Search results for "viol"

showing 10 items of 2848 documents

MINOS and CPT violating neutrinos

2009

We review the status of CPT violation in the neutrino sector. Apart from LSND, current data favors three flavors of light stable neutrinos and antineutrinos, with both halves of the spectrum having one smaller mass splitting and one larger mass splitting. Oscillation data for the smaller splitting are consistent with CPT. For the larger splitting, current data favor an antineutrino mass-squared splitting that is an order of magnitude larger than the corresponding neutrino splitting, with the corresponding mixing angle less than maximal. This CPT-violating spectrum is driven by recent results from MINOS, but is consistent with other experiments if we ignore LSND. We describe an analysis tech…

AstrofísicaQuarkPhysicsNuclear and High Energy PhysicsParticle physicsMuonCPT symmetryHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesWeinberg angleNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)MINOSHigh Energy Physics::ExperimentNeutrinoNeutrinosCPT violationNeutrino oscillationLepton
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Effects of radiation in accretion regions of classical T Tauri stars

2019

Models and observations indicate that the impact of matter accreting onto the surface of young stars produces regions at the base of accretion columns, in which optically thin and thick plasma components coexist. Thus an accurate description of these impacts requires to account for the effects of absorption and emission of radiation. We study the effects of radiation emerging from shock-heated plasma in impact regions on the structure of the pre-shock downfalling material. We investigate if a significant absorption of radiation occurs and if it leads to a pre-shock heating of the accreting gas. We developed a radiation hydrodynamics model describing an accretion column impacting onto the su…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)X-rays: starsAstrophysicsradiation: dynamics01 natural sciencesaccretion0103 physical sciencesThermalRadiative transferAstrophysics::Solar and Stellar Astrophysics010306 general physicsAbsorption (electromagnetic radiation)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysicsultraviolet: starsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsstars: variables: T Tauristars: formationaccretion disksHerbig Ae/BeAstronomy and AstrophysicsPlasmaThermal conductionAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomena
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SphinX soft X-ray spectrophotometer: Science objectives, design and performance

2011

The goals and construction details of a new design Polish-led X-ray spectrophotometer are described. The instrument is aimed to observe emission from entire solar corona and is placed as a separate block within the Russian TESIS X- and EUV complex aboard the CORONAS-PHOTON solar orbiting observatory. SphinX uses silicon PIN diode detectors for high time resolution measurements of the solar spectra in the range 0.8–15 keV. Its spectral resolution allows for discerning more than hundred separate energy bands in this range. The instrument dynamic range extends two orders of magnitude below and above these representative for GOES. The relative and absolute accuracy of spectral measurements is e…

Astrophysics::High Energy Astrophysical PhenomenaInstrumentationExtreme ultraviolet lithographyspectrumlaw.inventionX-raySettore FIS/05 - Astronomia E AstrofisicaOpticssolar corona; spectrum; X-ray; abundances; instrumentation; SphinXObservatorylawAstrophysics::Solar and Stellar AstrophysicsSpectral resolutioninstrumentationPhysicsabundanceDynamic rangebusiness.industrysolar coronaSphinXDetectorPIN diodeAstronomy and AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsbusinessOrder of magnitudeSolar System Research
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A photometric redshift of z = 1.8$^{\sf{+0.4}}_{\sf{-0.3}}$ for the AGILE GRB 080514B

2008

Aims: The AGILE gamma-ray burst GRB 080514B is the first burst with detected emission above 30 MeV and an optical afterglow. However, no spectroscopic redshift for this burst is known. Methods: We compiled ground-based photometric optical/NIR and millimeter data from several observatories, including the multi-channel imager GROND, as well as ultraviolet \swift UVOT and X-ray XRT observations. The spectral energy distribution of the optical/NIR afterglow shows a sharp drop in the \swift UVOT UV filters that can be utilized for the estimation of a redshift. Results: Fitting the SED from the \swift UVOT $uvw2$ band to the $H$ band, we estimate a photometric redshift of $z=1.8^{+0.4}_{-0.3}$, c…

Astrophysics::High Energy Astrophysical PhenomenaUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica::OtrasFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstrophysicsmedicine.disease_causemedicineAstrophysics::Solar and Stellar AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicasQCAstrophysics::Galaxy AstrophysicsQB:ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica::Otras [UNESCO]Photometric redshiftGamma rays: burstsPhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsRedshiftAfterglowbursts [Gamma rays]Space and Planetary ScienceSpectral energy distributionMillimeterGamma-ray burst:ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicas [UNESCO]UltravioletAstronomy & Astrophysics
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Multiple accelerated particle populations in the Cygnus Loop with Fermi-LAT

2021

The Cygnus Loop (G74.0-8.5) is a very well-known nearby supernova remnant (SNR) in our Galaxy. Thanks to its large size, brightness, and angular offset from the Galactic plane, it has been studied in detail from radio to $\gamma$-ray emission. The $\gamma$ -rays probe the populations of energetic particles and their acceleration mechanisms at low shock speeds. We present an analysis of the $\gamma$-ray emission detected by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope over 11 years in the region of the Cygnus Loop. We performed detailed morphological and spectral studies of the $\gamma$-ray emission toward the remnant from 100 MeV to 100 GeV and compared it with X-ra…

Astrophysics::High Energy Astrophysical Phenomenabrightnesscosmic radiation: energyFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeV01 natural sciencesGLASTthermalX-raycosmic raysSpitzer Space Telescope0103 physical sciencesultravioletsupernovaRadiative transferopticalcloudcosmic radiation: acceleration010306 general physicsSupernova remnant010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsacceleration of particlesISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cygnus LoopAstronomy and Astrophysicsshock wavesGalactic planeGalaxy13. Climate actionSpace and Planetary Sciencegamma raystatisticsspectralgalaxyAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Fermi Gamma-ray Space Telescope
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Introduction. A nagging thought of a scholar

2019

This paper is – as introduction of volume “Proximity violence in migration times” – is the result of the nagging thought of a scholar and the support the European Commission decided to provide her with in order to favour the theoretical challenge the project envisaged and allowing her to conduct these two years of research supported by a network of partners comprising universities, research centres and non-profit organisations. It is the product of a combined, reasoned in-the-field research and desk analysis regarding recognition and reception of refugee-asylum seekers, victims of violence within their places of origin, during the journey to the European states bordering on the Mediterranea…

Asylum seekers proximity violence reception system care services best practicesSettore SPS/07 - Sociologia Generale
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Sociedades fragiles

2001

AtentadosMal absolutoPoder norteamericanoVidal-Beneyto José11-SBlanqueoPOLÍTICADiferenciaTerrorismoFragilidad colectivaGrandes sociedadesPublicaciones: Obra periodística: Columnas y artículos de opiniónAtonomíaTráficoCambio socialResistenciaOperaciones financieras ocultasViolenciaSociedadesSectarismoGLOBALIZACIÓNDesarrollo tecnológicoHipersimplificación mediáticaJusticia infinita
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Antiamericanismo

2002

AtentadosTorres GemelasPazVidal-Beneyto JoséRiqueza11-SAntiamericanismoAversión exteriorRevolución liberalPublicaciones: Obra periodística: Columnas y artículos de opiniónLíderes mundialesLiberalismoPolítica económicaArgumentario antiamericanoNorteaméricaViolenciaPotencia mundialInseguridad ciuadanaImperialismo políticoEEUUIneficacia servicios públicos
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Data flow of spectral UV measurements at Sodankylä and Jokioinen

2016

Abstract. The data flow involved in a long-term continuous solar spectral UV irradiance monitoring program is investigated and structured to provide an overall view on the multiphase process from data acquisition to the final products. The program employing Brewer spectrophotometers as measuring instruments is maintained by the Finnish Meteorological Institute (FMI) ever since the 1990s at two sites in Finland: Sodankylä (67° N) and Jokioinen (61° N). It is built upon rigorous operation routines, processing procedures, and tools for quality control (QC) and quality analysis (QA) under continuous development and evaluation. Three distinct levels of data emerge, each after certain phase in th…

Atmospheric ScienceMeteorology010504 meteorology & atmospheric sciencesRETRIEVALIrradiance010502 geochemistry & geophysicsOceanography114 Physical sciencesColumn (database)01 natural sciencesData acquisitionBREWER SPECTROPHOTOMETERS0103 physical sciencesOZONE DEPLETION010303 astronomy & astrophysicsRemote sensing0105 earth and related environmental scienceslcsh:QC801-809GeologyINSTRUMENTSMonitoring programIRRADIANCEData flow diagramlcsh:Geophysics. Cosmic physicsSPECTRORADIOMETERGeographySpectroradiometerCOLUMNMeasuring instrumentAEROSOL OPTICAL DEPTHRaw dataULTRAVIOLET-RADIATIONGROUND-LEVELGeoscientific Instrumentation, Methods and Data Systems
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Operational considerations to improve total ozone measurements with a Microtops II ozone monitor

2012

A Microtops II "ozone monitor" with UV channels centered at 305.5, 312.5, and 320 nm has been used routinely in six experimental campaigns carried out in several geographic locations and seasons, covering latitudes from 35 to 68° N during the last ten years (2001–2011). The total ozone content is retrieved by Microtops II by using different combinations (Channel I, 305.5/312.5 nm; Channel II, 312.5/320 nm; and Channel III, 305.5/312.5/320 nm) of the signals at the three ultraviolet wavelengths. The long-term performance of the total ozone content determination has been studied taking into account the sensitivities to the calibration, airmass, temperature and aerosols. When a calibration was…

Atmospheric ScienceOzoneMeteorologylcsh:TA715-787lcsh:Earthwork. FoundationsOzone monitorMicrotops IITotal ozoneGeofísicamedicine.disease_causelcsh:Environmental engineeringLatitudeRoot mean squarechemistry.chemical_compoundWavelengthAtmosferaUltraviolet solar radiationchemistrySunphotometerCalibrationmedicinelcsh:TA170-171Total column ozoneUltravioletCommunication channel
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