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interest are identified by coincident spectroscopy of electrons and photons in a β/γ coincidence spectrometer (BGCS). The β spectrometer is a plastic scintillator, manufactured as a cylindrical cell containing the separated xenon sample. This cell is surrounded by the NaI(Tl) γ spectrometer. We report here the development of a calibration process for the BGCS suitable for use in remote sampling systems. This procedure is based upon γ-ray
Compton scattering, resulting in a true coincident signal in both detectors, generation of electrons over a wide energy range that matches the energy distribution of electrons from radioxenon decay, and a relative insensitivity to source location. In addition to gain calibration, this procedure determines the resolution of the β detector as a function of energy.
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Detection and measurement of atmospheric radioxenon is an important component of international monitoring systems for nuclear weapons testing. Monitoring stations separate xenon from air and perform isotopic analysis of the radioxenon. In one such radioxenon measurement scheme, the isotopes of
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from the air in batch mode, processing approximately 48 m in an 8-hour period. The average amount of xenon collected in this period is approximately 2 cc. The xenon gas is then transferred into a nuclear detection system consisting of a beta–gamma coincidence spectrometer.
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2003 – The ARSA was sent to
Guangzhou, China for further participation in the International Noble Gas Experiment
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1997 – ARSA underwent a field test at the
Environmental Measurements Laboratory in New York City
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2002 – The commercialization of the ARSA was transferred to
General Dynamics Corporation
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2000 – The ARSA system was sent to
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in the late 1990s with funding and support from the
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179:1995 – ARSA concept first proven in the laboratory
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66:"Automated radioxenon sampler analyzer"
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