Gamma-ray Full Spectrum Analysis for Environmental Radioactivity by HPGe Detector
Research Paper
J. Astron. Space Sci. 31(4), 317-323 (2014)
http://dx.doi.org/10.5140/JASS.2014.31.4.317
Gamma-ray Full Spectrum Analysis for Environmental Radioactivity
by HPGe Detector
Meeyoung Jeong1,2, Kyeong Beom Lee2†, Kyeong Ja Kim3, Min-Kie LEE2, Ju-Bong HAN1
1
Radiation Measurement and Radiation Safety, University of Science and Technology, Daejeon, Korea
Korea Research Institute of Standards and Science, Daejeon 305-600, Korea
3
Korea Institute of Geoscience & Mineral Resources, Daejeon, Korea
2
Odyssey, one of the NASA’s Mars exploration program and SELENE (Kaguya), a Japanese lunar orbiting spacecraft have
a payload of Gamma-Ray Spectrometer (GRS) for analyzing radioactive chemical elements of the atmosphere and the
surface. In these days, gamma-ray spectroscopy with a High-Purity Germanium (HPGe) detector has been widely used
for the activity measurements of natural radionuclides contained in the soil of the Earth. The energy spectra obtained
by the HPGe detectors have been generally analyzed by means of the Window Analysis (WA) method. In this method,
activity concentrations are determined by using the net counts of energy window around individual peaks. Meanwhile, an
alternative method, the so-called Full Spectrum Analysis (FSA) method uses count numbers not only from full-absorption
peaks but from the contributions of Compton scattering due to gamma-rays. Consequently, while it takes a substantial
time to obtain a statistically significant result in the WA method, the FSA method requires a much shorter time to reach
the same level of the statistical significance. This study shows the validation results of FSA method. We have compared
the concentration of radioactivity of 40K, 232Th and 238U in the soil measured by the WA method and the FSA method,
respectively. The gamma-ray spectrum of reference materials (RGU and RGTh, KCl) and soil samples were measured by
the 120% HPGe detector with cosmic muon veto detector. According to the comparison result of activity concentrations
between the FSA and the WA, we could conclude that FSA method is validated against the WA method. This study implies
that the FSA method can be used in a harsh measurement environment, such as the gamma-ray measurement in the Moon,
in which the level of statistical significance is usually required in a much shorter data acquisition time than the WA method.
Keywords: gamma-ray full spectrum analysis, gamma-ray spectrometer, lunar orbiter payload, anticoincidence background
suppression
1. INTRODUCTION
The geological matrix in the Earth and the Moon contain
the primary natural radionuclides. These are the single
nuclide as 40K and the decay series of 232Th and 238U. The
decay series of 232Th and 238U emit three different types of
radiation: alpha particles, beta particles and gamma-rays. As
gamma-rays have more extreme radiation penetration than
alpha and beta particles, gammas are used in the radiation
measurement. The activity concentrations of 232Th and
238
U are same as those of their progenies due to radioactive
equilibrium (secular equilibrium).
Typically, gamma-ray spectroscopic system utilizes
Window Analysis (WA) method in order to measure soil
based radioactivity. Hendriks, PHGM et al. (2001) utilized
Full Spectrum Analysis (FSA) method in the development
of high-efficiency BGO scintillation detector system for a
comparison with conventional WA system which uses NaI
detector. Also, Maphoto KP (2004) compared two analysis
methods using an HPGe detector, and utilized FORTRAN
program for FSA. The two methods showed a difference of
1% ~ 61 % depending on the samples.
In this study, a FORTRAN program was developed for the
technology development of FSA to replace the WA method
This is an Open Access article distributed under the terms of the
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provided the original work is properly cited.
Received Nov 6, 2014 Revised Dec 3, 2014 Accepted Dec 4, 2014
†Corresponding Author
E-mail: , ORCID: 0000-0002-5202-2004
Tel: +82-42-868-5379, Fax: +82-42-868-5671
Copyright © The Korean Space Science Society
317
http://janss.kr plSSN: 2093-5587 elSSN: 2093-1409
J. Astron. Space Sci. 31(4), 317-323 (2014)
Table 1. The data of used materials.
and a low-level background gamma-ray spectrometer
developed by Korea Research Institute of Standards and
Science (KRISS) was used. This gamma-ray spectrometer is
equipped with a passive shield to reduce background signals
and an active shield to eliminate cosmic rays. It is operated
by anti-coincidence mode with HPGe detectors. The
purpose of this study is to ensure the validity of FSA method
by evaluating uncertainties between the measurement and
analysis results of the WA and the FSA.
WA method requires long measurement time and only
takes into account of the interested peaks in measured spectra,
thus, the accuracy is low. Moreover, it has a disadvantage of
slow analyzing speed. In this study, a validation is performed
for the Full Spectrum Analysis (FSA) method which
complements the WA method to account for all the energy
peaks from full spectrum in addition to the contributions
of the Compton scattering, thus enabling measurement of
statistical significance in a short period of time.
Mesh
Mass
(kg)
Density
(g/cm3)
Activity
concentration
(Bq/kg)
RGU(238U)
RGTh(232Th)
KCl(40K)
soil
240
240
200
200
0.1076
0.1089
0.0825
0.0855
1.196
1.210
0.916
0.950
4940
3250
16602
2.2 Methods
Gamma-ray spectroscopic system detects gammas emitted
from sample materials using a High Purity Germanium
(HPGe) detector (Khandaker 2011). As radioactive isotopes
emit gammas of intrinsic energy, if we measure the energy of
gammas, we can tell apart the kind of isotope and its activity.
Gamma-ray spectroscopic system is used to identify the
isotopes and activities by measuring gammas from a sample
material. Most of HPGe detectors use high-density and high
atomic numbered lead as a shield to reduce background
noise due to radiation and radioactive dirt existing around the
detectors. HPGe gamma-ray spectrometers are used widely
for the measurement of environment radiations (Murray et al.
1987).
2. MATERIALS AND METHODS
2.1 Materials
The reference materials, IAEA-RGU-1 and IAEA-RGTh-1,
were prepared by the Canada Centre for Mineral and Energy
Technology on behalf of the International Atomic Energy
Agency (IAEA), while the 40K reference material (KCl of
99.5% purity) was produced in Japan (Wieser 2006). The
reference materials were sampled in a 90 ml can and were
kept for radioactive equilibrium between radium and radon
daughter nuclides. For the background data acquisition,
a 90 ml can was filled with pure water. Table 1 lists the
information of the reference sources from the samples, such
as mass and activity concentration. The detailed sample
preparation process is summar (...truncated)