Search results for "synchrotron radiation"

showing 10 items of 146 documents

Surface magnetism studied by photoelectron spectromicroscopy with high spatial and time resolution

2004

Abstract Photoemission electron microscopy (PEEM) is widely used for the study of magnetic surfaces and thin films. Ferromagnetic and antiferromagnetic microstructures are investigated exploiting magnetic circular and linear dichroism in the soft X-ray range using tuneable synchrotron radiation. Local dichroism spectroscopy gives access to magnetic moments of the elements in compounds or multilayer materials. Beyond these achievements, the method bears a high future potential with respect to an increased lateral resolution via aberration correction of the electron optics and a high time resolution in the 100 ps range for the study of dynamic processes. In addition, photoelectron spin polari…

RadiationMaterials scienceMagnetic momentCondensed matter physicsMagnetismAnalytical chemistrySynchrotron radiationDichroismCondensed Matter PhysicsLinear dichroismAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsCondensed Matter::Materials SciencePhotoemission electron microscopyFerromagnetismElectron opticsPhysical and Theoretical ChemistrySpectroscopyJournal of Electron Spectroscopy and Related Phenomena
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XMM-Newton observation of the supernova remnant Kes 78 (G32.8-0.1): Evidence for shock-cloud interaction

2017

The Galactic supernova remnant Kes 78 is surrounded by dense molecular clouds, whose projected position overlaps with the extended HESS gamma-ray source HESS J1852-000. The X-ray emission from the remnant has been recently revealed by Suzaku observations, which have shown indications for a hard X-ray component in the spectra, possibly associated with synchrotron radiation. We aim at describing the spatial distribution of the physical properties of the X-ray emitting plasma and at revealing the effects of the interaction of the remnant with the inhomogeneous ambient medium. We also aim at investigating the origin of the gamma-ray emission, which may be Inverse Compton radiation associated wi…

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaHadronSynchrotron radiationFOS: Physical sciencesElectronAstrophysicsISM: individual objects: Kes 7801 natural sciencesSpectral linelaw.inventionlawISM: cloud0103 physical sciencesSupernova remnant010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Molecular cloudAstronomy and AstrophysicsPlasmaAstronomy and AstrophysicAcceleration of particleSynchrotronX-rays: ISM13. Climate actionSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena
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Numerical study of emission and dynamics from a TDE-powered jet

2012

A transient event Swift J1644+57 is thought to be caused by the emission from a collimated relativistic jet. The jet, powered by the sudden onset of accretion onto a supermassive black hole following the tidal disruption of a star, collides with the gaseous circumnuclear medium and produces forward and reverse shocks which emit synchrotron radiation. We perform 1D and 2D relativistic hydrodynamic simulations using the MRGENESIS code. The aim of the simulations is to study the dynamics of a jet thought to exist in transient events such as Swift J1644+57, as discussed in recent literature. We discuss 1D and 2D jet evolution, on-axis radio light curves and differences between 1D and 2D jet dyn…

PhysicsJet (fluid)Supermassive black holeAccretion (meteorology)PhysicsQC1-999Astrophysics::High Energy Astrophysical PhenomenaSynchrotron radiationAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLight curve7. Clean energy01 natural sciencesCollimated light13. Climate action0103 physical sciencesTransient (oscillation)010306 general physics010303 astronomy & astrophysicsEvent (particle physics)Astrophysics::Galaxy AstrophysicsEPJ Web of Conferences, 39, id.04003 (2012)
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The evolution of the large-scale emission in Fanaroff-Riley type I jets

2011

Recent observations in X-rays and gamma-rays of nearby Fanaroff-Riley type I (FR I) radio galaxies have raised the question of the origin of the emission detected in the termination structures of their jets. The study of these structures can give information on the conditions for particle acceleration and radiation at the front shocks. In addition, an evolutionary scenario can help to disentangle the origin of the detected X-ray emission in young FR I sources, like some gigahertz peaked spectrum active galactic nuclei. This work focuses on the nature and detectability of the radiation seen from the termination regions of evolving FR I jets. We use the results of a relativistic, two-dimensio…

PhysicsPhotonActive galactic nucleusRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaCosmic microwave backgroundCosmic background radiationSynchrotron radiationAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLight curveParticle accelerationSpace and Planetary ScienceMonthly Notices of the Royal Astronomical Society
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The polytron as a cw electron accelerator in the 10 GeV range

1991

Abstract This article is concerned with a generalized microtron, characterized essentially by the number of magnet pairs in its bending system. It is shown that the most serious physical energy limit of the microtron, emittance growth due to synchrotron radiation, may be overcome if this number is raised essentially above what has been considered in the past. The main properties of such “polytrons” are investigated and several design examples for 15 GeV output energy are discussed.

PhysicsNuclear and High Energy PhysicsRange (particle radiation)Synchrotron radiationParticle acceleratorBendinglaw.inventionNuclear physicslawMagnetLimit (music)Physics::Accelerator PhysicsThermal emittanceNuclear ExperimentInstrumentationMicrotronNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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First analysis of the ν3+ν5 combination band of SF6 observed at Doppler-limited resolution and effective model for the ν3+ν5-ν5 hot band

2018

Abstract Sulfur hexafluoride is a greenhouse gas with a long lifetime in the atmosphere and an important tracer for air mass circulation atmospheric models. The IR spectrum of this heavy species, however, features many hot bands at room temperature (at which only 30% of the molecules lie in the ground vibrational state), especially those originating from the lowest, v 6 and v 5 = 1 vibrational states. Using a cryogenic long path cell with variable optical path length and temperatures regulated between 168 and 163 K, coupled to Synchrotron Radiation and a high resolution interferometer, Doppler-limited spectra of the very weak ν 3 + ν 5 band near 1450 cm−1 have been recorded. Low temperature…

Physics010304 chemical physics010504 meteorology & atmospheric sciencesAtmospheric modelsInfrared spectroscopySynchrotron radiation01 natural sciences7. Clean energyAtomic and Molecular Physics and OpticsSpectral lineHot bandSulfur hexafluoridechemistry.chemical_compoundFar infraredchemistry13. Climate action0103 physical sciencesPhysical and Theoretical ChemistryAtomic physicsSpectroscopyOptical path length0105 earth and related environmental sciencesJournal of Molecular Spectroscopy
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Synchrotron x-ray transmission measurements and modeling of filters investigated for Athena

2020

International audience; Advanced Telescope for High-Energy Astrophysics is a large-class astrophysics space mission selected by the European Space Agency to study the theme "Hot and Energetic Universe." The mission essentially consists of a large effective area x-ray telescope and two detectors: the X-ray Integral Field Unit (X-IFU) and the Wide Field Imager (WFI). Both instruments require filters to shield from out-of-band radiation while providing high transparency to x-rays. The mission is presently in phase B; thus, to consolidate the preliminary design, investigated filter materials need to be properly characterized by experimental test campaigns. We report results from high-resolution…

synchrotron radiationComputer scienceAstrophysics::High Energy Astrophysical PhenomenaMechanical EngineeringAstrophysics::Instrumentation and Methods for AstrophysicsSynchrotron radiationtelescopesAstronomy and AstrophysicsElectronic Optical and Magnetic Materialslaw.inventionTelescopeFilter designSettore FIS/05 - Astronomia E AstrofisicaTransmission (telecommunications)Space and Planetary ScienceControl and Systems EngineeringlawFilter (video)[SDU]Sciences of the Universe [physics]CalibrationOptical filterInstrumentationDigital filterastrophysics space mission Athena optical and thermal filters Wide Field Imager X-ray Integral Field Unit x-ray transmissionRemote sensing
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Generation and excitation of point defects in silica by synchrotron radiation above the absorption edge

2010

We report photoluminescence measurements carried out on amorphous SiO{sub 2} upon excitation by synchrotron light. Exposure of the as-grown material to above-edge light at low temperature induces the formation of nonbridging oxygen hole centers (NBOHC), localized in a thin layer below the surface limited by the penetration depth (tens of nm) of impinging light. After concluding the exposure to 11 eV light, stable defects are revealed by observing their characteristic 1.9 eV photoemission band excited at 4. 8eV. The local concentration of induced defects, supposedly formed by nonradiative decay of excitons, is very high (close to approx10{sup 21} cm{sup -3}) and independent of the previous h…

Materials sciencePhotoluminescencesynchrotron radiationExcitonpoint defectSettore FIS/01 - Fisica SperimentaleSynchrotron radiationCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsAbsorption edgesilicaExcited stateddc:530Atomic physicsLuminescencePenetration depthExcitation
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Luminescence and ultraviolet excitation spectroscopy of SrI2 and SrI2:Eu2+

2013

Abstract We report measurements of luminescence and its ultraviolet excitation spectra in SrI2 and SrI2:Eu2+ at temperatures of 10 and 300 K. Attention is focused on determining the exciton energy and its temperature shift from features of the excitation spectra and limits placed by absorption spectroscopy on a 120 μm thin crystal, on observation of a broadened Eu emission band attributed to trace Eu associated with oxygen in nominally undoped crystals, and on adding observations concerning the 3.4 eV band at low temperature attributed by Pustovarov et al. to the self-trapped exciton.

RadiationAbsorption spectroscopyExcitonchemistry.chemical_elementSynchrotron radiationmedicine.disease_causeOxygenStrontium iodidechemistry.chemical_compoundchemistrymedicinePhotoluminescence excitationAtomic physicsLuminescenceInstrumentationUltravioletRadiation Measurements
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Natural gas hydrate investigations by synchrotron radiation X-ray cryo-tomographic microscopy (SRXCTM)

2008

[1] We report the 3D microstructure analyses of natural gas hydrates sampled from Gulf of Mexico. The samples were characterized by synchrotron radiation X-ray cryo-tomographic microscopy (SRXCTM) using the ‘TOMCAT’ beam line at the Swiss Light Source (SLS). The SRXCTM demonstrates its applicability to unlock some microscopic features of the marine hydrates, in particular of crystallite size and grain boundary network. The gas hydrate domains are surrounded by a network of pores of typically a few micrometers, which are largely due to decomposition. Out of the SRXCTM data, the porosity, total volume of the voids, the void surface area and number of the total gas-filled voids have been calcu…

010504 meteorology & atmospheric sciencesbusiness.industryClathrate hydrateSynchrotron radiationMineralogy010502 geochemistry & geophysics01 natural sciencesGeophysicsNatural gasGeneral Earth and Planetary SciencesGrain boundaryCrystallitePorositybusinessHydrateGeologySwiss Light Source0105 earth and related environmental sciencesGeophysical Research Letters
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