Search results for "COSMIC"

showing 10 items of 656 documents

EDGE: explorer of diffuse emission and gamma-ray burst explosions

2009

How structures on various scales formed and evolved from the early Universe up to present time is a fundamental question of astrophysical cosmology. EDGE will trace the cosmic history of the baryons from the early generations of massive star by Gamma-Ray Burst (GRB) explosions, through the period of cluster formation, down to very low redshifts, when between a third and one half of the baryons are expected to reside in cosmic filaments undergoing gravitational collapse by dark matter (Warm Hot Intragalactic Medium: WHIM). In addition EDGE, with its unprecedented observational capabilities, will provide key results on several other topics. The science is feasible with a medium class mission …

Vision[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Warm–hot intergalactic mediumAstrophysicsAstrophysics7. Clean energy01 natural sciencesCosmologySettore FIS/05 - Astronomia E AstrofisicaIntergalactic MediumWarm-Hot Intergalactic MediumX-rays Cosmology Clusters Gamma-ray bursts Warm-hot intergalactic medium Missions010303 astronomy & astrophysicsX-ray telescopesX-rays; Cosmology; Clusters; Gamma-ray bursts; Warm– hot intergalactic medium; MissionsPhysicsEquipment and servicesSatellite MissionSpectrometersAstrophysics (astro-ph)X-rays Cosmology Clusters Gamma-ray bursts Warm– hot intergalactic medium MissionsTemperatureAstrophysics::Instrumentation and Methods for AstrophysicsCosmologyGamma-ray burstsCosmic VisionSpectral resolutionGalaxy ClustersAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesWarm&ndashAstrophysics::Cosmology and Extragalactic AstrophysicsMissionshot intergalactic mediumAbsorptionNO010309 opticsX-rayClustersWarm–hot intergalactic mediumGalaxy groups and clusters0103 physical sciencesX-raysGalaxy groups and clustersImaging systems010306 general physicsGamma-ray burstWarm&ndashGalaxy clusterSpatial resolutionSensorsAstronomyX-rays clusters Gamma-Ray Bursts Warm-Hot Intergalactic Medium missionsAstronomy and AstrophysicsGalaxyRedshiftCluster13. Climate actionSpace and Planetary ScienceGamma-ray burstOptics for EUV, X-Ray, and Gamma-Ray Astronomy III. Edited by O'Dell, Stephen L.; Pareschi, Giovanni. Proceedings of the SPIE
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Diffuse soil CO2 degassing from Linosa island

2014

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Volcano monitoringLineamentGeochemistrysoil degassingfluid geochemistryCO2lcsh:QC851-999Instruments and techniques; Soil degassing; Volcano monitoring; GeophysicsSequential Gaussian simulationSoil co2 fluxFlux (metallurgy)Soil degassingGeomorphologygeographygeography.geographical_feature_categoryRiftlcsh:QC801-809Instruments and techniquesSettore GEO/08 - Geochimica E VulcanologiaTectonicslcsh:Geophysics. Cosmic physicsGeophysicsVolcanoLinosaSoil CO_2 fluxlcsh:Meteorology. ClimatologyGeologyChannel (geography)
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Continuous SO2 flux measurements for Vulcano Island, Italy

2012

<p>The La Fossa cone of Vulcano Island (Aeolian Archipelago, Italy) is a closed conduit volcano. Today, Vulcano Island is characterized by sulfataric activity, with a large fumarolic field that is mainly located in the summit area. A scanning differential optical absorption spectroscopy instrument designed by the Optical Sensing Group of Chalmers University of Technology in Göteborg, Sweden, was installed in the framework of the European project "Network for Observation of Volcanic and Atmospheric Change", in March 2008. This study presents the first dataset of SO<sub>2</sub> plume fluxes recorded for a closed volcanic system. Between 2008 and 2010, the SO<sub>2</…

Vulcano Islanddata setSO2lcsh:QC851-999fumaroleNetwork for Observation of Volcanic and Atmospheric ChangeVulcanoFlux (metallurgy)Optical sensingemissionsulfur dioxideSicilyGeomorphologyAeolian archipelagoLipari Islandvolcanology Fossa Cratergeographygeography.geographical_feature_categoryplumeDifferential optical absorption spectroscopylcsh:QC801-809Atmospheric changedegassingSettore GEO/08 - Geochimica E VulcanologiaPlumelcsh:Geophysics. Cosmic physicsGeophysicsOceanographyDifferential optical absorption spectroscopyItalyVolcanoMessina [Sicily]lcsh:Meteorology. ClimatologyGeologyAnnals of Geophysics
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A multiscale method for gamma/h discrimination in extensive air showers

2011

We present a new method for the identification of extensive air showers initiated by different primaries. The method uses the multiscale concept and is based on the analysis of multifractal behaviour and lacunarity of secondary particle distributions together with a properly designed and trained artificial neural network. The separation technique is particularly suited for being applied when the topology of the particle distribution in the shower front is as largely detailed as possible. Here, our method is discussed and applied to a set of fully simulated vertical showers in the experimental framework of ARGO-YBJ, taking advantage of both the space and time distribution of the detected sec…

Wavelet MethodNeural NetworksCosmic Rays; Extensive Air Showers; Multiscale Analysis; Wavelet Methods; Neural NetworksMultiscale AnalysiSettore FIS/01 - Fisica SperimentaleExtensive Air ShowerCosmic Ray
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ATHENA WFI optical blocking filters development status toward the end of the instrument phase-A

2018

Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. The Wide Field Imager (WFI) is one of the two instruments of the ATHENA astrophysics space mission approved by ESA as the second large mission in the Cosmic Vision 2015-2025 Science Programme. The WFI, based on a large array of depleted field effect transistors (DEPFET), will provide imaging in the 0.2-15 keV band over a 40'x40' field of view, simultaneously with spectrally an…

X-ray detectorCosmic VisionPhotonX-ray detectorWide Field ImagerField of viewCondensed Matter Physic7. Clean energy01 natural sciences010309 opticsX-ray astronomyOpticsSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesAthenaSpectral resolutionElectrical and Electronic EngineeringOptical blocking filter010303 astronomy & astrophysicsPhysicsCMOS sensorbusiness.industryElectronic Optical and Magnetic MaterialDetectorComputer Science Applications1707 Computer Vision and Pattern RecognitionPhoton countingApplied MathematicActive pixel sensor13. Climate actionbusinessDEPFET
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ATHENA X-IFU thermal filters development status toward the end of the instrument phase-A

2018

Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. The X-ray Integral Field Unit (X-IFU) is one of the two instruments of the Athena astrophysics space mission approved by ESA in the Cosmic Vision 2015-2025 Science Programme. The X-IFU consists of a large array of transition edge sensor micro-calorimeters that will operate at 100 mK inside a sophisticated cryostat. A set of thin filters, highly transparent to X-rays, will be m…

X-ray detectorCryostatCosmic VisionPhotonComputer scienceShieldsCondensed Matter Physicmicrocalorimeter01 natural sciences7. Clean energySettore FIS/05 - Astronomia E AstrofisicaX-ray Integral Field Unit (X-IFU)0103 physical sciencesthermal thin-film filterElectrical and Electronic EngineeringAerospace engineering010306 general physics010303 astronomy & astrophysicsbusiness.industryElectronic Optical and Magnetic MaterialDetectorAstrophysics::Instrumentation and Methods for AstrophysicsShot noiseComputer Science Applications1707 Computer Vision and Pattern RecognitionTransition Edge SensorApplied MathematicATHENA X-ray observatoryRadio frequencyTransition edge sensorbusinessSpace Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
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The LOFT mission concept: a status update

2016

The Large Observatory For x-ray Timing (LOFT) is a mission concept which was proposed to ESA as M3 and M4 candidate in the framework of the Cosmic Vision 2015-2025 program. Thanks to the unprecedented combination of effective area and spectral resolution of its main instrument and the uniquely large field of view of its wide field monitor, LOFT will be able to study the behaviour of matter in extreme conditions such as the strong gravitational field in the innermost regions close to black holes and neutron stars and the supra-nuclear densities in the interiors of neutron stars. The science payload is based on a Large Area Detector (LAD, >8m2 effective area, 2-30 keV, 240 eV spectral resolut…

X-ray timing[ SDU.ASTR.GA ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Field of viewAstrophysics01 natural scienceslaw.inventionlawObservatorytiming010303 astronomy & astrophysicsQBPhysicsmicrochannel plates. PROPORTIONAL COUNTER ARRAYCALIBRATIONX-ray astronomyElectronic Optical and Magnetic MaterialApplied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science Applications1707 Computer Vision and Pattern RecognitionX-ray detectorsCondensed Matter Physicscompact objectsX-ray spectroscopy[SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]spectroscopyCosmic Vision[ INFO ] Computer Science [cs]Silicon detectorAstrophysics::High Energy Astrophysical PhenomenaCondensed Matter PhysicTelescopeX-rayX-ray astronomySilicon detectors; spectroscopy; timing; X-ray astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Applied Mathematics; Electrical and Electronic EngineeringSettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesElectronic[INFO]Computer Science [cs]Optical and Magnetic MaterialsSpectral resolutionElectrical and Electronic EngineeringDETECTORta115X-ray astronomy Silicon detectors timing spectroscopy010308 nuclear & particles physicsX-ray imagingX-ray timing; X-ray spectroscopy; X-ray imaging; compact objects; X-ray detectors; microchannel plates. PROPORTIONAL COUNTER ARRAY; CALIBRATION; DETECTORApplied MathematicNeutron starQB460-466 AstrophysicsSilicon detectors; spectroscopy; timing; X-ray astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringSilicon detectors; spectroscopy; timing; X-ray astronomySilicon detectorsLarge Observatory For x-ray Timing (LOFT) Large Area Detector (LAD) Wide Field Monitor (WFM) Large Area Silicon Drift Detectors (SDD)Gamma-ray burst
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Bayesian chronological analyses consistent with synchronous age of 12,835-12,735 Cal BP for Younger Dryas boundary on four continents

2015

The Younger Dryas impact hypothesis posits that a cosmic impact across much of the Northern Hemisphere deposited the Younger Dryas boundary (YDB) layer, containing peak abundances in a variable assemblage of proxies, including magnetic and glassy impact-related spherules, high-temperature minerals and melt glass, nanodiamonds, carbon spherules, aciniform carbon, platinum, and osmium. Bayesian chronological modeling was applied to 354 dates from 23 stratigraphic sections in 12 countries on four continents to establish a modeled YDB age range for this event of 12,835-12,735 Cal B.P. at 95% probability. This range overlaps that of a peak in extraterrestrial platinum in the Greenland Ice Sheet …

Younger DryasBayesian probabilityCALIFORNIAGreenland ice sheetBayesianlaw.inventionPaleontologycometsynchroneitylawTERMINATIONDEPTH MODELSYounger DryasRadiocarbon datingIMPACT HYPOTHESISCOSMIC IMPACTNANODIAMONDSMultidisciplinaryWILDFIRENorthern HemispherePNAS PlusYounger Dryas impact hypothesisEXTRATERRESTRIAL IMPACTradiocarbonBLACK MATGeologySPHERULES
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Recent changes in measured wind in the NE Atlantic and variability of correlation with NAO

2010

The paper deals with wind measurements, recorded since the 1950s, at twelve meteorological stations along a transect near the westernmost European border, between 64° and 44° N. Extreme wind speed tends to decrease sharply near the northern boundary (at Reykjavick), near the middle of the study area (at Shannon and Valentia) and near the southern boundary (at Brest and Cap Ferret), to increase at Thorshavn, with less significant trends at the other stations. Average wind speeds confirm the above tendencies, with an additional increasing speed at Lerwick, Kirkwall, Malin Head, Belle-Ile and Cap Ferret. To compare changes in wind activity, the data have been subdivided into three periods: unt…

[ SDU.OCEAN ] Sciences of the Universe [physics]/Ocean AtmosphereAtmospheric Science010504 meteorology & atmospheric sciencesCorrelation coefficientMeteorologyKeywords. Meteorology and atmospheric dynamics (Climatology[SDE.MCG]Environmental Sciences/Global Changes010502 geochemistry & geophysics01 natural sciencesWind speedLatitudeKeywords. Meteorology and atmospheric dynamics (Climatology; General circulation)Trend surface analysisEarth and Planetary Sciences (miscellaneous)lcsh:ScienceTransectExtreme value theory0105 earth and related environmental sciences[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereClimatologyAtmospheric dynamicsGeneral circulationlcsh:QC801-809General circulation)GeologyAstronomy and AstrophysicsWesterlieslcsh:QC1-999lcsh:Geophysics. Cosmic physics[ SDE.MCG ] Environmental Sciences/Global Changes[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology13. Climate actionSpace and Planetary ScienceNorth Atlantic oscillationClimatologylcsh:Q[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/Climatologylcsh:PhysicsGeologyAnnales Geophysicae
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Global atmospheric response to specific linear combinations of the main SST modes. Part I: numerical experiments and preliminary results

1996

Abstract. This article investigates through numerical experiments the controversial question of the impact of El Niño-Southern Oscillation (ENSO) phenomena on climate according to large-scale and regional-scale interhemispheric thermal contrast. Eight experiments (two considering only inversed Atlantic thermal anomalies and six combining ENSO warm phase with large-scale interhemispheric contrast and Atlantic anomaly patterns) were performed with the Météo-France atmospheric general circulation model. The definition of boundary conditions from observed composites and principal components is presented and preliminary results concerning the month of August, especially over West Africa and the …

[ SDU.OCEAN ] Sciences of the Universe [physics]/Ocean AtmosphereAtmospheric Science010504 meteorology & atmospheric sciencesMeteorologyAtmospheric circulation010502 geochemistry & geophysics01 natural sciencesWest africaEarth and Planetary Sciences (miscellaneous)Linear combinationlcsh:ScienceSouthern Hemisphere0105 earth and related environmental sciences[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereAnomaly (natural sciences)lcsh:QC801-809Northern HemisphereGeologyAstronomy and Astrophysics[ SDU.STU ] Sciences of the Universe [physics]/Earth Scienceslcsh:QC1-999lcsh:Geophysics. Cosmic physicsEl Niño Southern Oscillation13. Climate actionSpace and Planetary Science[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/ClimatologyGeneral Circulation ModelClimatologyEnvironmental sciencelcsh:Qlcsh:Physics
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