Physical Review Special Topics. Accelerators and Beams (Dec 2010)

Characterization and error analysis of an N×N unfolding procedure applied to filtered, photoelectric x-ray detector arrays. II. Error analysis and generalization

  • D. L. Fehl,
  • G. A. Chandler,
  • W. A. Stygar,
  • R. E. Olson,
  • C. L. Ruiz,
  • J. J. Hohlfelder,
  • L. P. Mix,
  • F. Biggs,
  • M. Berninger,
  • P. O. Frederickson,
  • R. Frederickson

DOI
https://doi.org/10.1103/PhysRevSTAB.13.120403
Journal volume & issue
Vol. 13, no. 12
p. 120403

Abstract

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A five-channel, filtered-x-ray-detector (XRD) array has been used to measure time-dependent, soft-x-ray flux emitted by z-pinch plasmas at the Z pulsed-power accelerator (Sandia National Laboratories, Albuquerque, New Mexico, USA). The preceding, companion paper [D. L. Fehl et al., Phys. Rev. ST Accel. Beams 13, 120402 (2010)PRABFM1098-4402] describes an algorithm for spectral reconstructions (unfolds) and spectrally integrated flux estimates from data obtained by this instrument. The unfolded spectrum S_{unfold}(E,t) is based on (N=5) first-order B-splines (histograms) in contiguous unfold bins j=1,…,N; the recovered x-ray flux F_{unfold}(t) is estimated as ∫S_{unfold}(E,t)dE, where E is x-ray energy and t is time. This paper adds two major improvements to the preceding unfold analysis: (a) Error analysis.—Both data noise and response-function uncertainties are propagated into S_{unfold}(E,t) and F_{unfold}(t). Noise factors ν are derived from simulations to quantify algorithm-induced changes in the noise-to-signal ratio (NSR) for S_{unfold} in each unfold bin j and for F_{unfold} (ν≡NSR_{output}/NSR_{input}): for S_{unfold}, 1≲ν_{j}≲30, an outcome that is strongly spectrally dependent; for F_{unfold}, 0.6≲ν_{F}≲1, a result that is less spectrally sensitive and corroborated independently. For nominal z-pinch experiments, the combined uncertainty (noise and calibrations) in F_{unfold}(t) at peak is estimated to be ∼15%. (b) Generalization of the unfold method.—Spectral sensitivities (called here passband functions) are constructed for S_{unfold} and F_{unfold}. Predicting how the unfold algorithm reconstructs arbitrary spectra is thereby reduced to quadratures. These tools allow one to understand and quantitatively predict algorithmic distortions (including negative artifacts), to identify potentially troublesome spectra, and to design more useful response functions.