Search results for "Sphere"

showing 10 items of 2121 documents

Bright Hot Impacts by Erupted Fragments Falling Back on the Sun: Magnetic Channelling

2016

Dense plasma fragments were observed to fall back on the solar surface by the Solar Dynamics Observatory after an eruption on 7 June 2011, producing strong EUV brightenings. Previous studies investigated impacts in regions of weak magnetic field. Here we model the $\sim~300$ km/s impact of fragments channelled by the magnetic field close to active regions. In the observations, the magnetic channel brightens before the fragment impact. We use a 3D-MHD model of spherical blobs downfalling in a magnetized atmosphere. The blob parameters are constrained from the observation. We run numerical simulations with different ambient density and magnetic field intensity. We compare the model emission i…

010504 meteorology & atmospheric sciencesField (physics)FOS: Physical sciencesAstrophysics01 natural sciencesAtmosphereSettore FIS/05 - Astronomia E AstrofisicaSun: activity0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsMagnetic pressureSun: magnetic field010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSun: coronaAstronomy and AstrophysicsSun: UV radiation Supporting material: animationPlasmaCoronal loopAstronomy and AstrophysicRam pressureMagnetic fieldStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space Physics
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A tale of two emergences: Sunrise II observations of emergence sites in a solar active region

2017

R. Centeno et. al.

010504 meteorology & atmospheric sciencesField (physics)photosphere [Sun]Field lineFOS: Physical sciencesFluxchromosphere [Sun]Astrophysicspolarimetric [Techniques]01 natural sciences0103 physical sciencesSunrise010303 astronomy & astrophysicsChromosphereSun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSunspotsSun: chromosphereTechniques: polarimetricSun: photosphereAstronomy and AstrophysicsMagnetic reconnectionMagnetic fluxMagnetic fieldmagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science
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2021

Intracratonic basins tend to subside much longer than the timescale predicted by thermal relaxation of the lithosphere. Many hypotheses have been suggested to explain their longevity, yet few have been tested using quantitative thermo-mechanical numerical models, which capture the dynamic of the lithosphere. Lithospheric-scale geodynamic modelling preserving the tectono-stratigraphic architecture of these basins is challenging because they display only few kilometres of subsidence over 1000 of km during time periods exceeding 250 Myr. Here we present simulations that are designed to examine the relative role of thermal anomaly, tectonics and heterogeneity of the lithosphere on the dynamics …

010504 meteorology & atmospheric sciencesGeologySubsidenceForcing (mathematics)010502 geochemistry & geophysics01 natural sciencesUnconformityTectonics13. Climate actionLithosphereErosionCompression (geology)Accretion (geology)SeismologyGeology0105 earth and related environmental sciencesBulletin de la Société géologique de France
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Microbiology and atmospheric processes: biological, physical and chemical characterization of aerosol particles

2008

Abstract. The interest in bioaerosols has traditionally been linked to health hazards for humans, animals and plants. However, several components of bioaerosols exhibit physical properties of great significance for cloud processes, such as ice nucleation and cloud condensation. To gain a better understanding of their influence on climate, it is therefore important to determine the composition, concentration, seasonal fluctuation, regional diversity and evolution of bioaerosols. In this paper, we will review briefly the existing techniques for detection, quantification, physical and chemical analysis of biological particles, attempting to bridge physical, chemical and biological methods for …

010504 meteorology & atmospheric sciencesIndoor bioaerosollcsh:LifeBiological particles[SDU.STU]Sciences of the Universe [physics]/Earth SciencesNanotechnology[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph]01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]03 medical and health scienceslcsh:QH540-549.5[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environmentEcology Evolution Behavior and Systematics0105 earth and related environmental sciencesEarth-Surface Processes[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere0303 health sciences[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.OCEAN] Sciences of the Universe [physics]/Ocean Atmosphere030306 microbiologyChemistrylcsh:QE1-996.5[SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environmentAerosolCharacterization (materials science)lcsh:Geologylcsh:QH501-531[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]13. Climate action[SDU.STU] Sciences of the Universe [physics]/Earth SciencesIce nucleuslcsh:EcologyBiochemical engineeringAerosol sampling
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Applications of a new set of methane line parameters to the modeling of Titan's spectrum in the 1.58 μm window

2012

International audience; In this paper we apply a recently released set of methane line parameters (Wang et al., 2011) to the modeling of Titan spectra in the 1.58 mu m window at both low and high spectral resolution. We first compare the methane absorption based on this new set of methane data to that calculated from the methane absorption coefficients derived in situ from DISR/Huygens (Tomasko et al., 2008a; Karkoschka and Tomasko, 2010) and from the band models of Irwin et al. (2006) and Karkoschka and Tomasko (2010). The Irwin et al. (2006) band model clearly underestimates the absorption in the window at temperature-pressure conditions representative of Titan's troposphere, while the Ka…

010504 meteorology & atmospheric sciencesInfraredCASSINI VIMSHUYGENS PROBEMONODEUTERATED METHANEAtmospheric sciences01 natural sciences7. Clean energyMethaneSpectral lineTropospherechemistry.chemical_compoundsymbols.namesake0103 physical sciencesSpectral resolutionSpectroscopy010303 astronomy & astrophysicsCLOUD STRUCTURE0105 earth and related environmental sciencesPhysics[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Astronomy and Astrophysics9500 CM(-1)SPECTROSCOPIC DATABASEM TRANSPARENCY WINDOWComputational physicsAerosolchemistry[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]TEMPERATURE-DEPENDENCE13. Climate actionSpace and Planetary SciencesymbolsSHIFT COEFFICIENTSOUTER SOLAR-SYSTEMTitan (rocket family)
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Gas mass derived by infrasound and UV cameras: Implications for mass flow rate

2016

Abstract Mass Flow Rate is one of the most crucial eruption source parameter used to define magnitude of eruption and to quantify the ash dispersal in the atmosphere. However, this parameter is in general difficult to be derived and no valid technique has been developed yet to measure it in real time with sufficient accuracy. Linear acoustics has been applied to infrasonic pressure waves generated by explosive eruptions to indirectly estimate the gas mass erupted and then the mass flow rate. Here, we test on Stromboli volcano (Italy) the performance of such methodology by comparing the acoustic derived results with independent gas mass estimates obtained with UV cameras, and constraining th…

010504 meteorology & atmospheric sciencesInfrasoundMass flowVolcano acousticMagnitude (mathematics)ThrustGeophysicsMass flow rate010502 geochemistry & geophysics01 natural sciencesAtmosphereGeophysicsSulphur dioxide cameraThermal imagery13. Climate actionGeochemistry and PetrologyMass flow rateRange (statistics)WaveformGeology0105 earth and related environmental sciencesJournal of Volcanology and Geothermal Research
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Melange: A viscoelastic lattice-particle model applicable to the lithosphere

2012

[1] This article introduces the software Melange, a 3D lattice-particle hybrid model. The software was specifically designed in order to simulate ductile visco-elasto-plastic deformation and can be used to study tectonic processes in the lithosphere from the micro to the macro scale. Melange is under an open source license. The code takes both relevant yield mechanisms for the deformation of lithospheric material into account: dynamic brittle failure and ductile creep, where ductile creep is modeled as viscoelasticity. The software considers effects of the local geology, of the inherent disorder of geomaterials, of rheological layering of the lithosphere and applies repulsion when the mater…

010504 meteorology & atmospheric sciencesIsotropyModulusMechanics010502 geochemistry & geophysics01 natural sciencesViscoelasticityPhysics::GeophysicsGeophysicsBrittlenessRheologyCreepGeochemistry and PetrologyLithosphereMacroscopic scaleGeotechnical engineeringGeology0105 earth and related environmental sciencesGeochemistry, Geophysics, Geosystems
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High time resolution fluctuations in volcanic carbon dioxide degassing from Mount Etna

2014

Abstract We report here on the first record of carbon dioxide gas emission rates from a volcano, captured at ≈ 1 Hz. These data were acquired with a novel technique, based on the integration of UV camera observations (to measure SO2 emission rates) and field portable gas analyser readings of plume CO2/SO2 ratios. Our measurements were performedat the North East crater of Mount Etna, southern Italy, and the data reveal strong variability in CO2 emissions over timescales of tens to hundreds of seconds, spanning two orders of magnitude. This carries importantimplications for attempts to constrain global volcanic CO2 release to the atmosphere, and will lead to an increased insight into short te…

010504 meteorology & atmospheric sciencesLagPlume imagingInduced seismicity010502 geochemistry & geophysicsAtmospheric sciencesPassive degassing01 natural sciencesAtmospherechemistry.chemical_compoundImpact craterGeochemistry and Petrology0105 earth and related environmental sciencesCarbon dioxide; Passive degassing; Plume imaging; Volcanic remote sensing; Volcano seismology; Geophysics; Geochemistry and PetrologyBasaltgeographygeography.geographical_feature_categoryVolcano seismologyPlumeVolcanic remote sensingGeophysicsVolcanochemistryCarbon dioxide13. Climate actionCarbon dioxideCarbon dioxide; Passive degassing; Plume imaging; Volcanic remote sensing; Volcano seismology; Geochemistry and Petrology; GeophysicsSeismologyGeology
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Pre- and syn-eruptive geochemistry of volcanic gases from Soufriere Hills of Montserrat, West Indies

1998

International audience; Soufriere Hills fumaroles contained magmaderived volatiles before and during the eruption initiated in 1995 but also preserved a typical and quite steady hydrothermal coinposition. Chemical changes due to increased boiling and a greater input of oxidizing magmatic gas occurred only at Galway's Soufriere, the most active fumarolic field. Hydrothermal buffering of the fumaroles has been favoured by their remote location (!-2 km) froin the eruptive vents and by a preferential degassing of the uprising magma through intrusive conduits under the crater. High temperature (720øC) gas collected froin the extruding lava dome in Feb. 1996 was chemically and isotopically repres…

010504 meteorology & atmospheric sciencesLava75252 Paris cedex 05GeochemistryLSCEitaly (e-mail: pare!io010502 geochemistry & geophysics01 natural sciencesHydrothermal circulationBritish Geological SurveyVolcanic Gaseslsce.saclay.cea.ff) PalermoCEA-CNRSImpact craterevent[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environment0105 earth and related environmental sciencesevent.disaster_type[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereLGSCFrance (semetg?)ipgp.j ussieu.t¾). -SS.R. YoungLava domeIPGPFumaroleGeophysics4 place JussieuDomoMagmambox.unipa.it). 4M.p. SemetGeneral Earth and Planetary Sciences91190 GiftYvette2p. Ailard and P. Jean-BaptisteFrance (e-mail: ailardGeology
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Is there a global carbonate layer in the oceanic mantle?

2021

co-auteur étranger; International audience; Previous modeling of carbonate subduction by high‐pressure experimentation has allowed to propose scenarios for bulk carbon return to the mantle, but the detailed transfer mechanisms have seldom been studied. We monitored carbonate – silicate reactions by combining high‐pressure experiments and synchrotron‐based x‐ray diffraction. Carbonates break down at moderate pressure and high temperature and CO2 is trapped at grain boundaries. Further isothermal compression yields melting, which may control continuous carbon introduction, first in the mantle wedge, and next, away from the wedge. Carbon presence has been discussed in a variety of magmatic con…

010504 meteorology & atmospheric sciencesMantle wedgeSubductionchemistry.chemical_element010502 geochemistry & geophysics01 natural sciencesIsothermal processMantle (geology)Plate tectonicschemistry.chemical_compoundGeophysicschemistry13. Climate actionLithosphere[SDU]Sciences of the Universe [physics]General Earth and Planetary SciencesCarbonateGrain boundaryCompression (geology)PetrologyCarbonGeology0105 earth and related environmental sciences
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