Paper
19 November 1993 Marshall Space Flight Center imaging x-ray experiment (MIXE)
Brian D. Ramsey, Jeff A. Apple, Kurtis L. Dietz, Martin C. Weisskopf, Robert A. Austin, Jeffery J. Kolodziejczak, Takahisa Minamitani
Author Affiliations +
Abstract
The MIXE includes a state-of-the-art imaging proportional counter which utilizes fluorescence gating in order to achieve high sensitivity in the bandwidth from the xenon k-edge (35 keV) to 100 keV. The current detector system includes a parallel amplification stage to allow for improved energy resolution without sacrificing spatial resolution. Another novel feature is the molybdenum/stainless steel pressure vessel, which is an important factor in achieving low background rates. In this paper we compare the results of Monte Carlo simulations with laboratory experiments and present data obtained during a recent balloon flight from Palestine, Texas.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Brian D. Ramsey, Jeff A. Apple, Kurtis L. Dietz, Martin C. Weisskopf, Robert A. Austin, Jeffery J. Kolodziejczak, and Takahisa Minamitani "Marshall Space Flight Center imaging x-ray experiment (MIXE)", Proc. SPIE 2006, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IV, (19 November 1993); https://doi.org/10.1117/12.162822
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Cited by 2 scholarly publications.
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KEYWORDS
Sensors

Spatial resolution

Monte Carlo methods

Luminescence

Molybdenum

X-ray imaging

X-rays

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