Search results for "Universe"

showing 10 items of 2171 documents

Unrest at the Nevados de Chillán volcanic complex: a failed or yet to unfold magmatic eruption?

2018

Resuming erupting activity at volcanoes that have been long quiescent poses a significant challenge to hazard assessment, as it require assessment of whether the change in activity is an isolated event or the beginning of a new eruptive sequence. Such inception is often poorly characterised as quiescent volcanoes tend to be poorly equipped and not extensively monitored, especially with respect to gas geochemistry. Here, we report gas composition and flux measurements from a newly opened vent at the very onset of eruptive activity at the Nevados de Chillán volcanic complex (Chile) in January-February 2016. The molar proportions of H2O, CO2, SO2, H2S and H2 gases are found to be 98.4, 0.97, 0…

event.disaster_typeBasaltTrail By FireQE1-996.5geographygeography.geographical_feature_categoryAndesiteGeochemistryUV cameraGeologyEruption triggerDaciteVolcanic GasesBasaltic andesiteLithic fragmentVolcanoVolcanic unrestMagma[SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/Volcanologyevent[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environmentVolcanic gasesMulti-GASGeology
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The importance of fracture-healing on the deformation of fluid-filled layered systems

2014

International audience; Understanding the fracturingehealingerefracturing cycle is a fundamental part of studying the deformation dynamics and the permeability evolution of rock systems. Previous studies, however, have not examined the influence of healing i.e. fracture-closure through vein formation and the mechanical properties of the " healed " fractures (veins) on the rock deformation. We present results from a two-dimensional coupled hydro-mechanical model which simulates large time and spatial scale dynamic fracturing and healing of a porous medium under the influence of gravity, tectonic stretching and elevated fluid pressures. Our results show that healing decreases the local porosi…

fault010504 meteorology & atmospheric sciences[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph][SDU.STU]Sciences of the Universe [physics]/Earth SciencesBone healing010502 geochemistry & geophysics01 natural sciencesjointevolution[PHYS.MECA.SOLID]Physics [physics]/Mechanics [physics]/Solid mechanics [physics.class-ph]Fluid dynamicstectonicsGeotechnical engineering[PHYS.MECA.MEFL]Physics [physics]/Mechanics [physics]/Fluid mechanics [physics.class-ph]PorosityElastic modulus0105 earth and related environmental sciences[SDU.STU.TE]Sciences of the Universe [physics]/Earth Sciences/TectonicsGeologyhealingPermeability (earth sciences)fracturenetwork[PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]Delayed fractureSaturation (chemistry)Porous mediumGeology
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Os, Sr, Nd, Pb, O isotope and trace element data from the Ferrar flood basalts, antarctica: evidence for an enriched subcontinental lithospheric sour…

1996

Os, Sr, Nd, Pb and O isotopes and trace element data are reported for basaltic andesite and andesite whole rocks and, in part, for selected mineral separates from the Jurassic Ferrar flood basalt province. Radiogenic Sr (> 0.709), unradiogenic Nd (εNd= −3 to −5), and radiogenic Pb isotopes, as well as low Nb/La ratios of 0.4 – 0.6 and Nb/La ratios between 0.45 and 0.6 are found for all rocks including our most primitive sample (Mg# = 71.9). This indicates involvement of either continental crust or enriched lithospheric mantle in magma genesis. 187Re/188Os correlates strongly with 187Os/188Os, with an age of 172 ± 5 Ma, in agreement with published Arsingle bondAr data. Initial 187Os/188Os of…

flood basalts010504 meteorology & atmospheric sciencesGeochemistryFerrar Group551010502 geochemistry & geophysics01 natural sciencesMantle (geology)magma contaminationBasaltic andesite[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/PlanetologyGeochemistry and Petrology[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/GeochemistryEarth and Planetary Sciences (miscellaneous)[SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/Volcanology0105 earth and related environmental sciencesgeochemistryPeridotiteBasaltAndesiteContinental crustTrace elementGeophysics13. Climate actionSpace and Planetary ScienceFlood basaltFerrar Group; flood basalts; magma contamination; geochemistryGeology
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Zones d'ammonites et de foraminifères du Vraconnien au Turonien : Une comparasion entre les domaines boréal et téthysien (NW Europe / Tunisie central…

2008

International audience; Depuis la fin du 19ème siècle, l'intervalle comprenant l'Albien supérieur élevé, le Cénomanien, le Turonien et le Coniacien basal a été subdivisé d'abord en zones d'ammonites puis, à partir du milieu du 20ème siècle, en zones de foraminifères planctoniques, deux groupes de macro- et de microfossiles particulièrement efficaces en bio-chronostratigraphie grâce à leur taux d'évolution rapide. Toutefois, des différences de compositions fauniques entre le domaine boréal (Europe du Nord-Ouest) et le domaine téthysien (Méditerranée) ont longtemps empêché des corrélations précises entre ces deux domaines. Aujourd'hui, dans un intervalle de temps couvrant environ 16 millions …

foraminifèresCrétacéStratigraphyzones[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy[SDE.MCG.CPE] Environmental Sciences/Global Changes/domain_sde.mcg.cpe[ SDE.MCG.CPE ] Environmental Sciences/Global Changes/domain_sde.mcg.cpezonationlcsh:StratigraphyCénomanienTéthys[SDU.STU.GC] Sciences of the Universe [physics]/Earth Sciences/Geochemistrylcsh:QE701-760lcsh:QE640-699ammonitesAlbienlcsh:QE1-996.5PaleontologyGeology[ SDU.STU.GC ] Sciences of the Universe [physics]/Earth Sciences/GeochemistryVraconnienTuronienlcsh:GeologyGeographylcsh:Paleontology[SDU.STU.ST] Sciences of the Universe [physics]/Earth Sciences/StratigraphyCenomanianHumanitiesCarnets de géologie (Notebooks on geology)
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Analysis of cloudiness and solar radiation diurnal cycles for a better understanding of the forests greenness mean annual cycle in Central Africa.

2016

To better understand the Central Africa forests sensitivity toclimate variability, we jointly analyse the mean annual cycles of greenness, rainfall, cloudiness and solarradiation for the target region 0-5°N/12-19°E using high resolution satellite data. Our results demonstrate theimportance of the diurnal scale for understanding the mean annual cycles of rainfall, cloudiness and solarradiation and the way they shape those of forest greenness. They also suggest that whereas the March-Mayrainy season appears optimal for greenness especially because of favorable light conditions, water availabilityis the main controlling factor in December-January the main dry season and in February at the star…

forests[ SDV.BV ] Life Sciences [q-bio]/Vegetal BiologyAfrique CentraleCentral Africacycles diurnessolar radiationcloudinessforêtsradiation solaire[SDU.STU.CL] Sciences of the Universe [physics]/Earth Sciences/Climatology[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology[SDV.BV]Life Sciences [q-bio]/Vegetal Biologynébulosité[SDV.BV] Life Sciences [q-bio]/Vegetal Biologydiurnal cycles[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/Climatology
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Cycles diurnes de rayonnement solaire et forets en Afrique Centrale.

2018

The sunlightconditions prevailing in Central Africa, and their potential impact on forests traits and functioning, have neverbeen fully explored. Using satellite estimates documenting mostly the period 2005-2013, and accounting forscale interactions between the diurnal and annual cycles, we demonstrate that the seasonality of sunlight levelsstrongly vary across Central Africa forests. Gabon stands out with a main dry season strongly light-deficient,cool and moist. An original map of terra firme forest types developed by CIRAD shows that most of theevergreen forests of Central Africa develop in Gabon. We postulate that despite a mean annual precipitationamount below 2000 mm/yr, the Gabonese …

forestsforêtsAfrique Centrale[SDU.STU.CL] Sciences of the Universe [physics]/Earth Sciences/ClimatologyCentral Africacycles diurnes[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatologysolar radiationdiurnal cyclesrayonnement solaire
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Évolution du stress gélif et idéotypes de pois d'hiver dans le contexte de changement climatique, à une échelle régionale.

2017

11 pages; International audience; Pea (Pisum sativum L.) is an important crop in temperate regions for its high seed protein concentration that is particularly sensitive to abiotic stresses. The abrupt temperature increase known as the “1987/1988 temperature regime shift” that occurs over Europe is questioning how winter pea will perform in the changing climate. This study assessed the winter frost damage evolution along from 1961 to 2015 in Burgundy-Franche-Comté by using: (1) daily observed and gridded regional temperature data and (2) a validated crop winter frost stress model calibrated for pea. This study shows a global decrease of the frost stress nevertheless resulting from a subtle …

frost resistance010504 meteorology & atmospheric sciencesmodeling;temperature abrupt shift;winter pea;frost resistance;Burgundy-Franche-ComteBurgundy-Franche-Comté[SDV.SA.AGRO]Life Sciences [q-bio]/Agricultural sciences/AgronomyContext (language use)lcsh:TP670-69901 natural sciencesBiochemistryBourgogne Franche-Comtéwinter peatemperature abrupt shift[ SDV.SA.AGRO ] Life Sciences [q-bio]/Agricultural sciences/AgronomyEffects of global warmingTemperate climateRegime shiftmodélisation0105 earth and related environmental sciences2. Zero hungerAbiotic componentGlobal warmingIdeotypemodeling04 agricultural and veterinary sciences15. Life on landpois d'hiverrésistance au gelGeographyAgronomy[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology13. Climate actionClimatologyrupture des températuresFrost040103 agronomy & agriculture0401 agriculture forestry and fisheries[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/Climatologylcsh:Oils fats and waxesAgronomy and Crop ScienceFood ScienceOilseeds and fats, crops and lipids
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High-energy monitoring of NGC 4593 II. Broad-band spectral analysis: testing the two-corona model

2019

It is widely believed that the primary X-ray emission of AGN is due to the Comptonisation of optical-UV photons from a hot electron corona, while the origin of the 'soft-excess' is still uncertain and matter of debate. A second Comptonisation component, called warm corona, was therefore proposed to account for the soft-excess, and found in agreement with the optical-UV to X-ray emission of a sample of Seyfert galaxies. In this context, we exploit the broadband XMM-Newton and NuSTAR simultaneous observations of the Seyfert galaxy NGC 4593 to further test the so called "two corona model". The NGC 4593 spectra are well reproduced by the model, from the optical/UV to the hard X-rays. Moreover, …

galaxie [X-rays]High energyPhotonAstrophysics::High Energy Astrophysical Phenomenablack hole physicsgalaxies: activeFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesmagnetohydrodynamics (MHD)Spectral lineCorona (optical phenomenon)X-rays: binariesaccretionPrimary (astronomy)Seyfert [galaxies]0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsSpectral analysis010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)individuals: (NGC 4593) [X-rays][SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsaccretion disks[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsAstronomy and AstrophysicGalaxygalaxies: SeyfertX-rays: galaxiesISM: jets and outflowsSpace and Planetary Science[SDU]Sciences of the Universe [physics]active [galaxies]Astrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-rays: individuals: (NGC 4593)
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Testing warm Comptonization models for the origin of the soft X-ray excess in AGNs

2018

The X-ray spectra of many active galactic nuclei (AGN) show a soft X-ray excess below 1-2 keV on top of the extrapolated high- energy power law. The origin of this component is uncertain. It could be a signature of relativistically blurred, ionized reflection, or the high-energy tail of thermal Comptonization in a warm (kT $\sim$ 1 keV), optically thick ($\tau\simeq$ 10-20) corona producing the optical/UV to soft X-ray emission. The purpose of the present paper is to test the warm corona model on a statistically significant sample of unabsorbed, radio-quiet AGN with XMM-newton archival data, providing simultaneous optical/UV and X-ray coverage. The sample has 22 objects and 100 observations…

galaxie [X-rays]Seyfert [Galaxies]Active galactic nucleusactive [Galaxies][ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical Phenomenagalaxies: activeFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesPower lawSpectral lineAccretion discIonization0103 physical sciencesThermalAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Soft x ray010308 nuclear & particles physicsAstronomy and AstrophysicsAstronomy and AstrophysicGalaxygalaxies: SeyfertX-rays: galaxiesSpace and Planetary Science[SDU]Sciences of the Universe [physics]Astrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the Intracluster Medium out to $R_{200}$ in Abell 2319

2018

We present the joint analysis of the X-ray and SZ signals in A2319, the galaxy cluster with the highest signal-to-noise ratio in Planck maps and that has been surveyed within our XMM Cluster Outskirts Project (X-COP). We recover the thermodynamical profiles by the geometrical deprojection of the X-ray surface brightness, of the SZ comptonization parameter, and an accurate and robust spectroscopic measurements of the temperature. We resolve the clumpiness of the density to be below 20 per cent demonstrating that most of this clumpiness originates from the ongoing merger and can be associated to large-scale inhomogeneities. This analysis is done in azimuthally averaged radial bins and in eigh…

galaxies: clusters: general ; galaxies: clusters: intracluster medium – X-rays; galaxies: clusters – intergalactic mediumgalaxies: clusters: intracluster medium – X-raysCosmology and Nongalactic Astrophysics (astro-ph.CO)galaxies: clusters: intracluster medium[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionlawIntracluster medium0103 physical sciencesROSATCluster (physics)Surface brightnessTotal pressure010303 astronomy & astrophysicsGalaxy clusterComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhysicsgalaxies: clusters – intergalactic medium[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsSettore FIS/05Astronomy and AstrophysicsAstronomy and AstrophysicX-rays: galaxies: clusterGalaxySpace and Planetary Sciencegalaxies: clusters: generalX-rays: galaxies: clustersintergalactic mediumHydrostatic equilibrium[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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