Search results for "Drift chamber"

showing 4 items of 14 documents

Resolution of the ATLAS muon spectrometer monitored drift tubes in LHC Run 2

2019

The momentum measurement capability of the ATLAS muon spectrometer relies fundamentally on the intrinsic single-hit spatial resolution of the monitored drift tube precision tracking chambers. Optimal resolution is achieved with a dedicated calibration program that addresses the specific operating conditions of the 354 000 high-pressure drift tubes in the spectrometer. The calibrations consist of a set of timing offsets and drift time to drift distance transfer relations, and result in chamber resolution functions. This paper describes novel algorithms to obtain precision calibrations from data collected by ATLAS in LHC Run 2 and from a gas monitoring chamber, deployed in a dedicated gas fac…

Wire chambers (MWPCdrift tube13000 GeV-cmsPhysics::Instrumentation and DetectorsmuonsTracking (particle physics)01 natural sciences030218 nuclear medicine & medical imagingHigh Energy Physics - ExperimentSubatomär fysikMWPCHigh Energy Physics - Experiment (hep-ex)Gaseous detectors0302 clinical medicineWire chambersDrift tubesSubatomic Physicsscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]tracking detectorProportional chambersmomentum resolutionInstrumentationImage resolutionMathematical Physicsdrift tubesPhysicsLarge Hadron ColliderDrift chamberstrack data analysisMuon spectrometersResolution (electron density)DetectorSettore FIS/01 - Fisica SperimentaleATLAS:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]Wire chambers (MWPC Thin-gap chambers drift chambers drift tubes proportional chambers etc)medicine.anatomical_structureCERN LHC Collproportional chambers etc)Gaseous detectors; Muon spectrometers; Particle tracking detectors (gaseous detectors); Wire chambers (MWPC thin-gap chambers drift chambers drift tubes proportional chambers etc)MDT chambersWire chambers (MWPC)LHCcolliding beams [p p]Particle Physics - Experimentp p: scatteringspectrometer [muon]Ciências Naturais::Ciências Físicas530 PhysicsParticle tracking detectors (Gaseous detectors):Ciências Físicas [Ciências Naturais]610FOS: Physical sciencesdrift chamber [muon]gas [monitoring]programming03 medical and health sciencesOpticsAtlas (anatomy)Muon spectrometer0103 physical sciencesCalibrationmedicinemuon: drift chamberGaseous detectorddc:610drift chambersHigh Energy Physicsspatial resolutionMuonScience & Technology010308 nuclear & particles physicsbusiness.industryhep-ex:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]Thin-gap chamberscalibrationmonitoring: gasExperimental High Energy Physicsbusinessp p: colliding beamsmuon: spectrometerexperimental results
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LOFT: the Large Observatory For X-ray Timing

2012

The LOFT mission concept is one of four candidates selected by ESA for the M3 launch opportunity as Medium Size missions of the Cosmic Vision programme. The launch window is currently planned for between 2022 and 2024. LOFT is designed to exploit the diagnostics of rapid X-ray flux and spectral variability that directly probe the motion of matter down to distances very close to black holes and neutron stars, as well as the physical state of ultra-dense matter. These primary science goals will be addressed by a payload composed of a Large Area Detector (LAD) and a Wide Field Monitor (WFM). The LAD is a collimated (<1 degree field of view) experiment operating in the energy range 2-50 keV,…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]VisionX-ray timingAstronomySPIE ProceedingsObservatoriesX-ray timing X-ray spectroscopy X-ray imaging compact objectsSilicon Drift ChambersFOS: Physical sciencesddc:500.2X-ray missionsSpace (mathematics)Astrophysics01 natural sciences7. Clean energySettore FIS/05 - Astronomia E AstrofisicaX-rays0103 physical sciencesElectronicOptical and Magnetic MaterialsInstrumentation (computer programming)Electrical and Electronic EngineeringAerospace engineeringDiagnosticsCompact objects010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsSpatial resolutionsezeleSensors010308 nuclear & particles physicsbusiness.industryApplied MathematicsX-ray imagingSilicon Drift ChamberComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicsCompact objects; X-ray imaging; X-ray spectroscopy; X-ray timing; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic Engineering[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]X-ray spectroscopySilicon Drift Chambers; X-ray missionsInstrumentation and Methods for AstrophysicsAstrophysics - Instrumentation and Methods for Astrophysicsbusiness
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Efficiencies of the drift chambers in the EMMA experiment

2013

Cosmic rays are high-energy subatomic particles which travel almost at the speed of light all over the space. The shape of the cosmic ray energy spectrum is measured experimentally, but it is not perfectly understood. The slope of the spectrum at high energies is constant up to the knee energy (about 10^15 eV) where the slope steepens. The knee has been tried to be explained by several models which aim to describe the origin and the acceleration mechanisms of the cosmic ray. The stars and the shockwaves from supernova explosions are believed to be at least a part of cosmic ray evolution. The cosmic rays were found in the early 20th century and they have been studied with several methods. Wh…

drift chamberkosminen säteilycosmic rayajautumiskammiot
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The OLYMPUS Experiment

2014

Nuclear instruments & methods in physics research / A 741, 1 - 17 (2014). doi:10.1016/j.nima.2013.12.035

two-photon [exchange]Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsHadronluminosity: monitoringRecoil4-MOMENTUM TRANSFERSNuclear Experiment (nucl-ex)Nuclear ExperimentInstrumentationNuclear ExperimentPhysicsElastic scatteringLuminosity (scattering theory)ELECTROMAGNETIC FORM-FACTORSInstrumentation and Detectors (physics.ins-det)elastic scattering [cross section]positron p: elastic scatteringAntimatterdrift chamberelastic scattering [electron p]target [hydrogen]proportional chamberCROSS-SECTIONNuclear and High Energy PhysicsELECTRON-PROTONDESY DORIS StorFOS: Physical sciencesmonitoring [luminosity]time-of-flight530electron p: elastic scatteringNuclear physicsCross section (physics)RATIO(GEV/C)(2)p: form factor: ratiocalorimeterddc:530cross section: elastic scatteringactivity reporthydrogen: targetexchange: two-photonScatteringPOSITRONSDESYelastic scattering [positron p]magnetic spectrometerELECTROMAGNETIC FORM-FACTORS; PROTON ELASTIC-SCATTERING; 4-MOMENTUM TRANSFERS; ELECTRON-PROTON; CROSS-SECTION; RATIO; (GEV/C)(2); POSITRONSform factor: ratio [p]gas electron multiplierPhysics::Accelerator PhysicsPROTON ELASTIC-SCATTERINGHigh Energy Physics::Experiment
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