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Physical Sciences Inc. 20 New England Business Center Andover, MA 01810
Physical
Sciences Inc.
Bogdan R. Cosofret, Kirill Shokhirev and Phil Mulhall
Physical Sciences Inc., Andover MA
David Payne, Bernard Harris and Richard Moro Raytheon Integrated Defense Systems, Tewksbury MA
2013 IEEE Conference on Technologies for Homeland
Security (HST ’13)
12-14 November 2013
Utilization of advanced clutter suppression
algorithms for improved spectroscopic
portal capability against radionuclide threats
ACKNOWLEDGEMENT:
This work has been supported by the US Department of Homeland Security, Domestic Nuclear Detection
Office, under competitively awarded contract/IAA HSHQDC-10-C-00171 and HSHQDC-11-C-00117. This
support does not constitute an express or implied endorsement on the part of the Government.
VG13-158
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Physical Sciences Inc.
Agenda
Motivation and General Objectives
Overview of PCS Algorithm and
Optimization for ASP
Experimental Setup
Results
Conclusions
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Motivation
Detection of threat R/N sources in moving
cargo is difficult due to the need to
acquire spectra at short integration time
– Low SNR regime
– Poisson noise and clutter mask weak threat
signals
Current systems: PVT-based RPM and
NaI-based ASP
Advanced Spectroscopic Portal
Capability gaps:
– RPMs are sensitive, cost effective, but lack energy resolution necessary for
threat ID high false warning rates that require secondary screenings
– PVTs have discrimination capability, but are expensive reduced sensitivity
imposes limits on how fast traffic moves through portal
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General Objectives
Improve overall performance of current ASP systems using
advanced algorithms for noise and clutter suppression
Demonstrate the achievement of ASP Key Performance Parameters
under improved and cost effective operational capability:
– Utilization of only 4 out of 12 NaI detectorscurrentlyintegratedwithRTN’s
ASP units
– Vehicle speeds through the portal in excess of 20 mph (> 6x improvement
over current throughput)
ASP Key Performance Parameters targeted:
– False alarm rate of 1 in 1000 occupancies
– Pd,ID > 90% for weak activity sources (< 10 µCi)
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Poisson/Clutter Split Model (PCS): Conceptual Approach and ASP Optimization
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GLRT Methodology for Threat Detection
PCS algorithm is based on the GLRT framework, where the
background is estimated within the Poisson/Clutter model
Background Estimation Data Set:
Background-only Spectra
Test Spectra:
Background + (Threat Signal)
GL
RT
Fra
me
wo
rk
Algorithm
Statistical
Model
Likelihood of H0
(no threat)
Likelihood of H1
(threat present)
Likelihood
ratio
Detection
and ID
CFAR
threshold
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PCS Model: Separation of Poisson and Clutter Noise
The variability among background radiological spectra can be attributed to
two mechanisms:
– Background clutter, i.e. the changes of the energy-dependent count rate due to
variations in isotopic composition depending on particular environments, weather
conditions, etc.
– The random process of radioactive decay, described by Poisson statistics
The key innovations behind the Poisson Clutter Split (PCS) algorithm are:
– The use of a novel probabilistic representation of radiological backgrounds
– Accurate modeling of gamma counts based on Poisson statistics
– The use of the Generalized Likelihood Ratio Test (GLRT) to simultaneously perform
detection and identification of sources.
PCS algorithm’s non-linear probabilistic model provides a better
characterization of the radiological environment than traditional linear
methods
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PCS Model: Separation of Poisson and Clutter Noise
Observed counts x, obey Poisson statistics corresponding to the local background
rate, b, and the integration time, Δt.
PCS calculates the mean rate as a function of energy and the dominant modes of
spectral variations, zk, observed across sampled environments:
The underlying rate, b, can be accurately parameterized with a limited number of
coefficients which determine the spectral variability of the rate:
– Clutter is reflected in the varying parameters, w
– zk capture the spectral features of the environment
In the presence of a radioactive source, the background rate, b , is elevated by an
energy-dependent contribution from the source:
)(~ tbPxb
1 x D vector, D is the number of channels
)},,..,({ 1 wzzbb k
),..,( 1 Kwww
),()( wswbsb
)()( wfwbpbp
f(w) is the probability distribution
of the clutter parameters
)(~ tPxTest
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PCS-based Background Estimation and
Threat Detection and Identification
Estimate the background (train) in single or multiple environments
N background spectra, { xi }, i = 1,..,N,
Estimate the modes of spectral variability and find parameter combinations, for each spectrum
Fit a probabilistic model to the distribution of w’s
Kkzk ,..,1,
distributionofw’s
Detection and ID: analyze new spectrum x
Given new spectrum x, maximize likelihood under two hypotheses:
H0: x is generated from a rate consistent with the background model
H1: x is generated from the rate consistent with the estimated background
spectrally perturbed by a threat isotope
Alarm and ID if likelihood ratio exceeds threshold
iw
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PCS Optimization for ASP
PCS background model developed using
previous ASP field data
– Background model developed for two operational modes:
1 sec and 0.5 sec integration time
– Spectra from 60 empty occupancies were used to create
background model
PCS CFAR threshold determination (Objective
1 in 1000 occupancies):
– 1000 available no-source occupancies contain ~200,000
1/10 sec live time spectra
– Processed spectra through PCS and analyzed results
– Set isotope specific CFAR threshold to be the highest PCS
signal value recorded under the 1000 observed occupancies
16 isotopes included in the PCS spectral library
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PCS Integration with ASP
Real-time PCS software installed on
Windows laptop
Laptop connected to ASP database
server which resides on an
Ethernet backbone
32-bit API allows calls across the
Ethernet backbone to pull spectra
and packet sequence number (PSN)
from database
Groups of 5 PSN were accumulated
to generate 0.5 sec integration time
spectra for ingestion into PCS
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Low Cost Identifier Portal (LCIP): Only 4 out 12 ASP detectors used: Aa3, Ba3, Ca1, Da1
96”
69” Aa1
Aa2
Aa3
Ba1
Ba2
Ba3
Da2
Da3
Ca1
Ca2
Ca3
Da1
NaI
Detectors
(4”x2”x16”)
Neutron
Detector
2.30m
2.36m
Speed (MPH)
Observation time (sec)
5 2.6
10 1.3
20 0.65
30 0.43
Spectra acquired at 0.5 second integration time
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Experimental Parameters
Vehicle: PSI Truck
Check sources emplaced inside truck:
– (1x) Cs-137 (8 µCi)
– (1x) Ba-133 (7 µCi)
– (1x) Co-57 (4 µCi)
Interferant: three 50 lb salt bags (~ 40 µCi of
K-40 signal)
Shielding:
¼” steel cap
– 30% reduction in peak
count for Cs-137
– 50% reduction in peak
count for Ba-133
– 67% reduction in peak
count for Co-57
Salt bags
Steel Cap
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LCIP Evaluation: Check Source Locations Inside Vehicle
12'
Salt Bags
Shielding (0.25” steel cap)
(when used)
29” 49”
40” 3x50 lbs
Salt bags
Source Locations
Positions for Cs-137 and Ba-133 used
during multi-source runs. Co-57 was
located on second stand
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Background Only (30 mph) 150 lbs of Salt Inside the Truck
Several runs through the portal were conducted without sources present
– Weak PCS responses observed for all 16 isotopes in the library
– No PCS responses exceeded the CFAR (1 in 1000 occ) isotope specific thresholds
– No false alarms were reported
Continuous acquisition of spectra over ~ 2 hrs also yielded no false alarms
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Truck with Unshielded Cs-137 (8 µCi) + Salt Vehicle Speed: 30 mph
PCS results with 4/12 NaI detectors: Pd,ID = 95% against unshielded Cs-137
at 30 mph (detected/ID in 18 out of 19 runs), CFAR = 1 in 1000 occ.
No false alarms or mis-identifications were reported
Note: Standard ASP software using with all 12/12 NaI detectors yielded
Pd,ID = 10% (2 out of 19 runs)
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Truck with Shielded Cs-137 (attenuated 8 µCi) + Salt Vehicle Speeds: 20 and 30 mph
PCS results with 4/12 detectors: Pd,ID = 93% at CFAR of 1 in 1000 occ.
against shielded Cs-137 at 20 - 30 mph (detected in 14 out of 15 runs)
No false alarms or mis-identifications were reported
Note: Standard ASP software with all 12/12 ASP detectors yielded Pd,ID = 0%
20 mph 30 mph
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Truck with Unshielded Ba-133 (7 µCi) + Salt Vehicle Speed: 30 mph
PCS results with 4/12 NaI detectors: Pd,ID = 93% against unshielded Ba-133 at 30
mph (detected/ID in 14 out of 15 runs), CFAR 1 in 1000 occ.
No false alarms or mis-identifications reported
Ba-133 presence leads to correlated I-131 PCS responses, but not strong enough to
exceed the I-131 isotope specific threshold. Cross-talk also addressed using
Dominant PCS
Note: Standard ASP software using all 12/12 NaI detectors yielded Pd,ID = 0%
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Truck with Shielded Ba-133 (attenuated 7 µCi) + Salt Vehicle Speed: 20 mph
PCS results with 4/12 NaI detectors: Pd,ID = 86% against shielded Ba-133 at
20 mph (detected/ID in 12 out of 14 runs), CFAR 1 in 1000 occ.
No false alarms or mis-identifications were reported
Note: Standard ASP software using all 12/12 NaI detectors yielded Pd,ID = 0%
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Truck with Unshielded Multiple Sources
(Co-57, Ba-133, Cs-137)
Vehicle Speed: 20 mph
PCS Results with 4/12 NaI detectors: Pd,ID(Cs-137) = 100%, Pd,ID(Ba-133) =
100%, Pd,ID(Co-57, 4 µCi) = 85% at 20 mph when all sources inside the truck
Note: Standard ASP software using all 12/12 NaI detectors yielded Pd,ID
(Cs-137) = 30%, Pd,ID (Ba-133) = 0%, Pd,ID (Co-57) = 0%
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Conclusions and Next Steps
Demonstrated Pd,ID = 100%, CFAR = 1 in 1000 occupancies at
20 mph
Successfully demonstrated Pd,ID > 90%, CFAR = 1 in 1000
occupancies at 30 mph
Successfully demonstrated isotope identification/discrimination
capability with no reported false alarms or mis-identifications
Demonstrated the ability to detect shielded check sources
Next Steps: Integrate C version of PCS (demonstrated
< 100 msec/spectrum processing time with 28-isotope library)
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