Search results for "gamma rays"

showing 8 items of 108 documents

Observation of intrinsically bright terrestrial gamma ray flashes from the Mediterranean basin

2015

Abstract  We present three terrestrial gamma ray flashes (TGFs) observed over the Mediterranean basin by the Reuven Ramaty High Energy Solar Spectroscope Imager (RHESSI) satellite. Since the occurrence of these events in the Mediterranean region is quite rare, the characterization of the events was optimized by combining different approaches in order to better define the cloud of origin. The TGFs on 7 November 2004 and 16 October 2006 came from clouds with cloud top higher than 10–12 km where often a strong penetration into the stratosphere is found. This kind of cloud is usually associated with heavy precipitation and intense lightning activity. Nevertheless, the analysis of the cloud type…

TLEAtmospheric ScienceAtmospheric ElectricityFOS: Physical sciencesAstrophysicsAerosol and CloudsTroposphereAltitudeRaigs gammaPhysics - Space PhysicsEarth and Planetary Sciences (miscellaneous):Matematikk og Naturvitenskap: 400 [VDP]StratosphereResearch ArticlesPhysics:Física [Àrees temàtiques de la UPC]Cloud topGamma raysGamma raythunderstormsLightningMonte Carlo techniqueSpace Physics (physics.space-ph)TGF:Energies::Energia elèctrica [Àrees temàtiques de la UPC]Physics - Atmospheric and Oceanic PhysicsGeophysicsterrestrial gamma ray flashx-ray13. Climate actionSpace and Planetary ScienceAtmospheric and Oceanic Physics (physics.ao-ph)Atmospheric ProcessesThunderstormSatellitelightningResearch ArticleJournal of Geophysical Research. Atmospheres
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First observations of the X-ray transient EXO 2030+375 with IBIS/ISGRI

2003

We present a first INTEGRAL observation of the 42s transient X-ray pulsar EXO 2030+375 with IBIS/ISGRI. The source was detected during Cyg X-1 observations in December 2002. We analyzed observations during the outburst period from 9 to 21 December 2002 with a total exposure time of ~770 kiloseconds. EXO 2030+375 was almost always detected during single ~30 minute exposures in the 18-45 energy bands. The source light curve shows the characteristic outburst shape observed in this source.

X-ray transientFOS: Physical sciencesIndividualAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsGamma rays ; Observations ; X-rays ; Individual ; EXO 2030+375 ; Telescopes ; INTEGRAL ; IBISPulsarX-raysObservations:ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica [UNESCO]PhysicsIbisEXO 2030+375biologyINTEGRALUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía ópticaGamma raysAstrophysics (astro-ph)Astronomy and Astrophysicsbiology.organism_classificationLight curveSpace and Planetary ScienceIBIS:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Telescopes
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γ-RAY AND PARSEC-SCALE JET PROPERTIES OF A COMPLETE SAMPLE OF BLAZARS FROM THE MOJAVE PROGRAM

2011

著者人数: 145名

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical Phenomenagalaxies: activePopulationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesRadio spectrumLuminosityRelativistic beamingquasars: generalgamma rays: galaxiesgalaxies0103 physical sciencesgalaxie [gamma rays]educationBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)radio continuum: galaxiesPhysicseducation.field_of_studygeneral [quasars]general [BL Lacertae objects]010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsQuasarBL Lacertae objects: generalgalaxies: jetsgalaxies [radio continuum]BL Lacertae objects: general; galaxies: active; galaxies: jets; gamma rays: galaxies; quasars: general; galaxies quasars: generaljet [galaxies]BL Lacertae objects: general; galaxies: active; galaxies: jets; gamma rays: galaxies; quasars: general; radio continuum: galaxiesSpace and Planetary Scienceactive [galaxies]Spectral energy distributionAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space TelescopeThe Astrophysical Journal
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The methodology for active testing of electronic devices under the radiations

2018

The methodology, developed for active testing of electronic devices under the radiations, is presented. The test set-up includes a gamma-ray facility, the hardware board/fixtures and the software tools purposely designed and realized. The methodology is so wide-ranging to allow us the verification of different classes of electronic devices, even if only application examples for static random access memory modules are reported.

business.industryComputer scienceSettore ING-IND/20 - Misure E Strumentazione NucleariTesting methodologies Electronic Devices Total Ionizing Dose Single Event Effects Gamma rays.Electrical engineeringelectronic devicetotal ionizing dosesingle event effectNuclear Energy and Engineeringtesting methodologygamma raylcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityElectronicsSafety Risk Reliability and QualitybusinessNuclear Technology and Radiation Protection
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Combined TL and 10B-alanine ESR dosimetry for BNCT

2004

The dosimetric technique described in this paper is based on electron spin resonance (ESR) detectors using an alanine-boric compound acid enriched with 1 0 B, and beryllium oxide thermoluminescent (TL) detectors; with this combined dosimetry, it is possible to discriminate the doses due to thermal neutrons and gamma radiation in a mixed field. Irradiations were carried out inside the thermal column of a TRIGA MARK II water-pool-type research nuclear reactor, also used for Boron Neutron Capture therapy (BNCT) applications, with thermal neutron fluence from 10 9 to 10 1 4 n t h cm - 2 . The ESR dosemeters using the alanine-boron compound indicated ESR signals about 30-fold stronger than those…

inorganic chemicalsMaterials scienceBeryllium oxidechemistry.chemical_elementBoron Neutron Capture TherapyRadiationRisk AssessmentSensitivity and SpecificityThermoluminescencelaw.inventiondosimeters electron paramagnetic resonancespin resonancechemistry.chemical_compoundRadiation ProtectionIsotopeslawHumansDosimetryRadiology Nuclear Medicine and imagingBoronElectron paramagnetic resonanceBoronNeutronsRadiationRadiological and Ultrasound Technologybusiness.industryRadiotherapy Planning Computer-AssistedRadiochemistryElectron Spin Resonance SpectroscopyPublic Health Environmental and Occupational HealthReproducibility of ResultsRadiotherapy DosageGeneral MedicineSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Neutron temperatureSystems IntegrationNeutron capturechemistryGamma RaysBody BurdenThermoluminescent DosimetryNuclear medicinebusinessRelative Biological EffectivenessRadiation Protection Dosimetry
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Dose calculation in biological samples in a mixed neutron-gamma field at the TRIGA reactor of the University of Mainz

2010

To establish Boron Neutron Capture Therapy (BNCT) for non-resectable liver metastases and for in vitro experiments at the TRIGA Mark II reactor at the University of Mainz, Germany, it is necessary to have a reliable dose monitoring system. The in vitro experiments are used to determine the relative biological effectiveness (RBE) of liver and cancer cells in our mixed neutron and gamma fi eld. We work with alanine detectors in combination with Monte Carlo simulations, where we can measure and characterize the dose. To verify our calculations we perform neutron fl ux measurements using gold foil activation and pin-diodes . Material and methods . When L- α -alanine is irradiated with ionizing …

inorganic chemicalsPhysics::Instrumentation and DetectorsQuantitative Biology::Tissues and OrgansPhysics::Medical PhysicsBoron Neutron Capture TherapyValidation Studies as TopicModels BiologicalIonizing radiationTRIGAHospitals UniversityNuclear ReactorsCell Line TumorGermanyRelative biological effectivenessMedicineDosimetryHumansRadiology Nuclear Medicine and imagingNeutronNeutronsbusiness.industryRadiotherapy Planning Computer-AssistedRadiochemistryLiver NeoplasmsRadiotherapy DosageHematologyGeneral MedicineHep G2 CellsNeutron temperatureNeutron captureOncologyGamma RaysAbsorbed dosebusinessNuclear medicineColorectal Neoplasms
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EPR DOSIMETRY IN A MIXED NEUTRON AND GAMMA RADIATION FIELD

2004

Suitability of Electron Paramagnetic Resonance (EPR) spectroscopy for criticality dosimetry was evaluated for tooth enamel, mannose and alanine pellets during the 'international intercomparison of criticality dosimetry techniques' at the SILENE reactor held in Valduc in June 2002, France. These three materials were irradiated in neutron and gamma-ray fields of various relative intensities and spectral distributions in order to evaluate their neutron sensitivity. The neutron response was found to be around 10% for tooth enamel, 45% for mannose and between 40 and 90% for alanine pellets according their type. According to the IAEA recommendations on the early estimate of criticality accident a…

inorganic chemicalsSafety ManagementMaterials scienceQuality Assurance Health CareRadiation DosageRisk AssessmentSensitivity and Specificitylaw.inventionRadiation Protectionstomatognathic systemlawNuclear ReactorsRisk FactorsmedicineDosimetryHumansRadiology Nuclear Medicine and imagingNeutronIrradiationElectron paramagnetic resonanceSpectroscopyRadiometryNeutronsObserver VariationRadiationRadiological and Ultrasound Technologybusiness.industryRadiochemistryPublic Health Environmental and Occupational HealthElectron Spin Resonance SpectroscopyReproducibility of ResultsGeneral MedicineReference StandardsTooth enamelEPR DOSIMETRY MIXED NEUTRON AND GAMMA RADIATION FIELDstomatognathic diseasesmedicine.anatomical_structureCriticalityGamma RaysAbsorbed doseBody BurdenFranceNuclear medicinebusinessRadioactive Hazard ReleaseRelative Biological Effectiveness
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GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2017

On August 17, 2017 at 12-41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×104 years. We infer the component masses of the binary to be between 0.86 and 2.26 M, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M, with the total mass of the system 2.74-0.01+0.04M. The source was localized within a sky region of 28 deg2 (90% probabili…

neutron star: binary[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]X-ray binaryADVANCED LIGOAstrophysicsKilonovagravitational waves; LIGO; binary neutron star inspiralspin01 natural sciencesLIGOGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Electromagnetic observationsGravitational-wave signals3100 General Physics and AstronomyPoint MassesAstrophysics - High Energy Astrophysical PhenomenaBlack-Hole MergersBinary neutron starsBlack HolesX-ray bursterCoalescing BinariesAstrophysics::High Energy Astrophysical Phenomena10192 Physics InstituteGeneral Relativity and Quantum Cosmology (gr-qc)Gravity wavesGravitational wavesNeutron starsPhysics and Astronomy (all)ddc:530Electromagnetic spectraNeutrons010308 nuclear & particles physicsVirgoGamma raysAstronomyRCUKVIRGOelectromagneticgravitational radiation: emissionStellar black holeGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Compact Binariesbinary: masscosmological modelAstronomyGeneral Physics and AstronomyAstrophysicsneutron starsGamma ray burstsGeneral Relativity and Quantum CosmologyGravitational wave detectorsUniverseDENSE MATTER010303 astronomy & astrophysicsastro-ph.HEPhysicsSignal to noise ratioSettore FIS/01 - Fisica SperimentaleGravitational effectsFalse alarm rateEQUATION-OF-STATEMergers and acquisitionsgravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]530 PhysicsMERGERSGeneral Relativity and Quantum Cosmology; General Relativity and Quantum Cosmology; astro-ph.HEFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstgravitational radiation: direct detectionMerging[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GAMMA-RAY BURSTLIGO (Observatory)binary: coalescenceGravitational waves neutron stars gamma-ray burst LIGO Virgo0103 physical sciencesGW151226MASSESSTFCAstrophysics::Galaxy AstrophysicsPhysiqueGravitational wavegravitational radiationPULSARgravitational radiation detectorNeutron starPhysics and AstronomygravitationRADIATIONDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikbinary neutron star inspiralSignal detectionPHYS REV LETT PHYSICAL REVIEW LETTERS
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