Search results for "solu"

showing 10 items of 7577 documents

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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First M87 Event Horizon Telescope Results. III. Data Processing and Calibration

2019

We present the calibration and reduction of Event Horizon Telescope (EHT) 1.3 mm radio wavelength observations of the supermassive black hole candidate at the center of the radio galaxy M87 and the quasar 3C 279, taken during the 2017 April 5–11 observing campaign. These global very long baseline interferometric observations include for the first time the highly sensitive Atacama Large Millimeter/submillimeter Array (ALMA); reaching an angular resolution of 25 μas, with characteristic sensitivity limits of ~1 mJy on baselines to ALMA and ~10 mJy on other baselines. The observations present challenges for existing data processing tools, arising from the rapid atmospheric phase fluctuations, …

010504 meteorology & atmospheric sciencesgalaxies: jetRadio galaxyAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesgalaxies: individualGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgalaxies: individual: M8701 natural sciencesSubmillimeter ArrayGeneral Relativity and Quantum CosmologyTechniques: high angular resolutionindividual (M87 3C279) [Galaxies]0103 physical sciencesInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysics0105 earth and related environmental sciencesRemote sensingPhysicsEvent Horizon TelescopeSupermassive black hole3C279Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsQuasarBlack hole physicsblack hole physicAstrophysics - Astrophysics of Galaxies3. Good healthhigh angular resolution [Techniques]InterferometryAmplitudeSpace and Planetary ScienceGalaxies: jetsAstrophysics of Galaxies (astro-ph.GA)Techniques: interferometricinterferometric [Techniques]jets [Galaxies]Astrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Galaxies: individual (M87 3C279)Radio wave
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Implementation of a comprehensive ice crystal formation parameterization for cirrus and mixed-phase clouds in the EMAC model (based on MESSy 2.53)

2018

A comprehensive ice nucleation parameterization has been implemented in the global chemistry-climate model EMAC to improve the representation of ice crystal number concentrations (ICNCs). The parameterization of Barahona and Nenes (2009, hereafter BN09) allows for the treatment of ice nucleation taking into account the competition for water vapour between homogeneous and heterogeneous nucleation in cirrus clouds. Furthermore, the influence of chemically heterogeneous, polydisperse aerosols is considered by applying one of the multiple ice nucleating particle parameterizations which are included in BN09 to compute the heterogeneously formed ice crystals. BN09 has been modified in order to co…

010504 meteorology & atmospheric sciencesglobal climate modelNucleationMineral dustnucleation parameterizations010502 geochemistry & geophysicsAtmospheric sciences01 natural sciencesempirical parameterizationTroposphereinsoluble particlesddc:5500105 earth and related environmental sciencesmineral dustIce crystalssubmodel system messylcsh:QE1-996.5Northern Hemisphereatmospheric aerosollcsh:Geology13. Climate actionupper troposphereIce nucleusEnvironmental scienceCirrustransport sectorsWater vapordroplet number concentration
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First M87 Event Horizon Telescope Results. II. Array and Instrumentation

2019

The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comparable to the diameter of the Earth. At a nominal operating wavelength of ~1.3 mm, EHT angular resolution (λ/D) is ~25 μas, which is sufficient to resolve nearby supermassive black hole candidates on spatial and temporal scales that correspond to their event horizons. With this capability, the EHT scientific goals are to probe general relativistic effects in the strong-field regime and to study accretion and relativistic jet formation near the black hole boundary. In this Letter we describe the system design of th…

010504 meteorology & atmospheric sciencesindividual (M87) [galaxies]Event horizonAstronomyAstrophysics::High Energy Astrophysical Phenomenainterferometers [instrumentation]black hole physicsFOS: Physical sciencesgalaxies: individualGeneral Relativity and Quantum Cosmology (gr-qc)galaxies: individual: M8701 natural sciencesGeneral Relativity and Quantum Cosmologygalaxies: individual (M87)instrumentation: interferometer0103 physical sciencesVery-long-baseline interferometryAngular resolutionInstrumentation (computer programming)instrumentation: interferometers010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy Astrophysics0105 earth and related environmental scienceshigh angular resolution [echniques]Event Horizon TelescopePhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Supermassive black holeGalaxy: centerhigh angular resolution [techniques]Astronomytechniques: high angular resolutiongravitational lensing: strongAstronomy and Astrophysicscenter [Galaxy]Hydrogen maserblack hole physicAstrophysics - Astrophysics of Galaxiesechniques: high angular resolutionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)strong [gravitational lensing]MillimeterAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]The Astrophysical Journal Letters
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First M87 Event Horizon Telescope Results. I. the Shadow of the Supermassive Black Hole

2019

When surrounded by a transparent emission region, black holes are expected to reveal a dark shadow caused by gravitational light bending and photon capture at the event horizon. To image and study this phenomenon, we have assembled the Event Horizon Telescope, a global very long baseline interferometry array observing at a wavelength of 1.3 mm. This allows us to reconstruct event-horizon-scale images of the supermassive black hole candidate in the center of the giant elliptical galaxy M87. We have resolved the central compact radio source as an asymmetric bright emission ring with a diameter of 42 ± 3 μas, which is circular and encompasses a central depression in brightness with a flux rati…

010504 meteorology & atmospheric sciencesindividual (M87) [galaxies]Event horizonAstronomyblack hole physicsjets [galaxies]galaxies: individualAstrophysicshigh-resolution7. Clean energy01 natural sciencesPhoton sphereGeneral Relativity and Quantum Cosmologyaccretionsagittarius-a-asterisk010303 astronomy & astrophysicsgalactic-centerHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsradio-sourcesaccretion disksGalactic Centergrmhd simulations3. Good healthenergy-distributionsactive [galaxies]AnatomyAstrophysics - High Energy Astrophysical PhenomenaActive galactic nucleusAstrophysics::High Energy Astrophysical Phenomenagalaxies: activeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgalaxies: individual: M87galaxies: individual (M87)Cell and Developmental BiologyGeneral Relativity and Quantum Cosmology0103 physical sciences(M87)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEvent Horizon TelescopeSupermassive black holeghz vlbi observationsfaraday-rotationAstronomy and Astrophysicsgalaxies: jetsAstrophysics - Astrophysics of GalaxiesBlack holeRotating black holeSpace and Planetary SciencegravitationAstrophysics of Galaxies (astro-ph.GA)advection-dominated accretion[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]ionized-gas
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First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole

2019

We present measurements of the properties of the central radio source in M87 using Event Horizon Telescope data obtained during the 2017 campaign. We develop and fit geometric crescent models (asymmetric rings with interior brightness depressions) using two independent sampling algorithms that consider distinct representations of the visibility data. We show that the crescent family of models is statistically preferred over other comparably complex geometric models that we explore. We calibrate the geometric model parameters using general relativistic magnetohydrodynamic (GRMHD) models of the emission region and estimate physical properties of the source. We further fit images generated fro…

010504 meteorology & atmospheric sciencesindividual (M87) [galaxies]Event horizonGeneral relativityAstronomyAstrophysics::High Energy Astrophysical Phenomenablack hole physicsFOS: Physical sciencesgalaxies: individualAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)galaxies: individual: M8701 natural sciences7. Clean energyGeneral Relativity and Quantum Cosmologygalaxies: individual (M87)GravitationGeneral Relativity and Quantum Cosmology0103 physical sciences(M87)010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsEvent Horizon TelescopeHigh Energy Astrophysical Phenomena (astro-ph.HE)high angular resolution [techniques]techniques: high angular resolutionAstronomy and Astrophysicsblack hole physicAstrophysics - Astrophysics of GalaxiesGalaxyinterferometric [techniques]Black holeRotating black holeSpace and Planetary Sciencegravitationtechniques: interferometricAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaSchwarzschild radius
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Debitage by fracturing in the osseous industry of Cova del Parpalló (Gandía-Valencia, Spain): A preliminary study

2016

Abstract The excavations carried out by L. Pericot from 1929 to 1931 in the Cova del Parpallo documented the Gravettian in the base, a Solutrean layer, and a Magdalenian. This sequences comprise an exceptional assemblage of portable art because of the number of plaquets/objects and the great chronological amplitude. With all this information, Parpallo was included in the reduced list of reference sites to organize the European Upper Paleolithic sequence in the first half of the 20th century. The Magdalenian layers were organized in four phases, following H. Breuil's classical proposal. Changes in bases morphology and decorative topics on osseous points permitted this correlation, identifyin…

010506 paleontology060102 archaeology06 humanities and the artsSolutrean01 natural sciencesArchaeologyDebitagelaw.inventionPaleontologySequence (geology)lawUpper PaleolithicPortable artAssemblage (archaeology)0601 history and archaeologyRadiocarbon datingMagdalenianGeology0105 earth and related environmental sciencesEarth-Surface ProcessesQuaternary International
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The Solutrean - Magdalenian Transition: a view from Iberia

2012

The paper examines the Upper SolutreaneArchaic Magdalenian/Badegoulian succession on the base of lithic and bone tool production, chrono-stratigraphic data and radiocarbon dates from the Cantabrian and Mediterranean regions of Iberia, mainly the areas of Asturias and Valencia (Spain). The discussion considers a reduced number of variables (characteristic stone tools, bone points and decoration techniques) and highlights the elements in common. The analysis concerning the transformation of lithic production at Cova del Parpallo provides new data for the Upper SolutreaneArchaic Magdalenian/ Badegoulian transition.

010506 paleontology060102 archaeologyBone tool06 humanities and the artsPaleolíticSolutrean01 natural sciencesArchaeologyPrehistòrialaw.inventionGeographyEvolució culturallaw0601 history and archaeologyRadiocarbon datingMagdalenian0105 earth and related environmental sciencesEarth-Surface Processes
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Consolidation of earthen building materials: a comparative study

2019

The consolidation and protection of mud bricks are a challenge in the field of conservation of archeological sites. One of the solutions is represented by the coverage of the entire excavation that assures a protection against mud dissolution. Unfortunately, this is not always feasible, both for economical and practical issues. For these reasons, alternative solutions are needed. In this work, laboratory experimentation has been carried out in order to test the efficacy of some products to slow down the dissolution process and increase the brick toughness. Three typologies of raw materials taken from different outcrops (one from the Republic of Azerbaijan and two from Calabria region, Italy…

010506 paleontologyArcheologyBrickPotassium hydroxide060102 archaeologyWaste managementConsolidation (soil)Alkaline solutions Consolidation Laboratory test Mud bricks06 humanities and the artsRaw material01 natural sciencesSilicatechemistry.chemical_compoundchemistrySodium hydroxideAnthropologyEnvironmental science0601 history and archaeologyDissolutionSettore GEO/09 -Georis. Miner.e Appl.Mineral.-Petrogr. per l'Ambi.ed i B.Cult.Potassium silicate0105 earth and related environmental sciencesArchaeological and Anthropological Sciences
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A new method for the identification of archaeological soils by their spectral signatures in the vis-NIR region

2020

Abstract This paper introduces a statistical method to identify spectral signatures of buried archaeological remains and distinguish them from spectra of the background soil in the visible to near infrared region. The proposed method is based on the Principal Component Analysis (PCA). The difference between an archaeological spectrum and non-archaeological soil spectra is quantified by a so-called R value. R values larger than 1 indicate that the spectrum represents an archaeological material. The method is successfully applied to samples from five study sites in Italy and Hungary with special conditions. The reflection spectra are taken in a time-efficient way with a field spectrometer. Th…

010506 paleontologyArcheologySpectral signature060102 archaeologySpectrometerNear-infrared spectroscopy06 humanities and the artsCC01 natural sciencesArchaeologyField (geography)Spectral linePrincipal component analysisReflection (physics)0601 history and archaeologySpectral resolutionGeology0105 earth and related environmental sciencesJournal of Archaeological Science: Reports
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