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Prinja, A.K.; Gleicher, F.; Dunham, G.; Morel, J.E.
Univ. of New Mexico, Albuquerque, NM (United States)1999
Univ. of New Mexico, Albuquerque, NM (United States)1999
AbstractAbstract
[en] Inelastic ion interactions with target electrons are dominated by extremely small energy transfers that are difficult to resolve numerically. The continuous-slowing-down (CSD) approximation is then commonly employed, which, however, only preserves the mean energy loss per collision through the stopping power, S(E) = ∫0∞ dEprime (E minus Eprime) σs (E → Eprime). To accommodate energy loss straggling, a Gaussian distribution with the correct mean-squared energy loss (akin to a Fokker-Planck approximation in energy) is commonly used in continuous-energy Monte Carlo codes. Although this model has the unphysical feature that ions can be upscattered, it nevertheless yields accurate results. A multigroup model for energy loss straggling was recently presented for use in multigroup Monte Carlo codes or in deterministic codes that use multigroup data. The method has the advantage that the mean and mean-squared energy loss are preserved without unphysical upscatter and hence is computationally efficient. Results for energy spectra compared extremely well with Gaussian distributions under the idealized conditions for which the Gaussian may be considered to be exact. Here, the authors present more consistent comparisons by extending the method to accommodate upscatter and, further, compare both methods with exact solutions obtained from an analog Monte Carlo simulation, for a straight-ahead transport problem
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American Nuclear Society 1999 Winter Meeting; Long Beach, CA (United States); 14-18 Nov 1999
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Journal Article
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Conference
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Miller, S.; Laudal, D.; Dunham, G.
Eleventh annual coal preparation, utilization, and environmental control contractors conference: Proceedings1995
Eleventh annual coal preparation, utilization, and environmental control contractors conference: Proceedings1995
AbstractAbstract
[en] The ability to remove mercury from power plant flue gas may become important because of the Clean Air Act amendments' requirement that the U.S. Environmental Protection Agency (EPA) assess the health risks associated with these emissions. One approach for mercury removal, which may be relatively simple to retrofit, is the injection of sorbents, such as activated carbon, upstream of existing particulate control devices. Activated carbon has been reported to capture mercury when injected into flue gas upstream of a spray dryer baghouse system applied to waste incinerators or coal-fired boilers. However, the mercury capture ability of activated carbon injected upstream of an electrostatic precipitator (ESP) or baghouse operated at temperatures between 200 degrees and 400 degrees F is not well known. A study sponsored by the U.S. Department of Energy and the Electric power Research Institute is being conducted at the University of North Dakota Energy ampersand Environmental Research Center (EERC) to evaluate whether mercury control with sorbents can be a cost-effective approach for large power plants. Initial results from the study were reported last year. This paper presents some of the recent project results. Variables of interest include coal type, sorbent type, sorbent addition rate, collection media, and temperature
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USDOE Pittsburgh Energy Technology Center, PA (United States); 440 p; 1995; p. 129-136; 11. annual coal preparation, utilization, and environmental control contractors conference; Pittsburgh, PA (United States); 12-14 Jul 1995; Also available from OSTI as DE95017240; NTIS; GPO; US Govt. Printing Office Dep
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Report
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Conference
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INIS IssueINIS Issue
Olsen, L.C.; Huber, D.A.; Dunham, G.; Addis, F.W.
Twenty first IEEE photovoltaic specialists conference 1990 (Conference Record)1990
Twenty first IEEE photovoltaic specialists conference 1990 (Conference Record)1990
AbstractAbstract
[en] This paper involves theoretical studies of current loss mechanisms in GaAs solar cells using PC-1D. In particular, the contribution to current-voltage characteristics of depletion layer recombination via traps at various locations in the forbidden gap has been modeled using PC-1D. The results of these studies are used to interpret experimental data for high efficiency GaAs solar cells. It is found that the double mechanism characteristic observed for high efficiency GaAs cells can usually be interpreted in terms of two mechanisms acting in parallel, one due to recombination via a midgap trap with n = 2, and another at higher voltages due to emitter/base recombination with n = 1, or a component characterized by n on the order of 1.1 to 1.5 due to recombination via a trap located between midgap and the conduction or valence band edge
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Anon; 1673 p; 1990; p. 415-419; IEEE Service Center; Piscataway, NJ (USA); 21. Institute for Electrical and Electronics Engineers (IEEE) photovoltaic specialists conference; Kissimmee, FL (USA); 21-25 May 1990; CONF-900542--; IEEE Service Center, 445 Hoes Ln., Piscataway, NJ 08854 (USA)
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Book
Literature Type
Conference; Numerical Data
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INIS VolumeINIS Volume
INIS IssueINIS Issue
AbstractAbstract
[en] Fuji TR image plate is frequently used as a replacement detector medium for x-ray imaging and spectroscopy diagnostics at NIF, Omega, and Z facilities. However, the familiar Fuji BAS line of image plate scanners is no longer supported by the industry, and so a replacement scanning system is needed. While the General Electric Typhoon line of scanners could replace the Fuji systems, the shift away from photo stimulated luminescence units to 16-bit grayscale Tag Image File Format (TIFF) leaves a discontinuity when comparing data collected from both systems. For the purposes of quantitative spectroscopy, a known unit of intensity applied to the grayscale values of the TIFF is needed. The DITABIS Super Micron image plate scanning system was tested and shown to potentially rival the resolution and dynamic range of Kodak RAR 2492 x-ray film. However, the absolute sensitivity of the scanner is unknown. In this work, a methodology to cross calibrate Fuji TR image plate and the absolutely calibrated Kodak RAR 2492 x-ray film is presented. Details of the experimental configurations used are included. An energy dependent scale factor to convert Fuji TR IP scanned on a DITABIS Super Micron scanner from 16-bit grayscale TIFF to intensity units (i.e., photons per square micron) is discussed.
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(c) 2016 Author(s); Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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AbstractAbstract
[en] At Sandia National Laboratories, the x-ray generator Manson source model 5 was upgraded from 10 to 25 kV. The purpose of the upgrade is to drive higher characteristics photon energies with higher throughput. In this work we present characterization studies for the source size and the x-ray intensity when varying the source voltage for a series of K-, L-, and M-shell lines emitted from Al, Y, and Au elements composing the anode. We used a 2-pinhole camera to measure the source size and an energy dispersive detector to monitor the spectral content and intensity of the x-ray source. As the voltage increases, the source size is significantly reduced and line intensity is increased for the three materials. We can take advantage of the smaller source size and higher source throughput to effectively calibrate the suite of Z Pulsed Power Facility crystal spectrometers.
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(c) 2016 Author(s); Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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Reference NumberReference Number
INIS VolumeINIS Volume
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External URLExternal URL
AbstractAbstract
[en] The Advanced Light Source beamline-9.3.1 x-rays are used to calibrate the rocking curve of bent potassium acid phthalate (KAP) crystals in the 2.3-4.5 keV photon-energy range. Crystals are bent on a cylindrically convex substrate with a radius of curvature ranging from 2 to 9 in. and also including the flat case to observe the effect of bending on the KAP spectrometric properties. As the bending radius increases, the crystal reflectivity converges to the mosaic crystal response. The X-ray Oriented Programs (XOP) multi-lamellar model of bent crystals is used to model the rocking curve of these crystals and the calibration data confirm that a single model is adequate to reproduce simultaneously all measured integrated reflectivities and rocking-curve FWHM for multiple radii of curvature in both 1st and 2nd order of diffraction.
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(c) 2016 Author(s); Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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ALKALI METALS, BOSONS, COHERENT SCATTERING, CONFIGURATION, DIFFRACTION, ELECTROMAGNETIC RADIATION, ELEMENTARY PARTICLES, ELEMENTS, ENERGY RANGE, IONIZING RADIATIONS, KEV RANGE, MASSLESS PARTICLES, METALS, OPTICAL PROPERTIES, PHYSICAL PROPERTIES, RADIATION SOURCES, RADIATIONS, SCATTERING, STORAGE RINGS, SURFACE PROPERTIES, SYNCHROTRON RADIATION SOURCES
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INIS VolumeINIS Volume
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AbstractAbstract
[en] We disucss the line broadening analysis of argon-doped deuterium-filled implosion cores driven by a dynamic hohlraum z-pinch. The observed line spectra include emissions from the Lyα, Lyβ, Lyγ, Heα, Heβ, Heγ and Heδ lines in H- and He-like argon ions, respectively. The data recorded using a crystal spectrometer with space-resolving slits and coupled to a framing camera yields time- and spatially-resolved argon line spectra in the implosion core. The analysis accounts for opacity and Stark line broadening to determine electron density, Ne, and areal-density, NΔR, values for the ground state populations of H- and He-like argon ions. In this connection, a set of Stark-broadened line shapes was computed considering the effect of differing ion and electron temperatures, which impacts the calculation of the ion microfield distribution function, the Doppler broadening, and the ion dynamic's effect. Analysis results will be discussed emphasizing the relevance of using these detailed Stark-broadened line shapes
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18. international conference on spectral line shapes; Auburn, AL (United States); 4-9 Jun 2006; (c) 2006 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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Conference
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INIS VolumeINIS Volume
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External URLExternal URL
AbstractAbstract
[en] Recent experiments on the Z accelerator have produced high-energy (17 keV) inner-shell K-alpha emission from molybdenum wire array z-pinches. Extensive absolute power and spectroscopic diagnostics along with collisional-radiative modeling enable detailed investigation into the roles of thermal, hot electron, and fluorescence processes in the production of high-energy x-rays. We show that changing the dimensions of the arrays can impact the proportion of thermal and non-thermal K-shell x-rays
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(c) 2014 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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Ampleford, D. J.; Hansen, S. B.; Jennings, C. A.; Jones, B.; Coverdale, C. A.; Harvey-Thompson, A. J.; Rochau, G. A.; Dunham, G.; Moore, N. W.; Harding, E. C.; Cuneo, M. E.; Chong, Y.-K.; Clark, R. W.; Ouart, N.; Thornhill, J. W.; Giuliani, J.; Apruzese, J. P., E-mail: damplef@sandia.gov2014
AbstractAbstract
[en] Aluminum wire array z pinches imploded on the Z generator are an extremely bright source of 1–2 keV radiation, with close to 400 kJ radiated at photon energies >1 keV and more than 50 kJ radiated in a single line (Al Ly-α). Opacity plays a critical role in the dynamics and K-shell radiation efficiency of these pinches. Where significant structure is present in the stagnated pinch this acts to reduce the effective opacity of the system as demonstrated by direct analysis of spectra. Analysis of time-integrated broadband spectra (0.8–25 keV) indicates electron temperatures ranging from a few 100 eV to a few keV are present, indicative of substantial temperature gradients
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(c) 2014 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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INIS VolumeINIS Volume
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AbstractAbstract
[en] The Z-pinch dynamic hohlraum is an x-ray source for high energy-density physics studies that is heated by a radiating shock to radiation temperatures >200 eV. The time-dependent 300-400 eV electron temperature and 15-35 mg/cc density of this shock have been measured for the first time using space-resolved Si tracer spectroscopy. The shock x-ray emission is inferred from these measurements to exceed 50 TW, delivering >180 kJ to the hohlraum
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(c) 2008 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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