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Core Neutronics Model
The Exitech Core Neutronics model, AMON™ (Advanced Model of Neutronics) is used at several simulators and faithfully reproduces core data, parameters,and transients. Example sections of the AMON handbook are provided here.
Table of Contents
1.0 Introduction This document provides the engineering equation development for the EXITECH AMONTM (Advanced Model Of Neutronics). This model calculates the neutron flux level and flux distribution within the reactor core as well as the thermal power deposited in the fuel and coolant. The thermal power values are passed to the Thermal-Hydraulics model. Core neutron flux level and distribution are passed to the NIS (Nuclear Instrumentation System) Model which simulates the source range (SRM), intermediate range (IRM) and local power range (LPRM) detectors and instrument channels. The AMON receives fuel temperature, coolant density, coolant void and boron concentration (of importance during ATWS events) as the major interface parameters from the Thermal-Hydraulics model. The AMON also receives control rod position information from the CRDH (Control Rod Drive Hydraulic System) Model.
1.1 Core Neutronics Model Nodalization Figure 1 and 2 show the 137 (radial) by 8 (axial) nodalization utilized for the AMONTM BWR Core Neutronics Model.
8.0 Nuclear Instrumentation The core nuclear instrumentation SRM, IRM, and LPRM Detector responses, as well as the core power calibration TIP machine probe signals are calculated dynamically. For each of the nuclear instrumentation detectors, a total of nine (9) signals are calculated, seven (7) dynamically varying averaged-signals inside the active core region plus two (2) fixed-zero-signals at extrapolated distances from the top and bottom of the core. These nine (9) signals are curve fitted by the cubic spline method. The curve fit coefficients for each of the detector channels are used to reconstruct the detector signal at specific detector positions The SRM/IRM detectors are movable detectors. Each of the seven (7) dynamically varying averaged-signals inside the core are calculated by averaging the eight (8) surrounding AMONTM nodal neutron fluxes (four (4) neighboring AMONTM nodes on each of the two (2) neighboring layers). If the detector resides within the reactor core, the reconstructed flux level signal of the detector is multiplied by a fixed detector efficiency constant to convert the flux signal into a counts per second (cps) signal (for SRM detectors) or a percentage power signal (for IRM detectors). If the detector is located below the reactor core bottom, the flux signal will be calculated by using the core bottom position neutron flux signal and attenuating this signal according to the detector’s distance below the core bottom. This attenuated neutron flux signal will then be multiplied by the same detector efficiency constants to convert the flux signal into cps (for SRM detectors) or percentage power (for IRM detectors). The LPRM detectors are fixed in the reactor core. In each LPRM string, there are four (4) detectors located at four elevations in the core to measure the core fission power in units of watts per centimeter square (watts/cm2). Seven (7) dynamically varying averaged-unit-area-fission-power values in the vicinity of the LPRM string are calculated by averaging the eight (8) surrounding AMONTM nodal fission powers (four (4) neighboring AMONTM nodes on each of the two (2) neighboring layers). Nine (9) cubic-spline-method curve fit coefficients for each LPRM string are used to reconstruct the four (4) LPRM detector signals at the specific detector elevations. The signals for the moveable TIP probe for each of the TIP channels (coexisting along with the LPRM strings in the core) are calculated by using the nine (9) cubic spline curve fit coefficients generated in the calculation of the corresponding LPRM string detector signals. The core unit area fission power along the channel direction is calculated by inserting the gradually changing probe position into the cubic spline curve fit reconstruction formula. If the probe has traveled below the bottom of the core, the core bottom position is inserted into the formula to generate a base value and the base value is attenuated according to the TIP detector’s distance below the bottom of the core. A rod shadow effect is modeled when the tip of a control rod comes within two notches (of the axial distance) around the detector. Four rods that surround the detector is considered:
Xi is a number ranged between -1 and 1 that represents the normalized axial distance between the ith rod tip and the detector with respect to the distance of two notches of the control rod. If the rod tip is withdrawn but within two notches of the detector, X equals 1. If the rod tip is at the same axial position as the detector, X equal 0. If the rod tip is inserted but within two notches of the detector, X is -1. The constant C is used to control the effectiveness of the rod shadow effect. It is implemented as a local constant in the nuclear instrument routine. To turn off the rod shadow effect, this constant is set to zero.
9.0 Assumptions and Simplifications The following Assumptions and Simplifications are applicable to the AMONTM core neutronics model:
10.0 References
APPENDIX A Neutronics Data Formalism A1.0 Introduction The format of the terms in Eq. (3.0-1) to (3.0-6) along with the nodal averaged fuel-assembly migration area and macroscopic fission cross sections are shown in this appendix. Referring to Figure 1 and Figure 2 (Core Nodalization Diagrams), the core cycle dependent (BOC, MOC, EOC as defined by the established simulator initial conditions) data noted in the following sections are required to parameterize and optimize the AMON Core Neutronics Model to a specific reference plant. The fuel exposure, void history and control history corrected equivalent one-group three-dimensional AMON model "coarse-node" (137 x 8) data should be generated from fuel exposure, void history and control history corrected two-group fine-mesh (560 x 25) data by a flux weighting scheme based upon the reference plant flux distributions at HFP and ARI cold conditions respectively. The nuclear data which are a function of moderator density can either be provided in the form of polynomial functions (as proposed herein) or in tabular form or in a combination of the two. The amount of coarse-node nuclear data collapsed from two group fine-mesh data is large, and it needs to be reduced by some scheme in order to be loaded in the AMON Model. And in reducing the amount of nuclear data the fidelity of AMON Model and the characteristics of the core cycle loaded have to be maintained. In the model, there are two (2) reduced data types are used, the nodal property dependent data type and core averaged property data type. The nodal nuclear data which will affect nodal power or flux heavily and whose properties are sensitive to the fuel lattice design, such as k-infinity k4R , migration area M2R and fission cross section 3fR are categorized as the nodal property dependent data. The number of grouped nodal property dependent data is determined by the fuel loading symmetry condition in the core, e.g. mirror symmetry, reflection symmetry, rotational symmetry, etc. This approach will usually reduce the data required by a factor of four (4) or more. Nodal nuclear data which will affect nodal power or flux slightly and whose properties are not that sensitive to the fuel lattice design will be treated and used as core averaged property data in the model. These data include boron reactivity coefficients, Doppler reactivity coefficients, Xe microscopic cross section and reactivity coefficients, and Sm microscopic cross section and reactivity coefficients.
A2.0 Nodal Property Dependent Data The homogenized nodal neutronic data k-infinity k4R , migration area M2R and fission cross section 3fR are processed in the same way in the AMON Model. Those nodal neutronic data, given for each symmetric group in the core, exclude Doppler (average fuel temperature) effects and Iodine, Xenon, Promethium, Samarium and Boron effects in node R. They are functions of exposure rate, void history, control history, moderator density, and control rod effective volumetric control fraction.. In the model, these data are grouped into four sets according to exposure (core-life dependency). Within each set of data at a given exposure rate, there are two subsets of base data given at ARO (uncontrolled), and ARI (controlled) conditions. Each subset of base data are fitted into a polynomial as a function of moderator density:
The A's are curve fit polynomial coefficients, and χR is the moderator density (gm/Cm3) of node R. Similarly, for the controlled case (ARI):
The final nodal property data N_DATAR(fR) will be linearly interpolated between the base N_DATAR's of Eqs. (A2.0-1) and (A2.0-2) according to the nodal control rod effective volumetric control fraction fR.
A3.0 Core-Averaged Data The data cited in the following subsections are to be provided on a core-averaged basis.
A3.1 Boron Reactivity Correction Data Since boron is transported and resides within the liquid phase of the coolant or moderator only, even if the concentrations remain constant for a given amount of boron in the system, the differences in void fraction will yield different boron number densities. The boron reactivity worth is calculated as the product of boron number density and the boron worth coefficient which is a function of the moderator density and boron number density, f:
A3.2 Doppler Reactivity Correction The Doppler correction is a function of the core-averaged moderator temperature, density as well as the nodal average fuel temperature. The format of the reactivity calculation is as follows:
A3.3 Xenon & Samarium Reactivity Corrections The Xenon and Samarium reactivity worth are proportional to Xenon and Samarium number density as follows:
A3.4 Equivalent One-Group Neutron Flux The flux is an equivalent one-group value converted from two-group data. Since this flux is an initial value used to establish the reference case simulator IC only (e.g. for model initialization during testing), the core-averaged value at hot full power will be sufficient.
A3.5 Delayed Neutron Precursor Data Core-averaged six group delayed neutron precursor data are required in the form of a table of constants for use in Parameterization of the amplitude function.
A3.6 Decay Heat Group Data The core-averaged eleven group decay heat precursor data are required in the form of a table of constants. If no reference plant specific data is provided, EXITECH will utilize the eleven group decay heat data presented in revision 2 of the RETRAN user's manual.
A3.7 Nuclear Fission-Energy And Neutron Poison Data The following data are required as core-averaged constant values.
APPENDIX B Parameterization And Optimization Data Request List B1.0 Introduction The performance and accuracy of the EXITECH Advanced MOdel of Neutronics (AMON) code is mainly dependent on the level of detail and accuracy of the reference plant reactor core design and performance data provided by the licensee. Data required for implementation of the AMON code may be divided into two (2) types:
B2.0 AMON Parameterization Data The data required to parameterize the AMON code for a specific reference plant reactor core fuel load must reflect the status of the specific fuel load cycle. As a precursor to the Licensee data generation process, the Licensee simulator training organization typically will define the simulator core life states (e.g. BOC, MOC, EOC, ...) required to support the Licensee’s operator training and examination program. In addition, for each core life state, the following global NSSS thermal hydraulic data at Hot Full Power (HFP) must be provided:
To provide a high fidelity simulation in the real-time environment, the AMON code requires core-life dependent equivalent one (1) group nuclear data. This data may be divided into the following two (2) categories:
B3.0 AMON Optimization Data In order to optimize the AMON model to match reference plant operating conditions, the following multi-dimensional distribution nuclear data are required. These data can be provided either collapsed to the AMON nodal configuration or as quarter (¼) core, 3D fine mesh (N/4 fuel assembly x 25 axial mesh) data. These data must be corrected for the corresponding fuel exposure, void (density) history and control history.
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