Search results for "Instrumentation"

showing 10 items of 4914 documents

Ultra-Fast Flash Observatory for the observation of early photons from gamma-ray bursts

2013

One of the least documented and understood aspects of gamma-ray bursts (GRBs) is the rise phase of the optical light curve. The Ultra-Fast Flash Observatory (UFFO) is an effort to address this question through extraordinary opportunities presented by a series of space missions including a small spacecraft observatory. The UFFO is equipped with a fast-response Slewing Mirror Telescope (SMT) that uses a rapidly moving mirror or mirror array to redirect the optical beam rather than slewing the entire spacecraft to aim the optical instrument at the GRB position. The UFFO will probe the early optical rise of GRBs with sub-second response, for the first time, opening a completely new frontier in …

PhysicsSpacecraftbusiness.industrySpace instrumentAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsGeneral Physics and AstronomyAstronomyCosmic rayAstrophysicsSpace explorationGamma ray burstslaw.inventionTelescopeFlash (photography)ObservatorylawGRB 090423Gamma-ray bursts (GRBs)businessGamma-ray burstScientific instrument
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Spectrum and charge ratio of vertical cosmic ray muons up to momenta of 2.5 TeV/c

2013

The ALEPH detector at LEP has been used to measure the momentum spectrum and charge ratio of vertical cosmic ray muons underground. The sea-level cosmic ray muon spectrum for momenta up to 2.5 TeV/c has been obtained by correcting for the overburden of 320 meter water equivalent (mwe). The results are compared with Monte Carlo models for air shower development in the atmosphere. From the analysis of the spectrum the total flux and the spectral index of the cosmic ray primaries is inferred. The charge ratio suggests a dominantly light composition of cosmic ray primaries with energies up to 10^15 eV.

PhysicsSpectral indexMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesFluxCosmic rayAstronomy and AstrophysicsHigh Energy Physics - ExperimentNuclear physicsMomentumHigh Energy Physics - Experiment (hep-ex)Air showerHigh Energy Physics::ExperimentUltra-high-energy cosmic rayParticle Physics - ExperimentAstroparticle Physics
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Penning discharge in the KATRIN pre-spectrometer

2014

The KArlsruhe TRItium Neutrino (KATRIN) experiment is a next-generation, large-scale tritium β-decay experiment to determine the neutrino mass by investigating the kinematics of tritium β-decay with a sensitivity of 200 meV/c2 using the MAC-E filter technique. In order to reach this sensitivity a low background level of 10−2 counts per second (cps) is required. A major background concern in MAC-E filters is the presence of Penning traps. A Penning trap is a special configuration of electromagnetic fields that allows the storage of electrically charged particles. This paper describes the mechanism of Penning discharges and the corresponding measurements performed at the test setup of the KAT…

PhysicsSpectrometerCyclotronElectronPenning trapCharged particlelaw.inventionNuclear physicslawIon trapNeutrinoAtomic physicsInstrumentationMathematical PhysicsKATRINJournal of Instrumentation
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Compton imaging with AGATA and SmartPET for DESPEC

2011

DESPEC (DEcay SPECtroscopy) is a spectrometer, currently under construction, which is to be used at the FAIR (Facility for Antiproton and Ion Research) facility at GSI Darmstadt, Germany, as part of the NuSTAR (Nuclear STructure, Astrophysics and Reactions) project. Its goal is to analyse the decay of exotic nuclei produced via the Super-FRS (SUPERconducting FRagment Separator). The optimal configuration of certain elements of the spectrometer, namely a HPGe (High Purity Germanium) tracking array, is still under consideration. Work currently being carried out at the University of Liverpool using a segmented, coaxial HPGe detector (AGATA B009) and a pixelated, planar HPGe detector (SmartPET …

PhysicsSpectrometerPhysics::Instrumentation and DetectorsCompton imagingDetectorGamma rayCompton cameraSemiconductor detectorNuclear physicsFacility for Antiproton and Ion ResearchHigh Energy Physics::ExperimentAGATANuclear ExperimentInstrumentationMathematical PhysicsJournal of Instrumentation
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Endcap Disc DIRC for PANDA at FAIR

2018

The Endcap Disc DIRC (EDD) has been developed to provide an excellent particle identification in the future PANDA experiment by separating pions and kaons up to a momentum of 4 GeV/c with a separation power of 3 s.d.. The detector is placed in the forward endcap of the PANDA target spectrometer. It consists of a fused silica plate and focusing elements placed at the outer rim, which focus the Cherenkov light on the photo cathodes of the attached MCP-PMTs. A compact and fast readout of the signals is realized with special ASICs. The performance has been studied and validated with different prototype setups in various testbeam facilities.

PhysicsSpectrometerPhysics::Instrumentation and Detectorsbusiness.industryCherenkov detectorDetectorParticle identificationlaw.inventionOpticslawHigh Energy Physics::ExperimentNuclear ExperimentbusinessCherenkov radiation
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The Cryogenic Anticoincidence Detector for ATHENA-XMS

2012

The TES cryogenic detectors, due to their high spectral resolution and imaging capability in the soft X-ray domain, are the reference devices for the next proposed space missions whose aims are to characterize the spectra of faint or diffuse sources. ATHENA is the re-scoped IXO mission, and one of its focal plane instrument is the X-ray Microcalorimeter Spectrometer (XMS) working in the energy range 0.3-10 keV. XMS will be able to achieve the proposed scientific goals if a background lower than 0.02 cts/cm2/s/keV is guaranteed. The studies performed by GEANT4 simulations depict a scenario where it is mandatory to use an active Anti-Coincidence (AC) to reduce the expected background in the L…

PhysicsSpectrometerPhysics::Instrumentation and Detectorsbusiness.industryDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysicsCondensed Matter PhysicsAtomic and Molecular Physics and OpticsSpace explorationSpectral lineLow temperature detectors · Astronomy and astrophysics · Superconductivity · Silicon · TESSettore FIS/05 - Astronomia E AstrofisicaCardinal pointOpticsOrbit (dynamics)General Materials ScienceSpectral resolutionbusinessEnergy (signal processing)Journal of Low Temperature Physics
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Enhancing the sensitivity of recoil-beta tagging

2013

Tagging with β-particles at the focal plane of a recoil separator has been shown to be an effective technique for the study of exotic proton-rich nuclei. This article describes three new pieces of apparatus used to greatly improve the sensitivity of the recoil-beta tagging technique. These include a highly-pixelated double-sided silicon strip detector, a plastic phoswich detector for discriminating high-energy β-particles, and a charged-particle veto box. The performance of these new detectors is described and characterised, and the resulting improvements are discussed.

PhysicsSpectrometerPhysics::Instrumentation and Detectorsbusiness.industryDetectorRecoil separatorNuclear physicsCardinal pointOpticsRecoilBeta (plasma physics)Phoswich detectorSensitivity (control systems)businessInstrumentationMathematical PhysicsJournal of Instrumentation
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Electrostatically operated micromirrors for a Hadamard transform spectrometer

2002

The paper presents the development of a linear micromirror array which can be used as a switchable entrance mask for a double-array Hadamard transform spectrometer. In addition to the detector array the double-array spectrometer has a linear multi-slit array realised by independently switchable micromirrors at the entrance side. Two different switch positions of the electrostatically operated mirrors allow the reflection of light into or away from the spectrometer. With this arrangement (mirror array, concave grating and array detector) and the use of the Hadamard transform principle it is possible to increase the signal-to-noise ratio and the resolution of the system compared to convention…

PhysicsSpectrometerPhysics::Instrumentation and Detectorsbusiness.industryResolution (electron density)DetectorMicromirror arrayPhysics::OpticsGratingOptical switchOpticsHadamard transformDetector arraybusiness1998 IEEE/LEOS Summer Topical Meeting. Digest. Broadband Optical Networks and Technologies: An Emerging Reality. Optical MEMS. Smart Pixels. Organic Optics and Optoelectronics (Cat. No.98TH8369)
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A Mott polarimeter operating at MeV electron beam energies.

2011

We have developed a Mott electron polarimeter for the Mainzer microtron (MAMI) accelerator in Mainz, Germany. At beam energies ranging between 1.0 and 3.5 MeV two double focusing magnet spectrometers collect elastically backscattered electrons from gold targets. In spite of the small spectrometer acceptance, a sufficient statistical efficiency is achieved to provide very fast measurements if beam currents typical for experiments at MAMI are being used. High reproducibility is achieved, demonstrating that the results of asymmetry measurements are independent of the primary beam current in a range from 0.004 to 45 μA at a level of <1% relative variation. Compared to low energy polarimeters of…

PhysicsSpectrometerbusiness.industryCyclotronPolarimeterParticle acceleratorMott scatteringlaw.inventionNuclear physicsOpticslawElectron opticsPhysics::Accelerator PhysicsNuclear ExperimentbusinessInstrumentationMicrotronBeam (structure)The Review of scientific instruments
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Oscillating ultra-cold neutron spectrometer

2019

The energy spectrum of ultra-cold neutrons (UCN) is very often a key point to determine the systematic effects in precision measurements utilizing UCN. The proposed novel method allows the in-situ measurements of the UCN velocity distribution and its time evolution. In addition, the proposed UCN spectrometer can be a handy diagnostic tool for monitoring the UCN spectrum in critical places in the transport system connecting an UCN source with experiments. In this paper, we present the preliminary results from measurements and simulations using the oscillating UCN spectrometer at the PSI UCN source.

PhysicsSpectrometerbusiness.industryPhysics::Instrumentation and DetectorsPhysicsQC1-999Time evolutionKey pointOpticsEnergy spectrumNeutronbusinessNuclear ExperimentTransport system
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