164 research outputs found

    SARNET benchmark on QUENCH-11. Final report

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    In den QUENCH-Versuchen wird der Wasserstoffquellterm bei der Einspeisung von Notkühlwasser in einen trockenen, überhitzten Reaktorkern eines Leichtwasserreaktors untersucht. Ferner wird in den Versuchen das Verhalten von überhitzten Brennelementen unter verschiedenen Flutbedingungen untersucht, eine Datenbasis zur Modellentwicklung und eine Weiterentwicklung von Rechenprogrammen zu Schweren Störfällen (engl. SFD – Severe Fuel Damage) erstellt. Der Ausdampf-Versuch QUENCH-11 wurde am 8. Dezember 2005 durchgeführt. Es war das zweite Experiment im Rahmen des EU-geförderten LACOMERA-Programms. Es sollte einen Kühlmittelpumpenausfall während eines Kühlmittelverluststörfalls (hier ein sog. Small Break LOCA) oder einer plötzlichen Stromabschaltung (eng. „station blackout“) mit einer späten Druckentlastung des Primärsystems simulieren. Verbunden mit dem Unfallszenario ist das Ausdampfen eines teilgefüllten Reaktorkerns bzw. des Versuchsbündels. Das Ziel war die Untersuchung des Bündelverhaltens während des Ausdampfens und des nachfolgenden Abschreckens mit reduzierter Wassereinspeiserate. Es war das erste Experiment, in dem der gesamte Unfallablauf von der Ausdampfphase bis zur verzögerten Flutung des Bündels bei einer geringen Wasser-Einspeiserate untersucht werden sollte. Das Ausmaß der Wechselwirkungen von Thermalhydraulik und Materialien war in dem Experiment ausgeprägter als in früheren QUENCH-Versuchen. Das Experiment wurde von INRNE Sofia (Bulgarische Akademie der Wissenschaften) vorgeschlagen und zusammen mit dem Forschungszentrum Karlsruhe definiert. Nach dem Experiment wurde entschieden, die QUENCH-11-Daten für ein Rechenprogramm-Benchmark, bei dem die Rechenergebnisse mit den experimentellen Daten verglichen werden, im Rahmen des Europäischen Exzellenz-Netzwerks SARNET anzubieten, um die Zuverlässigkeit der Rechnungen für die verschiedenen Phasen von Unfall bzw. Experiment zu überprüfen. Die eingesetzten SFD-Rechenprogramme waren ASTEC, ATHLET-CD, ICARE-CATHARE, MELCOR, RATEG/SVECHA, RELAP/SCDAPSIM, und SCDAP/RELAP5. Die Koordination für den Vergleich übernahm INRNE. Als Grundlage für den Vergleich dienten die zeitlichen Verläufe von Temperaturen, Wasserstofferzeugung und anderer wichtiger Daten. Außerdem wurden Axialprofile, in erster Linie die der Temperatur zum Zeitpunkt des Flutbeginns und des Endstadiums, d. h. bei der Testzeit von 7000 s, verglichen. Für die meisten Rechenergebnisse kann ein gemeinsamer Trendverlauf angegeben werden. Größere Unterschiede zeigen die Ergebnisse für die Wasserstofferzeugung und die zugehörige Oxidschichtdicke. Der Grad der Übereinstimmung zwischen Rechnung und Experiment wird von den Schwachstellen der Rechnung und des Experiments gleichermaßen mitbestimmt. SFD-Rechenprogramme sind zur Analyse von typischen Kernreaktorunfällen entwickelt worden. Einzelne Besonderheiten der experimentellen Anordnung integraler Experimente (wie auch QUENCH-11) sind bedingt durch das Vorhandensein von Dampfführungsrohr (Shroud) und Elektrodenmaterial für die elektrische Stabheizung nicht reaktortypisch und können daher nicht in der gewünschten Einzelheit im Rechenprogramm nachgebildet werden. Hinzu kommen Effekte durch den Anwender. Da jedoch die Bandbreite der wesentlichen Rechenergebnisse einschließlich der Wasserstofferzeugung nicht extrem groß ist, kann das Ergebnis des SFD-Rechenprogramm-Benchmarks insgesamt als positiv bewertet werden. Ein Vergleich mit anderen Experimenten zeigt einen weiteren Bedarf an Verbesserungen besonders im Hinblick auf die Oxidation stark zerstörter Bündelstrukturen während des Flutens. Zusätzlich erwies sich das Rechenprogramm-Benchmark für einige Programmanwender als wertvoll, um sich mit den physikalischen Problematiken und der Anwendung von großen SFD-Rechenprogrammen vertraut zu machen. Es dient dem Erfahrungsaustausch mit jüngeren Wissenschaftlern und Ingenieuren und der Aufrechterhaltung des Standards der nuklearen Sicherheit

    CoreSOAR Core Degradation State-of-the Art Report Update: Conclusions [in press]

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    In 1991 the CSNI published the first State-of-the-Art Report on In-Vessel Core Degradation, which was updated to 1995 under the EC 3rd Framework programme. These covered phenomena, experimental programmes, material data, main modelling codes, code assessments, identification of modelling needs, and conclusions including the needs for further research. This knowledge was fundamental to such safety issues as in-vessel melt retention of the core, recovery of the core by water reflood, hydrogen generation and fission product release. In the last 20 years, there has been much progress in understanding, with major experimental series finished, e.g. the integral in-reactor Phébus FP tests, while others have many tests completed, e.g. the electrically-heated QUENCH series on reflooding degraded rod bundles, and one test using a debris bed. The small-scale PRELUDE/PEARL experiments study debris bed quench, while LIVE examines melt pool behaviour in the lower head using simulant materials. The integral severe accident modelling codes, such as MELCOR and MAAP (USA) and ASTEC (Europe), encapsulate current knowledge in a quantitative way. After two EC-funded projects on the SARNET network of excellence, continued in NUGENIA, it is timely to take stock of the vast range of knowledge and technical improvements gained in the experimental and modelling areas. The CoreSOAR project, in NUGENIA/SARNET, drew together the experience of 11 European partners to update the state of the art in core degradation, finishing at the end of 2018. The review covered knowledge of phenomena, available integral experiments, separate-effects data, modelling codes and code validation, then drawing overall conclusions and identifying needs for further research. The final report serves as a reference for current and future research programmes concerning core degradation in NUGENIA, in other EC research projects such as in Horizon2020 and for projects under the auspices of OECD/NEA/CSNI

    Technical Design Report EuroGammaS proposal for the ELI-NP Gamma beam System

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    The machine described in this document is an advanced Source of up to 20 MeV Gamma Rays based on Compton back-scattering, i.e. collision of an intense high power laser beam and a high brightness electron beam with maximum kinetic energy of about 720 MeV. Fully equipped with collimation and characterization systems, in order to generate, form and fully measure the physical characteristics of the produced Gamma Ray beam. The quality, i.e. phase space density, of the two colliding beams will be such that the emitted Gamma ray beam is characterized by energy tunability, spectral density, bandwidth, polarization, divergence and brilliance compatible with the requested performances of the ELI-NP user facility, to be built in Romania as the Nuclear Physics oriented Pillar of the European Extreme Light Infrastructure. This document illustrates the Technical Design finally produced by the EuroGammaS Collaboration, after a thorough investigation of the machine expected performances within the constraints imposed by the ELI-NP tender for the Gamma Beam System (ELI-NP-GBS), in terms of available budget, deadlines for machine completion and performance achievement, compatibility with lay-out and characteristics of the planned civil engineering

    Whole genome sequence and manual annotation of Clostridium autoethanogenum, an industrially relevant bacterium

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    Clostridium autoethanogenum is an acetogenic bacterium capable of producing high value commodity chemicals and biofuels from the C1 gases present in synthesis gas. This common industrial waste gas can act as the sole energy and carbon source for the bacterium that converts the low value gaseous components into cellular building blocks and industrially relevant products via the action of the reductive acetyl-CoA (Wood-Ljungdahl) pathway. Current research efforts are focused on the enhancement and extension of product formation in this organism via synthetic biology approaches. However, crucial to metabolic modelling and directed pathway engineering is a reliable and comprehensively annotated genome sequence

    A global database of dissolved organic matter (DOM) concentration measurements in coastal waters (CoastDOM v1)

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    Measurements of dissolved organic carbon (DOC), nitrogen (DON), and phosphorus (DOP) con-centrations are used to characterize the dissolved organic matter (DOM) pool and are important components ofbiogeochemical cycling in the coastal ocean. Here, we present the first edition of a global database (CoastDOMv1; available at https://doi.org/10.1594/PANGAEA.964012, L\uf8nborg et al., 2023) compiling previously pub-lished and unpublished measurements of DOC, DON, and DOP in coastal waters. These data are complementedby hydrographic data such as temperature and salinity and, to the extent possible, other biogeochemical variables(e.g. chlorophyll a, inorganic nutrients) and the inorganic carbon system (e.g. dissolved inorganic carbon andtotal alkalinity). Overall, CoastDOM v1 includes observations of concentrations from all continents. However,most data were collected in the Northern Hemisphere, with a clear gap in DOM measurements from the SouthernHemisphere. The data included were collected from 1978 to 2022 and consist of 62 338 data points for DOC,20 356 for DON, and 13 533 for DOP. The number of measurements decreases progressively in the sequenceDOC > DON > DOP, reflecting both differences in the maturity of the analytical methods and the greater focuson carbon cycling by the aquatic science community. The global database shows that the average DOC concen-tration in coastal waters (average \ub1 standard deviation (SD): 182 \ub1 314 μmol C L−1; median: 103 μmol C L−1) is13-fold higher than the average coastal DON concentration (13.6 \ub1 30.4 μmol N L−1; median: 8.0 μmol N L−1),which is itself 39-fold higher than the average coastal DOP concentration (0.34 \ub1 1.11 μmol P L−1; median:0.18 μmol P L−1). This dataset will be useful for identifying global spatial and temporal patterns in DOM and willhelp facilitate the reuse of DOC, DON, and DOP data in studies aimed at better characterizing local biogeochem-ical processes; closing nutrient budgets; estimating carbon, nitrogen, and phosphorous pools; and establishing abaseline for modelling future changes in coastal waters

    Uniform Selection as a Primary Force Reducing Population Genetic Differentiation of Cavitation Resistance across a Species Range

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    Background: Cavitation resistance to water stress-induced embolism determines plant survival during drought. This adaptive trait has been described as highly variable in a wide range of tree species, but little is known about the extent of genetic and phenotypic variability within species. This information is essential to our understanding of the evolutionary forces that have shaped this trait, and for evaluation of its inclusion in breeding programs. Methodology: We assessed cavitation resistance (P 50), growth and carbon isotope composition in six Pinus pinaster populations in a provenance and progeny trial. We estimated the heritability of cavitation resistance and compared the distribution of neutral markers (FST) and quantitative genetic differentiation (QST), for retrospective identification of the evolutionary forces acting on these traits. Results/Discussion: In contrast to growth and carbon isotope composition, no population differentiation was found for cavitation resistance. Heritability was higher than for the other traits, with a low additive genetic variance (h 2 ns = 0.4360.18, CVA = 4.4%). QST was significantly lower than FST, indicating uniform selection for P50, rather than genetic drift. Putativ

    Short-Lived Trace Gases in the Surface Ocean and the Atmosphere

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    The two-way exchange of trace gases between the ocean and the atmosphere is important for both the chemistry and physics of the atmosphere and the biogeochemistry of the oceans, including the global cycling of elements. Here we review these exchanges and their importance for a range of gases whose lifetimes are generally short compared to the main greenhouse gases and which are, in most cases, more reactive than them. Gases considered include sulphur and related compounds, organohalogens, non-methane hydrocarbons, ozone, ammonia and related compounds, hydrogen and carbon monoxide. Finally, we stress the interactivity of the system, the importance of process understanding for modeling, the need for more extensive field measurements and their better seasonal coverage, the importance of inter-calibration exercises and finally the need to show the importance of air-sea exchanges for global cycling and how the field fits into the broader context of Earth System Science

    Ocean carbon from space: Current status and priorities for the next decade

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    This is the final version. Available on open access from Elsevier via the DOI in this recordData availability: Data for Fig. 1a were generated from a free Scopus (https://www.scopus.com/) search of the terms "Ocean carbon satellite" (using All fields) in March 2022. Data from Fig. 1b and 1c were generated from the workshop registration and are available within the figure (participation number, geographical representation and gender split).The ocean plays a central role in modulating the Earth’s carbon cycle. Monitoring how the ocean carbon cycle is changing is fundamental to managing climate change. Satellite remote sensing is currently our best tool for viewing the ocean surface globally and systematically, at high spatial and temporal resolutions, and the past few decades have seen an exponential growth in studies utilising satellite data for ocean carbon research. Satellite-based observations must be combined with in-situ observations and models, to obtain a comprehensive view of ocean carbon pools and fluxes. To help prioritise future research in this area, a workshop was organised that assembled leading experts working on the topic, from around the world, including remote-sensing scientists, field scientists and modellers, with the goal to articulate a collective view of the current status of ocean carbon research, identify gaps in knowledge, and formulate a scientific roadmap for the next decade, with an emphasis on evaluating where satellite remote sensing may contribute. A total of 449 scientists and stakeholders participated (with balanced gender representation), from North and South America, Europe, Asia, Africa, and Oceania. Sessions targeted both inorganic and organic pools of carbon in the ocean, in both dissolved and particulate form, as well as major fluxes of carbon between reservoirs (e.g., primary production) and at interfaces (e.g., air-sea and land–ocean). Extreme events, blue carbon and carbon budgeting were also key topics discussed. Emerging priorities identified include: expanding the networks and quality of in-situ observations; improved satellite retrievals; improved uncertainty quantification; improved understanding of vertical distributions; integration with models; improved techniques to bridge spatial and temporal scales of the different data sources; and improved fundamental understanding of the ocean carbon cycle, and of the interactions among pools of carbon and light. We also report on priorities for the specific pools and fluxes studied, and highlight issues and concerns that arose during discussions, such as the need to consider the environmental impact of satellites or space activities; the role satellites can play in monitoring ocean carbon dioxide removal approaches; economic valuation of the satellite based information; to consider how satellites can contribute to monitoring cycles of other important climatically-relevant compounds and elements; to promote diversity and inclusivity in ocean carbon research; to bring together communities working on different aspects of planetary carbon; maximising use of international bodies; to follow an open science approach; to explore new and innovative ways to remotely monitor ocean carbon; and to harness quantum computing. Overall, this paper provides a comprehensive scientific roadmap for the next decade on how satellite remote sensing could help monitor the ocean carbon cycle, and its links to the other domains, such as terrestrial and atmosphere.European Space AgencySimons FoundationUK National Centre for Earth Observation (NCEO)UKRIAtlantic Meridional Transect ProgrammeSwiss National Science Foundatio
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