Upload
albania-energy-association
View
277
Download
5
Embed Size (px)
DESCRIPTION
Lecture 6-Radiation Shielding
Citation preview
Chapter 7
Section 2 Shielding
Radiation Shielding
Radiation Shielding Objectives Understand
How radiation is emitted from a source
The difference between fluence and flux
How to calculate flux (& fluence) at a known distance from a point source
Calculate dose at a point in space using a dose conversion factor
Nature of Radiation Emissions When a radionuclide
decays, the radiation goes out from the source in any direction
This is called isotropic emission
We measure the strength of the radiations (intensity) at some distance from the source
Radiation Intensity
The fluence () is the number of photons moving through a target area (/cm2)
The flux () is the number of photons moving through an area per time (/cm2s)
Why Calculate Flux?
Fluence and flux tell you: Photons per area, and Photons per area & time
If you know: Energy per photon
Then, you can calculate Energy deposited per area and, ultimately, dose
Calculating Flux
Need to answer two questions:
What is the source strength S0 (in photons/s) or the total number of disintegrations (D)?
What is the distance, r, from the source (at point P) where you want to calculate the flux?
r
P
Calculating Flux, continued
Consider each photon as it leaves the source
It moves further away from others that have been emitted
Therefore, the flux (/cm2s) decreases
Another Way to Look at It
If a source emits 4 photons/s, what is the flux at 1 cm, 10 cm, and 1m?
Consider the surface area of the sphere(s) the photons are passing through:
Surface Area of a Sphere
S.A.1 cm = 12.57 cm2
S.A.10 cm = 1257 cm2
S.A.100 cm = 125,664 cm2
24.. rAS
1 cm
10 cm
100 cm
Calculating Fluence and Flux, continued
= Fluence /cm2
= Flux /cm2sD = total number of photons emittedS0 = source strength (photons/s)R = distance from source (1, 10, 100 cm)
20
2
4
4
r
S
r
D
Calculating Fluence and Flux, continued
If source emits 4 photons/s, S0 = 4, The (flux) is then calculated:
At 1 cm = 4 /12.57cm2s = 0.318 /cm2s At 10 cm = 4 /1257 cm2s = 3.18 x 10-3 /cm2s
At 100 cm =4 /125,664 cm2s = 3.18 x 10-5 /cm2s
Calculating Fluence and Flux, continued
For this same problem, what is the photon fluence?
Can we calculate it at all? Why? Why not?
Calculating Flux
At any point from the source, the photon intensity (flux) can also be estimated as:
But, what happens if we put some photon absorbing material between the source and our measurement point?
2
0
4 r
S
Attenuation Occurs Remember the “universal” equation (or one
form of it):
This describes how a beam of photons is Reduced in intensity by absorbing material Absorber of thickness x is in the photon path
The source can be said to be “shielded”
xeIxI 0)(
Source Strength From Shielded Source The two equations can be combined to
yield:
The term 1/(4r2) is called the geometeric attenuation factor
xo
x
unshieldedshielded
er
S
ex
24
)(
Converting to a Dose Rate Photon intensity can be
converted to dose rate Called an “uncollided” dose rate Use tables of “dose conversion
factors”:S0 P
rxo
u
xoshielded
er
SEEkD
er
Sx
2
2
4)(
4)(
x
Previous Example, continued
Assume S0 = 4 photons/s Photon energy is 0.8 MeV Shielding material is 0.5 cm Uranium (U)
Calculate the exposure rate at 1, 10, and 100 cm.
Photon Energy Flux to Exposure Dose-rate Conversion Factors
1.56 E-062.0
1.62 E-061.8
1.67 E-061.6
1.73 E-061.4
1.78 E-061.2
1.84 E-061.0
1.87 E-060.9
1.90 E-060.8
1.92 E-060.7
1.94 E-060.6
1.96 E-060.5
Conversion Factor, k(E),
R/hr per MeV/cm2 sEnergy (E) in
MeV
Energy of photon being evaluated
Scientific notation commonly used, should be read as:
1.96 x 10-6
These are “look up” values
Total Linear Attenuation Coefficient Factors, (cm-1)
0.334
0.352
0.372
0.397
0.4285
0.468
0.493
0.523
0.557
0.599
0.652
Fe
(7.86)
0.117
0.123
0.131
0.140
0.151
0.166
0.174
0.184
0.196
0.210
0.227
Al
(2.70)*
0.838
0.889
0.949
1.022
1.114
1.233
1.349
1.492
1.705
1.988
2.490
W
(19.3)
0.298
0.314
0.332
0.354
0.382
0.417
0.445
0.479
0.523
0.578
0.666
Sn
(7.31)
0.510
0.544
0.585
0.635
0.699
0.782
0.866
0.971
1.136
1.361
1.746
Pb
(11.34)
0.8792.0
0.9441.8
1.0231.6
1.1211.4
1.2451.2
1.4101.0
1.5840.9
1.8030.8
2.1440.7
2.6180.6
3.4590.5
U
(18.7)
Energy (E)
in MeV
*Normal density () in g/cm3
Total Linear Attenuation Coefficient Factors, (cm-1), continued
0.152
0.160
0.170
0.181
0.196
0.214
0.227
0.243
0.262
0.286
0.317
Barytes Concrete
(3.50)
0.105
0.111
0.118
0.126
0.136
0.149
0.156
0.165
0.175
0.188
0.204
Ordinary Concrete
(2.35)*
0.202
0.213
0.226
0.241
0.260
0.285
0.299
0.317
0.337
0.363
0.395
Ferrophos. Concrete
(4.68)
0.155
0.163
0.173
0.185
0.200
0.219
0.230
0.243
0.259
0.278
0.303
Magnetite Concrete
(3.55)
0.0494
0.0522
0.0554
0.0594
0.0643
0.0707
0.0743
0.0786
0.0835
0.0895
0.0967
Water (1.0)
5.36E-52.0
5.66E-51.8
6.01E-51.6
6.44E-51.4
6.97E-51.2
7.66E-51.0
8.05E-50.9
8.52E-50.8
9.05E-50.7
9.70E-50.6
1.048E-40.5
Air (0.001205)**
Energy (E)
in MeV
*Normal density () in g/cm3
* * Air at 200C, 760 mm Hg
Calculating Exposure
The uncollided flux previously calculated is: At 1 cm, = 0.318 /cm2s At 10 cm, = 3.18 x 10-3 /cm2s At 100 cm, = 3.18 x 10-5 /cm2s
k(E) = 1.9 x 10-6 R/hr per MeV/cm2 s E= 0.8 MeV e-x is e-1.803*0.5 = 0.41 So, the exposure rate is:
1.98 x 10-7 R/hr at 1 cm; 1.98 x 10-9 R/hr at 10 cm; 1.98 x 10-11 R/hr at 100 cm
xou e
r
SEEkD
24)(
Calculating Flux From Complex Geometries
Point Kernel method Source broken into many
small kernels Contribution from each
kernel evaluated for a common point
Contributions are summed
P
Rule of Thumb #1 Some equations to memorize For estimating dose rate from a
gamma point source where the distance is in feet, and the source strength is in Ci, and the energy of the gamma is expressed in MeV, then:
hr
rad =
ft
Ci E 6.0 D 2
Rule of Thumb #2
For beta radiation, the equation is similar, where the maximum energy of the beta radiation is used.
hr
rad =
ft
Ci E 2 D 2
max
Rules of Thumb, continued
It is important to note that if a nuclide decays by multiple emissions (betas or gammas) that they have to be accounted for in the calculation. You can estimate the dose from each separately and sum the total.