6533b861fe1ef96bd12c5a02
RESEARCH PRODUCT
Laboratory astrophysics and microanalysis with NTD-germanium-based X-ray microcalorimeters
D.a. LandisE. E. HallerEndre TakacsJames V. PortoJohn D. GillaspySimon R. BandlerG TuckerM. BarberaJeffrey W. BeemanS. S. MurrayHerbert W. SchnopperNorman W. MaddenEric H. Silversubject
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 trapdescription
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.
year | journal | country | edition | language |
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2000-04-01 | Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |