1994
DOI: 10.1093/oxfordjournals.rpd.a082312
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Experimental Determination of the Response of Four Bonner Sphere Sets to Thermal Neutrons

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Cited by 29 publications
(14 citation statements)
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“…In all subsequent comparisons, the reference H * (10) value is given by the HMGU extended-range BSS system since the latter was previously calibrated with monoenergetic neutron beams of up to 387 MeV (Ref. 22), and H * (10) measurements were made with this detector set at all positions (1)(2)(3)(4). One should finally note that both BSS systems involve a dead time factor below 40 µs implicating a negligible error.…”
Section: C1 Bonner Sphere Systemsmentioning
confidence: 99%
“…In all subsequent comparisons, the reference H * (10) value is given by the HMGU extended-range BSS system since the latter was previously calibrated with monoenergetic neutron beams of up to 387 MeV (Ref. 22), and H * (10) measurements were made with this detector set at all positions (1)(2)(3)(4). One should finally note that both BSS systems involve a dead time factor below 40 µs implicating a negligible error.…”
Section: C1 Bonner Sphere Systemsmentioning
confidence: 99%
“…The data from these calculations for irradiation with a 252 Cf source show very close agreement with the measurements performed for this project (Table 1). The evidence from previous measurements is that the gas pressure tends to be a little lower (Thomas et al, 1994): on average the thermal neutron response of an SP9 counter was found to be about 2.65 cm 2 corresponding to a pressure of roughly 191 kPa. The measured values varied from 2.53 to 2.74 cm 2 , a range of roughly 8.3% in the thermal neutron response.…”
Section: 233mentioning
confidence: 85%
“…A bare 3 He proportional counter without any surrounding material is also used as the 18th measuring channel. This system enables accurate measurements of neutron fluence spectra, Ф(E), and ambient dose equivalent, H * (10), values, since the fluence response functions (HEMA99) of all spheres with 3 He proportional counter in their center were calculated by means of Monte Carlo (MC) simulations [5,6] and experimentally validated at 13 neutron energies between thermal and 14.8 MeV [7,8] as well as with quasi-mono-energetic neutron fields with peak energies at 244 MeV and 387 MeV [9].…”
Section: Extended Range Bonner Sphere Spectrometermentioning
confidence: 99%