Search results for "RADIATION"

showing 10 items of 5298 documents

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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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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Observation of classically 'forbidden' electromagnetic wave propagation and implications for neutrino detection.

2018

Ongoing experimental efforts in Antarctica seek to detect ultra-high energy neutrinos by measurement of radio-frequency (RF) Askaryan radiation generated by the collision of a neutrino with an ice molecule. An array of RF antennas, deployed either in-ice or in-air, is used to infer the properties of the neutrino. To evaluate their experimental sensitivity, such experiments require a refractive index model for ray tracing radio-wave trajectories from a putative in-ice neutrino interaction point to the receiving antennas; this gives the degree of signal absorption or ray bending from source to receiver. The gradient in the density profile over the upper 200 meters of Antarctic ice, coupled wi…

010504 meteorology & atmospheric sciencesWave propagationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciencesElectromagnetic radiationAtomicIce shelfParticle and Plasma Physics0103 physical sciencesddc:530NuclearInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics::Atmospheric and Oceanic Physics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)geographygeography.geographical_feature_categoryultra high energy photons and neutrinos010308 nuclear & particles physicsMolecularAstronomy and AstrophysicsNuclear & Particles PhysicsComputational physicsRay tracing (physics)Radio propagationNeutrino detectorcosmic ray experimentsNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstronomical and Space SciencesRadio wave
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Line parameters and shapes of high clusters: R-branch of the nu3 band of CH4 in He mixtures

2002

International audience; The IR absorption spectra of CH4 in pure gas and in mixture with helium were studied in the region of nu3 band at higher J line clusters R(17)-R(22). The frequencies and intensities of rotation-vibration lines were estimated from the experimental spectra at Doppler shape conditions. The line frequencies and intensities were calculated and used for the attribution of overlapped lines in clusters. The calculated line intensities are close to the experimental values. The calculated frequency structure of the higher J manifolds are somewhat wider than the observed one. The shapes of helium-broadened line clusters were compared with those calculated accounting for line mi…

010504 meteorology & atmospheric sciences[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]chemistry.chemical_elementSemiclassical physics01 natural sciencesSpectral linesymbols.namesakeLine parameters[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesRelaxation matrixSpectroscopyMixing (physics)Helium0105 earth and related environmental sciencesLine (formation)PhysicsRadiationIr absorption010304 chemical physicsVibration-rotation spectraLine mixingAtomic and Molecular Physics and OpticschemistrysymbolsAtomic physicsDoppler effectMethane
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Natural gas hydrate investigations by synchrotron radiation X-ray cryo-tomographic microscopy (SRXCTM)

2008

[1] We report the 3D microstructure analyses of natural gas hydrates sampled from Gulf of Mexico. The samples were characterized by synchrotron radiation X-ray cryo-tomographic microscopy (SRXCTM) using the ‘TOMCAT’ beam line at the Swiss Light Source (SLS). The SRXCTM demonstrates its applicability to unlock some microscopic features of the marine hydrates, in particular of crystallite size and grain boundary network. The gas hydrate domains are surrounded by a network of pores of typically a few micrometers, which are largely due to decomposition. Out of the SRXCTM data, the porosity, total volume of the voids, the void surface area and number of the total gas-filled voids have been calcu…

010504 meteorology & atmospheric sciencesbusiness.industryClathrate hydrateSynchrotron radiationMineralogy010502 geochemistry & geophysics01 natural sciencesGeophysicsNatural gasGeneral Earth and Planetary SciencesGrain boundaryCrystallitePorositybusinessHydrateGeologySwiss Light Source0105 earth and related environmental sciencesGeophysical Research Letters
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Gravitational wave signature of proto-neutron star convection: I. MHD numerical simulations

2021

Gravitational waves provide a unique and powerful opportunity to constrain the dynamics in the interior of proto-neutron stars during core collapse supernovae. Convective motions play an important role in generating neutron stars magnetic fields, which could explain magnetar formation in the presence of fast rotation. We compute the gravitational wave emission from proto-neutron star convection and its associated dynamo, by post-processing three-dimensional MHD simulations of a model restricted to the convective zone in the anelastic approximation. We consider two different proto-neutron star structures representative of early times (with a convective layer) and late times (when the star is…

010504 meteorology & atmospheric sciencesdimension: 3neutron star: magnetic fieldtorusAstrophysicsMagnetar01 natural sciencesrotationstarstrong fieldMagnetarsAstrophysics::Solar and Stellar Astrophysicsgravitational radiation: spectrumgravitational radiation: signatureSupernova core collapse010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMethods numerical[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]formationscalingSupernovaAmplitudeAstrophysics - Solar and Stellar AstrophysicsConvection zoneAstrophysics - High Energy Astrophysical PhenomenaDynamosupernova: collapseprotoneutron starFOS: Physical sciencesConvectionsymmetry: axialGravitational waves0103 physical sciencesstructurenumerical calculationsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesGravitational waveAstronomy and AstrophysicsmagnetarNeutron star13. Climate actionSpace and Planetary Scienceefficiencygravitational radiation: emissionMagnetohydrodynamics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph][PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]
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How much is enough? : The convergence of finite sample scattering properties to those of infinite media

2021

We study the scattering properties of a cloud of particles. The particles are spherical, close to the incident wavelength in size, have a high albedo, and are randomly packed to 20% volume density. We show, using both numerically exact methods for solving the Maxwell equations and radiative-transfer-approximation methods, that the scattering properties of the cloud converge after about ten million particles in the system. After that, the backward-scattered properties of the system should estimate the properties of a macroscopic, practically infinite system. (C) 2021 The Authors. Published by Elsevier Ltd. This is an open access article under the CC BY-NC-ND license (http://creativecommons.o…

010504 meteorology & atmospheric scienceseducationparticulate random mediapienhiukkasetoptiset ominaisuudet01 natural sciences114 Physical sciencesVolume densityScatteringsymbols.namesakelaskennallinen tiedeConvergence (routing)Radiative transferRadiative transferMaxwellin yhtälötsirontaSpectroscopy0105 earth and related environmental sciencesPhysicsRadiationScatteringscatteringAlbedoSample (graphics)Atomic and Molecular Physics and OpticsComputational physicsWavelengthMaxwell's equationsMaxwell equationsradiative transferParticulate random mediasymbolsapproksimointi
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Characterization of a Newly Developed Aircraft-Based Laser Ablation Aerosol Mass Spectrometer (ALABAMA) and First Field Deployment in Urban Pollution…

2011

We present here the development and first field deployment of a novel Aircraft-based Laser ABlation Aerosol MAss spectrometer (ALABAMA), which is capable of measuring the chemical composition and size of individual ambient aerosol particles in the size range between 150 and 900 nm. The instrument uses a continuous wave 532 nm laser to size and detect the particles, a pulsed 266 nm laser to ablate and ionize the particles, and a bipolar, Z-shaped time-of-flight mass spectrometer to detect positive and negative ions. The ALABAMA fits into a 19"-aircraft rack of 150 cm height and has a total weight of 140 kg, thus currently being one of the smallest and lightest-weight instruments of its type.…

010504 meteorology & atmospheric sciencesinstrument developmentaerosolMineralogy01 natural scienceslaw.inventionOpticslawparticle composition11. SustainabilityEnvironmental ChemistryGeneral Materials ScienceParticle beam0105 earth and related environmental sciencesRange (particle radiation)Laser ablationbusiness.industryChemistry010401 analytical chemistryAtmosphärische SpurenstoffeLaserPollution0104 chemical sciencesAerosol13. Climate actionMass spectrumParticleParticle sizeAerosol Mass spectrometerbusinessAerosol Science and Technology
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Les Ammonoïdes (Mollusca, Cephalopoda) : avancées et contributions récentes à la paléobiologie évolutive.

2009

12 pages; Les ammonoïdes qui perdurent 335 Ma constituent un modèle de choix dans l'analyse du fait évolutif. Cet article de synthèse se propose d'aborder (1) : leur place phylogénétique au sein des céphalopodes et le choix d'un modèle actuel de référence ; (2) : la construction d'espaces phénotypiques qui offrent un angle d'étude pertinent de l'évolution biologique ; (3) : les concordances et discordances entre reconstruction phylogénétique et registre fossile et (4) : les reconquêtes postcrises, modèles d'étude de l'évolution à grande échelle. Il ressort que les ammonoïdes peuvent servir d'appui à de nombreuses thématiques paléontologiques (dynamique de la biodiversité, analyse phylogénét…

010506 paleontologyPhylogénieCrise et radiationÉvolutionBiostratigraphy010502 geochemistry & geophysics01 natural sciencesTetrabranchiataAmmonoïdeAllométrieMesozoicRegistre fossile0105 earth and related environmental sciences[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/PaleontologyFossil Recordbiology[SDV.BID.EVO]Life Sciences [q-bio]/Biodiversity/Populations and Evolution [q-bio.PE]General EngineeringAmmonoideabiology.organism_classificationGeography[ SDV.BID.EVO ] Life Sciences [q-bio]/Biodiversity/Populations and Evolution [q-bio.PE]Crise et radiation.Espace morphologique[SDU.STU.PG]Sciences of the Universe [physics]/Earth Sciences/PaleontologyHumanities
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Electron Paramagnetic Resonance and petrographic analysis for dating Mesolithic and Neolithic pottery from Al Khiday (Sudan)

2016

Abstract Electron Paramagnetic Resonance (EPR) dating, like luminescence techniques, is based on the time-dependent accumulation of trapped charges at mineral defect centres. However, Fe(III) ions prevent the common Continuous Wave (CW-EPR) approach for dating pottery, which always contains iron. The Pulsed method (ED-EPR) allowed this limitation to be overcome, with recording of radiation-induced defect signals, as shown by increased signal intensity after artificial irradiation of samples. The method was applied to studying Mesolithic and Neolithic pottery from Al Khiday (Central Sudan), characterized by quartz-rich tempers and coming from dated contexts. As the occurrence of a natural ED…

010506 paleontologyRadiation060102 archaeologyAl Khiday; EPR dating; Prehistoric pottery; Quartz; Radiation; InstrumentationMineralogy06 humanities and the artsQuartz01 natural sciencesEPR datinglaw.inventionPetrographylawPrehistoric pottery0601 history and archaeologyPotterySignal intensityElectron paramagnetic resonanceAl KhidayQuartzInstrumentationGeologyMesolithic0105 earth and related environmental sciences
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