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Radiation Shielding
Chapter 7
Section 2 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 (Φ) is the
number of photons
moving through a target
area (γ/cm2)
The flux (φ) is the
number of photons
moving through an area
per time (γ/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 (γ/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. = 4 π r

2

S.A.1 cm = 12.57 cm2
1 cm
10 cm

100 cm

S.A.10 cm = 1257 cm2
S.A.100 cm = 125,664 cm2
Calculating Fluence and Flux,
continued
D
Φ=
4π r 2
S0
φ=
4π r 2
Φ = Fluence γ/cm2
φ = Flux γ/cm2s
D = total number of photons emitted
S0 = source strength (photons/s)
R = distance from source (1, 10, 100 cm)
Calculating Fluence and Flux,
continued
If source emits 4 photons/s, S0 = 4,
The φ (flux) is then calculated:
At 1 cm
= 4 γ /12.57cm2s
φ = 0.318 γ/cm2s
At 10 cm
φ = 4 γ /1257 cm2s
φ = 3.18 x 10-3 γ/cm2s
φ

At 100 cm
=4 γ /125,664 cm2s
φ = 3.18 x 10-5 γ/cm2s
φ
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:

S0
φ=
2
4π r
But, what happens if we put some photon absorbing
material between the source and our measurement
point?
Attenuation Occurs
Remember the “universal” equation (or one
form of it):
−µ x
0

I ( x) = I e

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”
Source Strength From
Shielded Source
The two equations can be combined to
yield:

φ ( x) shielded = φ unshielded e
So −µ x
=
e
2
4π r

−µ x

The term 1/(4πr2) is called the
geometeric attenuation factor
Converting to a Dose Rate

S0

P

Photon intensity can be
converted to dose rate
Called an “uncollided” dose
rate
Use tables of “dose
conversion factors”:

φ ( x) shielded
x
r

So −µ x
=
e
2
4π r

 = k ( E ) E So e−µ x
Du
2
4π r
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 Doserate Conversion Factors
Energy of
photon being
evaluated

Energy (E) in
MeV

Conversion Factor,
k(E),
R/hr per MeV/cm2 s

0.5

1.96 E-06

0.6

1.94 E-06

0.7

1.92 E-06

0.8

1.90 E-06

0.9

1.87 E-06

1.0

1.84 E-06

1.2

1.78 E-06

1.4

1.73 E-06

1.6

1.67 E-06

1.8

1.62 E-06

2.0

1.56 E-06

Scientific
notation
commonly
used, should be
read as:
1.96 x 10-6
These are
“look up”
values
Total Linear Attenuation Coefficient
Factors, µ (cm-1)
Energy (E)
in MeV

Al
(2.70)*

Fe
(7.86)

Sn
(7.31)

W
(19.3)

Pb
(11.34)

U
(18.7)

0.5

0.227

0.652

0.666

2.490

1.746

3.459

0.6

0.210

0.599

0.578

1.988

1.361

2.618

0.7

0.196

0.557

0.523

1.705

1.136

2.144

0.8

0.184

0.523

0.479

1.492

0.971

1.803

0.9

0.174

0.493

0.445

1.349

0.866

1.584

1.0

0.166

0.468

0.417

1.233

0.782

1.410

1.2

0.151

0.4285

0.382

1.114

0.699

1.245

1.4

0.140

0.397

0.354

1.022

0.635

1.121

1.6

0.131

0.372

0.332

0.949

0.585

1.023

1.8

0.123

0.352

0.314

0.889

0.544

0.944

2.0

0.117

0.334

0.298

0.838

0.510

0.879

*

Normal density (ρ) in g/cm3

µ
Total Linear Attenuation Coefficient
Factors, µ (cm-1), continued
Energy (E)
in MeV

Ordinary
Concrete
(2.35)*

Barytes
Concrete
(3.50)

Magnetite
Concrete
(3.55)

Ferrophos.
Concrete
(4.68)

Water
(1.0)

Air
(0.001205)**

0.5

0.204

0.317

0.303

0.395

0.0967

1.048E-4

0.6

0.188

0.286

0.278

0.363

0.0895

9.70E-5

0.7

0.175

0.262

0.259

0.337

0.0835

9.05E-5

0.8

0.165

0.243

0.243

0.317

0.0786

8.52E-5

0.9

0.156

0.227

0.230

0.299

0.0743

8.05E-5

1.0

0.149

0.214

0.219

0.285

0.0707

7.66E-5

1.2

0.136

0.196

0.200

0.260

0.0643

6.97E-5

1.4

0.126

0.181

0.185

0.241

0.0594

6.44E-5

1.6

0.118

0.170

0.173

0.226

0.0554

6.01E-5

1.8

0.111

0.160

0.163

0.213

0.0522

5.66E-5

2.0

0.105

0.152

0.155

0.202

0.0494

5.36E-5

Normal density (ρ) in g/cm3
**
Air at 200C, 760 mm Hg
*

Du = k ( E ) E

So
4π r

2

e

−µ x

Calculating
Exposure

The uncollided flux previously calculated is:
At 1 cm, φ = 0.318 γ/cm2s
At 10 cm, φ = 3.18 x 10-3 γ/cm2s
At 100 cm, φ = 3.18 x 10-5 γ/cm2s

k(E) = 1.9 x 10-6 R/hr per MeV/cm2 s
E= 0.8 MeV
e-µx 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
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:

6.0 Eγ Ci rad

=
Dγ ≈
2
hr
ft
Rule of Thumb #2
For beta radiation, the equation is
similar, where the maximum
energy of the beta radiation is
used.

2 E max Ci rad

=
Dβ ≈
2
hr
ft
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.

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Lecture 6-Radiation Shielding

  • 2. 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
  • 3. 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
  • 4. Radiation Intensity The fluence (Φ) is the number of photons moving through a target area (γ/cm2) The flux (φ) is the number of photons moving through an area per time (γ/cm2s)
  • 5. 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
  • 6. 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
  • 7. Calculating Flux, continued Consider each photon as it leaves the source It moves further away from others that have been emitted Therefore, the flux (γ/cm2s) decreases
  • 8. 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:
  • 9. Surface Area of a Sphere S . A. = 4 π r 2 S.A.1 cm = 12.57 cm2 1 cm 10 cm 100 cm S.A.10 cm = 1257 cm2 S.A.100 cm = 125,664 cm2
  • 10. Calculating Fluence and Flux, continued D Φ= 4π r 2 S0 φ= 4π r 2 Φ = Fluence γ/cm2 φ = Flux γ/cm2s D = total number of photons emitted S0 = source strength (photons/s) R = distance from source (1, 10, 100 cm)
  • 11. Calculating Fluence and Flux, continued If source emits 4 photons/s, S0 = 4, The φ (flux) is then calculated: At 1 cm = 4 γ /12.57cm2s φ = 0.318 γ/cm2s At 10 cm φ = 4 γ /1257 cm2s φ = 3.18 x 10-3 γ/cm2s φ At 100 cm =4 γ /125,664 cm2s φ = 3.18 x 10-5 γ/cm2s φ
  • 12. Calculating Fluence and Flux, continued For this same problem, what is the photon fluence? Can we calculate it at all? Why? Why not?
  • 13. Calculating Flux At any point from the source, the photon intensity (flux) can also be estimated as: S0 φ= 2 4π r But, what happens if we put some photon absorbing material between the source and our measurement point?
  • 14. Attenuation Occurs Remember the “universal” equation (or one form of it): −µ x 0 I ( x) = I e 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”
  • 15. Source Strength From Shielded Source The two equations can be combined to yield: φ ( x) shielded = φ unshielded e So −µ x = e 2 4π r −µ x The term 1/(4πr2) is called the geometeric attenuation factor
  • 16. Converting to a Dose Rate S0 P Photon intensity can be converted to dose rate Called an “uncollided” dose rate Use tables of “dose conversion factors”: φ ( x) shielded x r So −µ x = e 2 4π r  = k ( E ) E So e−µ x Du 2 4π r
  • 17. 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.
  • 18. Photon Energy Flux to Exposure Doserate Conversion Factors Energy of photon being evaluated Energy (E) in MeV Conversion Factor, k(E), R/hr per MeV/cm2 s 0.5 1.96 E-06 0.6 1.94 E-06 0.7 1.92 E-06 0.8 1.90 E-06 0.9 1.87 E-06 1.0 1.84 E-06 1.2 1.78 E-06 1.4 1.73 E-06 1.6 1.67 E-06 1.8 1.62 E-06 2.0 1.56 E-06 Scientific notation commonly used, should be read as: 1.96 x 10-6 These are “look up” values
  • 19. Total Linear Attenuation Coefficient Factors, µ (cm-1) Energy (E) in MeV Al (2.70)* Fe (7.86) Sn (7.31) W (19.3) Pb (11.34) U (18.7) 0.5 0.227 0.652 0.666 2.490 1.746 3.459 0.6 0.210 0.599 0.578 1.988 1.361 2.618 0.7 0.196 0.557 0.523 1.705 1.136 2.144 0.8 0.184 0.523 0.479 1.492 0.971 1.803 0.9 0.174 0.493 0.445 1.349 0.866 1.584 1.0 0.166 0.468 0.417 1.233 0.782 1.410 1.2 0.151 0.4285 0.382 1.114 0.699 1.245 1.4 0.140 0.397 0.354 1.022 0.635 1.121 1.6 0.131 0.372 0.332 0.949 0.585 1.023 1.8 0.123 0.352 0.314 0.889 0.544 0.944 2.0 0.117 0.334 0.298 0.838 0.510 0.879 * Normal density (ρ) in g/cm3 µ
  • 20. Total Linear Attenuation Coefficient Factors, µ (cm-1), continued Energy (E) in MeV Ordinary Concrete (2.35)* Barytes Concrete (3.50) Magnetite Concrete (3.55) Ferrophos. Concrete (4.68) Water (1.0) Air (0.001205)** 0.5 0.204 0.317 0.303 0.395 0.0967 1.048E-4 0.6 0.188 0.286 0.278 0.363 0.0895 9.70E-5 0.7 0.175 0.262 0.259 0.337 0.0835 9.05E-5 0.8 0.165 0.243 0.243 0.317 0.0786 8.52E-5 0.9 0.156 0.227 0.230 0.299 0.0743 8.05E-5 1.0 0.149 0.214 0.219 0.285 0.0707 7.66E-5 1.2 0.136 0.196 0.200 0.260 0.0643 6.97E-5 1.4 0.126 0.181 0.185 0.241 0.0594 6.44E-5 1.6 0.118 0.170 0.173 0.226 0.0554 6.01E-5 1.8 0.111 0.160 0.163 0.213 0.0522 5.66E-5 2.0 0.105 0.152 0.155 0.202 0.0494 5.36E-5 Normal density (ρ) in g/cm3 ** Air at 200C, 760 mm Hg *
  • 21.  Du = k ( E ) E So 4π r 2 e −µ x Calculating Exposure The uncollided flux previously calculated is: At 1 cm, φ = 0.318 γ/cm2s At 10 cm, φ = 3.18 x 10-3 γ/cm2s At 100 cm, φ = 3.18 x 10-5 γ/cm2s k(E) = 1.9 x 10-6 R/hr per MeV/cm2 s E= 0.8 MeV e-µx 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
  • 22. 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
  • 23. 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: 6.0 Eγ Ci rad  = Dγ ≈ 2 hr ft
  • 24. Rule of Thumb #2 For beta radiation, the equation is similar, where the maximum energy of the beta radiation is used. 2 E max Ci rad  = Dβ ≈ 2 hr ft
  • 25. 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.