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Ban, Young Suk,Masiello, Emiliano,Lenain, Roland,Joo, Han Gyu,Sanchez, Richard Elsevier 2018 Annals of nuclear energy Vol.115 No.-
<P><B>Abstract</B></P> <P>In order to examine the performance of two deterministic codes, nTRACER and the standalone developing version of the IDT solver of APOLLO3<B>®</B>, problems from 2D single assembly to 3D full core were computed with the same macroscopic cross-section library, so as to suppress the effects of physical modeling and to allow a direct comparison in terms of methodology, code architecture and performances. The problems we considered include cases for which the codes were not optimized in their initial design, allowing thus to analyze the potential for generalization and/or estimate possible improvements to broaden the scope of application of the codes.</P>
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Sanchez, Richard,Zmijarevi, Igor,Coste-Delclaux, M.,Masiello, Emiliano,Santandrea, Simone,Martinolli, Emanuele,Villate, Laurence,Schwartz, Nadine,Guler, Nathalie Korean Nuclear Society 2010 Nuclear Engineering and Technology Vol.42 No.5
This paper presents the mostortant developments implemented in the APOLLO2 spectral code since its last general presentation at the 1999 M&C conference in Madrid. APOLLO2 has been provided with new capabilities in the domain of cross section self-shielding, including mixture effects and transfer matrix self-shielding, new or improved flux solvers (CPM for RZ geometry, heterogeneous cells for short MOC and the linear-surface scheme for long MOC), improved acceleration techniques ($DP_1$), that are also applied to thermal and external iterations, and a number of sophisticated modules and tools to help user calculations. The method of characteristics, which took over the collision probability method as the main flux solver of the code, allows for whole core two-dimensional heterogeneous calculations. A flux reconstruction technique leads to fast albeit accurate solutions used for industrial applications. The APOLLO2 code has been integrated (APOLLO2-A) within the $ARCADIA^{(R)}$ reactor code system of AREVA as cross section generator for PWR and BWR fuel assemblies. APOLLO2 is also extensively used by Electricite de France within its reactor calculation chain. A number of numerical examples are presented to illustrate APOLLO2 accuracy by comparison to Monte Carlo reference calculations. Results of the validation program are compared to the measured values on power plants and critical experiments.
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RICHARD SANCHEZ,IGOR ZMIJAREVIC,M. COSTE-DELCLAUX,EMILIANO MASIELLO,SIMONE SANTANDREA,EMANUELE MARTINOLLI,LAURENCE VILLATE,NADINE SCHWARTZ,NATHALIE GULER 한국원자력학회 2010 Nuclear Engineering and Technology Vol.42 No.5
This paper presents the most important developments implemented in the APOLLO2 spectral code since its last generalpresentation at the 1999 M&C conference in Madrid. APOLLO2 has been provided with new capabilities in the domain ofcross section self-shielding, including mixture effects and transfer matrix self-shielding, new or improved flux solvers (CPMfor RZ geometry, heterogeneous cells for short MOC and the linear-surface scheme for long MOC), improved accelerationtechniques (DP1), that are also applied to thermal and external iterations, and a number of sophisticated modules and tools tohelp user calculations. The method of characteristics, which took over the collision probability method as the main fluxsolver of the code, allows for whole core two-dimensional heterogeneous calculations. A flux reconstruction technique leadsto fast albeit accurate solutions used for industrial applications. The APOLLO2 code has been integrated (APOLLO2-A)within the ARCADIAreactor code system of AREVA as cross section generator for PWR and BWR fuel assemblies.APOLLO2 is also extensively used by Electricité de France within its reactor calculation chain. A number of numericalexamples are presented to illustrate APOLLO2 accuracy by comparison to Monte Carlo reference calculations. Results of thevalidation program are compared to the measured values on power plants and critical experiments.
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