikelmassenspektren von Bakterien aufgenommen. Es konnte gezeigt werden, dass es prinzipiell möglich ist, Bakterien in Außenluft mittels Einzelpartikelmessungen nachzuweisen, jedoch wahrscheinlich nur bei sehr hohen Anzahlkonzentrationen. Der Nachweis von Bakterien und anderen primären biologischen Aerosolpartikeln mit dem AMS sollte daher in weiterführenden Experimenten noch optimiert werden.

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For more than 4 years, gaseous samples of 1-50 mu g carbon have been routinely measured with the gas ion source of the small AMS (Accelerator Mass Spectrometer) facility MICADAS (Mini CArbon DAting System) at ETH Zurich. The applied measurement technique offers a simple and fast way of C-14 measurements without the need of sample graphitization. A major drawback of gaseous C-14 measurements, however, is the relatively low negative ion current, which results in longer measurement times and lower precision compared to graphitized samples. In December 2009, a new, improved Cs sputter ion source was installed at MICADAS and we began to optimize conditions for the measurement of gaseous samples. C-12(-) currents from the new ion source were improved from initially 3 to 12-15 mu A for routine measurements and the negative ion yield was increased by a factor of 2, reaching 8 on average during routine operation. Moreover, the new measurement settings enable a doubled CO2 flow, thus substantially reducing measurement times. The achieved performance allows closing the sample size gap between gaseous and solid samples and makes the gas ion source a promising tool for dating with a measurement precision of 5 parts per thousand on samples as small as 50 mu g carbon. (C) 2012 Elsevier B.V. All rights reserved.

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The challenges of maintaining a building such as the Sydney Opera House are immense and are dependent upon a vast array of information. The value of information can be enhanced by its currency, accessibility and the ability to correlate data sets (integration of information sources). A building information model correlated to various information sources related to the facility is used as definition for a digital facility model. Such a digital facility model would give transparent and an integrated access to an array of datasets and obviously would support Facility Management processes. In order to construct such a digital facility model, two state-of-the-art Information and Communication technologies are considered: an internationally standardized building information model called the Industry Foundation Classes (IFC) and a variety of advanced communication and integration technologies often referred to as the Semantic Web such as the Resource Description Framework (RDF) and the Web Ontology Language (OWL). This paper reports on some technical aspects for developing a digital facility model focusing on Sydney Opera House. The proposed digital facility model enables IFC data to participate in an ontology driven, service-oriented software environment. A proof-of-concept prototype has been developed demonstrating the usability of IFC information to collaborate with Sydney Opera House’s specific data sources using semantic web ontologies.