Search results for "Particle"

showing 10 items of 15225 documents

Ray optics for absorbing particles with application to ice crystals at near-infrared wavelengths

2018

Abstract Light scattering by particles large compared to the wavelength of incident light is traditionally solved using ray optics which considers absorption inside the particle approximately, along the ray paths. To study the effects rising from this simplification, we have updated the ray-optics code SIRIS to take into account the propagation of light as inhomogeneous plane waves inside an absorbing particle. We investigate the impact of this correction on traditional ray-optics computations in the example case of light scattering by ice crystals through the extended near-infrared (NIR) wavelength regime. In this spectral range, ice changes from nearly transparent to opaque, and therefore…

010504 meteorology & atmospheric sciencesOpacityspektroskopiaIce crystalsPhysics::OpticsRay optics01 natural sciencesPOLARIZED-LIGHT SCATTERING114 Physical sciencesLight scattering010309 opticsScatteringMEDIAOptics0103 physical sciencesABSORPTIONInhomogeneous wavesCIRRUSray opticsSpectroscopy0105 earth and related environmental sciencesPhysicsta113absorbing mediaRadiationta115Geometrical opticsIce crystalsta114Scatteringbusiness.industryscatteringCLOUDSkiteetRayAtomic and Molecular Physics and OpticsoptiikkaSOLAR-RADIATIONWavelengthMAXWELLS EQUATIONSAbsorbing mediainhomogeneous wavesLight scattering by particlesPHASE MATRIXGEOMETRIC-OPTICSbusinessice crystalsAPPROXIMATION
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A Search for IceCube Events in the Direction of ANITA Neutrino Candidates

2020

During the first three flights of the Antarctic Impulsive Transient Antenna (ANITA) experiment, the collaboration detected several neutrino candidates. Two of these candidate events were consistent with an ultra-high-energy up-going air shower and compatible with a tau neutrino interpretation. A third neutrino candidate event was detected in a search for Askaryan radiation in the Antarctic ice, although it is also consistent with the background expectation. The inferred emergence angle of the first two events is in tension with IceCube and ANITA limits on isotropic cosmogenic neutrino fluxes. Here, we test the hypothesis that these events are astrophysical in origin, possibly caused by a po…

010504 meteorology & atmospheric sciencesPoint sourceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)Tau neutrino0103 physical sciencesTRACK RECONSTRUCTIONSource spectrum010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEIsotropyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicshep-phHigh Energy Physics - PhenomenologyAir showerPhysics and Astronomy13. Climate actionSpace and Planetary ScienceNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)
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The influence of the wind direction and plants on the variability of topsoil magnetic susceptibility in industrial and urban areas of southern Poland

2016

Volume magnetic susceptibility (κ) was measured on the soil surface and in the vertical topsoil profile within a 300 km2 area located in an urban-industrial conurbation. The results were compared to plant species compositions in the forest storeys, elevation above sea level, and terrain geomorphology. The content and mineral composition of the magnetic fraction were determined in the soil horizons. It was found that the extent of the area with enhanced topsoil magnetic susceptibility was similar to the dominant wind direction (south–west). Enhanced κ values were observed for the soil at the forest margin on the leeward side of the emitters as well as at sites located on exposed local elevat…

010504 meteorology & atmospheric sciencesSoil ScienceSoil science010501 environmental sciencesFraxinus01 natural sciencesforest topsoil IPrevailing windsEnvironmental ChemistrySea level0105 earth and related environmental sciencesEarth-Surface ProcessesWater Science and Technologypollution distributionGlobal and Planetary ChangeTopsoilbiologytechnogenic magnetic particlesGeologyWind directionbiology.organism_classificationPollutionDeciduousLitterEnvironmental scienceSoil horizonmagnetic susceptibilityEnvironmental Earth Sciences
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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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Modelling of stylolite geometries and stress scaling

2012

International audience; In this contribution we present numerical simulations of stylolite growth to decipher the effects of initial rock heterogeneity and stress on their morphology. We show that stylolite growth in a rock with a uniform grain size produces different patterns than stylolite growth in a rock with a bimodal grain size distribution. Strong pinning of large heterogeneities produce stylolite structures that are dominated by pronounced teeth, whereas a uniform grain size leads to spikes and a roughness that shows variable wavelengths. We compare the simulated stylolites with natural examples and show that the model can reproduce the real structures. In addition we show that stro…

010504 meteorology & atmospheric sciences[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]stress-gauge[SDE.MCG]Environmental Sciences/Global ChangesCompaction[SDU.STU]Sciences of the Universe [physics]/Earth Sciences[PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]Surface finishpressure solution010502 geochemistry & geophysics01 natural sciencesPhysics::Geophysics[PHYS.MECA.MEMA]Physics [physics]/Mechanics [physics]/Mechanics of materials [physics.class-ph]Stress (mechanics)Geochemistry and Petrology[SPI.MECA.MEMA]Engineering Sciences [physics]/Mechanics [physics.med-ph]/Mechanics of materials [physics.class-ph]Earth and Planetary Sciences (miscellaneous)compactionGeotechnical engineeringScaling0105 earth and related environmental sciencesstyloliteMechanicsself-affinityGrain sizeGeophysicsSpace and Planetary ScienceStyloliteParticle-size distributionPressure solutionnumerical modelGeology[SDU.STU.MI]Sciences of the Universe [physics]/Earth Sciences/MineralogyEarth and Planetary Science Letters
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Personal Exposure to Ultrafine Particles According to Different Environments and Modes of Transport in Schoolchildren: Results from a Spanish Cohort …

2017

Background Combustion, especially in diesel engines, emits a complex mixture of gases and particles that could be harmful for the respiratory and cardiovascular systems. Daily personal exposure to the smallest particulate matter (less than 0.1 µm and usually called nanoparticles or ultrafine particles – UFP) has been studied to a lesser extent compared to coarser particles. In this study we aim to assess personal exposure to UFP in different environments and transport modes among schoolchildren from a Spanish birth-cohort in the province of Valencia. Methods The study population consisted of 114 children aged 10-11 years. For each of them, personal exposure to UFP was measured continuously …

010504 meteorology & atmospheric sciencesbusiness.industryCold seasonHealth PolicyPublic Health Environmental and Occupational HealthTransportation010501 environmental sciences01 natural sciencesPollutionExposure levelEnvironmental healthUltrafine particleCohortMedicineSafety Risk Reliability and QualitybusinessSafety ResearchExposure dataSimulation0105 earth and related environmental sciencesJournal of Transport & Health
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Models and data analysis tools for the Solar Orbiter mission

2020

All authors: Rouillard, A. P.; Pinto, R. F.; Vourlidas, A.; De Groof, A.; Thompson, W. T.; Bemporad, A.; Dolei, S.; Indurain, M.; Buchlin, E.; Sasso, C.; Spadaro, D.; Dalmasse, K.; Hirzberger, J.; Zouganelis, I.; Strugarek, A.; Brun, A. S.; Alexandre, M.; Berghmans, D.; Raouafi, N. E.; Wiegelmann, T.; Pagano, P.; Arge, C. N.; Nieves-Chinchilla, T.; Lavarra, M.; Poirier, N.; Amari, T.; Aran, A.; Andretta, V.; Antonucci, E.; Anastasiadis, A.; Auchère, F.; Bellot Rubio, L.; Nicula, B.; Bonnin, X.; Bouchemit, M.; Budnik, E.; Caminade, S.; Cecconi, B.; Carlyle, J.; Cernuda, I.; Davila, J. M.; Etesi, L.; Espinosa Lara, F.; Fedorov, A.; Fineschi, S.; Fludra, A.; Génot, V.; Georgoulis, M. K.; Gilbe…

010504 meteorology & atmospheric sciencescorona [Sun]Solar windAstrophysics[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph]7. Clean energy01 natural scienceslaw.inventionData acquisitionlawCoronal mass ejectiongeneral [Sun]QB AstronomyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSun: magnetic fieldsQCComputingMilieux_MISCELLANEOUSQBPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]3rd-DASenergetic particlesSolar windCORONAL MASS EJECTIONSnumerical modelingmagnetic fields [Sun]solar windPhysics::Space PhysicsSystems engineeringAstrophysics::Earth and Planetary Astrophysicsatmosphere [Sun]fundamental parameters [Sun]Sun: generalFORCE-FREE FIELDSun: fundamental parametersSolar radiusContext (language use)STREAMER STRUCTUREOrbiter0103 physical sciencesOPTIMIZATION APPROACH[SDU.ASTR.SR] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]POLARIZATION MEASUREMENTSSun: Solar wind3-DIMENSIONAL STRUCTURE0105 earth and related environmental sciencesSpacecraftbusiness.industrySun: corona[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]solar coronaMAGNETIC-FLUX ROPESAstronomy and AstrophysicsSHOCKS DRIVEN115 Astronomy Space scienceSPECTRAL-LINESQC Physics13. Climate actionSpace and Planetary SciencebusinessHeliosphereSun: atmosphereELECTRON-DENSITY
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GRB 050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang

2005

We present optical and near-infrared observations of the afterglow of the gamma-ray burst GRB 050904. We derive a photometric redshift z = 6.3, estimated from the presence of the Lyman break falling between the I and J filters. This is by far the most distant GRB known to date. Its isotropic-equivalent energy is 3.4x10^53 erg in the rest-frame 110-1100 keV energy band. Despite the high redshift, both the prompt and the afterglow emission are not peculiar with respect to other GRBs. We find a break in the J-band light curve at t_b = 2.6 +- 1.0 d (observer frame). If we assume this is the jet break, we derive a beaming-corrected energy E_gamma = (4-12)x10^51 erg. This limit shows that GRB 050…

010504 meteorology & atmospheric sciencesgamma rays: burstsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsJet (particle physics)Astrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]gamma rays: individual: GRB 0509040103 physical sciences010303 astronomy & astrophysics0105 earth and related environmental sciencesPhotometric redshiftPhysicsCOSMIC cancer database[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Star formationAstrophysics (astro-ph)Astronomy and Astrophysicsearly UniverseLight curveRedshiftAfterglowSpace and Planetary Sciencecosmology: observationsGamma-ray burst
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Implementation of a comprehensive ice crystal formation parameterization for cirrus and mixed-phase clouds in the EMAC model (based on MESSy 2.53)

2018

A comprehensive ice nucleation parameterization has been implemented in the global chemistry-climate model EMAC to improve the representation of ice crystal number concentrations (ICNCs). The parameterization of Barahona and Nenes (2009, hereafter BN09) allows for the treatment of ice nucleation taking into account the competition for water vapour between homogeneous and heterogeneous nucleation in cirrus clouds. Furthermore, the influence of chemically heterogeneous, polydisperse aerosols is considered by applying one of the multiple ice nucleating particle parameterizations which are included in BN09 to compute the heterogeneously formed ice crystals. BN09 has been modified in order to co…

010504 meteorology & atmospheric sciencesglobal climate modelNucleationMineral dustnucleation parameterizations010502 geochemistry & geophysicsAtmospheric sciences01 natural sciencesempirical parameterizationTroposphereinsoluble particlesddc:5500105 earth and related environmental sciencesmineral dustIce crystalssubmodel system messylcsh:QE1-996.5Northern Hemisphereatmospheric aerosollcsh:Geology13. Climate actionupper troposphereIce nucleusEnvironmental scienceCirrustransport sectorsWater vapordroplet number concentration
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The chronic effects of fullereneC 60 -associated sediments in the midge Chironomus riparius – Responses in the first and the second generation

2017

Abstract The life cycle parameters of the benthic invertebrate Chironomus riparius make it a relevant organism for use in multi-generation chronic ecotoxicology tests. Since studies on chronic exposures with fullerene carbon nanoparticles have revealed adverse effects at lower concentration ranges, it is crucial to gain understanding of the consequences in following generations. The aims of this study were to investigate whether sediment-associated fullereneC 60 impacts on C. riparius emergence and breeding, thus affecting the growth of the second generation. Larvae were exposed to fullerene-spiked sediment at concentrations of 0.5, 10 and 40 mg/kg sediment dw. Total emergence and breeding …

010504 meteorology & atmospheric scienceshiilienvironmental effectsHealth Toxicology and Mutagenesista1172Populationved/biology.organism_classification_rank.speciesZoologymyrkyllisyys010501 environmental sciencesBiologyToxicology01 natural sciencesToxicologyzoobenthosEcotoxicologyeducation0105 earth and related environmental sciencesInvertebrateChironomus ripariuseducation.field_of_studyLarvaved/biologycarbonfullerenestoxicitySedimentGeneral Medicineselkärangattomatinvertebratesbiology.organism_classificationPollutionpohjaeläimistöfullereenitympäristövaikutuksetMidgeta1181nanohiukkasetnanoparticlesEcotoxicityEnvironmental Pollution
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