# Antineutrino Flux from the Laguna Verde Nuclear Power Plant

Authors: Marisol Chavez-Estrada; Alexis A. Aguilar-Arevalo
Journal: Advances in High Energy Physics
 (2015)

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## Abstract

We present a calculation of the antineutrino flux produced by the reactors at the Laguna Verde Nuclear Power Plant in México, based on the antineutrino spectra produced in the decay chains of the fission fragments of the main isotopes in the reactor core, and their fission rates, which have been calculated using the DRAGON simulation code. We also present an estimate of the number of expected events in a detector made of plastic scintillator with a mass of 1 ton, at 100 m from the reactor cores.


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## Body

## 1. Introduction

In recent years, there has been significant progress in understanding the properties of neutrinos; most notably, since 2012, the results of the reactor neutrino experiments, Daya Bay [1], Reno [2], and Double Chooz [3], have determined that the mixing angle θ13 is nonzero with a high level of significance. The current degree of development of neutrino detection technology is close to making a reality to nonintrusively monitor the operational status, power level, and fissile content of a nuclear reactor in real time using detectors placed at distances of a few tens of meters.For a technological application such as reactor monitoring, only antineutrinos with energies above the threshold of the Inverse Beta Decay (IBD) reaction (see (1)) on free protons (Eν>1.8 MeV) can be realistically considered at present:(1)ν¯e+p⟶e++n.IBD interactions of neutrinos on free protons can be identified through the correlation of the prompt positron signal and a delayed neutron capture signal in liquid or plastic scintillator-based detectors. In general, the spectrum of the antineutrinos from a nuclear reactor detected via IBD has a peak between 3.5 and 4 MeV. Since the number of emitted antineutrinos and their average energy depend on the amounts of  235U, 238U, 239Pu, and 241Pu isotopes present in the core, the measured energy spectrum provides a direct image of the fuel composition of the reactor core at a given time.Monitoring nuclear reactors through their antineutrino flux is a complimentary and promising new tool for supervising the operations of nuclear plants, which are bound to operate according to protocols established by the International Atomic Energy Agency (IAEA). This agency is responsible for ensuring that nuclear reactors worldwide operate legally, preventing the diversion of fissile material to activities which could lead to the manufacture of weapons.Many research groups worldwide [4–10] have studied this application aiming at adding antineutrino detection to the techniques used to implement reactor safeguards. In a medium term plan (5 to 8 years), IAEA [11] has proposed that antineutrino detectors for safeguard applications should be able to provide information on the thermal power, fissile content, and operational status of reactors while deployed aboveground in a compact volume like that of a standard 12 m ISO container, to minimize its intrusiveness with the nuclear power plant operations.One of the IAEA’s safeguards goals is to demonstrate the ability to detect the unauthorized removal of as little as 8 kg of plutonium (defined as a “significant quantity”) from a nuclear reactor within a 3-month period [12]. According to the agency, it is not possible to exclude the possibility that an explosive nuclear device is manufactured having this amount of material unaccounted for over this time.The accuracy to which the plutonium content in a nuclear reactor can be measured using neutrinos has been the subject of a number of studies [13–16]. One method [16], albeit with reduced sensitivity compared to IAEA’s “significant quantity,” consists of measuring the time evolution of the antineutrino count rate in a detector. Adding evolution of antineutrino spectrum shape as well as combination with standard IAEA safeguards methodologies may eventually allow reaching the desired goal set by the agency. Recent studies suggest that the observation of shape distortions with sufficient significance could be achieved with realistic energy resolutions [8] (~12% at 2 MeV neutrino energy).A recent demonstration that the ON/OFF cycle, thermal power stability, and fissile inventory of a reactor can be measured from the total antineutrino event rate in a compact (~1 m3 scale) and simple detector was given by the SONGS1 experiment [4], which used a gadolinium- (Gd-) loaded liquid scintillator detector, deployed under 25 MWe overburden, at 25 m from the reactor core of the 3.46 GWth San Onofre Nuclear Generating Station in Southern California in the United States. The experiment estimated a sensitivity to the removal of ~70 kg of 239Pu with 95% CL.Another recent development is the PANDA [5, 6] experiment, which used a segmented plastic scintillator detector located at ground level, with modules wrapped in Gd-coated sheets, at 36 m from Unit 2 reactor at the Ohi Power Station in Japan. This detector design uses event topology information to tag antineutrino events and to discriminate them from backgrounds such as fast neutrons, allowing operating it on the surface. Furthermore, it can be transported and operated easily inside a compact vehicle and has the advantage that, unlike the liquid scintillators, it is nonflammable. Studies from a 360 kg prototype have shown promise that this detector technology could be further developed to achieve the IAEA medium term goals.México has two nuclear fission reactors at the Laguna Verde Nuclear Power Plant (LVNPP), which has been operating commercially since 1990 (Unit 1) and 1995 (Unit 2). This is the only nuclear power plant in the country and it generates about 5% of its total electric power production. In this work, we calculate the antineutrino flux produced by these reactors and give some estimates of the number of events expected in a generic plastic scintillator detector located at a distance of 100 m from the reactor cores. Knowledge of the antineutrino flux produced by a particular reactor is an important step towards its monitoring using this method.While abundant literature exists about the calculation of neutrino fluxes from pressurized water reactors (PWR) [21–28], much less information is available about neutrino production at boiling water reactors (BWR) (see, e.g., [29]). These two reactor types operate under the same basic physical principles regarding nuclear fission, but differences in their operational procedures may affect differently the neutrino flux they produce, as well as its evolution along the reactor fuel cycle.This paper is organized as follows. In Section2, main technical data on the LVNPP and its reactors are detailed. In Section 3, a description about the production of antineutrinos from nuclear reactors is given, and the calculation of antineutrino flux is presented. In Section 4, parameters and characteristics of the DRAGON simulation code used to calculate fission rates of four major fissile isotopes for this paper are described. Section 5 shows the event rates or interactions that are expected to be observed with a 1-ton plastic scintillator detector placed at 100 meters from the LVNPP reactors. Finally, Section 6 presents the conclusions.


## 2. The Laguna Verde Nuclear Power Plant (LVNPP)

The LVNPP is located in the municipality of Alto Lucero, Veracruz, México. This plant has two twin units, each equipped with a BWR-5 second-generation reactor with a Mark II containment design, supplied by General Electric with a capacity of 2027 MWth, and net electrical output of 805 MWe. Both reactors operate with enriched uranium as fuel and demineralized water as moderator and coolant. It is the only nuclear power plant in the country and generates about 5% of the total electric power production in México [30].Each nuclear reactor core can be approximately represented by a cylinder ~4 m in height and 4 m in diameter containing 444 fuel assemblies and 109 control bars arranged as shown in Figure1. A fuel assembly is a square prism with sides of ~13 cm and 4 m in height, containing an array of fuel rods (configurations of 8×8, 10×10, or 12×12 have been either used or considered). Within a given fuel assembly, some of the rods contain uranium oxide (UO2) with various levels of enrichment, others contain a mixture of UO2 with gadolinium oxide (Gd2O3) at varying concentrations, and some of them are hollow in order to allow the flow of the refrigerant through them. Combining rods with different levels of enrichment and Gd2O3 concentrations permits adjusting the properties of the medium for the production, absorption, and diffusion of neutrons differently at various location across the core.Figure 1
Schematic of a cross section of one of the LVNPP reactor cores [17]. The “red” assemblies (0.711%) are located on the perimeter of the reactor core, while the “blue” assemblies (1.76%) are arranged in the central area. There are 109 control bars represented as crosses in the figure.


## 3. DRAGON Simulation of the Reactor Core

We used the numerical simulation code DRAGON [31] with the modifications described in [32] to implement a simulation for the LVNPP reactors and extract the time evolution of the fission rates (number of fission instances per second) of each of the main fissile isotopes in the core. Several research groups worldwide have implemented this simulation for PWR reactors, aiming at the same objective [33]. The code solves the neutron transport equations of individual fuel assemblies, whose detailed composition is given as an input. The overall behaviour of neutrons across the core can be calculated by summing over the various types of assemblies that compose a given core configuration.As described in Section2, a geometry with 444 fuel assemblies with 3 different types of 235U enrichment was considered. The initial fuel load that was assumed in this work is that shown in Figure 1. Note that in this model no assembly contains plutonium at the beginning of the operation cycle.In Figure2, we illustrate a single fuel assembly (in this case with a 10×10 rod configuration) [34] corresponding to one with average enrichment of 1.76% (blue assembly). The dimensions of a single unit cell (the place occupied by a single fuel rod) are shown in Figure 3. The three types of assembly (red, yellow, and blue) share the same geometry; however, the composition of the fuel rods within a given assembly is, in general, different. The number of assemblies of each type, NA, is Nred=68, Nyellow=280, and Nblue=96, totaling 444.Figure 2
Arrangement of fuel rods for blue assembly (half enrichment). (a) DRAGON code output. (b) Bar type (see Table2). Notice that initially there are no fuel bars with Pu.
(a)
(b)Figure 3
Cross section of a single unit cell. A fuel bar (in red) with Zircaloy cladding (white) immersed in demineralized water as moderator. Complete assembly is formed by 92 of these cells. The values forR1, R2, and L are described in Table 3.We considered eight different fuel rod compositions, labeledCX, with X=0,1,2,3,4,5,6,G, and used them to construct the various assemblies with the desired 235U enrichment and gadolinium concentration. Only fuel rods of type G contain gadolinium. Table 1 shows the number of fuel rods of each type which are used to build each of the three assemblies. As an example, Table 2 shows how we constructed the blue assembly.Table 1
Number of fuel bars of typeCX (X=0,…,6,G) for each assembly. There are a total of 92 bars for each assembly.
Assembly
C
0
C
1
C
2
C
3
C
4
C
5
C
6
C
G
Red
92
0
0
0
0
0
0
0
Blue
59
0
0
3
4
6
8
12
Yellow
34
9
19
0
0
0
0
30Table 2
Isotopic composition of fuel bars for blue assembly in Figure1. UO2 and UO2-Gd2O3 bars with overall average enrichment of 1.76% of 235U (relative to total U). Fuel rods with Gd admixture have enrichment of 5.2% (in total) and 3.792% (relative to U).
Rod type
Number of rods
234U
235U
238U
O16
Gd
(%)
(%)
(%)
(%)
(%)
C
0
59
0.005
0.627
87.517
11.852
—
C
3
3
0.029
2.468
85.651
11.852
—
C
4
4
0.029
2.821
85.298
11.852
—
C
5
6
0.029
3.173
84.945
11.852
—
C
6
8
0.029
3.482
84.637
11.852
—
C
G
12
0.028
3.142
79.691
11.933
5.206Table 3
Parameters of the BWR core used in the simulation with DRAGON code [20].
Thermal power (of each reactor)
2027 MWth
Specific power (of each reactor)
20.43 MW/ton
Moderator
Demineralized water
Temperature
600 K
Density
0.720 g/cm3
Coolant
Demineralized water
Temperature
400 K
Density
0.720 g/cm3
Fuel assemblies
444
Red assemblies
68
Blue assemblies
96
Yellow assemblies
280
Single unit cell (L×L)
1.295 cm × 1.295 cm
Fuel bars per assembly
92
Composition
UO2/UO2-Gd2O3
Cladding
Zircaloy 2
Zircaloy density
5.821 g/cm3
Zircaloy temperature
600 K
Fuel temperature
900 K
Fuel density
10.079 g/cm3
Fuel bar radius (R1)
0.438 cm
Zircaloy cladding radius (R2)
0.513 cm
Fuel bar height
400 cm
Coolant pipes per assembly
2
Composition
Zircaloy 2
Pipe radius (occupied by water)
1.0 cm
Pipe radius (occupied by Zircaloy)
1.2 cmTable3 lists the values used for the various parameters required by the simulation. Tests showed small dependence of the fission rates on variations of the coolant, moderator, and fuel temperatures, while maintaining the thermal power constant.A simulation was run for each of the three types of assemblyA (red, blue, or yellow in Figure 1), providing the fission rates fi(CX;A) for each type of fuel rod, and for each one of the fissile isotopes, i=1,2,3,4 (235U, 238U, 239Pu, and 241Pu, resp.).To obtain the fission rates for a given assembly,fiA, we multiply the fission rate for each type of fuel rod times the number of rods of its type in the assembly, Nrods, and sum over all fuel rod types in the assembly; that is,(2)fiA=∑CX∈ANrodsCX;AfiCX;A.Finally, to calculate the fission rates of isotopei in the complete reactor core, fi (Figure 4), we multiply the number of assemblies of each type times the corresponding fission rates for that assembly:(3)fi=∑ANAfiA.Figure 4
Fission rates (normalized) obtained with DRAGON for the 4 main fissile isotopes in the 444 fuel assemblies that make up the core of BWR-5 of 2.027 GWth like the LVNPP reactor.The simulation was run sequentially in time intervals of 5 days of evolution of the nuclear reactor core until completion of a full operation cycle of 400 days.As is expected for an initial load without plutonium, the fission rates of239Pu and 241Pu start at zero and rapidly grow to become comparable to those of the U isotopes within a few weeks of operation. A more realistic situation should consider that, between two fuel reloads, there will always be some remnant of plutonium inside the reactor, because when this action is performed, only a fraction of the spent fuel is replaced by new material.


## 4. The Antineutrino Flux

The power output of a nuclear reactor originates from the energy released in the fission of heavy elements, such as uranium and plutonium, into lighter fission fragments which are often unstable. The beta decay,(A,Z)→(A,Z+1)+e-+ν¯e, of the fission fragments produces a large number of electron antineutrinos ν¯e which are emitted isotropically from the core. During the fuel “burning” process, uranium isotopes breed 239Pu and 241Pu. The latter may in addition to 235U undergo a fission process only with slow (thermal) neutrons, while 238U is fissionable by fast neutrons only. The decay of 239Pu produces substantially less antineutrinos than the decay of 235U in the same energy range; therefore, during a typical reactor fuel cycle, the amount of antineutrinos decreases as uranium content decreases and the concentration of plutonium increases.Each fission releases on average ~200 MeV of energy and produces ~6ν¯e (~3 beta decays per fission fragment), with energies below ~10 MeV. This sets the number of antineutrinos emitted by a typical reactor to ~2 × 1020 ν¯e/s per GWth of thermal power. The energy spectrum of the antineutrinos depends on the fuel composition at a given time (239Pu antineutrinos are slightly less energetic than those of 235U fission products).The production of reactor antineutrinos is not exclusively through beta decay of the fission fragments of the four main fissile isotopes (235U, 238U, 239Pu, and 241Pu). The neutron capture in 238U(n,γ)239U also generates these particles in a process that contributes about 17% of the total antineutrino flux. This process occurs when a nucleus of 238U captures a neutron, leading to the following reaction: U238+n→U239→Np239→Pu239, and it produces two antineutrinos through two beta decays of 239U. This process occurs at a rate of ~0.6 per fission and produces antineutrinos with energies below 1.3 MeV.Let us now consider the antineutrinos emitted by one of the reactors at the LVNPP. Ignoring the neutron capture contribution, the antineutrino fluxΦi above 1.8 MeV can be calculated from the fission rates fi(t) and the antineutrino energy spectrum Si(Eν¯) of each isotope i, where i=1,2,3,4 corresponds to each of the main fissile isotopes of the reactor core: 235U, 238U, 239Pu, and 241Pu.Assuming neutrinos are emitted isotropically, using a sphere of radiusR, the flux at a time t for each isotope i is calculated as(4)ΦiEν¯,t=14πR2SiEν¯fit,with R being the distance from the reactor core to the detector.In our calculation of the antineutrino flux, we have used the new predictions of the energy spectra including the effect of the reactor antineutrino anomaly, as reported by [27, 35, 36]. The antineutrino energy spectra Si(Eν¯) between 1.8 and 8 MeV are shown in Figure 5. For the purposes of reactor monitoring, the effect of this anomaly can be ignored as long as only comparisons between the relative changes of the spectrum throughout the reactor operation cycle are made.Figure 5
Energy spectra of the emitted antineutrinos per fission of235U, 238U, 239Pu, and 241Pu. The dotted line at 1.8 MeV indicates the threshold for the Inverse Beta Decay (IBD) process.Figure6 shows the antineutrino flux for each of the main fissile isotopes of one of the reactors in the LVNPP, at day 5 (a) and then at day 200 (b); in the latter, the flux can be considered stable. The total flux (the sum of the four isotopes) for each time period is also shown in the gray curve in this figure. The total flux at day 200 is shown in Table 4.Table 4
Total antineutrino flux at day 200 for one of the reactors of the LVNPP, at 100 m from the reactor core. The last column shows the total systematic errorδ(sys).
E [MeV]
Φ
total [MeV−1 s−1 cm−2]
δ(sys) [%]
1.800
6.921E + 10
7.2
2.048
6.192E + 10
3.6
2.296
5.185E + 10
3.6
2.544
4.304E + 10
3.7
2.792
3.634E + 10
3.7
3.040
3.052E + 10
3.7
3.288
2.542E + 10
3.7
3.536
2.066E + 10
3.8
3.784
1.671E + 10
3.8
4.032
1.336E + 10
3.9
4.280
1.045E + 10
4.0
4.528
8.026E + 09
4.0
4.776
6.147E + 09
4.1
5.024
4.841E + 09
4.2
5.272
3.761E + 09
4.3
5.520
2.871E + 09
5.2
5.768
2.157E + 09
5.4
6.016
1.584E + 09
5.5
6.264
1.179E + 09
5.6
6.512
8.900E + 08
5.8
6.760
6.692E + 08
5.9
7.008
4.752E + 08
7.0
7.256
3.027E + 08
7.4
7.504
1.881E + 08
7.8
7.752
1.210E + 08
8.4
8.000
6.763E + 07
9.8Figure 6
Antineutrino flux produced by the fission of the 4 main fissile isotopes at 100 meters from one of the LVNPP reactors of 2.027 GWth at days 5 (a) and 200 (b) of operation. The gray curve (a) is the total flux.
(a)
(b)Two systematic uncertainties are associated with the calculation of the antineutrino flux: the error due to the energy spectra of antineutrinosδ(S(Eν¯)) and an error δ(Pth) associated with fluctuations in the thermal power of the reactor core, assumed to be 5% along one fuel cycle. The total error is the sum in quadrature of these uncertainties. The uncertainties in the antineutrino spectra are taken from [35, 36] and are of the order of 2–5% for the dominant parts of the spectra from 235U, 239Pu, and 239Pu and between 10 and 17% for the dominant part of the spectrum from 238U.The total flux per reactor at day 200 from our calculation is compared in Figure7 to that obtained according to the parametrization suggested by Vogel and Engel [18], setting the fission rates of the four main fissile isotopes to those output by the simulation (2.7×1019 fis/s for 235U, 7.7×1018 fis/s for 238U, 2.8×1019 fis/s for 239Pu, and 1.5×1018 fis/s for 241Pu). The two calculations agree well within the assumed uncertainties.Figure 7
Total antineutrino flux per reactor at day 200 (solid curve with error band). The error includes the sum of the relative uncertainties of each of the 4 main fissile isotopes in the reactor. The dashed curve shows the parametrization suggested in [18] with the fission rates calculated by DRAGON for the LVNPP. The continuous line shows the IBD cross section as given by [19].Spent fuel is stored temporarily in a nearby place to the reactor core and is expected to have a small contribution (<1%) to the antineutrino flux above the IBD reaction threshold [37] and was not considered for the calculation in this work.


## 5. Event Rates

Although the IBD reaction has a very small cross section (~10−43 cm2), the enormous flux emitted by a nuclear reactor allows the signal to be observed with a relatively small detector located at a relatively short distance from the reactor core (several tens of meters). The total IBD cross section as a function of the neutrino energy is shown in Figure 7 (right scale). Here we consider 1 ton of polyvinyl-toluene (PVT) plastic scintillator located at 100 m from each of the reactor cores, similar to the detector considered in [5, 6].This segmented detector is a one-cubic-meter array of 100 optically isolated plastic scintillator bars of dimensions 100 cm × 10 cm × 10 cm (10 kg per bar), instrumented with photomultiplier tubes (PMTs) at both ends and separated with sheets coated with gadolinium oxide (Gd2O3). The 100 m distance was chosen from aerial photographs of the LVNPP site, so as to place the detector equidistantly from both reactor cores, in an existing open space away from any discernible infrastructure.Following the IBD interaction (see (1)) of an antineutrino with a proton in the plastic scintillator, the prompt positron and the delayed neutron capture are detected independently. The positron will deposit its energy (comparable to the incident neutrino energy) through ionization in the scintillator and annihilate producing two gamma rays. The neutron will thermalize in the plastic and will eventually be captured by a gadolinium nucleus in one of the Gd2O3-coated sheets, with a typical capture time of several tens of μs, liberating a cascade of gamma rays with a total energy of ~8 MeV. Recording of the energy deposition in each bar allows for the implementation of powerful background rejection techniques [5, 6] which are unattainable with single-volume detectors.The number of IBD interactions associated with neutrinos from isotopei, emitted with energies between Emin and Emax, and occurring in a time interval Δt (ΔNev(i)) is calculated by integrating the product of the flux Φi, the IBD cross section σ(Eν¯) [19], and the number of targets (in this case free protons) Np, over the energy interval:(5)ΔNeviΔt=Np∫EminEmaxΦiEν¯,tσEν¯dEν¯.Depending on the characteristics of the detector, only a fraction of these interactions will be observed. For a simple estimate, let this fraction be a uniform efficiency factorϵ. For neutrinos coming from nuclear reactors, Emin is the threshold of 1.8 MeV and Emax is ~10 MeV. The number of detected events for each isotope is then approximated by(6)Nevi=ϵ×NpΔt4πR2∫EminEmaxSiEν¯fitσEν¯dEν¯,where Δt is a small exposure time compared with the time scale in which fission rates fi(t) change appreciably. Calculation for longer times requires integration over time.Finally, the total number of events is equal to the sum of the events for each isotope:(7)Nevtotal=∑i=14Nevi.These are shown in Figure8, considering four different detector efficiencies (5%, 20%, 30%, and 100%) and counting for two consecutive days.Figure 8
Number of events accumulated over 2 days of exposure along a complete cycle of 400 days at LVNPP with two reactors in 1 ton of plastic scintillator. Curves for detection efficiencies (lower to higher) of 5%, 20%, 30%, and 100% are shown.The authors of [5, 6] estimate an antineutrino detection efficiency of 9.24% and an antineutrino event rate of 147 events/day in a 1-ton detector with an uncertainty of the order of 30%. This is consistent, within errors, with our expected rate in a similar detector, from Figure 8, of 280 events/day with the two reactors and 100% efficiency (stable after day 350), after scaling for the difference in reactor power and distance and assuming the same efficiency.For our background estimate, we assume a similar analysis technique to [5, 6]. The authors measured an uncorrelated background, free of fast neutron events, of ~365 events/day with an uncertainty of 19%, operating a 360 kg detector with the reactor OFF for 21 days.Taking the above considerations into account, a 1-ton segmented detector of this type, with a 9.24% signal efficiency, deployed at 100 m from the cores of the LVNPP reactors would expect to observe an antineutrino event rate of 26 events/day, with a background (defined as in [5, 6]) of ~1013 events/day. At this reactor distance, the daily rate could be measured with a significance of 5σ, provided the background rate normalization is determined with a precision of 0.5% (±5 events/day), which would require significant improvements in the analysis and about a couple of months of reactor OFF data. Improvements in the detector design such as adding water or polyethylene shields to moderate the fast neutrons are expected to yield more efficient background rejection.Changes in the total antineutrino event rate over the fuel cycle are expected at the 10–15% level, corresponding to a variation of several tens of kg of Pu being produced in the reactor. Given the low statistics of the expected antineutrino signal at the proposed detector standoff with the projected efficiency, it will be desirable to add whatever spectral shape information is possible to the analysis. The capabilities of the detector in this regard will be the subject of a future work.


## 6. Conclusions

We calculated the antineutrino flux produced by the reactors at the LVNPP in México using the DRAGON simulation code in the energy range 1.8 MeV <Eν < 8 MeV. The simulation provided the time evolution of the fission rates and hence the change of the flux along the 400-day-long fuel cycle, starting with an initial load with no plutonium. A total systematic uncertainty on the flux ranging from 3.6% to 9.8%, depending on the antineutrino energy, was calculated assuming a 5% uncertainty on the reactor power and the uncertainties reported for the antineutrino spectra of the dominant fissile isotopes [35, 36]. Our calculation agrees well with frequently used parametrization [18] when used with the fission rates from the simulation of the LVNPP BWR reactors.The simulation code required the knowledge of generic parameters of the BWR reactors, at LVNPP, available in the literature, and showed the fission rates to have moderate dependence on variations of the coolant, moderator, and fuel temperatures for a fixed thermal power.A segmented plastic scintillator detector of the type considered in [5, 6] located at 100 m from the two reactors could in principle detect the emitted antineutrinos; however, new methods for background suppression and rejection for aboveground operation would need to be implemented. Operation at a significantly shorter distance from the cores must be pursued for its successful application to reactor monitoring.



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*Source: 109738-2015-12-08.xml*