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Buckling Correction for Experimental Power Distribution within Fuel Assemblies in a Finite System
Abstract:For design calculations to determine the local power distribution in a fuel assembly of a power reactor, the neutron flux is usually assumed to be symmetrical at the outer boundary of the assembly. In actuality, experimental data on power distributions are obtained in a finite system where this symmetry does not apply, so that the calculated values cannot be directly compared with observed data. In a zero power critical experiment in particular, the measurement must be performed in a fairly small core assembly so economize the amount of fuel materials to be used for simulation. This introduces the necessity of special considerations in the comparison between design and observed data.

The authors propose a method incorporating direct corrections to the experimentally determined. power distributions based on the geometrical buckling of the system. In this method the experimental power P 0 (r) is divided by the neutron flux Q (r) which is determined in the critical state with geometrical buckling in a bare (one neutron energy group) reactor, neglecting the reflector region of the experimental system. A sample application of the method to an actual light water lattice has confirmed the validity of the method.
Keywords:neutron counting statistics  family-first-pulse  first moment of neutron counts  Rossi alpha method  waiting time  correlation amplitude  uncorrelated counts  triggering probability  triggered-gate  time dependence
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