Search results for "Environment"

showing 10 items of 28487 documents

The Impact of a Very Weak and Thin Upper Asthenosphere on Subduction Motions

2019

Recent geophysical observations report the presence of a very weak and thin upper asthenosphere underneath subducting oceanic plates at convergent margins. Along these margins, trench migrations are significantly slower than plate convergence rates. We use numerical models to assess the role of a weak upper asthenospheric layer on plate and trench motions. We show that the presence of this layer alone can enhance an advancing trend for the motion of the plate and hamper trench retreat. This mechanism provides a novel and alternative explanation for the slow rates of trench migration and fast-moving plates observed globally at natural subduction zones.

010504 meteorology & atmospheric sciencesSubductionNumerical models010502 geochemistry & geophysics01 natural sciencesGeophysicsMantle convectionAsthenosphereOceanic crustLithosphereTransition zoneTrenchGeneral Earth and Planetary SciencesPetrologyGeology0105 earth and related environmental sciencesGeophysical Research Letters
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The tsunami phenomenon

2017

Abstract With human activity increasingly concentrating on coasts, tsunamis (from Japanese tsu = harbour, nami = wave) are a major natural hazard to today’s society. Stimulated by disastrous tsunami impacts in recent years, for instance in south-east Asia (2004) or in Japan (2011), tsunami science has significantly flourished, which has brought great advances in hazard assessment and mitigation plans. Based on tsunami research of the last decades, this paper provides a thorough treatise on the tsunami phenomenon from a geoscientific point of view. Starting with the wave features, tsunamis are introduced as long shallow water waves or wave trains crossing entire oceans without major energy l…

010504 meteorology & atmospheric sciencesSubmarineGeologyAquatic ScienceHazard analysis010502 geochemistry & geophysics01 natural sciencesWaves and shallow waterOceanographyWave shoalingNatural hazardSubmarine pipelineSedimentary rockTsunami earthquakeGeologySeismology0105 earth and related environmental sciencesProgress in Oceanography
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First study of the heat and gas budget for Sirung volcano, Indonesia

2017

International audience; With at least four eruptions over the last 20 years, Sirung is currently one of the more active volcanoes in Indonesia. However, due to its remoteness, very little is known about the volcano and its hyperacid crater lake. We report here on the first measurements of gas and heat emissions from the volcano. Notable is the substantial heat loss from the crater lake surface, amounting to 220 MW. In addition, 17 Gg of SO2, representing 0.8% of Indonesian volcanic SO2 contribution into the atmosphere, 11 Gg of H2S, 17 Gg of CO2, and 550 Gg of H2O are discharged into the atmosphere from the volcano annually. The volatiles degassed from Sirung magmas are subjected to hydroth…

010504 meteorology & atmospheric sciencesSulfideEarth science010502 geochemistry & geophysics01 natural sciencesHydrothermal circulationAtmosphereHeat loGeochemistry and PetrologyCrater lake[SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/VolcanologySedimentology0105 earth and related environmental scienceschemistry.chemical_classificationgeographygeography.geographical_feature_categoryLead (sea ice)Heat lossHeat lossesSirung volcanochemistryVolcano[SDU]Sciences of the Universe [physics]Degassing budgetCrater lakeGeologyBulletin of Volcanology
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Impulsive coronal heating from large-scale magnetic rearrangements: from IRIS to SDO/AIA

2019

The Interface Region Imaging Spectrograph (IRIS) has observed bright spots at the transition region footpoints associated with heating in the overlying loops, as observed by coronal imagers. Some of these brightenings show significant blueshifts in the Si iv line at 1402.77 A (logT[K] = 4.9). Such blueshifts cannot be reproduced by coronal loop models assuming heating by thermal conduction only, but are consistent with electron beam heating, highlighting for the first time the possible importance of non-thermal electrons in the heating of non-flaring active regions. Here we report on the coronal counterparts of these brightenings observed in the hot channels of the Atmospheric Imaging Assem…

010504 meteorology & atmospheric sciencesSun: activity Sun: corona Sun: UV radiation Astrophysics - Solar and Stellar AstrophysicsFOS: Physical sciencesAstrophysicsElectron01 natural sciences0103 physical sciencesmedicineAstrophysics::Solar and Stellar AstrophysicsIris (anatomy)010303 astronomy & astrophysicsSpectrographSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsAstronomy and AstrophysicsCoronal loopThermal conductionmedicine.anatomical_structureAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceCoronal planePhysics::Space PhysicsCathode rayAstrophysics::Earth and Planetary Astrophysics
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Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test

2018

Context. The determination from coronagraphic observations of physical parameters of the plasma embedded in coronal mass ejections (CMEs) is of crucial importance for our understanding of the origin and evolution of these phenomena. Aims. The aim of this work is to perform the first ever numerical simulations of a CME as it will be observed by future two-channel (visible light VL and UV Ly-α) coronagraphs, such as the Metis instrument on-board ESA-Solar Orbiter mission, or any other future coronagraphs with the same spectral band-passes. These simulations are then used to test and optimize the plasma diagnostic techniques to be applied to future observations of CMEs. Methods. The CME diagno…

010504 meteorology & atmospheric sciencesSun: coronal mass ejections (CMEs)Plasma parametersT-NDASContext (language use)Astrophysics01 natural sciencessymbols.namesakeMethods: data analysis0103 physical sciencesRadiative transferCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsQB Astronomydata analysis [Methods]010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesPhysicsUV radiation [Sun]numerical [Methods]Methods: numericalAstronomy and AstrophysicsPlasmaSun: UV radiationPolarization (waves)coronal mass ejections (CMEs) [Sun]Computational physicsQC PhysicsPlasmasSpace and Planetary SciencePhysics::Space PhysicssymbolsMagnetohydrodynamicsDoppler effectAstronomy & Astrophysics
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Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single Star and Binary Merger Progenitor Models for SN 1987A

2019

We perform three-dimensional hydrodynamic simulations of aspherical core-collapse supernovae focusing on the matter mixing in SN 1987A. The impacts of four progenitor (pre-supernova) models and parameterized aspherical explosions are investigated. The four pre-supernova models include a blue supergiant (BSG) model based on a slow merger scenario developed recently for the progenitor of SN 1987A (Urushibata et al. 2018). The others are a BSG model based on a single star evolution and two red supergiant (RSG) models. Among the investigated explosion (simulation) models, a model with the binary merger progenitor model and with an asymmetric bipolar-like explosion, which invokes a jetlike explo…

010504 meteorology & atmospheric sciencesSupergiant starAstrophysics::High Energy Astrophysical PhenomenaBinary numberchemistry.chemical_elementNeutron starFOS: Physical sciencesHydrodynamical simulationAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesCore-collapse supernovaeAstrophysics::Solar and Stellar AstrophysicsRed supergiant010303 astronomy & astrophysicsMixing (physics)HeliumStellar evolutionary modelSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesLine (formation)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astronomy and AstrophysicsSupernova dynamicSupernovaNeutron starchemistryAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceExplosive nucleosynthesisSupergiantAstrophysics - High Energy Astrophysical Phenomena
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Indication of a Pulsar Wind Nebula in the Hard X-Ray Emission from SN 1987A

2021

Since the day of its explosion, SN 1987A (SN87A) was closely monitored with the aim to study its evolution and to detect its central compact relic. The detection of neutrinos from the supernova strongly supports the formation of a neutron star (NS). However, the constant and fruitless search for this object has led to different hypotheses on its nature. Up to date, the detection in the ALMA data of a feature somehow compatible with the emission arising from a proto Pulsar Wind Nebula (PWN) is the only hint of the existence of such elusive compact object. Here we tackle this 33-years old issue by analyzing archived observations of SN87A performed Chandra and NuSTAR in different years. We fir…

010504 meteorology & atmospheric sciencesSupernova remnantsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSynchrotron radiationAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCompact starX-ray sources01 natural sciencesPulsar wind nebulaNeutron starsX-ray astronomy0103 physical sciencesPlasma astrophysicsEjectaX-ray point sources010303 astronomy & astrophysicsCompact objectsX-ray observatoriesShocksAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsX-ray astronomyAstronomy and AstrophysicsNeutron starSupernovaInterstellar synchrotron emissionSpace and Planetary ScienceNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Effect of soil management on soil erosion on sloping farmland during crop growth stages under a large-scale rainfall simulation experiment

2018

Soil erosion on farmland is a critical environmental issue and the main source of sediment in the Yellow River, China. Thus, great efforts have been made to reduce runoff and soil loss by restoring vegetation on abandoned farmland. However, few studies have investigated runoff and soil loss from sloping farmland during crop growth season. The objective of this study was to investigate the effects of soil management on runoff and soil loss on sloping farmland during crop growth season. We tested different soybean growth stages (i.e., seedling stage (R1), initial blossoming stage (R2), full flowering stage (R3), pod bearing stage (R4), and initial filling stage (R5)) and soil management pract…

010504 meteorology & atmospheric sciencesSòls ErosióManagement Monitoring Policy and Law01 natural sciencesRainwater harvestingSoil managementcrop growth stagessimulated rainfall0105 earth and related environmental sciencesEarth-Surface ProcessesWater Science and Technologysoil erosionbiologySowing04 agricultural and veterinary sciencesbiology.organism_classificationPE&RCTillageInfiltration (hydrology)Loess PlateauAgronomySeedling040103 agronomy & agriculturehoeing tillage0401 agriculture forestry and fisheriesEnvironmental scienceSurface runoffSoil conservationJournal of Arid Land
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FLEX/S3 Tandem Mission Performance Assessment: Evolution of the End-to-End Simulator Flex-E

2018

An End-to-end simulator (E2ES) is a tool to evaluate the performance of a satellite mission. Once a mission is approved for operation, E2ES evolves during Phase C/D to become a supporting tool for the development and validation of the ground data processor, as well as for simulating data sets to test the Prototype and Operational Processors. FLEX-E is the E2ES of the FLEX/Sentinel-3 tandem mission, which was selected in 2015 as ESA's eighth Earth Explorer. The FLEX-E evolution implies the consolidation of all the retrieval algorithms (e.g. fluorescence, reflectance, biophysical variables), the implementation of new scientific developments, as well the improvement of the co-registration proc…

010504 meteorology & atmospheric sciencesTandemComputer science0211 other engineering and technologiesAtmospheric correctionProcess (computing)02 engineering and technology01 natural sciencesData processing systemEnd-to-end principleFLEXSatelliteSimulation021101 geological & geomatics engineering0105 earth and related environmental sciencesIGARSS 2018 - 2018 IEEE International Geoscience and Remote Sensing Symposium
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Raindrop size distribution and terminal velocity for rainfall erosivity studies. A review

2019

Abstract The knowledge of the rainfall drop size distribution (DSD) at the land surface is essential for understanding precipitation mechanisms affecting soil erosion processes. Rainfall erosivity is defined as the potential of rain to cause erosion and it can be evaluated by rainfall kinetic power, which is determined by DSD and raindrop terminal velocity. This paper firstly deals with the raindrop terminal velocity estimate. Then the most widely used DSD are reviewed highlighting the difference between the raindrop size distribution per unit volume of air and that per unit area and time. The reliability of the available kinetic power-rainfall intensity relationships and their application …

010504 meteorology & atmospheric sciencesTerminal velocityRaindrop size distribution0207 environmental engineering02 engineering and technologyRainfall erosivitySeasonalitySeasonalityKinetic energyAtmospheric sciencesmedicine.disease01 natural sciencesRainfall kinetic powerDisdrometerDistribution (mathematics)ErosionmedicineEnvironmental scienceSettore AGR/08 - Idraulica Agraria E Sistemazioni Idraulico-ForestaliPrecipitationRainfall intensity020701 environmental engineeringIntensity (heat transfer)0105 earth and related environmental sciencesWater Science and Technology
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