0000000000041088

AUTHOR

E. E. Haller

showing 5 related works from this author

Microcalorimeter/EBIT measurements of X-ray spectra of highly charged ions

2001

Spectra of highly charged Ar, Kr, Xe and Fe ions, produced in an Electron Beam Ion Trap (EBIT), have been recorded in a broad X-ray energy band (0.2 keV to 10 keV) with a microcalorimeter detector. The first analysis of the Kr spectra has been completed and most of the spectral lines have been identified as transitions of B- to Al-like Kr. Line intensity ratios of Fe XVII have been measured and compared with theoretical models.

PhysicsAtomic and Molecular Physics and OpticPhysics::Instrumentation and DetectorsDetectorTheoretical modelsCondensed Matter PhysicsAtomic and Molecular Physics and OpticsSpectral lineIonSettore FIS/05 - Astronomia E AstrofisicaMathematical PhysicAtomic physicsElectronic band structureX ray spectraMathematical PhysicsLine (formation)Electron beam ion trap
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Astrophysics and spectroscopy with microcalorimeters on an electron beam ion trap

2003

The importance of the combination of electron beam ion trap (EBIT) spectroscopy with X-ray microcalorimeters in the field of astrophysics was discussed. X-ray astronomy involves heavily charged ion instruments , especially EBIT, to obtain improved quality atomic data. In this regard, the research program at the National Institute of Standards and Technology, which uses X-ray spectroscopic methods to study plasma and atomic physics, was also discussed.

PhysicsNuclear and High Energy PhysicsAstrophysics::Instrumentation and Methods for AstrophysicsX-rayHighly charged ionSurfaces Coatings and FilmFizikai tudományokSurfaces and InterfacesPlasmaAstrophysicsHighly charged ionIonX-rayNuclear physicsSettore FIS/05 - Astronomia E AstrofisicaTermészettudományokMicrocalorimeterIonizationCathode rayAtomic physicsLaboratory astrophysicSpectroscopyElectron beam ion trapInstrumentationElectron beam ion trapNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Analysis of broadband x-ray spectra of highly charged krypton from a microcalorimeter detector of an electron-beam ion trap

2001

Spectra of highly charged Kr ions, produced in an electron-beam ion trap (EBIT), have been recorded in a broad x-ray energy band (0.3 keV to 4 keV) with a microcalorimeter detector. Most of the spectral lines have been identified as transitions of B- to Al-like Kr. The transition energies have been determined with 0.2% uncertainty. A semi-empirical EBIT plasma model has been created to calculate a synthetic spectrum of highly charged Kr and to determine a charge state distribution of Kr ions inside the EBIT.

PhysicsDetectorKryptonchemistry.chemical_elementFizikai tudományokPlasmaCondensed Matter PhysicSpectral lineIonPhysics and Astronomy (all)Settore FIS/05 - Astronomia E AstrofisicaTermészettudományokchemistryPhysics::Atomic PhysicsIon trapAtomic physicsElectronic band structureMathematical PhysicsElectron beam ion trapStatistical and Nonlinear Physic
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The constellation-X focal plane microcalorimeter array: An NTD-germanium solution

2002

The hallmarks of Neutron Transmutation Doped (NTD) germanium cryogenic thermistors include high reliability, reproducibility, and long term stability of bulk carrier transport properties. Using micro-machined NTD Ge thermistors with integral “flying” leads, we can now fabricate two-dimensional arrays that are built up from a series of stacked linear arrays. We believe that this modular approach of building, assembling, and perhaps replacing individual modules of detectors is essential to the successful fabrication and testing of large multi-element spectrometers. Details of construction are presented.

PhysicsFabricationSpectrometerbusiness.industryThermistorDopingDetectorchemistry.chemical_elementGermaniummicrocalorimeterX-rayAstrophysicSurface micromachiningCardinal pointOpticsSettore FIS/05 - Astronomia E AstrofisicachemistryNTD GermaniumOptoelectronicsbusiness
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Laboratory astrophysics and microanalysis with NTD-germanium-based X-ray microcalorimeters

2000

With the ability to create cosmic plasma conditions in the laboratory it is possible to investigate the dependencies of key diagnostic X-ray lines on density, temperature, and excitation conditions that exist in astrophysical sources with X-ray optics and a high-resolution X-ray microcalorimeter. The same instrumentation can be coupled to scanning electron microscopes or X-ray fluorescence probes to analyze the elemental and chemical composition of electronic, biological, geological and particulate materials. We describe how our microcalorimeter and X-ray optics provide significantly improved capabilities for laboratory astrophysics and microanalysis.

PhysicsNuclear and High Energy PhysicsX-ray spectroscopyAstrophysics::High Energy Astrophysical PhenomenaResolution (electron density)X-ray opticsX-ray fluorescencechemistry.chemical_elementFizikai tudományokGermaniumAstrophysicsMicroanalysisSettore FIS/05 - Astronomia E AstrofisicaTermészettudományokchemistryAstrophysical plasmaInstrumentationElectron beam ion trapNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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