SINBAD ABSTRACT NEA-1553/73
FNS Clean Experiment on Vanadium Cube
1. Name of Experiment: ------------------ FNS/JAERI Clean Benchmark Experiment on Vanadium Cube Assembly (1996) 2. Purpose and Phenomena Tested: ---------------------------- A 25.4 cm x 25.4 cm x 25.4 cm cube vanadium assembly was irradiated in the D-T neutron source of Fusion Neutronic Source (FNS) facility at JAERI. Neutron spectra down to 1 eV, dosimetry reaction rates, gamma-ray spectra and gamma- ray heating rates were measured at 3 positions up to 17.78 cm inside the vanadium assembly. 3. Description of Source and Experimental Configuration: ---------------------------------------------------- The experimental configuration was basically the same as those used for some previous clean benchmark experiments like the Lithium-Oxide, Graphite, Copper, Beryllium, Tungsten assemblies. The vanadium assembly was a cube with a side of 254 mm. Four side surfaces and a rear surface of the vanadium assembly was covered with a graphite reflector with the thickness of 50.8 mm, as shown in Fig. 1, to reduce leakage neutrons from the rather small assembly and incoming background neutrons from the outside. Purity of vanadium was higher than 99.7 %. The material compositions of the vanadium assembly and the surrounding graphite reflector are given in Table 1. The experimental assembly was located in front of the neutron source at a distance of 200 mm from the target. The tritium-titanium target of ~3.7E11 Bq was bombarded by a deuteron beam of 350 keV energy to produce D-T neutrons. The number of source D-T neutrons generated during each measurement was determined by the alpha-particle detector with an accuracy of 2~3 %. The D-T neutron source can be roughly described as an isotropic point 14-MeV neutron source. The source neutron spectrum and intensity, however, depend slightly on the emission angle. The angle-dependent source characteristics were investigated experimentally and theoretically in detail, and a source subroutine for the Monte Carlo transport code MCNP-4 has been prepared to simulate the source condition precisely. This routine is listed in [3]. A comparison between the measured and calculated angular distribution is given in Fig. 3.2.7. in [4]. As an adequate alternative to the use of the MCNP routine it is suggested in [1] that the source spectrum of neutrons emitted toward the 0 degree direction with respect to the deuteron beam direction can be used for the incident neutron spectrum on the whole front surface of the assembly. No quantitative estimation of difference between both sources could be though found in the available literature. The 0 degree source neutron spectrum is shown in Fig. 2, and input cards of MCNP for description of the source spectrum are shown in the MCNP sample input file. The si1 and sp1 cards indicate upper neutron energies of the energy bins in MeV and probabilities in the bins, respectively. The dir and vec parameters with the sb2 card are used for variance reduction with the source biasing method. The weight of a source neutron specified by the wgt parameter, 1.1261, is larger than 1.0 because more D-T neutrons are emitted to the forward direction than in the backward direction with respect to the deuteron beam direction. The tritium target region is also a source of gamma-rays, namely, target gamma- rays, created by interaction of the source neutrons with structural materials of the target. Consideration of the target gamma-rays, however, is not needed in calculations of gamma-ray heating rates because contribution of the target gamma-ray to the measured heating rates has been already subtracted in the experimental data. On the other hand, the target gamma-ray contribution is involved in the measured gamma-ray spectra. The contribution at the detector positions deep inside the experimental assemblies is negligible, representing at most few percents, because the experimental assembly largely attenuates the target gamma-rays. Accordingly, it is not necessary to consider the target gamma-rays in transport calculations for the clean benchmark experiments. Since the V assemblies were located at least 4 m from the experimental room walls and floor, the contribution of the background neutrons and gamma-rays coming from the room walls and floor on the measured quantities was negligibly small. 4. Measurement System: ------------------ Two experimental channels for insertion of detectors were set on the lateral surface of the assembly, and detectors were placed on the central axis of the assembly at three positions: one on the front surface and other two inside the assembly at the depths of 76.2 and 177.8 mm. The report [1] states that the spectra measurements were performed one by one, we conclude therefore that the other experimental channels were closed (plugged with vanadium). The dosimetric foils were irradiated together and simultaneously in plural detector channels. No information on the background correction was found in the literature. Six techniques were employed to measure neutrons and gamma-rays. The detailed description of the experimental techniques is given in [1] (pages 5-20): (1) 14 mm-diameter spherical NE213 liquid organic scintillator was used as the fast (above 2 MeV) neutron spectrometer. It was inserted into the experimental channel hole of 22 mm diameter. Various sources of the NE213 measurement uncertainties are discussed in [1] (page 5) and the systematic errors are summarized in Table 2. (2) A pair of proton recoil gas proportional counters (PRC) was used to measure neutron spectrum in the 20 keV to 1 MeV energy range. The counter has a cylindrical shape with the outer diameter of 19 mm and the effective length of 127 mm. The counter is inserted into an experimental hole of 21 mm in diameter with its pre-amplifier. PRC is made of type 304 stainless steel of a thickness of 0.41 mm. Two types of counters were used to measure neutron spectrum in a wide energy range. Hydrogen gas at 0.5677 MPa (5.789 kgf/cm2) with 1 percent of CH4 filled counter was used for low-energy neutrons from 3 keV to 150 keV while for the high-energy neutrons from 150 keV to 1 MeV the counter was filled with 50-50 mixture of hydrogen and argon gases with 1.8 percent of nitrogen at 0.6102 MPa (6.222 kgf/cm2). Error Assessment: Possible error sources are gas pressure (number of hydrogen atom), n-p scattering cross section, fitting error for differentiation of recoil proton spectrum due to count statistics and calibration of recoil proton energy. The fitting error is the largest, ~ 3-10 % above 10 keV, while the other errors are expected to be less than 1%. Neutron spectra below 10 keV tend to become smaller due to the uncertainty of the W-value, which is the average energy loss per ion pair. The error due to W-value is not included in the experimental errors. (3) Slowing down time (SDT) method for the neutron spectrum from 1 eV to 300 eV. A BF3 gas proportional counter with an outer diameter of 14 mm and an effective length of 99 mm, containing 96 % boron-10 (B-10) enriched BF3 gas at the pressure of 71.5 kPa, was used for neutron detection. Using the standard thermal neutron field the effective number of B-10 atoms in the counter was determined to be 2.18E20 +- 3 %. The counter was inserted into one of the experimental holes of the experimental assembly. Experimental uncertainties associated with the measured spectra are summarized in Table 3. The overall experimental uncertainties are dominated mostly by the uncertainties of the energy calibration curves. The lowest and highest energies calibrated are 1.4 eV and 579 eV. In the energy ranges outside the calibration energies, roughly below 1 eV and above 1 keV, the adjusted calibration curves are used. (4) Dosimetry reaction rate of the Al-27(n,alpha)Na-24, Nb-93(n,2n)Nb-92m, In-115(n,n’)In-115m and Au-197(n,gamma)Au-198 reactions were measured by the foil activation method. Table 4 provides the characteristics for the reactions used. Typical Al and Nb sample size was 10 mm in diameter and 1 mm in thickness. Indium foils had dimensions of 10 x 10 x 1 mm3. In order to minimize the self-shielding effect for the Au-197(n,gamma) reaction, gold foils with a size of 10 x 10 x 0.001 mm3 were adopted. Experimental Error and Uncertainty: Major sources of the error for the reaction rate were the gamma-ray counting statistics (0.1 ~ several %) and the detector efficiency (2 ~ 3 %). The error for sum-peak correction was estimated less than 2 % depending on the decay mode and fraction of multiple gamma-ray cascade. The error for the decay correction was reflected from the error of half-life of the activity. If the half-life was accurate, the error for the saturation factor should be less than 1 % even for the short half-life activities. The other errors associated with foil weight, gamma-ray self-absorption, irradiation time, cooling time and counting time were negligibly small. The error for neutron yield was estimated to be 2 %. The overall error for the major part of reaction rate ranged between 3 ~ 6 %. Some data for high threshold reaction in the deep positions suffered from poor counting statistics due to low activation rate. (5) Prompt gamma-ray spectrum were measured by a 40 mm diameter spherical BC537 liquid organic scintillation counter. Outer diameter of the detector is 48 mm and length including a photomultiplier assembly is 262 mm. Experimental uncertainty: As explained in (6) below, typical experimental uncertainties of the gamma-ray heating rate measured by TLDs range between 7 ~ 15 %. The gamma-ray spectra are normalized to the gamma-ray heating rates. Uncertainties of about 10 % is introduced by the normalization procedure. All of the rest of experimental uncertainties, such as statistical errors, uncertainties of the response functions, determination of source D-T neutrons and subtraction of decay gamma-rays, are less than 5 %. Therefore, total experimental uncertainties are approximately 15 ~ 20 %. Note that only the statistical erorrs are included in the Table 10. (6) Gamma-ray heating rate were measured by thermoluminescent dosimeters (TLDs) in combination with the atomic number interpolation method. Gamma-ray heating rates of vanadium were deduced by interpolating the gamma-ray heating rates measured by three types of TLDs, Mg2SiO4 (MSO, effective atomic number Zeff = 11.1), Sr2SiO4 (SSO, Zeff = 32.5) and Ba2SiO4 (BSO, Zeff = 49.9). Sources of error in the measured gamma-ray heating rates are as follows: Statistical deviation of four TLDs 5 - 15 % Number of neutrons generated 2 - 3 % Calibration of the TLD reader 5 % Due to the subtraction of target gamma-rays and neutron response, the following uncertainties are to be added to the above errors according to the quadratic propagation of error. Response functions for neutrons 30 % Neutron energy spectra 10 % Target gamma-ray 20 % Overall errors for the obtained gamma-ray heating rates of vanadium are ~ 10%, except at the positions in the front surface of the assemblies where they are 20 ~ 25 %. 5. Description of Results and Analysis: ----------------------------------- The measured neutron spectra by the three methods at the depths of 76 mm and 178 mm are shown in Figs. 3 and 4, respectively. The numerical data of the spectra measured by the NE213, PRC and SDT methods are given in Tables 5 - 7, respectively. Table 8 summarises integral neutron fluxes derived from the measured neutron spectra. The measured dosimetry reaction rates are shown in Table 9. The measured gamma-ray spectra at the positions of 76 mm and 178 mm are shown in Figs. 5 and 6, and the numerical data of the spectra are shown in Table 10. Table 11 summarises the measured gamma-ray heating rates in vanadium. Example of Experiment Analysis: Transport calculations with the MCNP-4A code are presented in [2]. The calculations were performed using the JENDL-FF, JENDL-3.2, ENDF/B-VI and EFF-3 nuclear data libraries. The sample input for the MCNP-4A code is given in file mcnp-v.inp. The input was taken from [1], except that the 0 degree source was used instead of the source subroutine (not provided in the document [1]). 6. Special Features: ---------------- None 7. Author/Organizer: ---------------- Experiment and analysis: F. Maekawa, C. Konno, Y. Kasugai, Y. Oyama, Y. Ikeda Japan Atomic Energy Research Institute Tokai-mura, Naka-gun, Ibaraki-ken, 319-1195 Japan Phone: 81-292-82-6809 (for Y.O.) or -6015 (for H.M.) Fax: 81-292-82-5996 (for Y.O.) or -6365 (for H.M.) e-mail: oyama@cens.tokai.jaeri.go.jp or fujio@cens.tokai.jaeri.go.jp Compiler of data for Sinbad: I. Kodeli OECD/NEA, 12 bd des Iles, 92130 Issy les Moulineaux, France e-mail: ivo.kodeli@oecd.org Reviewer of compiled data: P. ORTEGO Sea Shielding Engineering And Analysis (SEA) Avda. Atenas 75 Local 9 Las Rozas 28230 MADRID seacandan@retemail.es 8. Availability: ------------ Unrestricted 9. References: ---------- [1] F. Maekawa, C. Konno, Y. Kasugai, Y. Oyama, Y. Ikeda: “Data Collection of Fusion Neutronics Benchmark Experiment Conducted at FNS/JAERI”, JAERI-Data/Code 98-021 (1998). [2] F. Maekawa, Y. Kasugai, C. Konno, I. Murata, Kokooo, M. Wada, Y. Oyama, Y. Ikeda and A. Takahashi: “Benchmark Experiment on Vanadium with D-T Neutrons and Validation of Evaluated Nuclear Data Libraries by Analysis of the Experiment“, J. Nucl. Sci. Technol., Vol. 36, No. 3, p. 242-249 (March 1999) [3] F. Maekawa, C. Konno, K. Kosako, Y. Oyama, Y. Ikeda and H. Maekawa: “Bulk Shielding Experiments on Large SS316 Assemblies Bombarded by D-T Neutrons, Volume II: Analysis“, JAERI-Research 94-044 (1994). [4] Y. Oyama: “Experimental Study of Angular Neutron Flux Spectra on a Slab Surface to Assess Nuclear Data and Calculational Methods for a Fusion Reactor Design“, JAERI-M 88-101 (1988). References to other useful documents can be found in the above reports. 10. Data and Format: --------------- DETAILED FILE DESCRIPTIONS -------------------------- Filename Size[bytes] Content ---------------- ----------- ------------- 1 fnsv-abs.htm 19,225 This information file 2 fnsv-exp.htm 26,157 Description of experiment 3 mcnp-v.inp 13,054 Input data for MCNP-4A calculations 4 fnsv-1.gif 25,282 Figure 1: Sectional view of the vanadium assembly 5 fnsv-2.gif 10,849 Figure 2: Source neutron spectrum emitted towards the 0 degree from the target. 6 fnsv-3.gif 20,330 Figure 3: Neutron spectra at z=7.6 cm in vanadium 7 fnsv-4.gif 20,231 Figure 4: Neutron spectra at z=17.8 cm in vanadium 8 fnsv-5.gif 17,683 Figure 5: Gamma-ray spectra at z=7.6 cm in vanadium 9 fnsv-6.gif 16,920 Figure 6: Gamma-ray spectra at z=17.8 cm in vanadium 10 j98-021.pdf 12,359,881 Reference JAERI-Data/Code 98-021 11 fns-v.pdf 893,812 Reference J. Nucl. Sci. Technol., Vol. 36, No. 3 File >fnsv-exp.htm contains the following tables: Table 1: Material specification Table 2: Systematic errors for neutron spectra measurements by NE213 Table 3: Uncertainties in measured neutron spectra by the SDT method Table 4: Dosimetry Reactions used in the foil activation method Tables 5-7: Measured neutron spectra Table 8: Integral neutron fluxes Table 9: Measured dosimetry reaction rates Table 10: Gamma-ray spectra Table 11: TLD Measurements Figures are included in GIF format. SINBAD Benchmark Generation Date: 09/2002 SINBAD Benchmark Last Update: 09/2002