Search results for "NIV"

showing 10 items of 7213 documents

Seafloor expression of oceanic detachment faulting reflects gradients in mid-ocean ridge magma supply

2019

International audience; Oceanic detachment faulting is a major mode of seafloor accretion at slow and ultraslow spreading mid-ocean ridges, and is associated with dramatic changes in seafloor morphology. Detachments form expansive dome structures with corrugated surfaces known as oceanic core complexes (OCCs), and often transition to multiple regularly-spaced normal faults that form abyssal hills parallel to the spreading axis. Previous studies have attributed these changes to along-axis gradients in lithospheric strength or magma supply. However, despite the recognition that magma supply can influence fault style and seafloor morphology, the mechanics controlling the transition from oceani…

010504 meteorology & atmospheric sciences[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]Fault (geology)010502 geochemistry & geophysics01 natural sciencesGeochemistry and PetrologyLithospheremagmatismEarth and Planetary Sciences (miscellaneous)PetrologyComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciences[SDU.STU.TE]Sciences of the Universe [physics]/Earth Sciences/Tectonicsgeographyoceanic core complexesgeography.geographical_feature_categoryMid-ocean ridgeSeafloor spreadingDetachment faultnumerical modelingGeophysicsSpace and Planetary ScienceRidgeAbyssal hillMagmatismmid-ocean ridgesmarine geologyfaultingGeologyEarth and Planetary Science Letters
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Hydrostratigraphic characterization of glaciofluvial deposits underlying an infiltration basin using ground penetrating radar.

2008

14 pages; International audience; An understanding of the heterogeneity of quaternary gravelly deposits is required to predict flow and contaminant transfer through these formations. In such deposits, preferential flow paths can lead to contamination at depths greater than predicted under the assumption of a homogeneous medium. The difficulties in characterizing their complex structure with conventional methods represent an obstacle for this prediction. In this study, we developed an approach relying on the use of ground penetrating radar (GPR) for the detection of sedimentary depositional units. A genetic interpretation of the radar stratigraphy allowed us to construct a distribution model…

010504 meteorology & atmospheric sciences[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph][SDE.MCG]Environmental Sciences/Global Changes0207 environmental engineeringInfiltration basinSoil Science[PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]02 engineering and technology[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy01 natural scienceslaw.inventionSedimentary depositional environment[ SDU.STU.GP ] Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph][ PHYS.PHYS.PHYS-GEO-PH ] Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]lawRadar020701 environmental engineeringPetrologyGeomorphologyWater content0105 earth and related environmental sciences6. Clean waterInfiltration (hydrology)[ SDE.MCG ] Environmental Sciences/Global Changes[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/StratigraphyGround-penetrating radarSedimentary rockSaturation (chemistry)Geology
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Growth of stylolite teeth patterns depending on normal stress and finite compaction

2007

Abstract Stylolites are spectacular rough dissolution surfaces that are found in many rock types. They are formed during a slow irreversible deformation in sedimentary rocks and therefore participate to the dissipation of tectonic stresses in the Earth's upper crust. Despite many studies, their genesis is still debated, particularly the time scales of their formation and the relationship between this time and their morphology. We developed a new discrete simulation technique to explore the dynamic growth of the stylolite roughness, starting from an initially flat dissolution surface. We demonstrate that the typical steep stylolite teeth geometry can accurately be modelled and reproduce natu…

010504 meteorology & atmospheric sciences[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph][SDE.MCG]Environmental Sciences/Global ChangesCompactionFOS: Physical sciencesMineralogyGeometry[PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]Surface finish010502 geochemistry & geophysics01 natural sciencesPhysics::GeophysicsPhysics - GeophysicsStress (mechanics)Geochemistry and Petrology[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/GeochemistryEarth and Planetary Sciences (miscellaneous)Scaling0105 earth and related environmental sciencesElastic energyDissipation[SDE.MCG.CPE]Environmental Sciences/Global Changes/domain_sde.mcg.cpeGeophysics (physics.geo-ph)GeophysicsAmplitudeSpace and Planetary ScienceStyloliteGeologyEarth and Planetary Science Letters
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Modelling of stylolite geometries and stress scaling

2012

International audience; In this contribution we present numerical simulations of stylolite growth to decipher the effects of initial rock heterogeneity and stress on their morphology. We show that stylolite growth in a rock with a uniform grain size produces different patterns than stylolite growth in a rock with a bimodal grain size distribution. Strong pinning of large heterogeneities produce stylolite structures that are dominated by pronounced teeth, whereas a uniform grain size leads to spikes and a roughness that shows variable wavelengths. We compare the simulated stylolites with natural examples and show that the model can reproduce the real structures. In addition we show that stro…

010504 meteorology & atmospheric sciences[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]stress-gauge[SDE.MCG]Environmental Sciences/Global ChangesCompaction[SDU.STU]Sciences of the Universe [physics]/Earth Sciences[PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]Surface finishpressure solution010502 geochemistry & geophysics01 natural sciencesPhysics::Geophysics[PHYS.MECA.MEMA]Physics [physics]/Mechanics [physics]/Mechanics of materials [physics.class-ph]Stress (mechanics)Geochemistry and Petrology[SPI.MECA.MEMA]Engineering Sciences [physics]/Mechanics [physics.med-ph]/Mechanics of materials [physics.class-ph]Earth and Planetary Sciences (miscellaneous)compactionGeotechnical engineeringScaling0105 earth and related environmental sciencesstyloliteMechanicsself-affinityGrain sizeGeophysicsSpace and Planetary ScienceStyloliteParticle-size distributionPressure solutionnumerical modelGeology[SDU.STU.MI]Sciences of the Universe [physics]/Earth Sciences/MineralogyEarth and Planetary Science Letters
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Influence of microporosity distribution on the mechanical behavior of oolithic carbonate rocks.

2015

Abstract The mechanical behavior of oolithic carbonate rocks was investigated for selected rocks with two different microstructural attributes: uniform (UP) and rimmed (RP) distribution of microporosity within ooids. These oolithic carbonate rocks are from the Oolithe Blanche formation, a deep saline aquifer in the Paris Basin, and a possible target for CO2 sequestration and geothermal production. Samples of similar physical properties (porosity, grain diameter, cement content) but different microporosity textures were deformed under triaxial configuration, in water saturated conditions, at 28 MPa of confining pressure, 5 MPa of pore pressure and at a temperature of 55 °C. During the experi…

010504 meteorology & atmospheric sciences[SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/PetrographyMineralogy010502 geochemistry & geophysics[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy01 natural sciencesTortuosityPore water pressureBrittlenessRock mechanicsMicroporosityParis BasinComputers in Earth SciencesOolithe Blanche formationSafety Risk Reliability and QualityPorosity0105 earth and related environmental sciences[ SDU.STU.PE ] Sciences of the Universe [physics]/Earth Sciences/PetrographyCarbonate rockGeotechnical Engineering and Engineering GeologyOverburden pressurePermeability (earth sciences)Rock mechanics[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/StratigraphyCarbonate rockGeology
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Trace element behaviour in seawater during Etna's pyroclastic activity in 2001: Concurrent effects of nutrients and formation of alteration minerals

2010

volcanic ash ; trace element leaching ; kinetic experiments ; chlorophyll-alpha; International audience; The eruption of Etna in Sicily on 13 July 2001 marked the most intense activity of the volcano in the last 300 years. The eruption occurred while the oceanographic cruise ANSIC 01 was being conducted to the east of Sicily, presenting a unique opportunity for the investigation of the chemical effects on the marine system during a period of significant (similar to 1 g m(-2)) ash deposition. Comparison of trace element data with measured concentrations from the oceanographic cruise JUVENILE 99, carried out two years before, indicates large enrichments of V. Cr, Mn, Fe, Co, Cu and Pb. We att…

010504 meteorology & atmospheric sciences[SDU.STU]Sciences of the Universe [physics]/Earth SciencesPyroclastic rockMineralogy010502 geochemistry & geophysics01 natural sciencesWater columnGeochemistry and Petrology14. Life underwaterLeaching (agriculture)Kinetic experiment0105 earth and related environmental sciencesgeographygeography.geographical_feature_categoryChlorophyll-αTrace elementGeophysicsDeposition (aerosol physics)Volcano13. Climate actionEnvironmental chemistryTrace element leachingSeawaterVolcanic ashGeologyVolcanic ashJournal of Volcanology and Geothermal Research
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Textural-chemical changes and deformation conditions registered by phyllosilicates in a fault zone (Pic de Port Vieux thrust, Pyrenees)

2017

International audience; Synkinematic phyllosilicates in fault zones can be used to deduce the deformation mechanisms and the conditions of fault activity, as their chemical composition, crystal structure and texture can record the different stages of deformation and fluid-rock interactions. The Pic de Port Vieux, a second-order thrust related to the major Gavarnie thrust in the southern central part of the Pyrenees Axial Zone, juxtaposes Triassic pelites of the hanging wall and Cretaceous limestones of the footwall. In order to investigate the mineralogical and geochemical changes and constrain the deformation conditions of thrusting, characterization of phyllosilicates was performed along …

010504 meteorology & atmospheric sciences[SDV]Life Sciences [q-bio]GeochemistryFault (geology)engineering.material010502 geochemistry & geophysics01 natural sciences[ SDE ] Environmental Scienceschemistry.chemical_compoundGeochemistry and PetrologyPeliteThrust faultQuartzChlorite0105 earth and related environmental sciencesgeographygeography.geographical_feature_categoryK-white micaThrust fault[ SDV ] Life Sciences [q-bio]MuscovitePyreneesGeologyHematitePhyllosilicatesFluid-rock interactionsDiagenesischemistry[SDU]Sciences of the Universe [physics]visual_art[SDE]Environmental Sciencesvisual_art.visual_art_mediumengineeringChloriteGeology[ SDU ] Sciences of the Universe [physics]
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Simulation of nitrous oxide emissions from wheat-cropped soils using CERES

2005

Estimation of nitrous oxide (N2O) emissions from arable soils, in relation to crop fertilization, is essential to devise strategies to mitigate the impact of agriculture on global warming. This paper presents the development and test of a N2O model resulting from the linkage of a dynamic soil-crop simulation model (CERES) with two sub-models of N2O production and reduction in soils. These sub-models (NOE and NGAS) account for both the nitrification and denitrification pathways. The resulting models (CERES–NOE and CERES–NGAS) were tested against experimental data collected on three contrasting wheat-cropped soils representative of the Beauce agricultural region in France. Although the input …

010504 meteorology & atmospheric sciences[SDV]Life Sciences [q-bio]Soil ScienceSoil scienceengineering.materialCERES01 natural sciencesModellingchemistry.chemical_compound[ SDU.ENVI ] Sciences of the Universe [physics]/Continental interfaces environmentAGRONOMIE[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environmentComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciences2. Zero hungerNitrous oxideGlobal warming04 agricultural and veterinary sciencesNitrous oxideCalcisol15. Life on landSoil type[SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environmentGreenhouse gaseschemistry13. Climate actionGreenhouse gasFertilizationSoil water[SDE]Environmental Sciences040103 agronomy & agricultureengineering0401 agriculture forestry and fisheriesEnvironmental scienceFertilizerArable landAgronomy and Crop Science
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Models and data analysis tools for the Solar Orbiter mission

2020

All authors: Rouillard, A. P.; Pinto, R. F.; Vourlidas, A.; De Groof, A.; Thompson, W. T.; Bemporad, A.; Dolei, S.; Indurain, M.; Buchlin, E.; Sasso, C.; Spadaro, D.; Dalmasse, K.; Hirzberger, J.; Zouganelis, I.; Strugarek, A.; Brun, A. S.; Alexandre, M.; Berghmans, D.; Raouafi, N. E.; Wiegelmann, T.; Pagano, P.; Arge, C. N.; Nieves-Chinchilla, T.; Lavarra, M.; Poirier, N.; Amari, T.; Aran, A.; Andretta, V.; Antonucci, E.; Anastasiadis, A.; Auchère, F.; Bellot Rubio, L.; Nicula, B.; Bonnin, X.; Bouchemit, M.; Budnik, E.; Caminade, S.; Cecconi, B.; Carlyle, J.; Cernuda, I.; Davila, J. M.; Etesi, L.; Espinosa Lara, F.; Fedorov, A.; Fineschi, S.; Fludra, A.; Génot, V.; Georgoulis, M. K.; Gilbe…

010504 meteorology & atmospheric sciencescorona [Sun]Solar windAstrophysics[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph]7. Clean energy01 natural scienceslaw.inventionData acquisitionlawCoronal mass ejectiongeneral [Sun]QB AstronomyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSun: magnetic fieldsQCComputingMilieux_MISCELLANEOUSQBPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]3rd-DASenergetic particlesSolar windCORONAL MASS EJECTIONSnumerical modelingmagnetic fields [Sun]solar windPhysics::Space PhysicsSystems engineeringAstrophysics::Earth and Planetary Astrophysicsatmosphere [Sun]fundamental parameters [Sun]Sun: generalFORCE-FREE FIELDSun: fundamental parametersSolar radiusContext (language use)STREAMER STRUCTUREOrbiter0103 physical sciencesOPTIMIZATION APPROACH[SDU.ASTR.SR] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]POLARIZATION MEASUREMENTSSun: Solar wind3-DIMENSIONAL STRUCTURE0105 earth and related environmental sciencesSpacecraftbusiness.industrySun: corona[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]solar coronaMAGNETIC-FLUX ROPESAstronomy and AstrophysicsSHOCKS DRIVEN115 Astronomy Space scienceSPECTRAL-LINESQC Physics13. Climate actionSpace and Planetary SciencebusinessHeliosphereSun: atmosphereELECTRON-DENSITY
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Gravitational wave signature of proto-neutron star convection: I. MHD numerical simulations

2021

Gravitational waves provide a unique and powerful opportunity to constrain the dynamics in the interior of proto-neutron stars during core collapse supernovae. Convective motions play an important role in generating neutron stars magnetic fields, which could explain magnetar formation in the presence of fast rotation. We compute the gravitational wave emission from proto-neutron star convection and its associated dynamo, by post-processing three-dimensional MHD simulations of a model restricted to the convective zone in the anelastic approximation. We consider two different proto-neutron star structures representative of early times (with a convective layer) and late times (when the star is…

010504 meteorology & atmospheric sciencesdimension: 3neutron star: magnetic fieldtorusAstrophysicsMagnetar01 natural sciencesrotationstarstrong fieldMagnetarsAstrophysics::Solar and Stellar Astrophysicsgravitational radiation: spectrumgravitational radiation: signatureSupernova core collapse010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMethods numerical[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]formationscalingSupernovaAmplitudeAstrophysics - Solar and Stellar AstrophysicsConvection zoneAstrophysics - High Energy Astrophysical PhenomenaDynamosupernova: collapseprotoneutron starFOS: Physical sciencesConvectionsymmetry: axialGravitational waves0103 physical sciencesstructurenumerical calculationsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesGravitational waveAstronomy and AstrophysicsmagnetarNeutron star13. Climate actionSpace and Planetary Scienceefficiencygravitational radiation: emissionMagnetohydrodynamics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph][PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]
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