Search results for " Gamma ray"

showing 10 items of 74 documents

Spectroscopic response of a CdZnTe multiple electrode detector

2007

Abstract The spectroscopic performances of a CdZnTe detector (crystal size: 5×5×0.9 mm 3 ) with five electrodes (cathode, anode and three steering electrodes) were studied. The anode layout, which consists of a circular electrode ( φ =80 μm) surrounded by two ring electrodes (gap=100 μm; radial width Δ r =100 μm) and by one electrode that extends to the edge of the crystal, is mostly sensitive to the electron carriers, overcoming the well known effect of the hole trapping in the measured spectra. We report on the spectroscopic response of the detector at different bias voltages of the electrodes and at various photon energies ( 109 Cd, 241 Am and 57 Co sources). The CdZnTe detector exhibits…

PhysicsNuclear and High Energy PhysicsSpectrometerbusiness.industryCdZnTe detectorSteering electrodeDetectorMultiple electrode detectorElectronSmall pixel effectCathodeAnodelaw.inventionCrystalFull width at half maximumX-ray and gamma ray spectroscopylawElectrodeOptoelectronicsbusinessInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Coronal fuzziness modelled with pulse-heated multistranded loop systems

2010

Coronal active regions are observed to get fuzzier and fuzzier (i.e. more and more confused and uniform) in harder and harder energy bands or lines. We explain this evidence as due to the fine multi-temperature structure of coronal loops. To this end, we model bundles of loops made of thin strands, each heated by short and intense heat pulses. For simplicity, we assume that the heat pulses are all equal and triggered only once in each strand at a random time. The pulse intensity and cadence are selected so as to have steady active region loops ($\sim 3$ MK), on the average. We compute the evolution of the confined heated plasma with a hydrodynamic loop model. We then compute the emission al…

PhysicsPhase (waves)FOS: Physical sciencesAstronomy and AstrophysicsPlasmaCoronal loopAstrophysicsSpectral lineComputational physicsPulse (physics)Loop (topology)Settore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceCoronal planeBundleSun: corona Sun: X-rays gamma raysSolar and Stellar Astrophysics (astro-ph.SR)
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Comparison of Hinode/XRT and RHESSI detection of hot plasma in the non-flaring solar corona

2009

We compare observations of the non-flaring solar corona made simultaneously with Hinode/XRT and with RHESSI. The analyzed corona is dominated by a single active region on 12 November 2006. The comparison is made on emission measures. We derive emission measure distributions vs temperature of the entire active region from multifilter XRT data. We check the compatibility with the total emission measure values estimated from the flux measured with RHESSI if the emission come from isothermal plasma. We find that RHESSI and XRT data analyses consistently point to the presence of a minor emission measure component peaking at log T ~ 6.8-6.9. The discrepancy between XRT and RHESSI results is withi…

PhysicsStellar atmosphereGamma rayFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPlasmaSolar atmosphereCoronaElectromagnetic radiationStarsSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSun: corona Sun: X-rays gamma raysMain sequenceSolar and Stellar Astrophysics (astro-ph.SR)
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Nonequilibrium of Ionization and the Detection of Hot Plasma in Nanoflare‐heated Coronal Loops

2008

Impulsive nanoflares are expected to transiently heat the plasma confined in coronal loops to temperatures of the order of 10 MK. Such hot plasma is hardly detected in quiet and active regions, outside flares. During rapid and short heat pulses in rarified loops the plasma can be highly out of equilibrium of ionization. Here we investigate the effects of the non-equilibrium of ionization (NEI) on the detection of hot plasma in coronal loops. Time-dependent loop hydrodynamic simulations are specifically devoted to this task, including saturated thermal conduction, and coupled to the detailed solution of the equations of ionization rate for several abundant elements. In our simulations, initi…

PhysicsSun: Corona Sun: X-Rays Gamma RaysAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsCoronal loopPlasmaAstrophysicsThermal conductionMagnetic fluxNanoflaresPulse (physics)Settore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceIonizationPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsAtomic physicsThe Astrophysical Journal
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Thermal structure of a hot non-flaring corona from Hinode/EIS

2014

In previous studies a very hot plasma component has been diagnosed in solar active regions through the images in three different narrow-band channels of SDO/AIA. This diagnostic from EUV imaging data has also been supported by the matching morphology of the emission in the hot Ca XVII line, as observed with Hinode/EIS. This evidence is debated because of unknown distribution of the emission measure along the line of sight. Here we investigate in detail the thermal distribution of one of such regions using EUV spectroscopic data. In an active region observed with SDO/AIA, Hinode/EIS and XRT, we select a subregion with a very hot plasma component and another cooler one for comparison. The ave…

PhysicsSun: corona Sun: UV radiation Sun: X-rays gamma rays techniques: spectroscopic techniques: imaging spectroscopyLine-of-sightSun: coronaExtreme ultraviolet lithographyTechniques: spectroscopicFOS: Physical sciencesAstronomy and AstrophysicsThermal distributionPlasmaAstrophysicsAstronomy and AstrophysicSun: UV radiationImaging dataCoronaSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSun: X-rays gamma raySpace and Planetary ScienceThermalTechniques: imaging spectroscopySolar and Stellar Astrophysics (astro-ph.SR)Line (formation)Astronomy & Astrophysics
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Characterization of Al-Schottky CdTe detectors

2011

In the last decades, great efforts are being devoted to the development of CdTe detectors for high resolution X-ray and gamma ray spectroscopy. Recently, new rectifying contacts based on aluminum (Al) are very appealing in the development of CdTe detectors with low leakage currents and anode pixellization. In this work, we report on preliminary results of electrical and spectroscopic investigations on Schottky CdTe diode detectors (4.1 × 4.1 × 0.75 and 4.1 × 4.1 × 2 mm3) with Au/Ti/Al/CdTe/Pt electrode configuration. The detectors are characterized by very low leakage currents even at room temperature (26 pA at 25 °C under a bias voltage of −100 V for the 2 mm thick detector). Polarization …

PhysicsX-ray spectroscopySpectrometerbusiness.industrySettore FIS/01 - Fisica SperimentaleDetectorSchottky diodeBiasingSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)AnodeCdTe detectorFull width at half maximumX-ray and gamma ray spectroscopyOpticsOptoelectronicsGamma spectroscopybusiness2011 IEEE Nuclear Science Symposium Conference Record
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Widespread Nanoflare Variability Detected with Hinode/X-Ray Telescope in a Solar Active Region

2011

It is generally agreed that small impulsive energy bursts called nanoflares are responsible for at least some of the Sun's hot corona, but whether they are the explanation for most of the multimillion-degree plasma has been a matter of ongoing debate. We present here evidence that nanoflares are widespread in an active region observed by the X-Ray Telescope on board the Hinode mission. The distributions of intensity fluctuations have small but important asymmetries, whether taken from individual pixels, multipixel subregions, or the entire active region. Negative fluctuations (corresponding to reduced intensity) are greater in number but weaker in amplitude, so that the median fluctuation i…

Physicsmedia_common.quotation_subjectAstronomy and AstrophysicsAstrophysicsPlasmaactivity Sun: corona Sun: X-rays gamma rays [Sun]Poisson distributionCoronaAsymmetryIntensity (physics)Nanoflareslaw.inventionTelescopesymbols.namesakeAmplitudeSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary SciencelawPhysics::Space PhysicssymbolsSun: activity Sun: corona Sun: X-rays gamma raysAstrophysics::Solar and Stellar Astrophysicsmedia_common
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Electrical Characterization of CdTe pixel detectors with Al Schottky anode

2014

Abstract Pixelated Schottky Al/p-CdTe/Pt detectors are very attractive devices for high-resolution X-ray spectroscopic imaging, even though they suffer from bias-induced time instability (polarization). In this work, we present the results of the electrical characterization of a (4×4) pixelated Schottky Al/p-CdTe/Pt detector. Current–voltage ( I–V ) characteristics and current transients were investigated at different temperatures. The results show deep levels that play a dominant role in the charge transport mechanism. The conduction mechanism is dominated by the space charge limited current (SCLC) both under forward bias and at high reverse bias. Schottky barrier height of the Al/CdTe con…

PhysicspolarizationNuclear and High Energy PhysicsSchottky contactbusiness.industrySchottky barrierSettore FIS/01 - Fisica SperimentaleSchottky diodeCdTeThermal conductionSpace chargeCadmium telluride photovoltaicsSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Settore FIS/03 - Fisica Della MateriaAnodeX-ray and gamma ray spectroscopypixel detectorOptoelectronicsPolarization (electrochemistry)businessCdTe; Schottky contacts; polarization; pixel detectors; X-ray and gamma ray spectroscopyInstrumentationVoltage
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INTEGRAL/SPI ground calibration

2003

Three calibration campaigns of the spectrometer SPI have been performed before launch in order to determine the instrument characteristics, such as the effective detection area, the spectral resolution and the angular resolution. Absolute determination of the effective area has been obtained from simulations and measurements. At 1 MeV, the effective area is 65 cm^2 for a point source on the optical axis, the spectral resolution ~2.3 keV. The angular resolution is better than 2.5 deg and the source separation capability about 1 deg. Some temperature dependant parameters will require permanent in-flight calibration.

Point source[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FOS: Physical sciencesInstrumentation ; Detectors ; Spectrographs ; Space vehicles ; Gamma rays ; ObservationsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]OpticsSpectrographs0103 physical sciencesCalibrationSource separationAngular resolutionSpectral resolutionspace vehicles: instrumentsInstrumentation010303 astronomy & astrophysicsObservations:ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica [UNESCO]instrumentation: spectrographsPhysicsSpectrometer[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryinstrumentation: detectorsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía ópticaGamma raysAntenna apertureAstrophysics (astro-ph)DetectorsSpace vehiclesAstronomy and AstrophysicsOptical axisSpace and Planetary Sciencebusiness:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]gamma rays: observations
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Recent trends in the development of CdTe and CdZnTe semiconductor detectors for astrophysical applications

2010

Cadmium telluride (CdTe) and cadmium zinc telluride (CdZnTe) offer great promise as x-ray and gamma ray detectors. Due to the high detection efficiency, the good room temperature performance and the recent improvements on crystal growth technology, CdTe and CdZnTe detectors have obtained an increasing interest in the field of hard x-ray and gamma ray astronomy. In this paper, we report on the R&D activities on CdTe and CdZnTe detectors for high energy space instrumentation. Our group has been involved in the design of new multilayer hard x and soft gamma ray Laue lens telescopes and, in particular on the development of focal plane detectors based on CdTe and CdZnTe. Here we present the acti…

Semiconductor detectorX-ray and gamma ray spectroscopySettore FIS/01 - Fisica SperimentaleCdTe and CdZnTeImaging
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