IEEE TRANSACTIONS ON NUCLEAR SCIENCE, VOL. 61, NO. 2, APRIL 2014 985
Effects of Background on Gamma-Ray Detection for
Mobile Spectroscopy and Imaging Systems
Timothy J. Aucott, Mark S. Bandstra, Victor Negut, Joseph C. Curtis, Daniel H. Chivers, and Kai Vetter
Abstract—The presence of gamma-ray background significantly
reduces detection sensitivity when searching for radioactive
sources in the field, particularly in mobile systems which must
contend with a variable background that is not known a priori.
An extensive survey of the background was performed in the San
Francisco Bay Area using both sodium iodide and high-purity
germanium detectors, covering a wide variety of environments
that might be encountered in an operational scenario. This data
was used as a basis for source injection in a moving detector sce-
nario in order to assess the effects of the background on different
detection approaches. Both imaging and spectroscopic algorithms
were implemented for the sodium iodide array, and their per-
formances are compared for a variety of source energies and
stand-off distances in the presence of the measured background.
Index Terms—Gamma-ray detection, radiation imaging,
spectroscopy.
I. INTRODUCTION
T
HERE are a number of scenarios in which a weakly
gamma-emitting source needs to be detected in the pres-
ence of a large background. For well-controlled cases, such as
those in low-count-rate laboratories, the background can be
minimized and then measured with a great deal of accuracy.
For many applications, however, a detector system is brought
out into the field and exposed to a background that may not
be well understood. This background may arise from a variety
of sources, both naturally-occurring and anthropogenic, but in
both cases will limit the detection of the source. Not only does
this background add significant statistical noise, but there are
large systematic uncertainties that arise from changes between
different environments [1], [2]. Mobile detector systems, in
particular, are constantly contending with a background that is
changing over time and location, and which is not necessarily
known or measurable a priori.
Manuscript received September 29, 2013; revised January 15, 2014; accepted
February 10, 2014. Date of current version April 10, 2014. This work was
supported by the U.S. Department of Homeland Security under Grant Award
2011-DN-077-ARI049-03.
T. J. Aucott, V. Negut, and J. C. Curtis are with the Department of Nu-
clear Engineering, University of California, Berkeley, CA 94720 USA (e-mail:
tjaucott@berkeley.edu).
D. H. Chivers and M. Bandstra are with the Nuclear Science Division,
Lawrence Berkeley National Laboratory, Berkeley, CA 94720 USA.
K. Vetter is with the Department of Nuclear Engineering, University of Cal-
ifornia, Berkeley, CA 94720 USA, and also with the Nuclear Science Division,
Lawrence Berkeley National Laboratory, Berkeley, CA 94720 USA.
Color versions of one or more of the figures in this paper are available online
at http://ieeexplore.ieee.org.
Digital Object Identifier 10.1109/TNS.2014.2306998
In any detection system, some threshold must be set as a de-
cision criterion for the presence or absence of a source. The
challenge faced by mobile detectors is that different environ-
ments contribute different rates of background. In particular, if a
threshold is chosen based on statistical variance alone, the false
alarm rate of the detector will likely be much higher than ex-
pected due to the systematic variance. This study focuses on
scintillator-based systems, which are commonly used in these
types of applications due to their relatively low cost per volume.
Because of their lower energy resolution (compared to semi-
conductor detectors), the effects of background are particularly
pronounced, as counts in the source peak will be convolved
with nearby background lines. One important goal is to mea-
sure the extent of these changes in the real-world environment
and to assess its impact on detection schemes that are commonly
employed.
Two well-established approaches for detecting these sources
are gamma spectroscopy and imaging. Both methods aim to in-
crease the signal-to-noise ratio of the system by looking for a
feature in some reduced space; for example, spectroscopy might
look for a photopeak in energy space, while imaging looks for a
peak pixel in the image space. Imaging is potentially less sensi-
tive to background uncertainty [3], but at the expense of lower
absolute efficiency. In this study, the imager in question is a
passive coded aperture, with an open fraction of 50%. Spec-
troscopy, on the other hand, has a higher efficiency, but may not
necessarily account for the background variability. Of course,
an imaging system has the additional ability to localize the ra-
diation source, and spectroscopy can identify the isotope being
detected, but this work focuses on the ability to compensate for
background and detect the source.
These two methodologies were compared by measuring the
gamma background and then injecting source photons into the
background data set to mimic a stationary source some dis-
tance from the path of the moving detector. This method cre-
ates two distributions, one for the background alone and one for
the source plus the background. By varying the alarm threshold
across the range of the two distributions, a receiver operator
characteristic (ROC) curve is created by plotting the probability
of true positives against the false positives. The background is
divided into separate runs, with a length determined by the par-
ticular standoff distance. The algorithms then report a single de-
cision on the presence or absence of a source in each run. In
order to make a fair comparison of false alarm rate, only one
isotope and standoff distance are considered at a time, which
are assumed by both algorithms. In a real system, of course, the
isotope and location are not known a priori; this simplification,
however, results in a more controlled study.
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