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Phillips, J.R.; Bosler, G.E.
Los Alamos National Lab., NM (USA)1983
Los Alamos National Lab., NM (USA)1983
AbstractAbstract
[en] The relative contributions of gamma rays originating in specific fuel pins to the total gamma-ray source strength were calculated as a function of initial gamma-ray energy for a pressurized-water-reactor fuel assembly. Gamma-ray energies used in the calculations ranged from 511 to 2186 keV, the energy range in which most long-lived fission and activation products emit gamma rays. Nondestructive gamma-ray measurement techniques use specific signatures of 137Cs or 134Cs/137Cs and 154Eu/137Cs isotopic ratios to determine the exposures of irradiated fuel assemblies. Nearly 92% of the measured 137Cs signature (661.6 keV) originates in the three outer rows of fuel pins. However, because only 78% of the 154Eu signature (1275 keV) originates in these three outer rows, a ratio of 154Eu/137Cs does not sample exactly the same volume segment of the fuel assembly. Other examples are presented that evaluate the effect of using a collimator at different angular orientations on quantifying the contributions from specific fuel pins to the total source strength
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Aug 1983; 21 p; Available from NTIS, PC A02/MF A01 as DE83016357
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