Search results for "PAC"

showing 10 items of 28794 documents

The Permeability Evolution of Tuffisites and Implications for Outgassing Through Dense Rhyolitic Magma

2019

There is growing evidence that outgassing through transient fracture networks exerts an important control on conduit processes and explosive‐effusive activity during silicic eruptions. Indeed, the first modern observations of rhyolitic eruptions have revealed that degassed lava effusion may depend upon outgassing during simultaneous pyroclastic venting. The outgassing is thought to occur as gas and pyroclastic debris are discharged through shallow fracture networks within otherwise low‐permeability, conduit‐plugging lava domes. However, this discharge is only transient, as these fractures become clogged and eventually blocked by the accumulation and sintering of hot, melt‐rich pyroclastic d…

010504 meteorology & atmospheric sciencesLava[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]SilicicLava domePyroclastic rock01 natural sciencesOutgassingGeophysics13. Climate actionSpace and Planetary ScienceGeochemistry and PetrologyRhyoliteMagmaEarth and Planetary Sciences (miscellaneous)Fracture (geology)PetrologyGeologyComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciences
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Shallow system rejuvenation and magma discharge trends at Piton de la Fournaise volcano (La Réunion Island)

2017

International audience; Basaltic magma chambers are often characterized by emptying and refilling cycles that influence their evolution in space and time, and the associated eruptive activity. During April 2007, the largest historical eruption of Piton de la Fournaise (Île de La Réunion, France) drained the shallow plumbing system (>240×106 m3>240×106 m3) and resulted in collapse of the 1-km-wide summit crater. Following these major events, Piton de la Fournaise entered a seven-year long period of near-continuous deflation interrupted, in June 2014, by a new phase of significant inflation. By integrating multiple datasets (lava discharge rates, deformation, seismicity, gas flux, gas composi…

010504 meteorology & atmospheric sciencesLavaeffusive paroxysmMagma chamber010502 geochemistry & geophysicseffusive trend01 natural sciencesEffusive eruptionImpact crater[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistryeffusive paroxysm; effusive trends; Piton de la Fournaise; shallow plumbing system; unloading; Geophysics; Geochemistry and Petrology; Earth and Planetary Sciences (miscellaneous); Space and Planetary ScienceGeochemistry and Petrologyunloading[SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/VolcanologyEarth and Planetary Sciences (miscellaneous)Petrology0105 earth and related environmental sciencesBasaltgeographygeography.geographical_feature_categoryeffusive trendsFumarolePiton de la FournaiseGeophysicsVolcanoshallow plumbing systemSpace and Planetary ScienceMagmaGeologySeismology
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Origin and Ion Charge State Evolution of Solar Wind Transients during 4 – 7 August 2011

2016

We present study of the complex event consisting of several solar wind transients detected by Advanced Composition Explorer (ACE) on 4 -- 7 August 2011, that caused a geomagnetic storm with Dst$=-$110 nT. The supposed coronal sources -- three flares and coronal mass ejections (CMEs) occurred on 2 -- 4 August 2011 in the active region (AR) 11261. To investigate the solar origin and formation of these transients we studied kinematic and thermodynamic properties of the expanding coronal structures using the Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) EUV images and the differential emission measure (DEM) diagnostics. The Helioseismic and Magnetic Imager (HMI) magnetic fie…

010504 meteorology & atmospheric sciencesMHDSolar windAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysics01 natural sciencesPhysics - Space PhysicsModelsIonization0103 physical sciencesCoronal mass ejectionQB AstronomyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesGeomagnetic stormPhysicsAstronomy and Astrophysics3rd-DASPlasmaCoronaSpace Physics (physics.space-ph)Solar windQC PhysicsMagnetic field13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsCoronal mass ejectionsMagnetohydrodynamicsSolar Physics
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Dynamic Triggering of Mud Volcano Eruptions During the 2016-2017 Central Italy Seismic Sequence

2017

On 24 August 2016 a seismic event (Mw 6.0) was the first of the long Central Italy sequence (ongoing at the end of 2017) of medium-to-high magnitude earthquakes, with nine Mw ≥5 up to October 2017, and with about 74.000 seismic events registered after one year. The largest was the Mw 6.5 30 October 2016 event near Norcia. After the major seismic events, seventeen mud volcanoes erupted around Monteleone di Fermo village (Marche region). Mud volcano eruptions generally occurred a few hours to a few days after the main earthquakes, suggesting a seismic triggering. We analyzed the peak ground velocities (PGV) and dynamic stresses during the three largest earthquakes. We also evaluated the stati…

010504 meteorology & atmospheric sciencesMagnitude (mathematics)010502 geochemistry & geophysics01 natural sciencesSequence (geology)GeophysicsSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Static stressSeismologyGeology0105 earth and related environmental sciencesDynamic stressMud volcanoJournal of Geophysical Research: Solid Earth
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Seismic sources and stress transfer interaction among axial normal faults and external thrust fronts in the Northern Apennines (Italy): A working hyp…

2016

In this study we analyse the main potential seismic sources in some axial and frontal sectors of the Northern Apennines, in Italy. This region was hit by a peculiar series of earthquakes that started in 1916 on the external thrust fronts near Rimini. Later, in 1917-1921, seismicity (up to Mw approximate to 6.5) shifted into the axial zone and clearly migrated north-westward, along the belt of active normal faults. The collection of fault-slip data focused on the active normal faults potentially involved in this earthquake series. The acquired data allowed us to better characterize the geometry and kinematics of the faults. In a few instances, the installation of local seismic networks durin…

010504 meteorology & atmospheric sciencesMagnitude (mathematics)ThrustInduced seismicity010502 geochemistry & geophysicsCluster (spacecraft)01 natural sciencesStress changeStress (mechanics)1916-1920 earthquake cluster0105 earth and related environmental sciencesEarth-Surface ProcessesSeismotectonicsStatic stress transferExternal thrust frontsAxial normal faultSeismic sourcesNorthern ApennineGeophysicsTime space1916–1920 earthquake clusterExternal thrust frontAxial normal faultsSeismic sourceSeismologyGeologyTectonophysics
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Strain rate dependence for evolution of steady state grain sizes: Insights from high-strain experiments on ice

2019

Abstract Understanding of the microstructural evolution and equilibrium grain size development during steady state tertiary flow is essential in order to improve our knowledge of ice and rock deformation. This contribution presents results from in situ transmitted light deformation experiments of natural glacier ice, with the development of the microstructure in a tertiary flow regime. We conducted one relative slower ( 1 × 10 − 6 1/s) and two relative faster-strain rate ( 2 × 10 − 6 1/s) pure shear experiments at −10 °C, up to a shortening of ∼57%. Microstructure development was followed by time-lapse observations, and two new microstructure-based indicators, the ‘seeding rate’ and the ‘mi…

010504 meteorology & atmospheric sciencesMechanicsSlip (materials science)Pure shearStrain rate010502 geochemistry & geophysicsMicrostructure01 natural sciencesGrain sizeGeophysicsSpace and Planetary ScienceGeochemistry and PetrologyParticle-size distributionEarth and Planetary Sciences (miscellaneous)SeedingGeology0105 earth and related environmental sciencesStress concentrationEarth and Planetary Science Letters
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Massive Oe/Be stars at low metallicity: Candidate progenitors of long GRBs?

2010

At low metallicity the B-type stars rotate faster than at higher metallicity, typically in the SMC. As a consequence, it was expected a larger number of fast rotators in the SMC than in the Galaxy, in particular more Be/Oe stars. With the ESO-WFI in its slitless mode, the SMC open clusters were examined and an occurence of Be stars 3 to 5 times larger than in the Galaxy was found. The evolution of the angular rotational velocity seems to be the main key on the understanding of the specific behaviour and of the stellar evolution of such stars at different metallicities. With the results of this WFI study and using observational clues on the SMC WR stars and massive stars, as well as the theo…

010504 meteorology & atmospheric sciencesMetallicityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesstars: rotation0103 physical sciencesMagellanic CloudsAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsStellar evolutionSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Astronomy and Astrophysicsgamma rays: general[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]GalaxyStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Sciencestars: supernovae: generalAstrophysics::Earth and Planetary AstrophysicsOpen cluster
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Pneumothorax and the environment: A systematic review of the impact of air pollution and meteorology, and a meta-analysis on meteorology factors.

2021

Abstract A relationship between the occurrence of spontaneous pneumothorax (SP) and meteorological factors has been observed but with contradictory results. The objectives of this systematic review was to synthesis the current body of evidence to the relationships between the occurrence of SP and environmental determinants such as meteorological factors and air pollutants. We conducted a systematic search of MEDLINE, Scopus, Cochrane Library and gray literature from inception up to 31st December 2020, to find published scientific research articles based on the following eligibility criteria: original studies and population-based articles describing the relationship between meteorological fa…

010504 meteorology & atmospheric sciencesMeteorological ConceptsHealth Toxicology and MutagenesisPopulationMEDLINEAir pollution010501 environmental sciencesCochrane LibraryToxicologymedicine.disease_cause01 natural sciencesMeteorologyAir pollutantsEnvironmental healthAir PollutionmedicineHumanseducation0105 earth and related environmental sciencesPotential impacteducation.field_of_studyAir PollutantsPneumothoraxGeneral MedicinePollutionMeta-analysisEnvironmental scienceSystematic searchEnvironmental pollution (Barking, Essex : 1987)
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A space-time rainfall generator for highly convective Mediterranean rainstorms

2003

Distributed hydrological models require fine resolution rainfall inputs, enhancing the practical interest of space-time rainfall models, capable of generating through numerical simulation realistic space-time rainfall intensity fields. Among different mathematical approaches, those based on point processes and built upon a convenient analytical description of the raincell as the fundamental unit, have shown to be particularly suitable and well adapted when extreme rainfall events of convective nature are considered. Starting from previous formulations, some analytical refinements have been considered, allowing practical generation of space-time rainfall intensity fields for that type of rai…

010504 meteorology & atmospheric sciencesMeteorology0207 environmental engineering[SDU.STU]Sciences of the Universe [physics]/Earth Sciences02 engineering and technologyMethod of moments (statistics)01 natural sciencesPoint processlcsh:TD1-1066lcsh:Environmental technology. Sanitary engineering020701 environmental engineering[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environmentlcsh:Environmental sciences0105 earth and related environmental scienceslcsh:GE1-350[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereComputer simulationRain gauge[SDU.OCEAN] Sciences of the Universe [physics]/Ocean AtmosphereSpace timelcsh:QE1-996.5lcsh:Geography. Anthropology. Recreation[SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environment6. Clean waterRunoff modellcsh:Geologylcsh:G13. Climate actionClimatology[SDU.STU] Sciences of the Universe [physics]/Earth SciencesGeneral Earth and Planetary SciencesEnvironmental scienceIntensity (heat transfer)Generator (mathematics)
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Ash-plume dynamics and eruption source parameters by infrasound and thermal imagery: The 2010 Eyjafjallajökull eruption

2013

During operational ash-cloud forecasting, prediction of ash concentration and total erupted mass directly depends on the determination of mass eruption rate (MER), which is typically inferred from plume height. Uncertainties for plume heights are large, especially for bent-over plumes in which the ascent dynamics are strongly affected by the surrounding wind field. Here we show how uncertainties can be reduced if MER is derived directly from geophysical observations of source dynamics. The combination of infrasound measurements and thermal camera imagery allows for the infrasonic type of source to be constrained (a dipole in this case) and for the plume exit velocity to be calculated (54–14…

010504 meteorology & atmospheric sciencesMeteorologyInfrasound Thermal cameras Volcanic Plume dynamicsInfrasoundPlume heightInfrasound010502 geochemistry & geophysicsAtmospheric sciences01 natural sciencesGeochemistry and PetrologyThermalEarth and Planetary Sciences (miscellaneous)ddc:5500105 earth and related environmental sciencesPlume heightLead (sea ice)Escape velocityPlumeGeophysics13. Climate actionSpace and Planetary ScienceParticle-size distributionEruption rateAsh eruptionsMass eruption rateGeology
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