Search results for " gamma-ray"

showing 10 items of 172 documents

On the ‘expanded local mode’ approach applied to the methane molecule: isotopic substitution CH2D2←CH4

2011

On the basis of a compilation of the ‘expanded local mode’ model and the general isotopic substitution theory, sets of simple analytical relations between different spectroscopic parameters (harmonic frequencies, ωλ, anharmonic coefficients, x λμ, ro-vibrational coefficients, , different kinds of Fermi- and Coriolis-type interaction parameters) of the CH2D2 molecule are derived. All of them are expressed as simple functions of a few initial spectroscopic parameters of the mother, CH4, molecule. Test calculations with the derived isotopic relations show that, in spite of a total absence of initial information about the CH2D2 species, the numerical results of the calculations have a very good…

010304 chemical physicsBasis (linear algebra)ChemistrySubstitution (logic)AnharmonicityBiophysicsThermodynamics010402 general chemistryCondensed Matter Physics01 natural sciences0104 chemical sciencesComputational chemistryAb initio quantum chemistry methodsSimple (abstract algebra)Simple function0103 physical sciencesMoleculePhysics::Chemical PhysicsPhysical and Theoretical ChemistryMolecular BiologyFermi Gamma-ray Space TelescopeMolecular Physics
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Tuning the Electronic Properties of the Dative N-B Bond with Associated O-B Interaction: Electron Localizability Indicator from X-Ray Wavefunction Re…

2016

Despite the immense growth in interest in difluoroborate dyes, the nature of the interactions of the boron atom within the N-BF2 -O kernel is not yet fully understood. Herein, a set of real-space bonding indicators is used to quantify the electronic characteristics of the dative N-B bond in difluoroborate derivatives. The atoms-in-molecules (AIM) partitioning scheme is complemented by the electron localizability indicator (ELI-D) approach, and both were applied to experimental and theoretical electron-density distributions (X-ray constrained wavefunction fitting vs. DFT calculations). Additionally, Fermi orbital analysis was introduced for small DFT models to support and extend the findings…

010405 organic chemistryChemistryX-raychemistry.chemical_elementElectron010402 general chemistry01 natural sciencesQuantum chemistryAtomic and Molecular Physics and Optics0104 chemical sciencesChemical bondChemical physicsKernel (statistics)Physical and Theoretical ChemistryAtomic physicsWave functionBoronFermi Gamma-ray Space TelescopeChemphyschem : a European journal of chemical physics and physical chemistry
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On the timing between terrestrial gamma ray flashes, radio atmospherics, and optical lightning emission

2017

On 25 October 2012 the Reuven Ramaty High Energy Solar Spectroscope Imager (RHESSI) and the Tropical Rainfall Measuring Mission (TRMM) satellites passed over a thunderstorm on the coast of Sri Lanka. RHESSI observed a terrestrial gamma ray flash (TGF) originating from this thunderstorm. Optical measurements of the causative lightning stroke were made by the lightning imaging sensor (LIS) on board TRMM. The World Wide Lightning Location Network (WWLLN) detected the very low frequency (VLF) radio emissions from the lightning stroke. The geolocation from WWLLN, which we also assume is the TGF source location, was in the convective core of the cloud. By using new information about both RHESSI a…

010504 meteorology & atmospheric sciencesGamma rayFOS: Physical sciencesRadio atmosphericLight curve01 natural sciencesLightningSpace Physics (physics.space-ph)GeophysicsPhysics - Space PhysicsSpace and Planetary Science0103 physical sciencesThunderstormEnvironmental scienceAtmosphericsVery low frequencyAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysics0105 earth and related environmental sciencesTerrestrial gamma-ray flashRemote sensingJournal of Geophysical Research: Space Physics
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Astrochronology of the Valanginian Stage from reference sections (Vocontian Basin, France) and palaeoenvironmental implications for the Weissert Even…

2013

12 pages; International audience; High-resolution gamma-ray measurements performed on five biostratigraphically well-dated reference sections from the Vocontian Basin (south-eastern France) are used to develop a new astrochronology of the Valanginian Stage and its subdivisions (i.e. ammonite and calcareous nannofossil zones and subzones). Spectral analyses show a pervasive dominance of 405-kyr eccentricity cycles with the expression of 100-kyr eccentricity, obliquity and precession. Previous rough estimates of Valanginian Stage duration ranged from 3.9 to 6.5 myr but were generally based on less reliable or indirect methods. This study provides a precise duration of 5.08 myr, tuning the ser…

010506 paleontologyBiozone[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy010502 geochemistry & geophysicsOceanographyPalaeoclimate01 natural sciencesPaleontologyGeologic time scaleStage (stratigraphy)Ecology Evolution Behavior and Systematics0105 earth and related environmental sciencesEarth-Surface ProcessesAmmoniteAstrochronologySeries (stratigraphy)High-resolution gamma-rayParaná-EtendekaPaleontologyCyclostratigraphylanguage.human_languageVocontian BasinStratigraphy13. Climate actionValanginian[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/StratigraphylanguageGeologyWeissert Event
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Low-Power, Subthreshold Reference Circuits for the Space Environment : Evaluated with -rays, X-rays, Protons and Heavy Ions

2019

The radiation tolerance of subthreshold reference circuits for space microelectronics is presented. The assessment is supported by measured results of total ionization dose and single event transient radiation-induced effects under &gamma

02 engineering and technologyHardware_PERFORMANCEANDRELIABILITYgammasäteily7. Clean energy01 natural sciencesanalog single-event transient (ASET)Ionizationsingle-event effects (SEE)0202 electrical engineering electronic engineering information engineeringAnnan elektroteknik och elektronikElectronic circuitPhysicsprotonsSubthreshold conductionionisoiva säteilyröntgensäteilyGamma raygamma-raysHardware and ArchitectureAtomic physicsVoltage referencemikroelektroniikkaprotonitComputer Networks and Communicationslcsh:TK7800-8360voltage referenceIonheavy-ions0103 physical sciencesionizationradiation hardening by design (RHBD)X-raysHardware_INTEGRATEDCIRCUITSMicroelectronicsElectrical and Electronic Engineeringhiukkassäteilybandgap voltage reference (BGR)Other Electrical Engineering Electronic Engineering Information Engineering010308 nuclear & particles physicsbusiness.industry020208 electrical & electronic engineeringlcsh:Electronicsspace electronicstotal ionization dose (TID)Analog single-event transient (ASET); Bandgap voltage reference (BGR); CMOS analog integrated circuits; Gamma-rays; Heavy-ions; Ionization; Protons; Radiation hardening by design (RHBD); Reference circuits; Single-event effects (SEE); Space electronics; Total ionization dose (TID); Voltage reference; X-raysmikropiiritsäteilyfysiikkaControl and Systems Engineeringreference circuitsSignal ProcessingbusinessSpace environmentHardware_LOGICDESIGNCMOS analog integrated circuits
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Dual-polarity pulse processing and analysis for charge-loss correction in cadmium–zinc–telluride pixel detectors

2018

Charge losses at the inter-pixel gap are typical drawbacks in cadmium–zinc–telluride (CZT) pixel detectors. In this work, an original technique able to correct charge losses occurring after the application of charge-sharing addition (CSA) is presented. The method, exploiting the strong relation between the energy after CSA and the beam position at the inter-pixel gap, allows the recovery of charge losses and improvements in energy resolution. Sub-millimetre CZT pixel detectors were investigated with both uncollimated radiation sources and collimated synchrotron X-rays, at energies below and above the K-shell absorption energy of the CZT material. The detectors are DC coupled to fast and low…

0301 basic medicine030103 biophysicsNuclear and High Energy PhysicsMaterials sciencePreamplifierPhysics::Instrumentation and Detectors01 natural sciencesCollimated lightCharge sharinglaw.invention03 medical and health scienceschemistry.chemical_compoundOpticslawcharge losse0103 physical sciencesInstrumentationenergy-resolved photon-counting detectorsNuclear and High Energy Physiccharge lossescharge sharingRadiationPixel010308 nuclear & particles physicsbusiness.industryCdZnTe detectorsCdZnTe detectorDetectorSettore FIS/01 - Fisica Sperimentaleenergy-resolved photon-counting detectorSynchrotronSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Cadmium zinc tellurideX-ray and gamma-ray detectorschemistryDirect couplingbusinessX-ray and gamma-ray detector
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An experimental search for a correlation between outdoor 222Rn concentration and 210Pb activity in air particulate samples

2018

This work was aimed to search for a correlation between outdoor 222Rn air concentration and 210Pb activity in particulate samples collected on a filter. The existence of a correlation could support the hypothesis that both 222Rn and its long-lived product 210Pb are embedded into the same air masses and undergo the same air transport phenomena. Lead-210 activity was determined by means of gamma ray spectrometric measurement carried out a few days after the sampling whereas 222Rn concentration was measured through a commercial monitor. Experimental tests allowed to obtain a weak correlation between 222Rn and 210Pb air concentration as a preliminary result due to high uncertainties of outdoor …

222Rn 210Pb air filtration atmospheric particulate gamma-ray spectrometry222RnSettore ING-IND/20 - Misure E Strumentazione Nucleariair filtrationParticulates010403 inorganic & nuclear chemistry01 natural sciences0104 chemical sciencesCorrelationatmospheric particulateNuclear Energy and Engineeringgamma ray spectrometryEnvironmental chemistrylcsh:QC770-798Environmental sciencelcsh:Nuclear and particle physics. Atomic energy. RadioactivitySafety Risk Reliability and Quality210PbNuclear Technology and Radiation Protection
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Response of AGATA segmented HPGe detectors to gamma rays up to 15.1MeV

2013

WOS: 000314826000009

AGATA; Gamma-ray spectroscopy; Gamma-ray tracking; HPGe detectors; Pulse-shape and gamma-ray tracking algorithms; Semiconductor detector performance and simulationsNuclear and High Energy PhysicsPulse-shape and gamma-ray tracking algorithmsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSemiconductor detector performance and simulationsTracking (particle physics)01 natural sciencesNuclear physicsGamma-ray tracking0103 physical sciencesGamma spectroscopyddc:530Gamma-ray spectroscopyNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentInstrumentationNuclear ExperimentDetectors de radiacióPhysicsSpectrometer010308 nuclear & particles physicsDetectorHPGe detectorsGamma ray81V35Semiconductor detectorAGATAFísica nuclearHpge detectorAGATA
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Search for neutrino emission from gamma-ray flaring blazars with the ANTARES telescope

2012

The ANTARES telescope observes a full hemisphere of the sky all the time with a duty cycle close to 100%. This makes it well suited for an extensive observation of neutrinos produced in astrophysical transient sources. In the surrounding medium of blazars, i.e. active galactic nuclei with their jets pointing almost directly towards the observer, neutrinos may be produced together with gamma-rays by hadronic interactions, so a strong correlation between neutrinos and gamma-rays emissions is expected. The time variability information of the studied source can be obtained by the gamma-ray light curves measured by the LAT instrument on-board the Fermi satellite. If the expected neutrino flux ob…

ASTROPHYSICSAstrofísicaAstrophysicsNeutrino Astronomy01 natural sciences7. Clean energyLARGE-AREA TELESCOPElaw.inventionlawWATERInstrumentation010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Time-dependent searchCATALOGLIGHTNeutrino astronomyFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaACTIVE GALACTIC NUCLEINuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Active galactic nucleus[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Point sourceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsfermi lat transient sources; neutrino astronomy; time-dependent search; antares; blazarsTelescopeMUONS0103 physical sciencesANTARES; Neutrino Astronomy; Fermi LAT transient sourcesBlazarANTARES010308 nuclear & particles physicsAstronomyAstronomy and AstrophysicsFermi LAT transient sourcesLight curveNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]MODEL13. Climate actionFISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]Neutrino astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]BlazarsFermi Gamma-ray Space Telescope
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First Multi-wavelength Campaign on the Gamma-ray-loud Active Galaxy IC 310

2017

The extragalactic VHE gamma-ray sky is rich in blazars. These are jetted active galactic nuclei viewed at a small angle to the line-of-sight. Only a handful of objects viewed at a larger angle are known so far to emit above 100 GeV. Multi-wavelength studies of such objects up to the highest energies provide new insights into the particle and radiation processes of active galactic nuclei. We report the results from the first multi-wavelength campaign observing the TeV detected nucleus of the active galaxy IC 310, whose jet is observed at a moderate viewing angle of 10 deg - 20 deg. The multi-instrument campaign was conducted between 2012 Nov. and 2013 Jan., and involved observations with MAG…

Active galactic nucleusAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesEnergy fluxAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxies: active; Galaxies: individual: IC 310; Gamma rays: galaxies; Astronomy and Astrophysics; Space and Planetary Science01 natural scienceslaw.inventionlawGalaxies: individual: IC 3100103 physical sciencesindividual: IC 310 [galaxies]Blazar010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsgalaxie [Gamma rays]010308 nuclear & particles physicsGamma rayAstronomy and AstrophysicsGalaxies: activeAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesSynchrotrongamma rays: galaxies ; galaxies: active ; individual (IC 310)Gamma rays: galaxiesSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)active [galaxies]galaxies [gamma rays]ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGSpectral energy distributionddc:520Astrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space TelescopeFlare
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