Search results for "Cryostat"

showing 10 items of 26 documents

A Temperature-Dependent X-Ray Absorption Characterization of Test Filters for the ATHENA Mission X-IFU Instrument

2018

In order to work properly, the X-ray Integral Field Unit of the ATHENA mission requires a set of thermal filters that block the infrared radiation, preventing it to reach the detector. Each filter will be mounted and thermally anchored onto a shield of the multistage cryostat and will be kept at the specific temperature of the stage. On the other hand, the filters partially absorb X-rays, and their transmittance has to be carefully characterized. The effect of temperature on the absorption edges of the elements that make up the filters has not been investigated yet. Here, we report the results of a preliminary run on the optical transmission data around the edges of C, N, and O at different…

CryostatAtomic and Molecular Physics and OpticMaterials scienceInfraredThermal filter-02 engineering and technology01 natural sciencesOptics0103 physical sciencesThermalTransmittanceGeneral Materials Science010306 general physicsAbsorption (electromagnetic radiation)X-IFUbusiness.industryDetector021001 nanoscience & nanotechnologyCondensed Matter PhysicsAtomic and Molecular Physics and OpticsATHENAK-edgeK-edgeFilter (video)Materials Science (all)0210 nano-technologybusinessJournal of Low Temperature Physics
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Baseline design of the thermal blocking filters for the X-IFU detector on board ATHENA

2014

ATHENA is an advanced X-ray observatory designed by a large European consortium to address the science theme "Hot and Energetic Universe" recently selected by ESA for L2 – the second Large-class mission within the Cosmic Vision science program (launch scheduled in 2028). One of the key instruments of the mission is the X-ray Integral Field Unit (X-IFU), an array of Transition Edge Sensor (TES) micro-calorimeters with high energy resolution (2.5 eV @ 6 keV) in the energy range 0.2÷12 keV, operating at the focal plane of a large effective area high angular resolution (5" HEW) grazing incidence X-ray telescope. The X-IFU operates at temperatures below 100 mK and thus requires a sophisticated c…

CryostatCosmic VisionVisionShieldsX-ray telescopeGrazing incidencelaw.inventionTelescopeOpticsSettore FIS/05 - Astronomia E AstrofisicalawX-raysElectronicmicro-calorimeterOptical and Magnetic MaterialsElectrical and Electronic EngineeringX-ray telescopesPhysicsX-IFUSpatial resolutionSounding rocketEquipment and servicesbusiness.industrySensorsApplied MathematicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsOptical Blocking FiltersComputer Science Applications1707 Computer Vision and Pattern RecognitionDetector arraysCondensed Matter PhysicsATHENAmissionsCultural heritageTransition edge sensorbusinessATHENA; micro-calorimeter; missions; Optical Blocking Filters; X-IFU; X-rays; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringTelescopes
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Temperature effects on the performances of the ATHENA X-IFU thermal filters

2016

The X-Ray Integral Field Unit (X-IFU) detector on-board ATHENA is an array of TES micro-calorimeters that will operate at ~50 mK. In the current investigated design, five thermal filters (TF) will be mounted on the cryostat shields to attenuate IR radiative load and avoid energy resolution degradation due to photon shot noise. Each filter consists of a thin polyimide film (~50 nm thick) coated with aluminum (~30 nm thick). Since the TF operate at different temperatures in the range 0.05-300 K, it is relevant to study how temperature affects their mechanical/optical performances (e.g. near edge absorption fine structures of the atomic elements in the filter material). Such results are crucia…

CryostatMaterials scienceAbsorption spectroscopybusiness.industrythermal filtersATHENA missionShot noise02 engineering and technologyAtmospheric temperature range021001 nanoscience & nanotechnologyATHENA mission thermal filters XANES01 natural sciencesXANESSettore FIS/05 - Astronomia E AstrofisicaOptics0103 physical sciencesRadiative transferCalibration010306 general physics0210 nano-technologybusinessAbsorption (electromagnetic radiation)PolyimideSPIE Proceedings
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On-line Mössbauer measurements at low temperatures of 83mKr implanted into Al

1978

Abstract A vacuum ion implantation chamber housing a helium flow cryostat and a Mossbauer transducer has been constructed and coupled directly to an ion separator for low temperature implantation and on-line Mossbauer measurements. 83m Kr, produced by thermal neutron activation of enriched 82 Kr gas, has been implanted into Al foils in the temperature range 15–300 K. Annealing effects and the temperature dependence of the Lamb-Mossbauer factor have been studied by Mossbauer measurements (at 15–35 K) using the implanted Al targets as sources and Kr/hydrochinone as absorber.

CryostatMaterials scienceAnnealing (metallurgy)Analytical chemistrychemistry.chemical_elementGeneral MedicineAtmospheric temperature rangeNeutron temperatureIonIon implantationNuclear magnetic resonancechemistryMössbauer spectroscopyHeliumNuclear Instruments and Methods
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Thermal modelling of the ATHENA X-IFU filters

2018

Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. The X-IFU instrument of the ATHENA mission requires a set of thermal filters to reduce the photon shot noise onto its cryogenic detector and to protect it from molecular contamination. A set of five filters, operating at different nominal temperatures corresponding to the cryostat shield temperatures, is currently baselined. The knowledge of the actual filter temperature profi…

CryostatMaterials scienceCondensed Matter Physic01 natural sciencesthermal simulationSettore FIS/05 - Astronomia E AstrofisicaOpticsthermal filter0103 physical sciencesThermalEmissivityRadiative transferElectrical and Electronic Engineering010306 general physicsThermal analysis010303 astronomy & astrophysicsX-IFUbusiness.industryElectronic Optical and Magnetic MaterialDetectorShot noiseComputer Science Applications1707 Computer Vision and Pattern RecognitionATHENAApplied MathematicFilter (video)businessSpace Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
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On the nuclear response of the helium-cooled lithium lead test blanket module in ITER

2005

Abstract The helium-cooled lithium lead (HCLL) concept has been recently selected as one of the two European reference designs foreseen for the breeding blanket of a demonstration fusion reactor. In particular, within the framework of the research and development activities on this blanket line, an HCLL test blanket module (TBM) has to be designed and manufactured to be implemented in ITER. At the Department of Nuclear Engineering (DIN) of the University of Palermo, a research campaign has been carried out to investigate the nuclear response of HCLL-TBM inside ITER by a numerical approach based on the Monte Carlo method. A realistic 3D heterogeneous model of HCLL-TBM has been set-up and ins…

CryostatMaterials scienceMechanical EngineeringNuclear engineeringMonte Carlo methodchemistry.chemical_elementBlanketFusion powerNuclear Energy and EngineeringchemistryTest blanket moduleHCLL-blanketNeutronicsRadiation damageNeutron sourceGeneral Materials ScienceLithiumSettore ING-IND/19 - Impianti NucleariHeliumCivil and Structural EngineeringFusion Engineering and Design
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Radio frequency shielding of thin aluminized plastic filters investigated for the ATHENA X-IFU detector

2018

Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. The X-ray Integral Field Unit (X-IFU) is one of the two detectors of the ATHENA astrophysics space mission approved by ESA in the Cosmic Vision 2015-2025 Science Programme. The X-IFU consists of a large array of transition edge sensors (TES) micro-calorimeters covering a field of view of 5' diameter, sensitive in the energy range 0.2-12 keV, and providing a spectral resolution…

CryostatMaterials sciencePhysics::Instrumentation and DetectorsX-ray detectorRF attenuationField of viewCondensed Matter Physic02 engineering and technologyreverberation chamber7. Clean energyElectromagnetic interferenceSettore FIS/05 - Astronomia E AstrofisicaOpticsX-ray Integral Field Unit (X-IFU)thermal thin-film filter0202 electrical engineering electronic engineering information engineeringElectrical and Electronic Engineeringbusiness.industryElectronic Optical and Magnetic Material020502 materialsDetectorAstrophysics::Instrumentation and Methods for Astrophysicsx-ray detectorComputer Science Applications1707 Computer Vision and Pattern Recognition020206 networking & telecommunicationsresonance modeApplied MathematicATHENA X-ray observatoryEMI shielding0205 materials engineeringElectromagnetic shieldingRadio frequencyAntenna (radio)businessSpace Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
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A study of the potential influence of frame coolant distribution on the radiation-induced damage of HCLL-TBM structural material

2008

Abstract Within the European Fusion Technology Programme, the Helium-Cooled Lithium Lead (HCLL) breeding blanket concept is one of the two EU lines to be developed for a Long Term fusion reactor, in particular with the aim of manufacturing a Test Blanket Module (TBM) to be implemented in ITER. The HCLL-TBM is foreseen to be located in an ITER equatorial port, being housed inside a steel-supporting frame, actively cooled by pressurized water. That supporting frame has been designed to house two different TBMs, providing two cavities separated by a dividing Plate 20 cm thick. As the nuclear response of HCLL-TBM might vary accordingly to the supporting frame configuration and composition, at t…

CryostatNeutron transportMaterials scienceMechanical EngineeringNuclear engineeringFrame (networking)Fusion powerBlanketCoolantNuclear Energy and EngineeringNeutron sourceGeneral Materials ScienceLithium-lead blanket TBM NeutronicsSettore ING-IND/19 - Impianti NucleariCivil and Structural EngineeringParametric statisticsFusion Engineering and Design
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Study of the helium-cooled lithium lead test blanket module nuclear behaviour under irradiation in ITER

2009

Abstract The present paper deals with the detailed investigation of the helium-cooled lithium lead test blanket module (HCLL-TBM) nuclear behaviour under irradiation in ITER, carried out at the Department of Nuclear Engineering of the University of Palermo adopting a numerical approach based on the Monte Carlo method. A realistic 3D heterogeneous model of the HCLL-TBM was set-up and inserted into an ITER 3D semi-heterogeneous model that realistically simulates the reactor lay-out up to the cryostat. A Gaussian-shaped neutron source was adopted for the calculations. The main features of the HCLL-TBM nuclear response were assessed, paying a particular attention to the neutronic and photonic d…

CryostatNeutron transportTokamakMaterials scienceMechanical EngineeringNuclear engineeringchemistry.chemical_elementFusion powerBlanketHCLL test blanket module Neutronics Monte Carlo methodlaw.inventionNuclear physicsNuclear Energy and EngineeringchemistrylawNeutron sourceGeneral Materials ScienceLithiumSettore ING-IND/19 - Impianti NucleariHeliumCivil and Structural EngineeringFusion Engineering and Design
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A Mössbauer cryostat equipped with a Gifford McMahon cryocooler

1989

A new cryostat for Mossbauer spectroscopic measurements has been developed around a cryogenerator of the Gifford McMahon type operating with helium gas in a closed circuit. Both source and absorber can be cooled to about 30K and the unwanted vibrations caused by the helium compression/expansion cycle have been limited to approximately 0.05–0.06 mms−1.

CryostatNuclear and High Energy PhysicsHelium gasChemistryThermodynamicschemistry.chemical_elementControl equipmentCryogenicsCryocoolerCondensed Matter PhysicsAtomic and Molecular Physics and OpticsMössbauer spectroscopyPhysical and Theoretical ChemistryAtomic physicsClosed circuitHeliumHyperfine Interactions
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