Search results for " env"

showing 10 items of 20374 documents

Mountain Building in Taiwan: Insights From 3‐D Geodynamic Models

2019

Taiwan is widely considered to be a typical example of an arc-continent collision surrounded by two opposite dipping subduction zones. The manner by which the interaction of the two neighboring slabs caused plate collision and mountain building is insufficiently understood. Various hypotheses have been proposed, but the geodynamic feasibility of those remains to be tested. Here we present 3-D thermomechanical models to study the geodynamic evolution process of a Taiwan-like setting after an initial transform fault was consumed. In our model setup, the boundary between the Eurasian plate and the South China Sea is northeast trending. The results show that all simulations result in toroidal m…

010504 meteorology & atmospheric sciencesSubductionContinental crustEurasian PlateTransform faultCrust01 natural sciencesGeophysicsMountain formationSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)ErosionSlabSeismologyGeology0105 earth and related environmental sciencesJournal of Geophysical Research: Solid Earth
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A geotraverse across two paleo-subduction zones in Tien Shan, Tajikistan

2017

Abstract We present first LA-ICP-MS U–Pb zircon ages as well as geochemical and Sr–Nd–Pb isotope data for 14 magmatic rocks collected along ca. 400 km profile across the Chatkal-Kurama terrane in the Mogol-Tau and Kurama ranges and the Gissar Segment of the Tien Shan orogen in Tajikistan. These new data from supra-subduction and post-collisional magmatic rocks of two Late Paleozoic active margins constrain a tectonic model for terrane motions across two paleo-subduction zones: (1) The 425 Ma old Muzbulak granite of the Mogol-Tau range formed in a supra-subduction setting at the northern margin of the Turkestan Ocean. The north-dipping plate was subducted from the Early Silurian to the earli…

010504 meteorology & atmospheric sciencesSubductionContinental crustGeochemistryGeology010502 geochemistry & geophysicsOphiolite01 natural sciencesBatholithPassive marginCarboniferousGeology0105 earth and related environmental sciencesTerraneZircon
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Whole-rock Nd–Hf isotopic study of I-type and peraluminous granitic rocks from the Chinese Altai: Constraints on the nature of the lower crust and te…

2017

Abstract The nature of the lower crust and tectonic setting of the Chinese Altai in the early to middle Paleozoic are still hotly debated. Decoupling between zircon Hf and whole-rock Nd isotopic systems for granites results in different interpretations for the above issues. In order to solve the problem, whole-rock Nd–Hf isotopic analyses were conducted on representative early to middle Paleozoic I-type granite and strongly peraluminous granites and rhyolites from the Chinese Altai. The I-type granites show metaluminous to weakly peraluminous feature and have eNd(t) values ranging from − 2.2 to + 0.8 and eHf(t) from + 3.9 to + 12.9, respectively. The strongly peraluminous granites and rhyol…

010504 meteorology & atmospheric sciencesSubductionMantle wedgeGeochemistryGeologyCrust010502 geochemistry & geophysics01 natural sciencesBasement (geology)MagmaIsland arcMetasomatismGeology0105 earth and related environmental sciencesZirconGondwana Research
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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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