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11
Lecture 5Lecture 5
Overview on the Analytical Procedures Overview on the Analytical Procedures (())
Moncef BenmansourMoncef BenmansourCNESTEN, Rabat MoroccoCNESTEN, Rabat Morocco
IAEA Regional Training Course
Sediment Core Dating Techniques - RAF/7/008 Project
CNESTEN, Rabat, 05-09 July 2010IAEA CNESTE
N
22
ContentsContents
Radionuclides and radiationsRadionuclides and radiations
Basis of Gamma spectrometryBasis of Gamma spectrometry
Hyper Germanium detectorsHyper Germanium detectors
Detection calibrationDetection calibration
Activity calculation, uncertainty, detection limitActivity calculation, uncertainty, detection limit
Correction factorsCorrection factors
Comparative measurements: Comparative measurements: 137137Cs, Cs, 210210Pb, Pb, 226226Ra, Ra, 241241AmAm
33
Radionuclides and RadiationsRadionuclides and Radiations
Natural Radionuclides Natural Radionuclides
– Cosmogenic RadionuclidesCosmogenic Radionuclides
1414C, C, 33H, H, 2222Na, Na, 77Be….Be….
– Primordial Radionuclides (Singly) Primordial Radionuclides (Singly)
4040K, K, 8787Rb, Rb, 5050V, V, 144144Nd...Nd...
– Primordial Radionuclides ( Natural series)Primordial Radionuclides ( Natural series)
238238U, U, 235235U, U, 232232Th seriesTh series
44
SERIE 238U
SERIE 232Th
SERIE 235U
Np
U 238U
4,49E9A 234U 2,48E5a
235U 7,13E8a
Pa 234Pa 1,18m
231Pa 3,25E4a
Th 234Th
24,1j 230Th 7,5E4a
232Th 1,39E10a
228Th 1,9a
231Th 25,6h
227Th 18,6j
Ac 228Ac
6,13h 227Ac
22,0a
Ra 226Ra
1622s 228Ra
6,7a 224Ra
3,64j 223Ra
11,1j
Fr
Rn 222Rn
3,825j 220Rn
54,5s 219Rn
3,92s
At
Po 218Po
3,05m 214Po 1,6E-4s
210Po 138,4j
216Po 0,158s
212Po 3,0E-7s
215Po 1,83E-3s
Bi 214Bi 19,7m
210Bi 5j
212Bi 60,5m
211Bi 2,16m
Pb 214Pb
26,8m 210Pb
21,4a 206Pb STABLE
212Pb 10,6h
208Pb STABLE
211Pb 36,1m
207Pb STABLE
Tl 210Tl
1,3m 206Tl 4,19m
208Tl 3,1m
207Tl 4,79m
55
Radionuclides and RadiationsRadionuclides and Radiations
Man made Man made RadionuclidesRadionuclides
– Fissions ProductsFissions Products
137137Cs, Cs, 9090Sr, Sr, 8989Sr, Sr, 131131I, I, 9999TcTc
– Activation ProductsActivation Products
239239Pu, Pu, 240240Pu, Pu, 241241Pu, Pu, 241241Am, Am, 242242Cm,Cm,
6060Co, Co, 6565Zn, Zn, 5454Mn, Mn, 5555FeFe……
- Nuclear Weapons testing
- Chernobyl Accident
- Discharges from reprocessing
66
Radionuclides and RadiationsRadionuclides and Radiations
Alpha particlesAlpha particles ( () helium) helium
Beta particles (Beta particles ( e- and e e- and e++
Electronic CaptureElectronic Capture
Gamma rays (Gamma rays (): Photons): Photons– 137137Cs, Cs, 210210Pb, Pb, 241241Am,…Am,…
Ee
Eg
77
Gamma-Matter Interaction: Gamma-Matter Interaction: Interaction processusInteraction processus
Photoelectric effect Compton Pair production
lc EEE
e-
)1(1 2
0
20
CmECm
EEc
20
)cos1(1
'
CmE
EE
202 CmEEE ee
2m0C2 = 1,02 MeV
88
Gamma-Matter InteractionGamma-Matter Interaction
Attenuation of Attenuation of
– II(x) = I (0) e(x) = I (0) e--xx
I(0) II(x)(x)
x
Attenuation Attenuation coefficientcoefficient
cmcm-1-1 or cm or cm22/g/g
99
Gamma attenuationGamma attenuation
Lead Aluminium
1010
Gamma spectrometry: General BasisGamma spectrometry: General Basis
Interaction of Interaction of photons with the detectorphotons with the detector Production of electric pulses : Amplitude proportionnel Production of electric pulses : Amplitude proportionnel
to photon energy emitted by the sourceto photon energy emitted by the source Whole information contained in a gamma spectrum Whole information contained in a gamma spectrum
( gamma energy, & activity)( gamma energy, & activity)
1111
Hyperpur Germanium DetectorsHyperpur Germanium Detectors
Semiconductor diodes having a p-i-n structureSemiconductor diodes having a p-i-n structure
Intrinsic (I) region is sensitive to ionizing radiation, Intrinsic (I) region is sensitive to ionizing radiation, particularly x rays and particularly x rays and rays rays
Under reverse bias, an electric field extends across Under reverse bias, an electric field extends across the intrinsic or depleted region.the intrinsic or depleted region.
When photons interact with the material charge When photons interact with the material charge
carriers (holes and electrons) are produced and are carriers (holes and electrons) are produced and are
swept by the electric field to the p and n electrodes.swept by the electric field to the p and n electrodes.
1212
Hyperpur Germanium DetectorsHyperpur Germanium DetectorsRelative efficiency, energy resolution, energy range, peak/compton ratio
1313
Hyperpur Germanium DetectorsHyperpur Germanium Detectors
Detector
Preamplifier Amplifier ADC
Multiplexer
High voltage supply
MCA
NIM Module (low voltage)
rays
Detector
Preamplifier Amplifier ADC
Multiplexer
High voltage supply
MCA
NIM Module (low voltage)
rays
1414
Electronic parmetersElectronic parmeters
Power Supply: H.VPower Supply: H.V
Amplifier Amplifier – Gain : Coarse and FineGain : Coarse and Fine– Shaping timeShaping time– Zero poleZero pole
Parameters of MCAParameters of MCA
1515
Hyperpur Germanium DetectorsHyperpur Germanium Detectors
1616
Energy CalibrationEnergy Calibration
Energy – Canal RelationEnergy – Canal Relation
– Two sources ( Two sources ( 137137Cs, Cs, 6060Co)Co)
– Multi-gamma sources Multi-gamma sources
661 keV 1173 keV
1332 keV
1836 keV
1717
Energy CalibrationEnergy Calibration
1818
Efficiency calibrationEfficiency calibration
Full – energy –peak efficiency: Full – energy –peak efficiency: (E)(E)
(E) (E) == N(E) N(E) /R/R– N (E): count rate in the peak corresponding to the N (E): count rate in the peak corresponding to the
Energy Energy EE– R: rate at which photons of Energy R: rate at which photons of Energy EE are emitted from are emitted from
the sourcethe source
R R = A.I= A.I– A :Source ActivityA :Source Activity
– II: : Gamma ( Gamma ( ) ray emission probability ) ray emission probability
1919
Efficiency calibrationEfficiency calibration
(E) (E) depends on: depends on: – Source dimension and source –detector distanceSource dimension and source –detector distance
– Dimensions of the detector housing and of the sensitive and Dimensions of the detector housing and of the sensitive and insensitive zones of the detectorinsensitive zones of the detector
– Elementary composition and density of all materials Elementary composition and density of all materials traversed by the photonstraversed by the photons
– Photon attenuation coefficients of these materialsPhoton attenuation coefficients of these materials
– Energy-and angle-dependent cross sections of the detector Energy-and angle-dependent cross sections of the detector material for the various photon interactionsmaterial for the various photon interactions
– Information on the electron and positron transport in the Information on the electron and positron transport in the detectorsdetectors
2020
Efficiency calibrationEfficiency calibration
Efficiency calculationEfficiency calculation– Monte Carlo codes, but many constraintsMonte Carlo codes, but many constraints
Uncertainties in the shape and size of the effective or Uncertainties in the shape and size of the effective or sensitive crystal volumesensitive crystal volume
Uncertainties on the photons and electron interaction Uncertainties on the photons and electron interaction probaility and angular distributionsprobaility and angular distributions
Efficiency measurementsEfficiency measurements– Calibration sources: easier and more accurate than Calibration sources: easier and more accurate than
calculation calculation
– (E) VS Energy (keV)(E) VS Energy (keV)
2121
Standard sourcesStandard sources
Liquid multi-gamma sources with certified Liquid multi-gamma sources with certified activities purchased from an international activities purchased from an international providerprovider
Different Marked matrixes prepared by the Different Marked matrixes prepared by the supplier in different geometries supplier in different geometries
Reference Materials: (e.g.. IAEA) Reference Materials: (e.g.. IAEA)
2222
Standard SourcesStandard Sources
Radionucléide Energie (keV) Nombre de
photons pour 100 désintégrations
Activité massique (Bq/g)
Periode ( j )
Am-241 59.537 0.001 35.9 0.4 2000 3 157935.5 296 Cd-109 88.034 0.002 3.65 0.06 9830 3.7 462.6 0.4 Co-57 122.061 0.001 85.68 0.13 463 3 271.77 0.10 Co-57 136.4740.001 10.67 0.13 463 3 271.77 0.10 Ce-139 165.8570.006 79.87 0.06 473 3 137.640 0.023 Cr-51 320.0840.001 9.85 0.09 14800 3 27.703 0.004
Sn-113 391.7020.004 64.89 0.17 2810 3.4 115.08 0.03 Sr-85 514.0090.012 99.29 0.04 1760 3 64.850 0.007
Cs-137 661.6600.003 85.2 0.2 2980 3 11004.75 7.3 Y-88 898.0420.004 94.1 0.5 2770 3 106.62 0.02 Co-60 1173.2380.004 99.89 0.02 2990 3 1923.915 0.365 Co-60 1332.5020.005 99.983 0.001 2990 3 1923.915 0.365 Y-88 1836.0640.013 99.36 0.05 2770 3 106.62 0.02
2323
Efficiency CurvesEfficiency CurvesHPGe, coaxial – P Type: Rel. Eff.30%HPGe, coaxial – P Type: Rel. Eff.30%
0
1
2
3
4
5
6
7
8
0 200 400 600 800 1000 1200 1400 1600 1800 2000
Energy (keV)
Eff
icie
ncy
(%
)
Cyl-20 ml
Cyl-200 ml
Mar-0,5 l
Mar-1,5 l
2424
Efficiency Curves Efficiency Curves P-type and N- type detectorsP-type and N- type detectors
0
1
2
3
4
5
6
7
0 200 400 600 800 1000 1200 1400
Energy (keV)
Eff
icie
ncy
(%
)
P-Type 30%
N-Type 45%
2525
Efficiency fittingEfficiency fitting
-6
-5
-4
-3
-2
-1
0
3 4 5 6 7 8
LN(E)
LN
(Eff
.)
0,001
0,01
0,1
1
10 100 1000 10000
Energy (keV)
Effic
ienc
y (%
)
n
j
jj EEa
00 )/(loglog
2626
Spectral EvaluationSpectral Evaluation
2727
a1, a2, b1 b2
N = Nt - Nb
2828
Spectral EvaluationSpectral Evaluation
Automatic peak search Evaluation of the peak positions in energy Identification of radionuclides by the use of a nuclide library Efficiency-calibration curve Calculation of the net peak area Calculation of activity concentrations in selected units Calculation of the detection limits for specific nuclides
Nt =
1
2
b
aiiN
Nb= ( )2
1
2
1 1
1
b
bii
a
aii NN
)(
)1(
1212
21
bbaa
ab
N = Nt - Nb
where: N = net count or net peak area Nb = background count Ni = counts in the channel i Nt = total counts
a1, a2,b1 and b2 = the number of the respective channel.
2929
Calcul of activityCalcul of activity
.)1(
0
ctcc
tc
eMtIF
etNA
At = activity or concentration of Radionculide in Bq kg-1 at the sampling date N = net peak area = decay constant (Ln2/T1/2), T1/2 for 137Cs is 30.17 year tc = counting time t0 = time difference between sampling and starting the measurement M = masse of the soil sample (kg) = absolute efficiency emission probability Fc =Correction factor
.0
cc
t
MtIF
NeA
General Case General Case If tc << T1/2 If tc << T1/2
3030
Calcul of activityCalcul of activity: Areal activity: Areal activity
S
CMA t
s C = activity of the sub-sample of the whole core (Bq kg-1)
Mt = total mass of the whole core (kg) S = corer area (m2)
i
iTs CMS
Ai
1 iTM Ci = activity of the i th sub-sample (Bq kg-1)
iTM = total mass of the i th (kg)
S = corer area (m2)
iiis HCA Ci = activity of the i th sub-sample (Bq kg-1) bulk density of the i th sub-sample (kg m-3) Hi = depth of the i th sub-sample (m)
3131
UncertaintiesUncertainties
.0
cc
t
MtIF
NeA
A/A)2 = (N/N)2 + ()2 + (I(Fc Fc
)/()(/ btbt NNNNNN
3232
UncertaintiesUncertainties
IAEA TECDOC 1401
3333
BackroundBackround
(i) Internal background
Natural radioactivity (238U, 235U, 232Th series and 40K) coming from the material used to build the detector
Natural radioactivity coming from the auxiliary equipments and shielding
(ii) External background
Natural radioactivity coming from surrounding environment; earth surface, walls, floor, etc.
Radiations coming from 222Rn (gas) daughters Cosmic rays
3434
Detection LimitDetection Limit
The detection limit is a term which expresses the detection capabilities of measurement system under certain conditions. A general accepted expression of the lower limit of detection (LLD) which contains a pre selected risk of 5% of concluding falsely that activity is present and a 95 % degree of confidence for detecting the presence of activity, is calculated as follows:
TI
BLLD
66.4
B = background count rate (counts/s) = absolute efficiency emission probability T = counting time
3535
Detection LimitDetection Limit
When introducing mass (kg) of the sample, the minimum detectable concentration (MDC) also termed Minimum Detection Activity (MDA) in Bq kg-1 can be expressed as:
TMI
BMDC
66.4
3636
Correction factorsCorrection factors
Factor corrections (Fc)Factor corrections (Fc)
– Coïncidence –summing corrections ( two or more Coïncidence –summing corrections ( two or more photons within the resolving time of the photons within the resolving time of the spectrometer). spectrometer).
– Dead –time and pil-up correctionsDead –time and pil-up corrections
– Attenuation correction: self-absorption Attenuation correction: self-absorption attenuationattenuation
3737
Coïncidence –summing corrections Coïncidence –summing corrections (eg. two Radionuclides )(eg. two Radionuclides )
– NN1 1 = A I= A I11 ( 1 – ( 1 – 1212))
– CC1 1 = 1/(1- = 1/(1- 1212))
– NN22 = AI = AI2 2 22 [1 – (I [1 – (I11/I/I22) ) 1212]]
– CC2 2 = 1 / [1—(I = 1 / [1—(I1 1 /I/I22) ) 1212]]
– NN33 = AI = AI3 3 ] ]
– CC3 3 = 1/[1+I= 1/[1+I11 /(I/(I3333))
1
3
E3 (I3) E1(I1)
E2 (I2)
3838
Dead time and pile-up correctionDead time and pile-up correction
MCA : Real and live timeMCA : Real and live time Pile - up correction rejector Pile - up correction rejector Pulser method:Pulser method:
– NN00 = N f t/N = N f t/Npp NN et Net N00: measured and true number of counts in the : measured and true number of counts in the
peak respectivelypeak respectively NNp: p: number of counts in the pulser peaknumber of counts in the pulser peak F: frequency of the pulserF: frequency of the pulser T: Counting timeT: Counting time
3939
Attenuation correctionAttenuation correction
Attnuation law: Attnuation law: II(x) = I (0) e(x) = I (0) e--dd– : masse attenuation coefficient: masse attenuation coefficient– d : tickness of the sample d : tickness of the sample – : density of the ample: density of the ample
Self-attenuation Facteur: Self-attenuation Facteur: – F (F (dd)= [1-exp(-)= [1-exp(-dd)]/ )]/ dd
Correction Facteur Correction Facteur – CCa a = F (= F (dd))sample sample //F(F(dd))standardstandard
– (E > 100 keV): (E > 100 keV): CCa a depends exclusively on the sample depends exclusively on the sample densitydensity
– (E <100 keV): (E <100 keV): CCa a depends also on the chemical composition depends also on the chemical composition
4040
Attenuation correctionAttenuation correction
Boshkova and Minev , ARI 54 (2001) 777-783
4141
Attenuation correctionAttenuation correction
Can be determinedCan be determined
– Using analytical methodsUsing analytical methods– Using the Monte-Carlo Computation Using the Monte-Carlo Computation
techniquestechniques– ExperimentallyExperimentally
4242
Attenuation correction: Attenuation correction: ExperimentallyExperimentally
Point Source on the top of Point Source on the top of containers:containers:– with unknown sample, standard, with unknown sample, standard,
and airand air
)/(1
)/ln(
0
0, II
IIF
s
ssatt
)/(1
)/ln(
0
0, II
IIF
st
ststatt
statt
sattatt F
FF
,
,
statts F
Cutshall et al., NIM PR A 206 (1983) 309-312
4343
Comparative Comparative measurementsmeasurements
137137Cs, Cs, 210210Pb, Pb, 226226Ra, Ra, 241241AmAm
4444
137137CsCs
4545
210210PbPb
4646
241241AmAm
4747
226226RaRa
4848
Comparison Comparison
Radionuclide
137Cs
210Pb
226Ra
241Am
T1/2 (ans) 30.17 22.3 1600 432 rays (keV) 661.66 46.52 186.21 and of
daughters 59.54
I 85.5 4.05 3.28 35.90
HPGe - Coaxial - BeGe, REGe
- BeGe, REGe - LEGe
- Coaxial - BeGe, REGe
- BeGe, REGe -LEGe - Coaxial
Précautions
- low activity & overlapping with 665 keV of 214Bi
- self absorption correction - Background
-self absorption correction - interference with 235U - Background - 222Rn variation
- self absorption correction
4949
137137Cs & Cs & 210210PbPbSelf-absorptionSelf-absorption
0
2
4
6
8
10
12
0.9 1.1 1.3 1.5
Density(g/cm3)
Eff
icie
ncy
(%
)
46.5 keV
662 keV
Sediment Samples (100 m)
HPGe 45% -N Type -
5050
ConclusionConclusion
Gamma spectrometry: Gamma spectrometry: Direct technique, without Direct technique, without radiochemical separation, but requires some radiochemical separation, but requires some precautions:precautions:
– Selection of suitable HPGe detectorsSelection of suitable HPGe detectors– Selection of suitable standardsSelection of suitable standards– Sample preparation and geometry of countingSample preparation and geometry of counting– Efficiency curveEfficiency curve– BackgroundBackground– FF actor effectsactor effects– All sources of uncertaintyAll sources of uncertainty– Quality Control ProgrammeQuality Control Programme