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Varian Linatron High-Energy X-ray Applications 2007

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<strong>Varian</strong> <strong>Linatron</strong> <strong>High</strong>-<strong>Energy</strong> X-<strong>ray</strong> <strong>Applications</strong><br />

<strong>2007</strong>


Table of Contents<br />

Page<br />

I Introduction 3<br />

II Characteristics of <strong>High</strong>-<strong>Energy</strong> Radiation 5<br />

Advantages of <strong>High</strong>-<strong>Energy</strong> X-<strong>ray</strong>s 5<br />

Generation of <strong>High</strong>-<strong>Energy</strong> X-<strong>ray</strong>s 5<br />

Measurement of <strong>High</strong>-<strong>Energy</strong> X-<strong>ray</strong>s 5<br />

Target Characteristics 5<br />

Radiation Absorption and Scattering in the Object 6<br />

Half-Value Layer and <strong>Energy</strong> Selection 7<br />

Half-Value Thickness versus <strong>Energy</strong> Spectrum 8<br />

III <strong>Linatron</strong> Radiographic Characteristics 9<br />

General Description 9<br />

X-<strong>ray</strong> Quality 9<br />

Field Coverage, Beaming, and Field Flatness 9<br />

• Field Coverage<br />

• Beaming and Field Flatness<br />

IV Theory, Variables, and Practices in<br />

<strong>Linatron</strong> Radiography 13<br />

Radiographic Setup 13<br />

• Collimation<br />

• Source-to-Film Distance<br />

• Object Placement and Image Formation<br />

• D/T Ratio, Magnification, and Image Sharpness<br />

• Reducing Scattered Radiation<br />

• Blocking<br />

• Lead Intensifying Screens as Filters<br />

• Filters<br />

• Film Holders<br />

Intensifying Screens 16<br />

• Metal Foil Screens<br />

• Metal-Phosphor Screens<br />

X-Ray Film Characteristics 18<br />

• Film Properties and Classification<br />

• Speed<br />

• Contrast and the Film Characteristic Curve<br />

• Multifilm Techniques<br />

Definition and Unsharpness 22<br />

Sensitivity and Image Quality 24<br />

• Thickness Sensitivity<br />

• Wire Penetrameter Sensitivity<br />

• Drilled Hole Plaque Penetrameter Sensitivity<br />

• Radiographic Sensitivity<br />

Exposure Curves 25<br />

• Method for Generating Exposure Curves<br />

• Latitude<br />

• Exposure Times and Material Densities<br />

• Using Film Response Curves to Generate<br />

New Exposure Curves<br />

• Increasing Latitude with Multiple Film Use<br />

Page<br />

V Radiographic Procedures 40<br />

General Considerations 40<br />

• Records and Logs<br />

• Exposure Room Equipment<br />

Castings Radiography 41<br />

• Radiographic Coverage<br />

• Layout and Marking<br />

• Casting Radiographic Procedures<br />

- Radiography of Flanges<br />

- Radiography of Valve Bodies<br />

Radiography of Welds 44<br />

• Radiographic Coverage<br />

- Circumferential Butt Welds<br />

- T-Sections<br />

• Design and Placement of Image Quality Indicators<br />

• Defect Location<br />

Radiography of Rocket Motors 47<br />

• Motor Attitude and Support Equipment<br />

• Rocket Motor Radiographic Procedures<br />

• Grain Radiography Coverage Requirements<br />

• Tangential Radiography<br />

• Tangential Radiography Coverage Requirements<br />

Assembly Radiography 51<br />

VI Bibliography 52<br />

VII <strong>High</strong>-<strong>Energy</strong> Real-Time Radiographic Imaging 53<br />

VIII Glossary 59


Preface<br />

This manual presents theory, principles, and practical<br />

application of radiography. It is intended to provide<br />

general guidance only in performing radiography with a<br />

<strong>Linatron</strong> system. It is not intended to supersede or preempt<br />

the requirements of applicable inspection procedures,<br />

specifications, standards, safety procedures, or regulations.<br />

Where statements in this manual conflict with local, state,<br />

national or international regulations, the regulations must<br />

take precedence.<br />

Although this document is intended primarily for <strong>Linatron</strong><br />

users, the principles of high-energy radiography presented<br />

here are generally applicable to other high-energy X-<strong>ray</strong><br />

equipment. Not all questions concerning <strong>Linatron</strong><br />

applications can be covered here. Any specific questions<br />

may be directed to <strong>Varian</strong> Security and Inspection Products<br />

(SIP) representatives. A list of <strong>Varian</strong> offices is given on<br />

the back cover.<br />

page 1<br />

The principle objectives of this manual are to<br />

provide:<br />

1) <strong>Applications</strong> information for prospective<br />

industrial radiographic uses of a <strong>Linatron</strong><br />

2) Technical information concerning <strong>Linatron</strong><br />

radiography not readily available elsewhere.<br />

Conventions and Terminology<br />

This manual uses the convention of designating an X-<strong>ray</strong><br />

energy distribution as MeV or KeV, i.e., 2 MeV designates<br />

a distribution of X-<strong>ray</strong> energies up to 2 MeV.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Introduction<br />

X-<strong>ray</strong>s are a type of electromagnetic energy that occupies a<br />

particular place in the electromagnetic spectrum. What we<br />

refer to as X-<strong>ray</strong>s is a type of energy that can be understood<br />

as both particles and waves because they have characteristics<br />

of both. Photons are the particle aspect of X-<strong>ray</strong>s, which<br />

are mass-less and travel at the speed of light. These are<br />

produced by <strong>Linatron</strong>s when high energy electrons are<br />

accelerated and strike a high density metal target. This<br />

releases photons in the X-<strong>ray</strong> frequency band as shown in<br />

Fig. 1-1.<br />

FIGURE 1-1. Spectrum<br />

Nondestructive testing using high energy (greater than 1<br />

MeV) radiographic techniques has been in use for more<br />

than 60 years. During this period, a number of highenergy<br />

X-<strong>ray</strong> sources have been developed for the detection<br />

of flaws in heavy metal sections. More recently, these x-<strong>ray</strong><br />

sources have found important uses in cargo screening and<br />

related security inspections applications. Please consult<br />

other <strong>Varian</strong> documentation for information on cargo<br />

screening applications.<br />

The first commercial high-energy X-<strong>ray</strong> source was the 1<br />

MeV resonant transformer, introduced by General Electric<br />

in 1939. A few years later there appeared 2 MeV versions<br />

of the resonant transformer, Van de Graaff generators with<br />

energies of 1 MeV and 2 MeV, and Betatrons with electron<br />

beam energies ranging from 15 MeV to 25 MeV.<br />

page 3<br />

The maximum X-<strong>ray</strong> output of these early machines was<br />

limited. Electron linear accelerators, which became available<br />

commercially about 1956, offered a way to substantially<br />

increase the X-<strong>ray</strong> output and made practical the<br />

radiography of steel sections greater than 2 feet thick. This<br />

met the need of modern nuclear technology which required<br />

radiographic examination of assemblies containing relatively<br />

thick sections of very dense material, such as uranium and<br />

tungsten alloys. Linear accelerators proved capable of<br />

penetrating and recording flaws or other anomalies on x-<strong>ray</strong><br />

film through many inches of such materials.<br />

<strong>Varian</strong> SIP (Security and Inspection Products) first<br />

extended its linear accelerator technology into the highenergy<br />

radiography field in December 1959 with the<br />

delivery to the U.S. Navy of a 10 MeV machine designed<br />

to produce high-quality radiographs of the Polaris missile<br />

and other solid rocket motors. In the years that followed,<br />

<strong>Varian</strong> SIP continued to supply similar machines to<br />

government and industrial customers.<br />

In 1968, <strong>Varian</strong> SIP introduced the <strong>Linatron</strong>®, a line of<br />

industrial linear accelerators with energy ranges from 1 to<br />

15 MeV. The <strong>Linatron</strong> represented a significant advance<br />

in reliability and ease of operation and handling. A typical<br />

<strong>Linatron</strong> installation includes an X-<strong>ray</strong> head (Figs. 1-2 and<br />

FIGURE 1-2. <strong>Linatron</strong> M9 X-<strong>ray</strong> head.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 1-3. <strong>Linatron</strong> M System Diagram<br />

1-3), a Control Console (Fig. 1-4), a modulator cabinet<br />

(Fig. 1-5). Among the more important characteristics of<br />

the <strong>Linatron</strong>s are:<br />

• Small focal spot size<br />

• Appropriate energy selection for the material to be<br />

radiographed<br />

• Ease of handling and beam positioning<br />

• <strong>High</strong> radiation output<br />

• <strong>High</strong> reliability<br />

• Low maintenance cost<br />

FIGURE 1-4. The standard operator interface to the <strong>Linatron</strong> is a<br />

Touchscreen Control Console.<br />

page 4<br />

FIGURE 1-5. <strong>Linatron</strong> modulator cabinet contains main power<br />

supplies, pulse modulator, and power distribution electronics.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Characteristics of <strong>High</strong>-<strong>Energy</strong> Radiation<br />

Advantages of <strong>High</strong>-<strong>Energy</strong> X-Rays<br />

The high energy x-<strong>ray</strong>s produced by <strong>Linatron</strong>s provide a<br />

number of advantages over traditional x-<strong>ray</strong> radiography.<br />

These include:<br />

• Making the radiography of very thick sections<br />

economically feasible.<br />

• Making it possible to achieve large source-toobject/object-to-film<br />

distance (D/T) ratios to<br />

minimize object distortion.<br />

• Allowing short exposure times for high<br />

throughput rates.<br />

• Combining high film latitude with reduced<br />

scatter allowing high detail resolution in<br />

radiographs of large complex assemblies.<br />

• Making it possible to use slower fine-grained X<strong>ray</strong><br />

film and real time radiography systems.<br />

Generation of <strong>High</strong> <strong>Energy</strong> X-Rays<br />

Electrons are injected at moderately high energies into a<br />

tuned resonant waveguide structure and accelerated<br />

toward a target by high electric fields. When these<br />

electrons strike the target, they rapidly decelerate. This<br />

deceleration creates high-energy bremsstrahlung X-<strong>ray</strong><br />

spectrum. The spectrum is characteristic of the target<br />

material, the target design, and the energy spectrum of<br />

the incident electron beam. The same process takes place<br />

in conventional X-<strong>ray</strong> equipment, but the higher energy<br />

<strong>Linatron</strong> electron beam produces a higher efficiency<br />

conversion of electrons into X-<strong>ray</strong>s.<br />

Measurement of <strong>High</strong> <strong>Energy</strong> X-Rays<br />

The “Roentgen” is the standard unit of measure for x-<strong>ray</strong>s,<br />

which quantifies exposure to a source of ionizing radiation.<br />

“Exposure”* is fundamentally a property of the beam<br />

rather than a measure of the effect of the beam on the<br />

object to be irradiated. The basic quantity that<br />

characterizes the energy imparted to matter by ionizing<br />

particles is the absorbed dose. The unit of absorbed dose is<br />

page 5<br />

the G<strong>ray</strong>, often abbreviated “Gy”**. Gy is defined as the<br />

amount of energy imparted to matter per unit mass of<br />

irradiated material and is equal to 1 joule per kilogram.<br />

In practice, the radiation output of a <strong>Linatron</strong> is measured<br />

by first measuring exposure, the charge produced by the x<strong>ray</strong><br />

beam in a given volume of air using an ionization<br />

chamber dosimeter. Correction factors are then used to<br />

calculate the absorbed dose in a material. Ion chamber<br />

measurements are normally made at a given depth in a<br />

water phantom or with the ion chamber surrounded by a<br />

plastic cylinder or equilibrium cap in order to achieve<br />

electronic equilibrium. For low-atomic-number materials,<br />

a Roentgen measured in air is approximately equivalent to<br />

one rad of absorbed dose. <strong>Linatron</strong> outputs are described<br />

in units of Gy per minute at one meter.<br />

*The term “exposure” is used primarily to describe the fact that<br />

film has received X-<strong>ray</strong> radiation during radiography of an<br />

object under test in subsequent sections of this manual.<br />

Exposure refers to the effect of the X-<strong>ray</strong> beam on the film in<br />

this context.<br />

**This manual uses Gy values for absorbed energy dose values.<br />

1 Gy (G<strong>ray</strong>) = 100 rad.<br />

Target Characteristics<br />

The target is a component in the <strong>Linatron</strong>, which absorbs<br />

high energy electrons and produces x-<strong>ray</strong>s. The intensity<br />

of the X-<strong>ray</strong>s produced at the target is a function of the<br />

electron beam intensity and the X-<strong>ray</strong> production<br />

efficiency of the target. Target efficiency is defined as the<br />

ratio of the total X-<strong>ray</strong> radiation power produced to the<br />

total power of the impinging electron beam. This<br />

efficiency depends on both target composition and<br />

geometry. The most efficient targets are made of materials<br />

with a high atomic number (high Z elements). Tungsten<br />

(Z=74) offers the best combined efficiency and physical<br />

properties. This is the primary material used in the<br />

<strong>Linatron</strong> target. It has a thickness slightly greater than the<br />

range of the electrons in the target material.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


<strong>Linatron</strong> targets are specially designed to produce the<br />

minimum focal spot size consistent with their high<br />

radiation output. Focal spot sizes of less than 2 mm are<br />

achieved in operating <strong>Linatron</strong>s. Focal spot size and<br />

uniformity are routinely determined by using a special spot<br />

size camera.<br />

Radiation Absorption and Scattering in the<br />

Object<br />

The x-<strong>ray</strong>s produced in a <strong>Linatron</strong> target form a beam<br />

which passes through the object under inspection. The x<strong>ray</strong><br />

beam consists of photons at varying energy levels,<br />

which are attenuated because the photons interact with<br />

nuclei and atomic electrons of the object as it enters and<br />

passes through material. Depending on the energy of<br />

individual photons, three distinct processes contribute to<br />

the aggregate attenuation of the beam.<br />

In the “photoelectric absorption” process, the photon<br />

loses all of its energy to an atomic electron; that electron<br />

then leaves the orbit of the atom and continues to move<br />

through the material at high speed. This process occurs in<br />

steel with most of the low-energy photons (0.1 MeV and<br />

less). As photon energy increases above 0.1 MeV,<br />

probability of photoelectric absorption decreases and rarely<br />

happens to photons with energies of 1 MeV and higher.<br />

In the “Compton scattering” process, the primary photon<br />

is deflected from its initial line of travel. It loses some of<br />

its energy due to interaction, and continues passing<br />

through the material in the new direction as a lower energy<br />

photon. The atomic electron involved in the interaction is<br />

ejected from its bound position. Compton scattering is<br />

the major attenuation process for photons with energies<br />

between 0.1 and 10 MeV. A high intensity of scattered<br />

radiation can emanate from an object being radiographed<br />

because many of the photons in a high-energy X-<strong>ray</strong> beam<br />

are in this energy range. For example, the intensity of<br />

scatter from a wall or hardware bracket behind the film can<br />

easily reach values that nearly equal the intensity of the<br />

transmitted primary beam<br />

page 6<br />

“Pair production” is the third process. This occurs<br />

when the photon is completely absorbed and an<br />

electron-positron particle pair is created. Pair<br />

production has a threshold energy of 1.02 MeV, and<br />

becomes significant when enough photons with energies<br />

above 4 MeV are present.<br />

The total attenuation of a high-energy X-<strong>ray</strong> beam is a<br />

combination of all three processes, plus other processes<br />

such as the generation of secondary X-<strong>ray</strong>s within an object<br />

by the slowing-down process of the scattered electrons.<br />

The amount of absorption and the total attenuation<br />

depends on the atomic number(s) of the material, the<br />

density and thickness of the object, and the X-<strong>ray</strong> energies<br />

of the photons that make up the beam. Figure 2-1 is a<br />

plot of absorber atomic numbers versus electron beam<br />

energy. This shows the range of absorber atomic number<br />

and photon beam energy where the photoelectric process,<br />

Compton scattering, and pair production dominate the<br />

attenuation process.<br />

FIGURE 2-1. Dominant x-<strong>ray</strong> attenuation process for each<br />

element (atomic number = Z) at each x-<strong>ray</strong> energy.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Half-Value Layer and <strong>Energy</strong> Selection<br />

An X-<strong>ray</strong> beam that enters an absorber is attenuated as it<br />

passes through, and is then measured by a detector at some<br />

fixed point behind the absorber material. The relationship<br />

between the intensity of the X-<strong>ray</strong>s at the detector and the<br />

absorber thickness is expressed by the familiar exponential<br />

law of attenuation:<br />

Ix = Ioe -μx<br />

where:<br />

e = 2.71828 (natural log base).<br />

I o = measured intensity at the detector with no<br />

absorber in the beam.<br />

I x = measured intensity at the detector with the<br />

absorber of thickness x in the beam.<br />

μ = total linear attenuation coefficient.<br />

x = absorber thickness.<br />

There is a single value for the linear attenuation coefficient<br />

when the absorber is a fixed composition and density for<br />

X-<strong>ray</strong>s of a single wavelength or energy.<br />

X-<strong>ray</strong>s emitted by the <strong>Linatron</strong> are not of a single energy,<br />

but contain all energies up to the nominal energy rating of<br />

the unit. Therefore, the actual linear attenuation<br />

coefficient for a substance does not take on a single value<br />

for all conditions of irradiation because of this wide energy<br />

spectrum. For a thin absorber, the attenuation is mostly<br />

caused by the lower energy X-<strong>ray</strong>s. Only the more<br />

energetic X-<strong>ray</strong>s pass through a thick absorber while nearly<br />

all of the lower energy X-<strong>ray</strong>s are absorbed completely.<br />

The thicker absorber will appear to have an attenuation<br />

coefficient value that corresponds to a higher X-<strong>ray</strong> energy.<br />

The attenuation reflects a constant value attenuation<br />

coefficient for thickness over one or two half-value layers<br />

(HVLs). HVL is defined as the thickness of material that<br />

reduces the intensity of the transmitted X-<strong>ray</strong>s by a factor<br />

of two.<br />

In general, the linear attenuation coefficient is proportional<br />

to the density of the absorber material, and it is sometimes<br />

necessary to use the mass attenuation coefficient (μ m )<br />

which is independent of density:<br />

where:<br />

μ m = μ d (cm2 /gm)<br />

page 7<br />

d = density (gm/cm 3 )<br />

If the mass attenuation coefficient is used, the exponential<br />

attenuation equation becomes:<br />

Ix = loe (-μmdx) It is often very useful to identify the X-<strong>ray</strong> attenuation of<br />

material with the HVL. HVL is related to the linear<br />

attenuation coefficient by:<br />

HVL = 0.693/μ<br />

The linear attenuation coefficient and the HVL are also<br />

used to express the quality, or energy makeup, of the<br />

beam from an X-<strong>ray</strong> generator since they have definite<br />

values for each material and for each photon energy.<br />

Practical radiography set-ups use broad-beam radiation,<br />

which produces a scatter effect in the exposure. The<br />

amount of scatter received by a detector will affect the<br />

measured HVL.<br />

The slope of the exposure curve and the contrast and<br />

latitude achieved in a step block exposure are indicators of<br />

the HVL and the effect of scatter. The selection of<br />

generator energy should be governed by the type and<br />

thickness of materials that are required to be radiographed<br />

in a specific application. The broadbeam HVL is the most<br />

useful material index for the radiographer to use for energy<br />

selection since it is related directly to exposure time.<br />

Figures 2-2 through 2-5 illustrate HVL as a function of<br />

incident electron energy for steel, rocket propellant, lead,<br />

and concrete.<br />

FIGURE 2-2. Half-value layer for steel as a function of energy.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 2-3. Half-value layer for propellant as a function of energy.<br />

FIGURE 2-4. Half-value layer for lead as a function of energy.<br />

I<br />

Z<br />

0<br />

a<br />

a<br />

I<br />

6<br />

0<br />

0<br />

0 5 10 15 20 25 30<br />

TARGET INCIDENT ELECTRON ENERGY(MeV)<br />

FIGURE 2-5. Half-value and tenth-value layer for concrete as a<br />

function of energy.<br />

page 8<br />

19.8<br />

13.2<br />

6.6<br />

E<br />

0<br />

z<br />

a<br />

a<br />

I-<br />

Z<br />

w<br />

Half-Value Thickness Versus <strong>Energy</strong> Spectrum<br />

The unfiltered X-<strong>ray</strong>s emitted by the <strong>Linatron</strong> target<br />

contain photons varying in energy, with the highest being<br />

equal to the incident electron energy. This collection of<br />

photons makes up the energy spectrum of the <strong>Linatron</strong> X<strong>ray</strong><br />

beam. This continuous spectrum of energies is often<br />

termed “white” radiation.<br />

The emerging <strong>Linatron</strong> X-<strong>ray</strong> beam becomes filtered and<br />

modified by the obstacles in its path. If an absorber with a<br />

thickness that reduces beam intensity to one-half is placed<br />

in the beam, that thickness can be identified as the first<br />

HVL. That first layer will be thinner than subsequent<br />

HVLs because less material is needed to reduce the<br />

intensity of a beam containing large numbers of lower<br />

energy photons. The first two layers modify the beam,<br />

filter it, and make it “harder”. After about two HVLs,<br />

additional absorber material no longer changes the<br />

distribution of X-<strong>ray</strong> energies and a constant value of the<br />

HVL results. This is described as the equilibrium state.<br />

The values plotted in Figures 2-2 to 2-5 are equilibrium<br />

values.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


<strong>Linatron</strong> Radiographic Characteristics<br />

General Description<br />

The <strong>Linatron</strong> is an RF-powered electron linear accelerator<br />

system that produces a very intense beam of high-energy<br />

X-<strong>ray</strong>s for industrial radiography. The system consists of<br />

an RF unit, an X-<strong>ray</strong> head, a modulator and a control<br />

console. In addition, an optional temperature control unit<br />

is available to provide the required 30° C. liquid coolant<br />

supply to the <strong>Linatron</strong>. Table 3-1 lists the important<br />

performance characteristics of <strong>Linatron</strong> Models M3, M6,<br />

M9 and K15.<br />

X-<strong>ray</strong> Quality<br />

As noted in Section 2, the most useful measurement of X<strong>ray</strong><br />

beam quality is the Half-Value Layer (HVL), which is<br />

derived from the broadbeam attenuation curve or from the<br />

attenuation coefficient. Table 3-2 lists the broadbeam<br />

HVL for several common materials for the LINATR0N<br />

energies.<br />

<strong>Linatron</strong> Model<br />

M3<br />

M3A<br />

M6<br />

M6A<br />

M9<br />

M9A<br />

K15A<br />

Table 3-1 <strong>Linatron</strong> Performance Characteristics<br />

<strong>Energy</strong> (Nominal Peak)<br />

(MeV)<br />

3<br />

1 - 3<br />

6<br />

3.5 -6<br />

9<br />

5 - 9<br />

9 - 15<br />

page 9<br />

Field Coverage, Beaming and Field Flatness<br />

Field Coverage. X-<strong>ray</strong>s emitted from an X-<strong>ray</strong> machine<br />

create secondary radiation (scatter) that can blur and<br />

distort the image on the radiograph when they strike<br />

objects located near the item under inspection. Scatter can<br />

also fog the film and cause a corresponding loss in image<br />

contrast and sensitivity. Therefore, the primary X-<strong>ray</strong><br />

beam should be restriced to the approximate size and area<br />

of the actual inspection. This is accomplished by a device<br />

known as a source collimator, which is a shielding device<br />

located at the source of the x-<strong>ray</strong> beam. These vary in<br />

geometry and density to control the shape of the beam.<br />

Frequently, custom collimators are specified by the<br />

customer to meet the needs of a specific application. The<br />

standard collimator opening for the Model M9 <strong>Linatron</strong> is<br />

a 30° cone and the standard collimator opening for the<br />

K15 <strong>Linatron</strong> is a 15° x 20° pyramid.<br />

Maximum Dose Rate<br />

(Gy/min-m)<br />

3.0<br />

0.2 - 3.0<br />

8.0<br />

2.0 - 8.0<br />

30.0<br />

6.0 - 30.0<br />

60.0 - 150.0<br />

<strong>Varian</strong> <strong>Linatron</strong> applications<br />

Focal Spot Size (mm)<br />

≤2<br />

≤2<br />

≤2<br />

≤2<br />

≤2<br />

≤2<br />

≤2


Beaming and Field Flatness. Electrons reach velocities<br />

approaching the speed of light in the <strong>Linatron</strong> accelerator.<br />

Most of the electrons continue to travel in the forward<br />

direction after their initial interaction with the X-<strong>ray</strong><br />

target. The deflection angle of scatter tends to be small,<br />

and decreases further as the energy of the incident electrons<br />

increases. X-<strong>ray</strong> radiation across the cone of the <strong>Linatron</strong><br />

is not uniform or “flat”. There is a “beaming” effect which<br />

increases with increased energy. Both X-<strong>ray</strong> energy and<br />

intensity (dose rate) are lower at off-center beam angles.<br />

Material<br />

Tungsten (18 gm/cc)<br />

HVL (cm)<br />

HVL (in.)<br />

Lead (11.3 gm/cc)<br />

HVL (cm)<br />

HVL (in.)<br />

Steel (7.85 gm/cc)<br />

HVL (cm)<br />

HVL (in.)<br />

Aluminum (2.70 gm/cc)<br />

HVL (cm)<br />

HVL (in.)<br />

Concrete (2.35 gm/cc)<br />

HVL (cm)<br />

HVL (in.)<br />

Solid Propellant (1.7 gm/cc)<br />

HVL (cm<br />

HVL (in.)<br />

Lucite (1.2 gm/cc)<br />

HVL (cm)<br />

HVL (in.)<br />

Rubber (1.11 gm/cc)<br />

HVL (cm)<br />

HVL (in.)<br />

1MV<br />

0.55<br />

0.21<br />

0.75<br />

0.30<br />

1.60<br />

0.63<br />

3.90<br />

1.50<br />

4.50<br />

1.80<br />

6.10<br />

2.40<br />

10.50<br />

4.10<br />

11.18<br />

4.40<br />

Table 3-2 Typical Broadbeam Half-Value Layer at Characteristic <strong>Linatron</strong> Energies<br />

page 10<br />

2MV<br />

0.90<br />

0.36<br />

1.25<br />

0.49<br />

2.00<br />

0.79<br />

5.40<br />

2.10<br />

6.20<br />

2.40<br />

8.40<br />

3.30<br />

12.10<br />

4.80<br />

12.70<br />

5.00<br />

Because <strong>Linatron</strong> targets are slightly thicker than the<br />

electron path length of the most energetic electron, a<br />

proportionately larger number of lower energy photons are<br />

produced, when compared with a thin target. This reduces<br />

the beaming effect, broadens field coverage, and increases<br />

sensitivity when inspecting thin and low-density materials.<br />

Typical Half-Value Layer*<br />

* Values measured by film techniques may vary somewhat depending upon actual material characteristics, scatter control and other factors.<br />

4MV<br />

1.15<br />

0.45<br />

1.60<br />

0.63<br />

2.50<br />

1.00<br />

7.50<br />

2.90<br />

8.60<br />

3.40<br />

11.60<br />

4.60<br />

16.80<br />

6.60<br />

19.30<br />

7.60<br />

<strong>Varian</strong> <strong>Linatron</strong> applications<br />

6MV<br />

1.20<br />

0.48<br />

1.57<br />

0.62<br />

2.80<br />

1 .10<br />

8.90<br />

3.50<br />

10.20<br />

4.00<br />

13.80<br />

5.40<br />

19.90<br />

7.80<br />

21.00<br />

8.30<br />

9MV<br />

1.20<br />

0.48<br />

1.52<br />

0.60<br />

3.00<br />

1.20<br />

9.60<br />

3.80<br />

11.00<br />

4.30<br />

14.90<br />

5.90<br />

21.50<br />

8.50<br />

24.40<br />

9.60<br />

15MV<br />

1.15<br />

0.45<br />

1.37<br />

0.54<br />

3.30<br />

11.30<br />

11.0<br />

4.30<br />

12.70<br />

5.00<br />

20.40<br />

8.00<br />

29.50<br />

11.60<br />

29.80<br />

11.75


With high-energy <strong>Linatron</strong>s, the intensity of the X-<strong>ray</strong><br />

beam is so much greater at its centerline than at small<br />

angles off-center that a compensator or beam flattener may<br />

be used to reduce the centerline intensity and produce a<br />

more uniform intensity across the field.<br />

In radiography, accurate film exposures require uniform x<strong>ray</strong><br />

beam intensity. Lower energy x-<strong>ray</strong> sources have a<br />

characteristically more uniform beam and can be employed<br />

if exposure times are not excessively long. Some<br />

conditions, such as x-<strong>ray</strong>ing thicker or denser objects,<br />

covering larger areas, or utilizing lengthy source to film<br />

distances, require higher beam power. For these<br />

conditions, a higher energy source may be combined with<br />

a beam compensator.<br />

FIGURE 3-1. <strong>Linatron</strong> x-<strong>ray</strong> intensity distribution, models M3 and M6<br />

page 11<br />

Figure 3-1 shows X-<strong>ray</strong> intensity distribution across<br />

uncompensated beams of 1 MeV, 2 MeV, and 6 MeV<br />

<strong>Linatron</strong>s. Figure 3-2 gives beam profiles for compensated<br />

and uncompensated 9 MeV <strong>Linatron</strong>s. Figure 3-3 shows<br />

plots for the uncompensated and compensated 15 MeV<br />

<strong>Linatron</strong>. These plots, which illustrate the beaming effect<br />

and the degree of flatness of the field, can determine<br />

variation in final film density from the center to the edge<br />

of a film.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 3-2. <strong>Linatron</strong> x-<strong>ray</strong> intensity distribution at 9 MV.<br />

page 12<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Theory, Variables, and Practices in <strong>Linatron</strong> Radiography<br />

Radioagraphic Setup<br />

Collimation. Collimation is the term used to describe the<br />

methods to eliminate the unwanted portion of the X-<strong>ray</strong><br />

beam cone. Collimation is accomplished in three stages:<br />

a. Source (Primary) Collimation. Each <strong>Linatron</strong> has a builtin<br />

collimator which limits the maximum field size the unit<br />

will produce. The collimators are purposely designed to<br />

cover wide areas so that multiple detectors can be exposed<br />

simultaneously. However, for maximum scatter control,<br />

additional inserts must be placed in the collimators or in<br />

front of them to narrow the beam to the detector area. A<br />

variable jaw collimator is set to the proper size by electric<br />

motor adjustment. Some variable collimator jaw openings<br />

are set from the control console by remote control. This is<br />

very useful when performing real time imaging.<br />

b. Pre-Collimation. This is the term used when shielding is<br />

placed between the X-<strong>ray</strong> source and the object. Precollimation<br />

is used to restrict the beam to just the area of<br />

the projected size of the detector.<br />

c. Post-Collimation. This is similar to pre-collimation except<br />

the shielding is placed between the object and the<br />

recording media. Post-collimation is one of the most<br />

important and least used practices in achieving an<br />

optimum X-<strong>ray</strong> image. Although most radiographic<br />

techniques do not require the extensive collimation<br />

described above, it can be of valuable assistance where high<br />

quality radiographs are required or when performing real<br />

time imaging.<br />

Source-to-Film Distance (SFD). Radiation intensity<br />

varies inversely as the square of the distance from the<br />

source (target) to the object. If d1 and d2 are the sourceto-film<br />

distances (SFD), and t1, and t2 are the exposure<br />

times (or dose) respectively, then the terms are related by:<br />

t1 /(d1 ) 2 = t2 /(d2 ) 2<br />

page 13<br />

An exposure technique plan will specify an SFD. The<br />

exposure time and dose must change with distance square<br />

relationship if that distance is changed for a particular<br />

application.<br />

Example<br />

If the original exposure was obtained for an SFD of 4 feet,<br />

and the new SFD must be 6 feet, then the new exposure<br />

time for each thickness is obtained by multiplying the old<br />

values by the factor (f):<br />

f = (6) 2 /(4) 2 = 2.25<br />

Object Placement and Image Formation. Unlike some<br />

other nondestructive testing methods, high-energy x-<strong>ray</strong><br />

radiography can be performed with objects and assemblies<br />

of every conceivable size, shape, and makeup. The<br />

inspections can be done with the object in any one of<br />

many orientations. The exterior and interior of the object<br />

can have any configuration, and the front and back<br />

surfaces need not be flat or parallel.<br />

Regardless of their location or orientation in the object,<br />

internal conditions such as voids and inclusions usually<br />

project interpretable images. Cracks and gaps form the<br />

best images when they are aligned with the X-<strong>ray</strong>s, i.e.<br />

when the X-<strong>ray</strong>s are permitted to stream through the open<br />

space of the gap to reach the film. This also applies to the<br />

inspection of assemblies for internal adjacent solid surfaces<br />

and for internal parts. The best image will require a<br />

particular orientation of the object because of the<br />

relationship of the internal surfaces to the X-<strong>ray</strong> beam.<br />

D/T Ratio, Magnification, and Image Sharpness. The<br />

D/T ratio is the source-to-object distance, D, divided by<br />

the object-to-film distance, T. The value of T is obtained<br />

by measuring the distance from the source side of the<br />

object to the film. T is the object thickness when the film<br />

is directly behind the object.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


It is most convenient to have exposure curves and<br />

technique plans for materials based on the SFD (source to<br />

film distance) for which the work will usually be<br />

performed. Normally, in <strong>Linatron</strong> radiography, the SFD<br />

D/T ratio is about 4 or more. The optimum D/T ratio for<br />

a particular application depends on the same factors that<br />

affect other variables in the radiography procedure.<br />

Among these are object thickness, screen material and<br />

thickness, type of X-<strong>ray</strong> film, filters used, and amount of<br />

magnification that can be tolerated.<br />

Because the X-<strong>ray</strong> film is located in back of the object, the<br />

images of all internal conditions are projected and<br />

magnified. Images of cracks and other defects that occur<br />

on the back and adjacent to the film have very little<br />

projection and magnification. These images are usually<br />

sharper than others for this reason. Because radiography<br />

utilizes a non-point source, the sharpness of all images in<br />

high-energy X-<strong>ray</strong> radiography depends on the projection<br />

involved and the distance to the film.<br />

Images of small voids, gaps, etc., that are located deep<br />

within the object (i.e., not at the back surface) may have<br />

very limited sharpness. They may still be visible, however,<br />

because of high contrast. Many penetrameter images are<br />

have minimal sharpness, yet are still visible and<br />

interpretable because of adequate contrast.<br />

Within the practical limits permitted by focal spot size and<br />

other factors, moving the film away from the object will<br />

reduce the intensity of scatter originating in the object.<br />

This may improve sensitivity where the film-screen unsharpness<br />

greatly exceeds geometrical un-sharpness.<br />

Projection radiography will benefit most from image<br />

magnification because of the inherently larger system unsharpness<br />

in real time imaging.<br />

Reducing Scattered Radiation. Scattered radiation is<br />

present in almost every high-energy radiography<br />

application. Scatter control during <strong>Linatron</strong> use is<br />

important because the scatter may be equally intense as<br />

(and sometimes greater than) the primary <strong>ray</strong>s that reach<br />

the film. If not eliminated or minimized, scatter can<br />

reduce film contrast, obscure and distort image visibility,<br />

and cause false images to appear on the film. A<br />

radiographer must deal with two types of scatter:<br />

page 14<br />

(1.) OBJECT SCATTER is secondary X-<strong>ray</strong> and electron<br />

radiation emitted in all directions from the object, and is<br />

mainly due to the Compton scattering process. For<br />

example, when radiographing 10 HVLs of material, only<br />

0.1% of the primary beam intensity reaches the film, and<br />

99.9% of the incident primary beam is absorbed or<br />

scattered. A large amount of that scatter may reach the<br />

film holder. It can arrive at the film at all angles other<br />

than the primary beam to blur and diffuse images.<br />

(2.) EXTRANEOUS SCATTER is scattered radiation from<br />

material and structures around the object, or from areas in<br />

back of the film (“backscatter”). Another source is the<br />

leakage radiation from the X-<strong>ray</strong> head itself which also<br />

contributes to this scatter.<br />

The radiographer can do the following to eliminate and<br />

minimize scatter:<br />

• Limit the primary beam to the area of interest by<br />

shielding, blocking, or using special collimators.<br />

• Avoid irradiating nearby structures.<br />

• Protect the film from extraneous scatter by suitable<br />

blocking.<br />

• Prevent backscattered radiation from reaching the film<br />

with back lead filters and absorbers.<br />

• Increase the object-to-film distance.<br />

• Use suitable object-film filtration to reduce forward<br />

scatter.<br />

Blocking. Blocking eliminates unwanted portions of the<br />

X-<strong>ray</strong> beam at the object through the use of lead bricks,<br />

shot-filled bags, and other shielding material. Blocking is<br />

needed when large thickness differences in an object<br />

produces high-intensity scatter, or when the object<br />

thickness is many HVLs and the object is smaller than the<br />

radiation field.<br />

A radiographer can judge the effectiveness of the blocking<br />

in a particular setup by observing the film density in the<br />

area of the radiograph over which the blockimg projects. If<br />

that area is absolutely clear (or of very low density), it is a<br />

good indication the desired imaging area also received little<br />

or no scatter.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Comparing the exposure and density for the particular<br />

application with standard exposures and densities from an<br />

exposure curve or other reference is another way to<br />

determine blocking effectiveness. If a shorter exposure of<br />

the material corresponds to a higher film density, when<br />

compared with other well-blocked exposures, it is very<br />

likely that scatter has contributed to the exposure.<br />

Lead Intensifying Screens as Filters. The thin metal foil<br />

(usually lead) intensifying screens that are placed in front<br />

and back of the film to intensify the primary beam and<br />

shorten the exposure also function as filters to reduce the<br />

amount of scattered radiation that reaches the film. Much<br />

of the scatter can be stopped by the lead screen since the<br />

average energy of the scattered radiation is lower than the<br />

energy of the primary beam.<br />

Example<br />

At 10 MeV, a front lead foil 0.01 inch (0.25 mm) thick<br />

will reduce scatter reaching the film by 35% when<br />

exposing about 5 HVLs of low-Z material.<br />

It is customary to select the front lead screen thickness so<br />

the screen provides both intensification and filtration.<br />

However, this practice may not always give the optimum<br />

image quality results. The thickness of a front lead screen<br />

should never exceed 0.050 inch (1.3 mm). The<br />

radiographer should consider using a composite filter<br />

placed in front of the film holder if additional filtration is<br />

needed beyond that. The quality of the image should be<br />

the basis for deciding whether filtration is effective. Some<br />

radiographers eliminate backscatter by using external<br />

(back) lead shielding rather than using lead foils.<br />

Filters. Absorbing plates or assemblies placed between the<br />

object and the film holder may be necessary to achieve the<br />

best image quality when:<br />

• The object shape, position, or composition produces<br />

extensive scatter.<br />

• Large object thickness produces scatter greatly in excess<br />

of the primary radiation.<br />

• The object is smaller than the radiation field.<br />

• Large thickness differences exist in the object.<br />

• <strong>High</strong>-speed photoelectrons produced in the object may<br />

reach the film holder.<br />

page 15<br />

In most cases, the front metal foil intensifying screen will<br />

provide enough filtration to obtain good image quality.<br />

However, in applications (e.g., assembly radiography),<br />

where image sharpness is paramount and a number of the<br />

conditions listed above may exist, an object-film filter of<br />

suitable design is recommended. The filter should be<br />

placed as close behind the object as practicable. The ideal<br />

filter can be layers of high-Z material (such as lead) closer<br />

to the source with subsequent layers of decreasing Z<br />

materials since the filter itself may be a source of scatter. In<br />

some applications a simple filter of lead and brass may be<br />

sufficient.<br />

Screen choices depend on the application, the details of the<br />

radiographic procedure, the energy level, and the degree of<br />

blocking used. For an application in which the<br />

collimation, blocking, and shielding have not minimized<br />

the amount of scatter reaching the film holder, and the<br />

setup geometry must not be modified, the use of external<br />

filters may provide an effective solution. A radiographer<br />

can judge the effectiveness of a filter by comparing image<br />

quality with and without the filter.<br />

Film Holders. The film holder, or cassette, has two<br />

functions. In addition to securing the film from light, it<br />

also maintains firm contact between the film and screens.<br />

Loss of good contact between film and screens results in a<br />

loss of contrast and sharpness in the image.<br />

Three types of film holders or cassettes are frequently used:<br />

semirigid, rigid, and vacuum. The best choice of holder<br />

depends on the requirements of the application.<br />

The Semirigid cardboard or plastic holder is the most<br />

common type. It offers low cost, ease of handling, and<br />

flexibility. Soft plastic, semirigid film holders should be<br />

used when the film must be curved to fit the shape of the<br />

object being inspected.<br />

Rigid holders with mounted screens and spring-loaded<br />

backs are also common. The rigid holder provides more<br />

positive film-screen contact than the semi-rigid holder,<br />

especially when the film must be held in a vertical<br />

orientation.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Vacuum cassettes are recommended where high detail<br />

resolution is needed and where good film-screen contact<br />

cannot be assured by any other means. Vacuum cassettes<br />

may also be required if precise measurements must be<br />

made from the radiograph.<br />

Intensifying Screens<br />

Metal Foil Screens. The previous section described the<br />

filtering action of lead foil screens placed inside the film<br />

holder in front and back of the film. These screens prevent<br />

the scatter from reaching the film by acting as filters.<br />

Contrast is not reduced, and image quality is enhanced as<br />

when other filters are used outside of the film holder.<br />

A second and equally important function of the lead foil is<br />

to increase the speed of exposure and image formation by<br />

intensifying the photographic effect of the primary beam.<br />

Most of this intensification is from the emission of<br />

photoelectrons and Compton electrons from the screen<br />

into the films. Intimate contact of the film and screens is<br />

always required in applied radiography. This sometimes<br />

necessitates using vacuum cassettes or spring-loaded<br />

holders. Intensification will be slightly reduced for the<br />

situation when emulsion that does not touch the screen<br />

because two or more films are placed in the same holder<br />

for the same exposure.<br />

Metal foil screens may be used either un-mounted or<br />

mounted on flexible plastic or cardboard. Mounting<br />

<strong>Energy</strong><br />

(MeV)<br />

1<br />

2<br />

4<br />

6<br />

8<br />

9<br />

11<br />

15<br />

Table 4-1<br />

Front Lead Thickness for Maximum<br />

Intensification<br />

inches mm<br />

0.005 0.13<br />

0.01 0.25<br />

0.02 0.51<br />

0.03 0.76<br />

0.04 1.02<br />

0.04 1.02<br />

0.05 1.02<br />

0.05 1.27<br />

page 16<br />

does not effect the intensification action. Lead is the<br />

screen material most commonly used because of its low<br />

cost, high intensification capabilities, and filtering<br />

effect. However, the lead must have a uniform surface<br />

finish and purity required to characterize the screen as<br />

“radiographic quality”.<br />

Lead screens have a few significant disadvantages. For<br />

instance, they are easily damaged and produce “lead marks”<br />

and phantom images on the film. Also, lead may oxidize<br />

over years of use and require abrasive cleaning to restore its<br />

surface. Some screen suppliers furnish the lead foil either<br />

with the surface chemically treated to resist deterioration or<br />

with a thin Mylar film for protection. Before removing the<br />

protective film, it is advisable to perform tests to determine<br />

how the image quality is affected.<br />

In most X-<strong>ray</strong> procedures, it is routine to use a back lead<br />

screen for intensification and filtering. The thickness of<br />

the back screen is not critical for intensification, since<br />

maximum effect is achieved at about 0.01 inch at all<br />

<strong>Linatron</strong> energies.<br />

The front screen provides a somewhat larger range of<br />

variability of intensification and image quality. As<br />

shown in Figure 4-1, maximum intensification at each<br />

energy is obtained from the approximate thicknesses<br />

listed in Table 4-1.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications<br />

Screen Thickness for Optimum<br />

Image<br />

inches mm<br />

0.002-0.005 0.051-0.13<br />

0.005-0.010 0.13-0.25<br />

0.010 0.025<br />

0.010 0.025<br />

0.020-0.030 0.51-0.76<br />

0.030 0.76<br />

0.030 0.76<br />

0.030-0.050 0.76-1.27


The intensification with a specific screen and for a given<br />

application can be determined experimentally by making<br />

exposures with and without the screen. With “narrow”<br />

beam geometry (i.e., where the collimation and spacing<br />

between the absorber and the film is less than 0.01<br />

steradian of angle), the increase in film density with the<br />

thicker screens is entirely due to the increased intensifying<br />

effect of the screen.<br />

In “broad beam” geometry, a normal amount of scatter is<br />

present, and the filtering of the lead screen determines the<br />

relative amount of scatter that exposes the film. As<br />

indicated in Figure 4-1, intensification for narrow beam,<br />

low front-scatter conditions reach maximum values for<br />

each energy.<br />

Example<br />

At 2 MeV a film density increase of about 0.8 density units<br />

is observed for a 0.01 inch- lead screen compared to an<br />

exposure without a front screen. This corresponds to a<br />

film exposure increase of about 110%. If normal amounts<br />

of front scatter impinge on the film holder and screen, an<br />

apparent intensification of from 20% to 40% may occur<br />

when compared with an exposure without a front screen.<br />

<strong>High</strong> sensitivity in <strong>Linatron</strong> radiography usually requires<br />

sharp images and high contrast. Image contrast is affected<br />

by the screen and film responses. Screens must be selected<br />

and used carefully in order to obtain optimum results at<br />

each energy level and for each application. Unlike kilovoltrange<br />

radiography, where the radiographer can improve<br />

contrast by lowering the voltage, <strong>Linatron</strong> energies are<br />

fixed. Thus, for a <strong>Linatron</strong> system, after a specific type of<br />

X-<strong>ray</strong> film and screens are selected, and after optimum<br />

scatter reduction is accomplished, the radiographer can do<br />

little to improve contrast without changing the imaging<br />

system. Table 4-2 suggests lead screen and filter<br />

thicknesses that typically achieve optimum image quality.<br />

page 17<br />

FIGURE 4-1. Front lead screen intensification: 1 to 15 MV X-<strong>ray</strong>s.<br />

Metal-Phosphor Screens. Composite screens consist of a<br />

layer of fluorescent salt phosphor over a metal foil screen.<br />

The metal foil is a source of electrons that strike the<br />

phosphor, causing visible light photons to radiate the film.<br />

They can sometimes be used in <strong>Linatron</strong> radiography to<br />

shorten exposure times beyond that used with lead screens.<br />

This can allow radiographers to obtain higher contrast<br />

images when compared with the use of lead screens. These<br />

composite screens can be used with ordinary x-<strong>ray</strong> film, and<br />

do not require special “screen” film.<br />

Composite screens may also be constructed of lead or<br />

calcium tungstate. Rare earth phosphors such as<br />

gadolinium oxysulfide are also available.The shorter<br />

exposure times obtained with these screens make it possible<br />

to use thin phosphors to obtain sharper images. The<br />

higher speed screens usually have a thicker phosphor layer.<br />

Typically, metal foil thickness ranging from 0.01 to 0.06<br />

inch (0.25 to 1.5 mm) provide the optimum range of<br />

speed, contrast, and image sharpness.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Table 4-3 lists some relative speeds for the various types of<br />

fluorescent screens currently available. Fluorescent screens<br />

must be well maintained, carefully handled, and kept<br />

clean. Dust particles leave white spots as images on the<br />

film and screens deteriorate with age.<br />

X-Ray Film Characteristics<br />

Film Properties and Classification. Commercial X-<strong>ray</strong><br />

films that have been used for years in kilovoltage and<br />

megavoltage X-<strong>ray</strong> and gamma-<strong>ray</strong> radiography also meet<br />

the needs of high-energy <strong>Linatron</strong> radiography.<br />

Speed. The relative speed of commercial X-<strong>ray</strong> film can be<br />

established with the <strong>Linatron</strong> by exposing each film in a<br />

real radiography arrangement until it will produce a<br />

developed film darkening of a specified density.<br />

<strong>Energy</strong> (MeV)<br />

1-4<br />

6-9<br />

15<br />

Radiographic Conditions<br />

Flat object, low scatter, up<br />

to 4 inches steel or equal.<br />

Complex object, high<br />

scatter, or thick object<br />

over 4 in. of steel or equal.<br />

Flat object, low scatter, up<br />

to 5 inches steel or equal.<br />

Complex object, high<br />

scatter, or thick object<br />

over 5 in. of steel or equal.<br />

Flat objects, low scatter,<br />

up to 6 inches steel or<br />

equal.<br />

Complex object, high<br />

scatter, or thick object<br />

over 6 in. steel.<br />

Table 4-2 Suggested Screen and Filter Thickness Speed<br />

page 18<br />

Example<br />

A comparison chart can be created for various film types<br />

by exposing each film to produce a specified density, such<br />

as 2.0 on the H. & D. scale. If all other variables are held<br />

constant, a relative film speed index can be assigned to<br />

each film, with a numerical value that is proportional to<br />

the exposure level needed to obtain the 2.0 film density<br />

The data presented in Table 4-3 was obtained using this<br />

procedure.<br />

A change in screen material or thickness will cause<br />

shorter or longer exposures. Therefore, the film speed<br />

index will depend on the specific screen used. The<br />

specific developing technique can change the film speed<br />

index by up to 100%. Therefore, it is as important to<br />

quantify and control the developing process as carefully<br />

as the exposure itself.<br />

Screen Thickness<br />

Front Back<br />

0.010 in 0.010 in<br />

(0.25 mm) (0.25 mm)<br />

0.020 in 0.010 in<br />

(0.51 mm) (0.25 mm)<br />

0.020 in 0.010 in<br />

(0.51 mm) (0.25 mm)<br />

0.030 in 0.010 in<br />

(0.76 mm) (0.25 mm)<br />

0.030 in 0.010 in<br />

(0.76 mm) (0.25 mm)<br />

0.050 in 0.010 in<br />

(1.27 mm) (0.25 mm)<br />

* Back lead filters may be placed behind the film holder if there is a large amount of backscatter present. 0.250-inch (6.35 mm) thickness<br />

should be adequate for all cases.<br />

** Object filters are placed between the object and the film holder to reduce the effect of secondary or scatter radiation, or scatter generated by<br />

the object.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications<br />

Remarks<br />

Backing lead as needed.*<br />

0.030 in. lead or composite<br />

object filter may improve<br />

sensitivity.**<br />

Backing lead as needed.*<br />

0.030 in. lead or composite<br />

object filter may improve<br />

sensitivity.**<br />

Backing lead as needed.*<br />

0.125 in. lead or composite<br />

filter may improve<br />

sensitivity.**


A film’s response to scatter may be related to the primary<br />

radiation in conjunction with the relative film speed index.<br />

Therefore, changing to a different film type should not<br />

alleviate a scatter problem in applied radiography. The<br />

intensification index is an indicator that designates<br />

decreasing numbers for faster screens, corresponding to the<br />

exposure level needed to produce a specified film density.<br />

Table 4-4 lists the exposure factors (the index number that<br />

is proportional to the exposure rads) at different film<br />

densities for 12 film varieties in common use. This table is<br />

primarily used to produce a constant film density when<br />

changing film types. To accomplish this, a radiographer<br />

will multiply the film speed index of the new film times<br />

the initial film exposure level to get the new exposure level.<br />

In this way, the new density should be the same as the first<br />

film density.<br />

Contrast and Film Characteristic Curve. Each structural<br />

element, inclusion, void, and crack in the object being<br />

radiographed uniquely alters the radiation passing through<br />

Film Type<br />

DuPont NDT 75<br />

Kodak AA<br />

Agfa Gevaert D-7<br />

DuPont NDT 70<br />

DuPont NDT 65<br />

DuPont NDT 55<br />

Kodak T<br />

Agfa Gevaert 0-4<br />

Kodak M<br />

DuPont NDT 45<br />

Agfa Gevaert D-2<br />

Kodak R<br />

Table 4-3 Relative Intensification Index of Screens*<br />

page 19<br />

Film Type<br />

the object. These variations affect the attenuation in each<br />

area, which results in different image densities on the<br />

exposed film.<br />

FILM CONTRAST is the magnitude of the density<br />

difference between two areas that received different<br />

exposures. A radiographic image with large differences is<br />

said to have “high contrast”. A “low contrast” image<br />

occurs where film density differences are small across the<br />

image. Each type of film has a characteristic response curve<br />

that indicates its sensitivity to incremental exposure. For a<br />

particular film, a FILM RESPONSE CURVE can be made<br />

by plotting density versus exposure level. To create the<br />

data for a film response cure, a radiographer will make a<br />

series of radiographs using a single solid object with<br />

uniform thickness. Each film in the series will subject to a<br />

incrementally longer exposure, creating a range of film<br />

densities. Film response curves can be made for all the<br />

film used in a <strong>Linatron</strong> facility, and can be used to<br />

compare film speeds. Figure 4-2 shows such plots.<br />

Film Density (H. & D. Units)<br />

1.5 2.0 2.5 3.0 3.5<br />

Film Speed Index<br />

0.35 0.5 0.7 0.9 1.2<br />

0.7 1 1.3 1.6 2<br />

0.7 1 1.3 1.6 2<br />

0.7 1 1.3 1.6 2<br />

0.8 1 . I 1.4 1.7 2.1<br />

1.2 1.8 2.4 2.8 3.4<br />

1.4 2 2.5 3 3.7<br />

2.2 3 4 5 5.6<br />

2.7 4 5 6 7<br />

5 7 8.7 10 11<br />

5.5 7 8.7 10 11<br />

7 10 12.6 15 17<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Manufacturers publish density versus log relative exposure<br />

plots for their films, and identify them as FILM<br />

CHARACTERISTIC CURVES. Both response curves and<br />

characteristic curves illustrate the relationships between the<br />

gradient or contrast, which is the slope of the curve,<br />

exposure rads, density, and speed. In Figure 4-2, the steep<br />

rise in the curves above a density of 2.0 shows how much<br />

speed and contrast increase at higher densities. The curves<br />

also show that fine-grained (slower) films have higher<br />

gradients and contrast than faster films. If the exposure<br />

level for an object with a specific thickness is known for<br />

one type of film, the radiographer can find the:<br />

• Exposure time that would be required using another<br />

type of film.<br />

Screen, Front and Back<br />

Lead, optimum thickness<br />

Lead and Tungstate Salt Composites<br />

Very <strong>High</strong> Speed<br />

<strong>High</strong> Speed<br />

<strong>High</strong> Definition<br />

Lead and Gadolinium Oxysulfide<br />

Composites<br />

<strong>High</strong> Speed<br />

<strong>High</strong> Definition<br />

page 20<br />

X-Ray <strong>Energy</strong> (MV)<br />

• Film density that would occur with the second film,<br />

with the same exposure as the first film.<br />

Figure 4-3 shows a plot of film gradient, which is the slope<br />

of the film density versus log relative exposure<br />

(“characteristic”) curve, for three speeds of film.<br />

The exposure gradient shows a continuous increase with an<br />

increase in density, and the slower film shows the higher<br />

film gradients.<br />

The maximum usable density is determined by the<br />

limitations of the viewing equipment. Commercial variable<br />

brightness illuminators are adequate at densities up to about<br />

3.5. For films darker than 3.5, a very high-intensity spot<br />

illuminator with a variable iris should be used.<br />

1-3 4-6 9 15<br />

1 1 1 1<br />

0.14 0.20 0.33 0.50<br />

0.33 0.50 0.67 0.77<br />

0.60 0.70 0.80 1.00<br />

0.20 0.33 0.50 0.67<br />

0.55 0.67 0.80 1.00<br />

Table 4-4 Relative Speeds of Industrial X-Ray FilmAt <strong>Linatron</strong> X-Ray Energies With Lead Screens and Automatic Processing<br />

(With 2.5” Steel Absorber)<br />

* The intensification index is arranged with decreasing numbers for faster screens, corresponding to the exposure level needed to produce a<br />

specified film density.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-2. Film response curves for three industrial X-<strong>ray</strong> films<br />

with relative speeds (exposure factors, EF): 1 = Fast, 3 = Medium,<br />

7 = Slow.<br />

If an object with varying thicknesses (steps) is radiographed,<br />

the densities of the steps on each film, when plotted, will<br />

appear as shown in Figure 4-4. These points also show that<br />

the density differences, and therefore the contrast, are larger<br />

with slower film. This further illustrates the general rule<br />

that contrast increases with increased film density.<br />

A numerical value for contrast can be taken from this plot.<br />

Example<br />

For the 1/8th-inch steel steps, the slope of the curve is<br />

approximately 0.20 density units per 1 /8-inch step at the<br />

2.0 density point. This value corresponds to the contrast<br />

achieved with lead intensifying screens. It shows the<br />

increased contrast achieved with phosphor screens.<br />

page 21<br />

FIGURE 4-3. Curves of gradient versus film density for three X<strong>ray</strong><br />

films shown in Figure 4-2.<br />

FIGURE 4-4. Film density plot for step exposures of steel for lead<br />

screens at 2 MeV. *<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-5. Plot of density versus steel steps for lead and leadphosphor<br />

at 9 MeV. *<br />

Figure 4-5 is a plot of density versus steel steps for lead and<br />

metalphosphor screens. It shows the increased contrast<br />

achieved with phosphor screens.<br />

Multifilm Techniques. It has been shown that a single film<br />

will exhibit a range for film densities that bears a relationship<br />

to the range of thicknesses in the object. If there are<br />

thicknesses in the object being radiographed that exceed the<br />

corresponding limits of a single film, the thicknesses may<br />

still be covered in a single exposure by placing two or more<br />

films in the film holder. This is true with the additional film<br />

having the same or a different speed.<br />

Example<br />

It may be desired to maintain a minimum density of 1.5 to<br />

achieve the required radiographic quality for an exposure<br />

where the film density ranges from 1.0 to 1.7.<br />

If a second film of the same type is used and the two<br />

films are exposed simultaneously, the resultant exposure<br />

is about the same. The density of each film will again<br />

range from about 1.0 to 1.7. The two densities will sum<br />

and the density range will be 2.0 to 3.4 when they are<br />

viewed together.<br />

page 22<br />

For this example, there wasn’t an increase in exposure time<br />

to get a very desirable density range. Using two films of<br />

the same type also permits the interpreter to distinguish<br />

between an artifact (blemish or flaw) in the film and a<br />

defect in the object. This procedure can also be used with<br />

two films of different speeds. The first is exposed to a<br />

density ranging from 1.0 to 1.7, as before. If the second is<br />

a faster film, its density may range from 2.0 to 3.5. The<br />

interpreter may then view the darker portion of the lower<br />

density film and the low density portion of the higher<br />

density film, and thus obtain coverage of the entire<br />

thickness range in one exposure.<br />

Double film loads can be used between a single pair of<br />

screens. There is also mutual intensification of the<br />

touching film using this technique. Also, many electrons<br />

from metallic screens are sufficiently energetic to pass<br />

through multiple layers of film and intensify the<br />

succeeding layers. Using interleaved lead screens will<br />

ensure better resolution in each film. Interleaving is also<br />

employed to adjust the speed relationships. This makes the<br />

second layer darker. The interleaved lead foil screens must<br />

be without backing material and be between 0.005 and<br />

0.010 inch thick.<br />

Definition and Unsharpness<br />

It is often desirable to obtain the very best image available<br />

in radiography, i.e., one with high contrast, minimal<br />

distortion, low graininess, and optimum definition. To<br />

accomplish this, an intermediate exposure time is required,<br />

since it allows improved density variations to occur on the<br />

film. Therefore, compromises are required where there is a<br />

need for the shortest possible exposure times. Some<br />

approaches to this include:<br />

• Sharpness is increased by using thin screens (and<br />

sometimes eliminating the back screen), by using single<br />

emulsion film and fine-grained film, and by using<br />

effective filters between the object and the screen.<br />

HOWEVER,<br />

Exposure times are reduced by using thick screens,<br />

double-emulsion films, coarser- grained films, and by<br />

deleting a separate filter between the object and screen.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


• Moving the film farther from the object (increasing “TI’)<br />

reduces scatter, which improves image quality.<br />

HOWEVER,<br />

Exposure time and geometric unsharpness are increased.<br />

• Increasing the source-to-object distance provides greater<br />

area coverage and reduces geometric unsharpness.<br />

HOWEVER,<br />

Exposure time increases by the inverse square law.<br />

• Using composite metal-phosphor screens shortens<br />

exposure times and provides higher contrast in the<br />

image.<br />

HOWEVER,<br />

Composite metal-phosphor screens result in increased<br />

graininess and a loss of sharpness and detail resolution.<br />

Unsharpness in a radiograph can be defined as blurring of<br />

image edges. This causes a loss of fine crack definition,<br />

image detail, and penetrameter (Image Quality Indicator)<br />

detail. Unsharpness and lack of contrast are not<br />

synonymous. Film contrast is the difference in film<br />

density between two areas of a radiograph. A film may<br />

have high contrast but lack sharpness because of image<br />

edge blurring, and vice versa. Good image quality needs<br />

sharpness and high contrast for good radiographic<br />

sensitivity.<br />

Three sources of unsharpness have been identified in<br />

general radiography. These are geometric, inherent, and<br />

scatter (see Figure 4-6). U F (inherent unsharpness of the<br />

film and screens), and U G (geometric unsharpness due to<br />

focal spot size and object thickness and arrangement)<br />

contribute mostly to unsharpness. U F is usually the major<br />

element of unsharpness in high-energy X-<strong>ray</strong> radiography.<br />

It increases with increasing radiation energy and film grain<br />

size. It is a function of screen material and thickness, and<br />

is affected by the film processing technique. We can expect<br />

the following values of U F with <strong>Linatron</strong> radiography<br />

using lead screens, fine-grained film (i.e., speed index = 4,<br />

at density = 2.0), and automatic processing:<br />

page 23<br />

FIGURE 4-6. Sources of unsharpness.<br />

<strong>Energy</strong>, MeV UF, mm<br />

1 0.15<br />

2 0.3<br />

4 0.4<br />

6 0.5<br />

9 0.6<br />

15 1 .0<br />

U G is a linear unsharpness, described by the adjacent<br />

diagram and the expression:<br />

U G = S/(D/T)<br />

Where S = source spot size,<br />

D = distance from the source spot to the<br />

front surface of the object and<br />

T = distance from the front surface of the<br />

object to the film, or usually the thickness of<br />

the object.<br />

The total unsharpness (UTOT ) results from the combined<br />

effect of the inherent, scatter and geometric unsharpnesses,<br />

and can be expressed as the square root of the sum of the<br />

square of each.<br />

UTOT = (U 2<br />

F + UG2 + US2 ) 1/2<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


The total unsharpness is reduced to include only inherent<br />

and geometrical unsharpness because they contribute much<br />

more than spot size to unsharpness. This reduces the<br />

expression the expression above to the following.<br />

UTOT = (U 2<br />

F + UG2 ) 1/2<br />

Example<br />

Let energy equal 2 MeV and focal spot equal 2 mm. If we<br />

use double emulsion film and automatic development,<br />

with U F = 0.3 mm, and a radiography arrangement where<br />

6 inches of steel are exposed with a D/T = 12, U TOT is:<br />

U TOT = (0.3 2 + (2/12) 2 ) 1/2 = 0.34 mm<br />

From this example, it can be seen that with a film<br />

unsharpness of 0.3, the geometric value only has a slight<br />

effect on the total. Figure 4-7 shows total unsharpness<br />

plotted for the case where inherent unsharpness is 1 mm.<br />

The plots show the effect of various values of D/T on the<br />

total unsharpness.<br />

FIGURE 4-7. Total unsharpness as a function of source spotsize.<br />

page 24<br />

Sensitivity and Image Quality<br />

A standard requirement in most high-energy radiography<br />

applications with <strong>Linatron</strong> sources is that the inspection<br />

process demonstrates 2% sensitivity using penetrameter<br />

wires or holes. <strong>Linatron</strong> radiography regularly produces<br />

sensitivities better than 1% through a wide range of<br />

material thicknesses. Many factors determine image<br />

quality in all high-energy <strong>Linatron</strong> radiography<br />

applications. Thickness, wire penetrameter, plaque<br />

penetrameter, and radiographic sensitivity are four kinds of<br />

sensitivity commonly evaluated determine <strong>Linatron</strong><br />

capability.<br />

Thickness Sensitivity. Thickness sensitivity refers to the<br />

ability of the radiographic inspection to demonstrate a<br />

thickness step by seeing the density difference produced on<br />

the film. Under good viewing conditions a trained eye can<br />

reliably perceive 0.006 density units with a reasonably<br />

sharp step edge in the image. This minimum perceptible<br />

density difference varies with energy and object thickness<br />

depending on the energy of the source and the contrast<br />

achieved by the film and screens. All <strong>Linatron</strong> sources can<br />

provide approximately 1% thickness sensitivity from 1 inch<br />

(25.4 mm) of steel up to 10 HVL thicknesses using finegrained<br />

film, lead screens and good scatter control.<br />

Wire Penetrameter Sensitivity. Wire penetrameters are<br />

generally used in Europe, and in several special applications<br />

in the United States. The German D.I.N. wires come in<br />

16 sizes from 3.2 mm to 0.10 mm as follows: 3.2, 2.64,<br />

2.0, 1.6, 1.32, 1.0, 0.8, 0.66, 0.5, 0.4, 0.33, 0.25, 0.20,<br />

0.165, 0.15, and 0.10 mm.<br />

Data shows that all <strong>Linatron</strong> sources should demonstrate<br />

better than 1% sensitivity above 1 inch (24.5 mm) of steel,<br />

and should achieve better than 0.5% for steel thicknesses at<br />

about 6 inches (152.4 mm).<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Drilled Hole Plaque Penetrameter Sensitivity. The<br />

drilled hole plaque is the standard American penetrameter<br />

for all radiography. It consists of a small rectangular strip<br />

of material with three drilled holes. Thickness of the<br />

penetrameter is specified as 1%, 2%, or more, of the object<br />

thickness. The three hole diameters are equal to 1 x T, 2 x<br />

T, and 4 x T where the thickness of the penetrameter “T”.<br />

Sensitivity is described in terms of the thickness percent (1,<br />

2, 4) and the required hole size that must be discerned.<br />

Example<br />

2-2T is the standard way to describe a penetrameter whose<br />

thickness must be 2% of the object thickness and whose 2<br />

x T hole must be seen on the film.<br />

Drilled hole sensitivity data for each <strong>Linatron</strong> show that all<br />

sources should demonstrate better than 1% sensitivity<br />

above 2 inches (50.8 mm) of steel, up to 10 HVLs, and<br />

better than 2% for thicknesses down to 1 inch (25.4 mm).<br />

Radiographic Sensitivity. Radiographic sensitivity refers<br />

to the ability to see and recognize a variety of defects and<br />

other internal conditions in the radiograph in this manual.<br />

Standard penetrameters provide an indicator of the level of<br />

image quality that is achieved with a particular<br />

radiographic technique used. Penetrameters do not,<br />

however, give defect size. Penetrameters must be placed on<br />

the source side of an object since the image improves as the<br />

defect occurs closer to the film.<br />

Exposure Curves<br />

The plot of exposure level that corresponds to a specific<br />

film density (2.0 for example) for each thickness of<br />

material is called an exposure curve. Exposure curves<br />

should be made for the <strong>Linatron</strong> after it is completely<br />

operational for all applications. Such curves represent<br />

operational data that are indicative of the operating<br />

characteristics of the setup. Subsequent exposure curves for<br />

the same setup should provide consistent results.<br />

page 25<br />

Established exposure curves also allow the radiographer to<br />

simplify the exposure calculation process. With these<br />

curves, the radiographer only needs to look up the required<br />

exposure level for that thickness and make the exposure. If<br />

the source-to-film distance must be changed, using the<br />

inverse square law provides the new exposure level. A<br />

change to a different film can lead to an additional<br />

adjustment of exposure level using the relative speed table.<br />

Method for Making Exposure Curves. This process<br />

involves making a series of test exposures of an object with<br />

uniform density but varying thickness. Typically, a wedge<br />

or stair-step shaped block is used in conjunction with<br />

additional slabs of uniform thickness. Because exposure<br />

time can be represented as a straight line on semi-log graph<br />

paper, at least two measurements are needed to establish<br />

this line.<br />

FIGURE 4-8. Wedge-shaped block used for experimentally<br />

obtaining exposure curves. Standardized to a film density of 2.0.<br />

To make an exposure curve for a new material, a step or<br />

wedge-shape block (see Figure 4-8) of the same material<br />

that is being radiographed, and a slab of that material, are<br />

placed together to form the object for the first test exposure.<br />

It is most helpful if the slab thickness and the wedge center<br />

thickness are approximately 1 HVL. Note, the material<br />

used in this work should first be radiographed to assure that<br />

it is uniform and free of defects.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


This wedge block is then radiographed with substantially<br />

the same film, screens, focal-film distance, and<br />

arrangements for the same conditions as future routine<br />

inspection work. It should be noted that good collimation<br />

and shielding must be used for the test exposures to<br />

achieve a low amount of scatter at the film holder. The<br />

film is then inspected to determine where the film density<br />

is 2.0 on the step or wedge image. The total thickness of<br />

the wedge-slab combination corresponding to this spot is<br />

measured and the exposure level is recorded. This data<br />

provides the first point for the exposure curve. The<br />

assembly is then made thicker by adding several slabs, and<br />

the process is repeated to obtain the second point. These<br />

two points should then be plotted on semilog graph paper<br />

and connected by a straight line.<br />

The first check on the accuracy of this exposure curve is to<br />

determine from the slope of the line if the HVL equals the<br />

handbook values or other predicted value for the material.<br />

An accuracy check can be obtained by selecting a third<br />

exposure that should correspond to another point along<br />

the line. The line can be extended down to 1 HVL, and up<br />

to 12 HVLs or greater. The curve provides a good<br />

approximation of exposure times for the entire range of<br />

thickness the <strong>Linatron</strong> can inspect. Since the same wedge<br />

exposure will have a region where the film density is about<br />

3.0, it could provide points for an exposure curve for the<br />

density 3.0. These data also provide important<br />

information about contrast and latitude.<br />

Latitude. A common task in high-energy <strong>Linatron</strong><br />

installations is to radiograph objects that have varying<br />

shapes and thicknesses. A single film exposure can cover a<br />

range of useful film densities where sensitivity and<br />

interpretability are accurate and valid. The thickness range<br />

that corresponds to the range of useful densities, usually<br />

1.5 to 3, is called the latitude of the exposure. Latitude<br />

depends on the film gradient, or contrast, and the<br />

attenuation of the material, or HVL. By noting the points<br />

on the wedge image that correspond to densities 1.5 and 3,<br />

the wedge exposure used to generate the exposure curves<br />

can also be used to provide data for determining latitude.<br />

Figure 4-9 shows a plot of latitude for each energy.<br />

page 26<br />

FIGURE 4-9. Latitude ranges for <strong>Linatron</strong> exposures of steel.<br />

Hint:<br />

While a single film has a limited latitude, two films of<br />

different speed can be combined in one exposure to<br />

increase the total latitude of the exposure.<br />

Exposure Times and Material Densities. When all other<br />

variables remain constant the correct radiographic exposure<br />

time and level for an object depend on its thickness and<br />

density. Two objects with different densities (d 1 and d 2 )<br />

can have approximately the same exposure time, when<br />

their thickness (X 1 and X 2 ) are related by the expression<br />

Example<br />

d 1 X 1 = d 2 X 2<br />

A 1.00-inch-thick (25.4 mm) slab of copper alloy with a<br />

density of 8.8 gm/cc will have approximately the same<br />

exposure time and rads as a 1.13-inch (28.7 mm) thick<br />

slab of steel with a density of 7.87 gm/cc.<br />

Likewise, an object with unknown radiographic exposure<br />

characteristics may be compared with one whose exposure<br />

values are known. To accomplish this, first approximate the<br />

objects linear attenuation coefficient (μ 2 ) from its density<br />

(d2) by<br />

<strong>Varian</strong> <strong>Linatron</strong> applications<br />

μ 1 /d 1 = μ 2 /d 2


and then determining the approximate exposure level from<br />

the known value of exposure for object number 1 (Rl ), by<br />

R2e -μ2X2= R1e -μ1X1 Example<br />

The exposure of a 4-inch-thick (101.6 mm) bronze alloy<br />

(density = 9) may be estimated from the steel exposure<br />

curve at 2 MV by:<br />

μbronze = 0.693/0.8 X 9/7.85 = 1 inch-1 For 4 inches (101.6 mm) of steel, the exposure rads:<br />

R l = 150 rads.<br />

Therefore for bronze: R2 = 150 e-(.866)(4)<br />

e<br />

= 256 rads<br />

-(1)(4)<br />

Thus, an exposure curve for the bronze alloy can be<br />

constructed by calculating the exposure rads at two<br />

thicknesses, plotting these points, and connecting them<br />

with a straight line.<br />

Table 4-4 lists the physical density ratio conversion factors<br />

for converting steel or solid propellant exposure curve into<br />

curves for a wide variety of materials.<br />

• Physical density may be used for a first approximation,<br />

but a more accurate value results from t using linear<br />

attenuation coefficients.<br />

Multiply by factors belowto convert steel<br />

exposures to approximate exposures for these<br />

materials:<br />

Zirconium 0.83<br />

Copper 1.13<br />

Molybdenum 1.3<br />

Silver 1.33<br />

Lead 1.44<br />

Uranium or Tungsten 2.38<br />

Gold 2.45<br />

page 27<br />

Using Film Response Curves to Generate New Exposure<br />

Curves. When an exposure curve is obtained and verified<br />

for one film and at one value of film density, new exposure<br />

curves for other films and for other film densities can be<br />

generated without remaking the entire series of exposures.<br />

To determine response curves for new films, refer to the<br />

film response curves that plot film density versus the<br />

exposure level for X-<strong>ray</strong>s, in the <strong>Linatron</strong> energy ranges.<br />

Example<br />

Table 4-4 Physical Density Ratios for Common Materials When Using <strong>High</strong> <strong>Energy</strong> X-Rays<br />

If an exposure curve for steel is made with AGFA-Gevaert<br />

Type D-2 x-<strong>ray</strong> film for a density of 2.0, and it is desired<br />

to have a similar curve for Type D-4 film at density 2.0,<br />

the film response data of Table 4-3 (presented earlier) and<br />

the characteristic curve plots for x-<strong>ray</strong> film in the AGFA-<br />

Gevaert Handbook supply the data necessary for the new<br />

plot. Table 4-3 shows that at a film density of 2.0, D-2 has<br />

a film speed index of 7 and D-4 has a film speed index of<br />

3. These indices are in proportion to the exposure rads.<br />

Therefore, at each thickness, the factor of the D-4 film<br />

speed index relative to the D-2 film index (or 3/7 when<br />

multiplied by the exposure rads from the D-2 exposure<br />

curve) will determine the correct rad exposure at each<br />

thickness for the D-4 film. the Agfa-Gevaert Handbook<br />

indicates the same relative speed indices for these films, but<br />

with another series of index numbers.<br />

Multiply by factors below to convert propellant<br />

exposures to approximate exposures for these<br />

materials:<br />

Sodium 0.57<br />

Lucite 0.69<br />

Magnesium 1.02<br />

Carbon 1.3<br />

Concrete 1.38<br />

Aluminum 1.6<br />

Titanium 2.67<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Increasing Latitude With Multiple Film Use. The<br />

exposure curves for steel and solid propellant are shown in<br />

Figures 4-10 through 4-21. Figures 4-10 and 4-16 are for<br />

two typical films and a single film speed index (Exposure<br />

Factor) of 1. The remaining figures are for three film<br />

types, with film speed indices of 1,2, and 4. Note the<br />

overlapping of film densities. The densities in the three<br />

films are not equal at any one particular value of thickness<br />

and exposure, since the film speed indices and responses<br />

are unequal. Because the response characteristics of each<br />

film at any thickness and exposure, when the fast film (low<br />

film speed index) shows a density of 3.0, the slower film<br />

exposed to the same level and thickness may show a<br />

density of 1.6 or 1.7.<br />

FIGURE 4-10. <strong>Linatron</strong> tvpical exposure curves for steel.<br />

page 28<br />

Example<br />

The curves for the 9 MeV <strong>Linatron</strong> show a latitude of 2.8<br />

inches (71.12 mm) of steel between film densities of 1.0 to<br />

3.0. This means if an object is made of various<br />

thicknesses, and the range exceeds about 2.5 inches (63.5<br />

mm), the latitude limits of one film are exceeded, and a<br />

second film, either slower or faster (for the thinner or<br />

thicker section), is needed to extend the exposure range.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-11. <strong>Linatron</strong> 1 MeV typical exposure curves for steel.<br />

page 29<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-12. <strong>Linatron</strong> 2 MeV typical exposure curves for steel.<br />

page 30<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-13. <strong>Linatron</strong> 4 MeV typical exposure curves for steel.<br />

page 31<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-14. <strong>Linatron</strong> 9 MeV typical exposure curves for steel.<br />

page 32<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-15. <strong>Linatron</strong> 15 MV typical exposure curves for steel.<br />

page 33<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-16. <strong>Linatron</strong> typical exposure curves for solid propellant.<br />

page 34<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-17. <strong>Linatron</strong> 1 MeV typical exposure curves for solid propellant.<br />

page 35<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-18. <strong>Linatron</strong> 2 MeV typical exposure curves for solid propellant.<br />

page 36<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-19. <strong>Linatron</strong> 4 MeV typical exposure curves for solid propellant.<br />

page 37<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-20. <strong>Linatron</strong> 9 MeV typical exposure curves for solid propellant.<br />

page 38<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 4-21. <strong>Linatron</strong> 15 MeV typical exposure curves for solid propellant.<br />

page 39<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Radiographic Procedures<br />

General Considerations<br />

Practices in radiography of castings, welds, rocket motors,<br />

and assemblies are described in this section. The<br />

information presented here is intended as a general<br />

description only. Specific radiographic facilityoperating<br />

procedures are usually determined by unique facility<br />

requirements. These guidelines must not change, alter,<br />

supercede or take precedence over any controlling<br />

procedures, specifications or standards.<br />

Records and Logs. It is extremely important to keep<br />

careful records of all radiographic work. The daily log<br />

should show the names of the radiographers and the<br />

identification of each part radiographed.<br />

In addition to the job information, a daily log should be<br />

maintained containing information concerning radiation<br />

hazards and operation of all equipment, including all safety<br />

devices, interlocks, warnings. All malfunctions should be<br />

dated and identified. Checks of the equipment after<br />

repairs or adjustments should be logged.<br />

Exposure Room Equipment. In addition to the <strong>Linatron</strong><br />

and its manipulation system, an x-<strong>ray</strong> facility should have<br />

the following:<br />

• Materials handling crane, forklift, or other means to<br />

move and set up the parts that require x-<strong>ray</strong><br />

examination.<br />

• Electrical power outlets.<br />

• Grounding system leading to an outside earth ground.<br />

• Film cassette support and holders.<br />

page 40<br />

A facility designed to examine objects such as large rocket<br />

motors or similar assemblies should include yokes, belt<br />

slings, roller support frames, motorized turntables, and<br />

tangential shielding supports. Other accessories and<br />

supplies for radiography are listed below.<br />

• Image Quality Indicators (IQI) for the applicable<br />

standards and material being radiographed<br />

• Deep block lead numbers and letters<br />

• Film holders (all sizes), rigid cardboard, soft plastic, and<br />

vacuum cassettes<br />

• Lead screens from 0.010 inch (0.25 mm) to 0.030 inch<br />

(0.76 mm) thick, assorted sizes, some unbacked and<br />

some with cardboard backing<br />

• Lead sheets 1/8 inch (3.18 mm) to 1/2 inch (12.7 mm)<br />

thick, in all sizes<br />

• Lead or copper shot in canvas bags<br />

• Lead bricks<br />

• Calipers and other wall-thickness gages<br />

• Survey meters for radiation protection surveys; also Rmeters,<br />

pocket dosimeters, film badges, warning lights,<br />

signs, and other safety equipment<br />

• Automatic temperature-controlled film processing<br />

equipment<br />

• Film viewing equipment with variable intensity viewers<br />

• Magnifying glass, 3x to 5x, for film reading<br />

• Densitometer with capabilities up to density 4.0<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Casting Radiography<br />

Radiography of castings can reveal defects which can be<br />

repaired before expensive machining operations are<br />

performed. Therefore, it can be a very effective tool to<br />

determine the suitability of the casting. Radiography also<br />

reveals how well casting techniques are working.<br />

Most castings inspected by high-energy radiography are<br />

produced in sand mold flasks or in metal-framed<br />

containers. The upper section of the mold is referred to as<br />

the cope, the bottom section as the drag, and the junction<br />

of the two as the parting line. The mold of a large,<br />

complex casting may be assembled from a number of parts<br />

and cores. Radiography may also be required for large<br />

ingots that are cast in permanent molds and for parts<br />

suitably shaped for casting by the centrifugal process.<br />

Listed below are common casting defects that radiography<br />

can reveal.<br />

• COLD SHUTS are areas between two quantities of cast<br />

material that have cooled below the molten state before<br />

coming into contact with each other, thereby causing an<br />

unfused interface.<br />

• HOT TEARS show as crackline indications usually<br />

appearing singly near the surface and at hot spots or<br />

where temperature gradients are high.<br />

• CRACKS show as sharply defined indications, sometimes<br />

with penumbral shadows, caused by metal parting from<br />

itself. These are frequently caused by improper stress<br />

and temperature gradients. Cracks are often created<br />

when a core or mold resists the compression of the<br />

casting as it shrinks on solidification.<br />

• PIPING shows as elongated, cylindrical-shaped<br />

indications located at or near the center of the casting.<br />

These are caused by risers and feeders not being kept hot<br />

and liquefied, which causes a lack of metal flow to the<br />

center of the casting mold.<br />

• SHRINKAGE is generally associated with improper<br />

feeding of metal into the casting mold. Shrinkage<br />

manifests itself in the following three forms:<br />

- Sponge Shrinkage, found in heavier sections, appears<br />

on the radiograph as a dark, lacy area with a diffused<br />

outline.<br />

- Feather Shrinkage, found in thinner sections, appears<br />

on the radiograph as a sponge, with a feathery outline.<br />

page 41<br />

<strong>Varian</strong> <strong>Linatron</strong> applications<br />

- Linear Shrinkage, a continuous structure of connected<br />

lines with branches of variable lengths, widths, and<br />

densities.<br />

• GAS HOLES AND VOIDS are caused by trapped air or<br />

mold gases. They appear on the radiograph as round or<br />

elongated, smooth edged, dark spots and may appear<br />

individually, in clusters, or distributed throughout the<br />

casting.<br />

• DROSS represents oxidized metals. This appears as a<br />

series of lines in a swirl pattern sometimes combined<br />

with agglomerated irregular indications.<br />

• SEGREGATION is the result of certain elements of a<br />

metal to concentrate in the last liquid portion of the<br />

metal. This results in an uneven distribution of the<br />

chemical constituents. These can appear as uneven,<br />

irregularly shaped, dark areas on the radiograph.<br />

• MOLD MATERIAL, SAND, AND OTHER<br />

INCLU SIONS<br />

• UNFUSED CHAPLETS AND CHILLS<br />

• INCOMPLETE DEFECT REMOVAL<br />

• DEFECTIVE REPAIR WELDS<br />

Radiographic Coverage. The coverage on castings may be<br />

specified by the customer or it may be given by casting<br />

specifications. The radiographer is required to select<br />

optimum projections and techniques in the latter case.<br />

Visual inspection of rough-cleaned castings reveals where<br />

risers and gates have been removed. Pattern numbers are<br />

usually on the drag side. Areas typically radiographed<br />

include heavy sections in the drag, the flanges, the<br />

junctions of diaphragms and casting walls in the valve<br />

areas. Among the critical areas are valve seats, steam chest<br />

areas, and other parts where extensive machining is<br />

performed.<br />

Shrinkage defects usually lie in the centerline of cast<br />

sections and, unless they are extensive or in areas to be<br />

machined, are less critical than hot tears or cracks. Both<br />

hot tears and cracks tend to be perpendicular to cooling<br />

stress directions and are often difficult to examine unless<br />

the radiographic projection is parallel to the crack or tear<br />

direction.


When radiographing curved sections, the concave side<br />

should face the source and, when possible, flexible film<br />

holders should be formed to the casting contour. While<br />

this practice tends to improve film/screen contact, it may<br />

increase the image distortion at the edges of the curved<br />

film. To control for this, image quality indicators should<br />

be placed at the extreme widths of the film, and there<br />

should be adequate overlap in adjacent exposures to<br />

ensure complete coverage. While an oblique angle may<br />

be required in some regions, when possible, the X-<strong>ray</strong><br />

beam should enter the casting at right angles to the front<br />

surface, and the film should be set up perpendicular to<br />

the central <strong>ray</strong>.<br />

When the casting thickness varies more than 1/2-inch<br />

(12.7 mm) equivalent steel, the multiple-film technique<br />

can be employed to cope with the varying section<br />

thicknesses. These variations may also create significant<br />

scatter, which can be minimized using special procedures<br />

(see the discussion on scatter control).<br />

Layout and Marking. Radiographic assignments can<br />

involve fairly simple techniques. This can be as simple as<br />

placing the film cassette under or behind the casting and<br />

making the exposure. But, for large, heavy castings such as<br />

turbine bodies, the film placement and radiographic<br />

projections can be complex and may require careful<br />

planning and fixturing.<br />

Crane mounted <strong>Linatron</strong> used to examine large objects.<br />

page 42<br />

The radiographer should be furnished with either a marked<br />

print of the casting, showing the projections and areas to<br />

be covered, or a rough sketch showing the film locations,<br />

markers and other relevant information. The marked print<br />

or sketch should remain with the casting radiographs. The<br />

radiographer should retain a copy to add information<br />

about the film and screens used, image quality indicator<br />

selection and placement, filtration, exposure and resulting<br />

film density, and other pertinent facts about the job.<br />

Casting Radiographic Procedures. When compared with<br />

lower energy systems, <strong>Linatron</strong> radiography of castings can<br />

often produce significantly more readable film images.<br />

The increased latitude and reduced wide angle scatter<br />

provide major advantages not found in lower energy<br />

radiography. However, high-energy radiographs will have<br />

less contrast, and the imaging of fine cracks and<br />

filamentary porosity can be difficult. Cracks usually do<br />

not progress in a straight line and do not present welldefined<br />

edges to the X-<strong>ray</strong> path. This usually causes<br />

images to have penumbral edges, which makes detection<br />

difficult. Cracks which lie at angles to the X-<strong>ray</strong> beam can<br />

be seen if their width exceeds the limit imposed by the<br />

overall radiographic sensitivity, as determined from the<br />

equation;<br />

<strong>Varian</strong> <strong>Linatron</strong> applications<br />

Δx = W/sin ø (see Figure 5-1)<br />

where Δx = the crack width in the direction of the radiation<br />

W = the crack width<br />

ø = the angle of the crack to the x-<strong>ray</strong> beam


FIGURE 5-1. Relationships between crack width (W), projection<br />

angle (ø), and contrast sensitivity (Δx/x).<br />

Almost all castings contain discontinuities of various types<br />

(inclusions, microshrinkage, etc.) that have no effect on the<br />

strength or serviceability of the casting. Repairing these<br />

discontinuities is expensive and sometimes can do more<br />

harm than good. It is the radiographer’s task to determine<br />

the criticality of the various areas and to produce the best<br />

possible radiographs.<br />

• RADIOGRAPHY OF FLANGES. Whenever flanged<br />

areas of a casting are radiographed, the radiograph<br />

should cover the flanges, the cylindrical wall, and the<br />

corner between them. Film should be placed under the<br />

flange and inside the casting, as shown in Figure 5-2.<br />

Two or three projections may be required since an<br />

exposure that shows shrinkage defects might not show<br />

tears. It is important the exposures provide a clear<br />

picture of the junction between the flange and the wall.<br />

The radiographs must show shrinkage completely if<br />

there is shrinkage in the flange and wall areas. Cracks<br />

and tears must be found if they are present in the fillet.<br />

Flange exposures should be made for the average<br />

thickness of the section being radiographed. Multiple<br />

film techniques should be used as necessary if multiple<br />

thicknesses are present in the radiographed section.<br />

page 43<br />

• RADIOGRAPHY OF VALVE BODIES. <strong>High</strong>-energy X<strong>ray</strong>s<br />

can penetrate both outside walls and provide the<br />

necessary sensitivity for demonstrating internal section<br />

defect when applied to small and some large valve<br />

bodies. This is especially true in the critical valve seat<br />

areas. Exposures are made by placing the film behind<br />

the valve body and beaming into the object at the best<br />

angle to project the critical internal section onto the<br />

film. Blocking, filtering, or other scatter reduction<br />

techniques should be used to ensure maximum<br />

sensitivity. A large D/T ratio is needed to minimize<br />

distortion and undesirable enlargement.<br />

FIGURE 5-2. Typical flanged casting exposure plan showing 12<br />

exposures at 30˚ increments for three beam orientations (cr =<br />

central <strong>ray</strong>).<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Radiography of Welds<br />

Radiography is one of the most widely used inspection<br />

techniques and still remains the most reliable choice for<br />

weld inspection. Because radiographic weld inspections are<br />

often controlled by mandatory procedures with codified<br />

accept-reject criteria, the radiographer should know the<br />

specified requirements, and as much as possible about the<br />

specific fabrication before deciding to apply a certain<br />

procedure. To assure the appropriate inspection is<br />

conducted, the radiographer must know the ability of each<br />

radiographic procedure and technique to form images of<br />

defects. For example, the orientation of weld defects is<br />

often known and should determine the optimum<br />

radiographic coverage and angulation to provide the best<br />

inspection.<br />

Frequently, the defect of most concern is the crack, and<br />

small cracks are hardest to detect. The probability of crack<br />

detection by radiography is a function of crack width,<br />

orientation, and X-<strong>ray</strong> machine sensitivity. A<br />

supplementary test such as ultrasonic examination may be<br />

required since it is often not practical to exhaust all<br />

possible angulations of an X-<strong>ray</strong> beam in order to increase<br />

the crack detection probability. The following list describes<br />

defects that are common to most welding and can be<br />

revealed by radiography.<br />

• CRACKS can occur in the weld metal (centerline<br />

shrinkage cracks, root cracks, etc.), in the heat-affected<br />

zone and in the base metal. They appear on the<br />

radiograph as dark lines with sharp distinct edge, or<br />

edges that are fuzzy and diffused.<br />

page 44<br />

• LACK OF PENETRATION is failure to melt the base<br />

metal during the stringer pass weld. It appears on the<br />

radiograph as a straight dark line at the center of the<br />

weld This defect is usually caused by improper heat or<br />

choice of weld rod.<br />

• INCOMPLETE FUSION is failure of the weld metal to<br />

fuse to the base metal. This appears as slightly wavy<br />

lines running parallel to the weld length and off the<br />

centerline of the weld.<br />

• SLAG, TUNGSTEN, AND OTHER INCLUSIONS are<br />

caused by entrapment of foreign material in the weld<br />

metal. This defect appears on the radiograph as<br />

irregularly shaped high or low-density areas depending<br />

upon the material entrapped.<br />

• POROSITY is gas entrapped in the weld metal. This<br />

appears on the radiograph as small, globular shaped dark<br />

voids. This can be linear in nature or can be scattered<br />

throughout the weld metal.<br />

• UNDERCUT is base metal sucked into the cover pass<br />

causing a reduction of thickness at the juncture. This<br />

appears on the radiograph as darker lines along the edges<br />

of the weld.<br />

• CONCAVITY occurs on joints that are welded from one<br />

side only, where excessive melting of the underside<br />

occurs, causing it to be pulled into the joint.<br />

• CENTERLINE CREVICE.<br />

• JOINT DISTORTION, MISMATCH, AND WELD<br />

MISPLACEMENT.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Radiographic Coverage<br />

* There are special requirements for the radiography of all<br />

welds that may not be found in other radiographic<br />

applications. These requirements are as follows.<br />

(1) Film with the highest contrast gradient consistent with<br />

acceptable exposure times should be used.<br />

2) The exposure should obtain the highest film densities<br />

that can be viewed conveniently.<br />

Full Length Of Film<br />

Inches cm<br />

6 15.2<br />

8 20.3<br />

10 25.4<br />

12 30.5<br />

14 35.6<br />

16 40.6<br />

18 45.7<br />

19 48.3<br />

Angle from Central Ray to<br />

Film Edge (degrees)<br />

2.4<br />

3.2<br />

4.0<br />

4.8<br />

5.5<br />

6.3<br />

7.1<br />

7.5<br />

Table 5-3 Angle From Central Ray to Film Edge at 72 Inch (1.83 m) SF<br />

page 45<br />

(3) To demonstrate transverse cracks, longitudinal<br />

coverage per exposure should not exceed the<br />

maximum permissible projection angles that the<br />

radiation source makes with the film ends, unless<br />

otherwise specified. This is shown in Table 5-3 for a<br />

1.83 meter SFD distance as an example.<br />

The sensitivity required to demonstrate cracks at a<br />

projection angle of 3˚ for various crack separation widths<br />

and material thicknesses is shown in Table 5.4. These data<br />

are calculated from the relationship Δx = W/sin ø<br />

(See Figure 5-1).<br />

<strong>Varian</strong> <strong>Linatron</strong> applications<br />

Ratio of Crack Thickness & Width<br />

(T/W) that Presents an Open<br />

Channel For the x-<strong>ray</strong>s<br />

24 to 1<br />

18 to 1<br />

14 to 1<br />

12 to 1<br />

10 to 1<br />

9 to 1<br />

8 to 1<br />

7.6 to 1


The width of separation required for sensitivity<br />

demonstration is increased proportionately if the<br />

projection angle is increased. The demonstrated crack<br />

width is decreased proportionally if the sensitivity is<br />

improved, i.e. from 1% to 0.5%.<br />

The data given in Table 5-4 provide general guidelines<br />

only. Cracks do not follow a single plane and sometimes<br />

portions of the crack edges will not be parallel to the<br />

radiation beam in actual practice.<br />

Weld Thickness<br />

Inches cm<br />

2 5.1<br />

4 10.2<br />

6 15.2<br />

8 20.3<br />

10 25.4<br />

10 25.4<br />

1 30.5<br />

12 30.5<br />

15 38.1<br />

15 38.1<br />

Crack Separations<br />

Mils mm<br />

1.0 0.03<br />

2.0 0.05<br />

1.5 0.04<br />

2.0 0.05<br />

2.5 0.06<br />

5.0 0.13<br />

3.0 0.08<br />

6.0 0.15<br />

3.3 0.08<br />

7.5 0.19<br />

Table 5-4 Sensitivity Needed to Show Cracks at Angles 3˚ to the Beam<br />

page 46<br />

• CIRCUMFERENTIAL BUTT WELDS. Radiographs of<br />

circumferential butt welds in heavy sections usually are<br />

obtained with the source outside the circumference. Care<br />

must be exercised when radiographing curved sections<br />

with this technique. Be aware that small transverse<br />

cracks may be obscured if the projection angles are too<br />

large. Therefore, the film coverage must be reduced to<br />

control the projection angle through the curved section.<br />

Image quality indicator placement should be the same as<br />

linear welds. Distortion from projection is increased<br />

when film holders are made to conform to the inside<br />

curvature. Consequently, the use of rigid cassettes with a<br />

suitable front filter is recommended.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications<br />

Sensitivity Required (%)<br />

1.0<br />

1.0<br />

0.5<br />

1.0<br />

0.5<br />

1.0<br />

0.5<br />

1.0<br />

0.5<br />

1.0


• T-SECTIONS. T-Section welds present problems that<br />

are solved only by the radiographer ingenuity. It may be<br />

necessary to take two projections to ensure adequate<br />

examination. For example, when a dome is welded to a<br />

heavy flange (with a double-J bevel), orient one<br />

projection parallel to the flange surface and the other at a<br />

projection angle near the angle of the bevel. A<br />

projection parallel to the surface should be made if the<br />

flange material is rolled stock with the weld attachment<br />

perpendicular to the rolling direction. Many highly<br />

stressed T-weld failures occur because of cracking in the<br />

parent material beneath the weld.<br />

Design and Placement of Image Quality Indicators<br />

(IQI). A typical practice is to require at least two IQls per<br />

exposure area. These are placed at the limits of film<br />

coverage adjacent to the weld. If weld reinforcement is not<br />

removed, the IQI must be shimmed up so that the total<br />

thickness under the IQI is equal to the total thickness<br />

through the weld. This includes backing strips that were<br />

not removed. In the United States, ASTM plaque-type IQI<br />

are usually required. In Europe, DIN, International<br />

lnsitute of Welding (IIW), or AFNOR (French) IQls may<br />

be used. Reports correlating sensitivities of various IQls<br />

are listed in the Bibliography.<br />

FIGURE 5-3. Typical rocket motor configuration.<br />

page 47<br />

Defect Location. The linear extent of defects can be<br />

determined by comparing radiographs with markers placed<br />

adjacent to the welds. It is sometimes necessary to locate<br />

the depth of defects to determine which side of the weld<br />

should be excavated for repair. This is done by making a<br />

double exposure with a shift of the source across the length<br />

of the defect. Defect depth is a simple ratio of the defect<br />

shift compared to the shift of the marker on the surface,<br />

relative to the known weld thickness.<br />

Radiography of Rocket Motors<br />

Solid propellant rocket motors are made with a wide range<br />

of diameters, and with a variety of bore configurations as<br />

shown in Figure 5-3. A solid propellant rocket motor<br />

consists of a rigid case, an internally bonded insulator and<br />

liner, and solid propellant. These are shown in Figure 5-4.<br />

These propellant configurations have a burning surface<br />

area that normally produces a predictable pressure/flight<br />

curve. If this area is increased by the presence of a crack,<br />

void, or separation, overpressurization of the case can<br />

occur, causing a malfunction. One or more nozzles at the<br />

back end complete the basic motor.<br />

FIGURE 5-4. Cross section of front end of solid rocket motor,<br />

showing construction details for radiographic examination.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


The propellant in large motors is often adhesively bonded<br />

to the liner to provide structural support and to restrict the<br />

burning to the bore surfaces and typically provide low<br />

subject contrast when radiographed. Therefore, every<br />

precaution must be taken to increase the radiographic<br />

contrast. This contrast can be greatly enhanced by<br />

selecting the proper X-<strong>ray</strong> energy.<br />

MeV<br />

1<br />

2<br />

6<br />

9<br />

15<br />

Propellant Thickness Range<br />

inches cm<br />

2-25 5.1 - 63.5<br />

6-33 15.2 - 83.8<br />

8-48 20.3 - 121.9<br />

12-65 30.5 - 165.1<br />

16-100+ 40.6 - 254.0+<br />

Table 5-5 Thickness Range for Routine Radiography with<br />

<strong>Linatron</strong> Sources<br />

Table 5-5 lists practical radiography ranges for solid<br />

propellant. The table shows that a <strong>Linatron</strong> providing X<strong>ray</strong><br />

energies of 1, 2, 6, 9, and 15 MeV, covers the<br />

radiographic range for solid propellant from 2 inches (5.1<br />

cm) to over 100 inches (2.54 m) in thickness. Radiography<br />

of the propellant grain and the peripheral bonded regions,<br />

including the front and back domes, is normally required.<br />

Radiographs of the grain should reveal the presence of<br />

cracks, voids, non-uniform mixing, lack of bond between<br />

internal interfaces, bore deformation, foreign material,<br />

excessive porosity, low-density volumes, and other defects<br />

that are characteristic of the propellant type and the<br />

manufacturing process.<br />

Tangential radiography of peripheral areas reveals interpropellant<br />

bond failures, deterioration or separation of the<br />

liner-propellant bond, insulation failure, peripheral<br />

porosity, and other substandard conditions. Radiographs<br />

are also used to judge the quality of repair work in rocket<br />

motors.<br />

page 48<br />

FIGURE 5-5. Typical roll stand to support rocket motor for horizontal<br />

radiography.<br />

Motor Attitude and Support Equipment. Radiography<br />

of many solid propellant rocket motors is best<br />

accomplished with the motor horizontal on a roller<br />

support stand as illustrated in Figure 5-5. The structural<br />

strength of the motor must allow it to be placed in the<br />

horizontal position, and a method used for support during<br />

rotation. An effective arrangement is to position the X-<strong>ray</strong><br />

source above the motor with film for the grain exposures<br />

placed on a shelf below the area to be covered. It is easily<br />

changed to accommodate larger or smaller motors, it<br />

makes the bore accessible, and it allows tangential shields<br />

and film holders to be placed along both sides of the<br />

motor for tangential exposures. The vertical position is<br />

used when the structural strength of the motor case will<br />

not support the weight of the motor in the horizontal<br />

position. This type of radiography requires mounting<br />

equipment such as a turntable (see Figure 5-7). Adapter<br />

rings, handling yokes, belt slings and other specialized<br />

devices.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Rocket Motor Radiographic Procedures. Radiography<br />

of the grain of a solid propellant rocket motor is usually<br />

performed in accordance with an established layout and<br />

exposure plan designed to give complete coverage of the<br />

entire grain. The cylinder is divided into a number of<br />

segments that correspond to the film centers and range.<br />

These segments may be exposed individually, or they may<br />

be grouped into exposure regions, with several films<br />

exposed simultaneously. In addition to specifying the film<br />

locations, the plans should show the exact location and<br />

direction of the central <strong>ray</strong>. A significant amount of film<br />

overlap is used in most plans to ensure complete coverage.<br />

The overlap also allows some of the propellant to be<br />

exposed a second time at a different angle. This offers an<br />

added opportunity to show cracks that may be present but<br />

at an angle that would not show detection in the first<br />

exposure.<br />

FIGURE 5-6. Typical turntable for vertical rocket motor radiography.<br />

page 49<br />

The dome and tangential areas require separate exposures.<br />

Plaque or wire-type image quality indicators should be<br />

placed on the front (source side) of the motor, so that at<br />

least one such image appears on a film in each exposure.<br />

Plaque-type IQI thickness need not be more than 1% of<br />

the average propellant thickness penetrated. The source-tofilm<br />

distance should be as large as practical.<br />

The angle from the central <strong>ray</strong> to the edge of the film<br />

should not exceed 15 degrees when calculating the film<br />

coverage for a grain exposure layout. Lead front and back<br />

screens (or equivalent screens made of other materials such<br />

as tungsten, copper, tantalum, or fluorometallics), at a<br />

thickness of 20 mils (0.51 mm), should be used. In some<br />

instances, cassette filters may be required to control the<br />

effects of this scatter. The film holders should be placed as<br />

close to the back of the motor as possible for the through<br />

body exposures. Ideally they should be enclosed in an<br />

evacuated envelope to ensure film-screen contact. The<br />

film-screen contact should be maintained by springpressure<br />

cassettes or other mechanical means if a vacuum<br />

system is not available.<br />

For x-<strong>ray</strong>ing propellants, ideal film densities are from 1.5<br />

to 3.0. When thicknesses are greater than those that will<br />

render these densities, the multiple (two-speed) film<br />

technique should be used. Although film exposure curves<br />

will normally indicate film combinations that can be used<br />

for various thick- nesses, some experimental exposures are<br />

usually required to finalize film selection and exposure.<br />

Occasionally, a thin lead foil is used as a separator between<br />

films when optimum intensification and definition are<br />

required.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Grain Radiography Coverage Requirements. Contrast<br />

sensitivities of better than 1% can be achieved routinely<br />

with the <strong>Linatron</strong> using optimum radiographic production<br />

techniques. Defects such as voids and gross density<br />

variations in the solid propellant are readily detected at that<br />

sensitivity. The simplest radiographic procedure (e.g., one<br />

exposure through the grain or two exposures, one at 0˚ and<br />

the second at 90˚ may be used when these are the only<br />

concern. However, cracks and separations are also of great<br />

concern in rocket motors.<br />

Cracks with widths of 1 to 5 mils (0.03 - 0.13 mm) are<br />

detected only when they are aligned with the radiation<br />

source. Most propellants with cracks will open to a width<br />

of 10 to 30 mils (0.25 - 0.76 mm) minimum. At these<br />

widths cracks can readily be detected at almost any angle to<br />

the radiation, and through large thicknesses of propellant.<br />

FIGURE 5-7. Visualization of crack-like defects, as a function of<br />

propellant thickness and crack angle, for x/x = 0.2%.<br />

Figure 5-7 illustrates the width of crack-like defects that<br />

can be demonstrated through various thicknesses of<br />

propellant, at various projection angles, with an assumed<br />

contrast sensitivity of 0.2%. Refer to the approximate<br />

relationship Δx = W/ø. It can be seen from Figure 5-7, as<br />

propellant thickness increases, the ratio W/ø increases,<br />

which means that the same width crack will be shown at<br />

smaller angles. For example,<br />

page 50<br />

Propellant Thickness Ratio of Crack Width<br />

to Projection Angle<br />

inches cm<br />

<strong>Varian</strong> <strong>Linatron</strong> applications<br />

30-36 76.2 - 91.4 W/ø ≈ 1.0<br />

40-50 101.6 - 127.0 W/ø ≈ 1.5<br />

50-60 127.0 - 152.4 W/ø ≈ 2.0<br />

To observe the required rocket grain cracks, the number of<br />

exposures must be increased as the diameter increases. If<br />

the technique being used produces contrast sensitivity<br />

other thanAx/x = 0.2%, the procedures must be modified<br />

accordingly to obtain an equivalent defect detectability.<br />

Tangential Radiography. Propellant-to-insulation (liner<br />

separations) in the domes are considered critical defects<br />

wherever they occur in a rocket motor. Separations as small<br />

as 2 mils (0.05 mm) can be shown on the radiograph,<br />

when the separation occurs at the tangential point.<br />

FIGURE 5-8. Probability (P) of detecting propellant to insulation<br />

separation versus number of exposures (N) for various circumferential<br />

lengths of separation (Lc , for 54-inch (137 cm) diameter (D),<br />

rocket motor, P = Lc/n - D N.


Tangential radiography is performed by placing the area of<br />

inspection at nearly right angles to the x-<strong>ray</strong> beam. The x<strong>ray</strong><br />

forming the outermost part of the cone of radiation<br />

will pass through the interfaces formed by the successive<br />

diameters of the propellant, insulator, and case. By placing<br />

the film against the motor case, below the inspection area,<br />

a radiographic image of the tangential points of the<br />

successive interfaces is formed. The detectability of a<br />

separation depends upon the number of tangential<br />

exposures, as illustrated in Figure 5-8.<br />

Example<br />

12 tangential exposures evenly distributed around a 54inch-diameter<br />

(1 37.2 cm) motor have a 50% probability<br />

of showing an area of separation that extends 7 inches (1<br />

7.8 cm) around the periphery and 100% probability of<br />

showing an area extended 15 inches (38.1 cm) or more<br />

around the periphery.<br />

Tangential Radiography Coverage Requirements.<br />

Radiography of the peripheral areas of the dome and<br />

cylindrical areas of a solid propellant rocket motor requires<br />

an exposure plan similar to the plan for the grain. In fact,<br />

the same layout and marking may be used for the<br />

tangential exposures as for the grain. The central <strong>ray</strong><br />

positions depend on the size of the motor and on the<br />

particular source to be used. The grain exposure with<br />

simultaneous bilateral tangential exposures can be made by<br />

directing the central <strong>ray</strong> radially because of the <strong>Linatron</strong>’s<br />

high output intensities and large radiation cones. With a<br />

less powerful source or one with a small cone of radiation,<br />

only one side of the motor can be exposed at a time. In<br />

general there is no need to use the two-film technique,<br />

since one film may have sufficient latitude to show the<br />

critical areas inside the case. Some experimental exposure<br />

tests may be needed to finalize the optimum technique.<br />

Tangential shielding may be required to reduce the forward<br />

scatter that is characteristic tangential radiographs. This<br />

occurs because of the very small angle between the primary<br />

beam and the object during tangential radiography. A lead<br />

shield can be added to the outer surface of the motor at<br />

the tangential point when exposures with very high<br />

contrast sensitivity are required. The attenuation of the<br />

shield should be approximately the same as the average<br />

attenuation of the chord at the propellant interface.<br />

page 51<br />

Wires and slits with thicknesses often less than 1% of the<br />

total equivalent chord at the propellant interface have been<br />

employed in tangential radiography. Lead screen and filters<br />

should be used like grain exposures. The interface image is<br />

a projection since the curvature of a motor prevents the<br />

placement of film close to the tangent point. For this<br />

reason the largest source-to-film distance possible should<br />

be used.<br />

Assembly Radiography<br />

Assemblies such as jet engines, gas turbines, valves, nuclear<br />

fuel elements, and explosive devices (e.g. bombs and fuzes)<br />

are frequently radiographed with high-energy x-<strong>ray</strong>s to<br />

show internal conditions or dimensions. These assemblies<br />

may have material thicknesses that vary by several HVLs at<br />

adjacent regions. Also, many assemblies can have material<br />

and assembly characteristics that produce forward scatter,<br />

which obscures the sharpness of the radiographic image.<br />

The following good radiographic practices should be<br />

observed when establishing the techniques:<br />

• Use the highest practical x-<strong>ray</strong> energy to minimize the<br />

effect of forward scatter.<br />

• Use object-film filters and screen-film combinations that<br />

produce the highest contrast and best sharpness.<br />

• Use large D/T ratios to avoid distortion.<br />

• For radiography of a radioactive object, place the film at a<br />

distance from the object sufficient to reduce fogging of<br />

the film by the object’s radiation. Also, use an object-film<br />

filter in back of the object to further reduce object effects.<br />

• Use multifilm techniques where thickness variations<br />

exceed the range of a single film.<br />

• Exposure times for each film may be obtained from<br />

established exposure curves when the average thickness of<br />

the objects in the area of penetration is known.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Bibliography<br />

Books<br />

Practical Radiography for Industry<br />

H. R. Clauser<br />

Reinhold Publishing Co., N.Y. (1 952)<br />

Applied X- Rays<br />

G. L. Clark<br />

McGraw Hill Book Co., N.Y.<br />

4th Edition, (1 955)<br />

Handbook of Radiology<br />

Editors-R. H. Morgan & K. E. Corrigan<br />

The Year Book Publishers, Chicago (1 955)<br />

A Further Handbook of Industrial Radiology<br />

Editor-W. J. Wilshire<br />

Edward Arnold & Co., London (1957)<br />

Handbook of Nondestructive Testing<br />

Editor-R. C. McMaster<br />

Roland Press, N.Y. (1 960)<br />

Techniques of Nondestructive Testing<br />

Editors-C. A. Hogarth & J. Blitz<br />

Butterworth & Co., London (1 960)<br />

Nondestructive Testing<br />

W. J. McGonnagle<br />

McGraw Hill Book Co., N.Y. (1961)<br />

An Introduction to Industrial Radiology<br />

J. C. Rockley<br />

Butterworth & Co., London (1 964)<br />

Physics of Industrial Radiology<br />

Editor-R. Halmshaw<br />

American Elsevier Publishing Co., N.Y. (1966)<br />

Industrial X-Ray Interpretation<br />

Justin G. Schneeman<br />

lntex Publishing Co., IL (1968)<br />

Radiography in Modern Industry<br />

Eastman Kodak Company, Rochester, N.Y.<br />

4th Edition (1 979)<br />

Industrial Radiology Techniques<br />

R. Halmshaw<br />

Wykeham Publishing Co., London (1 971 )<br />

page 52<br />

Sections of Books and Technical Reports<br />

Radiography with <strong>High</strong>-<strong>Energy</strong> Radiation<br />

C. C. Pollitt<br />

Journal of the British Steel Castings<br />

Research Association, No. 65, Feb. 1962<br />

10-MeV X-Ray Technique<br />

D. T. O’Connor, E. L. Criscuolo, & A. L. Pace<br />

Special Technical Publication No. 96<br />

American Society for Testing & Materials<br />

Radiology with <strong>High</strong>-<strong>Energy</strong> X-Rays<br />

R. Halmshaw & C. C. Pollitt<br />

Progress i n Non- Des t ruct ive Testing<br />

Vol. 2, Heywood & Co., London (1959)<br />

10- MeV Rotating Target Linear Accelerator for<br />

Radiography of Large Rocket Motors<br />

J. H. Cusick & J. Haimson<br />

Proceedings, Missiles & Rockets Symposium,<br />

U.S. Naval Ammunition Depot, Concord, Ca.(1961)<br />

Radiography of Large Missiles<br />

With the Linear Electron Accelerator<br />

J. Haimson<br />

Nondestructive Testing, Mar-Apr 1963<br />

<strong>High</strong> - <strong>Energy</strong> Radiography in the 6- to 30-MeV Range<br />

J. H. Bly & E. A. Burrill<br />

Special Technical Publication No. 278<br />

American Society for Testing & Materials (1959)<br />

<strong>High</strong> Voltage Radiography<br />

Section No. 23 of the “Handbook of Nondestructive<br />

Testing”, Editor R. C. McMaster,<br />

Roland Press, N.Y. (1 960)<br />

Radiographic lnspection<br />

Section in “Metals Handbook”, Vol. 11, 8th<br />

Edition, American Society for Metals, 1978.<br />

Nondestructive Testing Handbook<br />

Editors - Paul Mclntire and Lawrence E. Bryant.<br />

American Society for Nondestructive Testing.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


<strong>High</strong> <strong>Energy</strong> Real-Time Radiographic Imaging<br />

Real Time Radiography can be defined as nondestructive<br />

radiographic testing where an image of the test object is<br />

viewed concurrently with the irradiation. This method of<br />

inspection is relatively new to nondestructive testing but is<br />

an outgrowth of fluoroscopy, which has been used in the<br />

industrial field for many years. The technology has made<br />

great leaps, with improvements in image processing,<br />

development of new fluors and camera designs.<br />

FIGURE 6-1. Typical real-time x-<strong>ray</strong> imaging system.<br />

page 53<br />

Imaging Heads - In general, high energy real time<br />

radiography imaging heads (cameras) have three main<br />

components, the imaging screen, lens system and low-light<br />

video camera. The imaging screen directly converts x-<strong>ray</strong>s<br />

into low-level light, usually in the yellow/green part of the<br />

visible spectrum. The lens system contains one or more<br />

large aperture lenses that couple the light to the low-light<br />

video camera.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Normally, the light generated in the imaging screen is<br />

coupled to the lens-camera system by a front surface mirror<br />

mounted at 45 degrees to the screen. This positions the<br />

camera and lenses outside the cone of direct radiation,<br />

minimizing damage to these components.<br />

In general, two types of low-light video cameras are used in<br />

real-time radiography, Silicon Intensified Target (SIT) and<br />

Image lsocon video tube cameras. SIT cameras have<br />

excellent low-light sensitivity and are compact, rugged and<br />

require no special cooling. Image lsocons have more<br />

dynamic range and spatial resolution but are very position<br />

sensitive and require special cooling.<br />

Because Image lsocons are physically larger tubes, these<br />

cameras are generally larger and vibration sensitive. SIT<br />

tubes are small, low cost and more adaptable to special<br />

applications.<br />

Signal Processing - Signals from real-time cameras are<br />

digitized and stored in digital memory for further<br />

processing or archival storage. The digital memory is part of<br />

an image processor, which is a specialized computer system<br />

designed to process image data, most often in real time.<br />

FIGURE 6-2. Schematic of ER real-time system functional elements.<br />

page 54<br />

Image processors can vary considerably from systems that<br />

only have the ability to acquire individual video frames to<br />

systems that can perform complicated image filtering<br />

and/or transforms. Images stored and processed by the<br />

image processor are displayed on a high resolution video<br />

monitor for interpretation. This is illustrated in Figure 6-2.<br />

Archival Storage - Archival storage is necessary to keep an<br />

image record of inspection procedures performed. Two<br />

basic methods are used to store real-time radiography<br />

images, analog and digital. The most popular, and<br />

presently least expensive, method to store real-time images<br />

is high bandwidth analog video tape. Any image presented<br />

on the video monitor will be recorded on video tape.<br />

Additionally, images can be annotated verbally on the<br />

video tape’s audio track.<br />

Images may also be stored digitally on hard disk, floppy<br />

diskette, magnetic tape and optical laser disk. Magnetic<br />

tape and optical laser disk have the most capacity, but<br />

magnetic tape is classified as a volatile medium with a<br />

definite possibility for the data to be corrupted by<br />

magnetic fields, erased or being overwritten.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Optical disks are classified as non-volatile because they can<br />

be written to once, read as many times as desired and<br />

cannot be erased. Therefore, optical disks are the digital<br />

equivalent to standard film. Additionally, optical disks have<br />

a very high capacity. Present optical disks can store up to<br />

8000 images per disk pack. Since disk packs are removable,<br />

virtually unlimited storage is possible.<br />

Hard disk storage is usually an intermediate digital storage<br />

before transferring the images to optical disk, magnetic<br />

tape or floppy diskette. This is because the hard disk has a<br />

definite limit on storage capacity. Therefore, image data<br />

must be regularly erased to make room for more data.<br />

Operator Control - Early real-time radiography system<br />

operator controls were a collection of the individual<br />

component controls mounted on an operators console.<br />

The trend for present systems is to integrate all of the<br />

controls from the separate components that make up a<br />

real-time system into one centralized control system. This<br />

is most often accomplished by controlling all system<br />

components with a centralized computer system.<br />

Today it is possible to use a real-time radiography system as<br />

the control core of an automated radiographic inspection<br />

system. This requires communication and control<br />

protocols between the imaging system and the parts<br />

handling device (manipulator) - and possibly other<br />

peripherals - and the ability for the imaging system to<br />

perform programmable inspection sequences. Then, after<br />

the part is loaded and the x-<strong>ray</strong> source and camera are<br />

aligned to an initial position, the control computer can<br />

control the rest of the inspection process.<br />

<strong>Applications</strong><br />

Real-time radiography applications can be generally<br />

divided into two subsections, actual real-time imaging<br />

where processes are examined for dynamic function and<br />

automated test sequences where high test throughput and<br />

low-cost is the primary function.<br />

Test procedures such as observing the pattern of metal<br />

filling molds and observing the function of motor<br />

components while the motor is actually running are typical<br />

dynamic function applications. It is also often necessary to<br />

use real-time systems to properly position test objects<br />

where the inner mechanism is unknown or obscure.<br />

page 55<br />

Automated testing has become more important in recent<br />

times because of an emphasis upon 100% testing of critical<br />

components. Real time systems, in conjunction with parts<br />

handling systems (manipulators) and integrated system<br />

control, allow automated test sequencing with higher<br />

throughputs and more coverage than previous film systems.<br />

Figure 6-3 illustrated a real-time automated inspection<br />

system.<br />

The following characteristics should be considered when<br />

planning a real-time radiography application:<br />

X-<strong>ray</strong> energy - Selection of an x-<strong>ray</strong> energy for real-time<br />

imaging should be based upon several considerations.<br />

Selection of an energy that is too great for the part being<br />

inspected can lead to difficulties. When the energy is so<br />

high that the material does not present at least 1.5 half<br />

value layers, small changes in attenuation may be lost.<br />

Additionally, radiation buildup can cause tremendous<br />

scatter problems when x-<strong>ray</strong>ing thin sections. This is<br />

stabilized after approximately 1.5 HVLs. This thickness is<br />

called the “equilibrium” thickness.<br />

Selecting too low an energy also presents problems,<br />

especially when actual real-time images are important. In<br />

general, dynamic real-time radiography is like taking<br />

pictures at a thirtieth of a second per image. If the<br />

radiation energy or output is too low, little detail will be<br />

seen in the image. This imaging time can be lengthened by<br />

averaging two or more frames together. However, enough<br />

radiation must be reaching the imaging screen to provide<br />

the amount of light on the conversion screen needed for<br />

proper image evaluation.<br />

Ideally, x-<strong>ray</strong> energy and output is chosen so that 4 to 7<br />

half value layers are being examined and the radiation to<br />

the imaging screen exceeds 15 to 25 rads/min. However,<br />

real-time systems can be useful at extremes outside of this<br />

ideal envelope.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FIGURE 6-3. Real-time automated inspection system.<br />

page 56<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Real-time inspection applications, using proper technique,<br />

have been successful for up to twelve half value layers.<br />

However, throughput suffers when the long image<br />

exposures for this type of imaging are used.<br />

Collimators - When real-time imaging is being performed,<br />

it is extremely important to restrict the x-<strong>ray</strong> beam to the<br />

area that is being inspected. Remote controlled collimators<br />

are very useful in real-time radiography because the size<br />

and shape of the collimated beam can be seen on the<br />

imaging screen in the control room in “real-time”, allowing<br />

the operator to select the exact area desired for viewing.<br />

Additional collimation may be needed at the object being<br />

inspected to control scattered radiation. This can be<br />

located either on the x-<strong>ray</strong> side of the object or on the<br />

screen side of the object, depending upon the needs of the<br />

situation.<br />

These are termed “pre-collimators” and “postcollimators”,<br />

respectively, and are similar to the practice of “blocking”<br />

except that these collimators restrict the beam to the size of<br />

the imaging screen, while blocking is only shielding placed<br />

around the item being inspected.<br />

Manipulators - A key factor in real-time radiography is the<br />

ability to manipulate the item under inspection<br />

automatically or by remote control.<br />

To inspect complicated items, manipulators (or parts<br />

handling systems) must be accurately controllable and<br />

repeatable. For automated imaging applications,<br />

manipulators are programmed to follow predictable,<br />

planned paths during the inspection.<br />

The design of manipulators is very applications specific<br />

and the system integration needed for automated test<br />

sequences is challenging. In general, the manipulator must<br />

have sufficient flexibility to position the inspected object<br />

under inspection properly for the total x-<strong>ray</strong> inspection.<br />

Control of the manipulator can be a remote manual<br />

console or the controls can be integrated into the imaging<br />

system. Integrating manipulator control with the imaging<br />

system allows completely autamatic inspection sequences.<br />

page 57<br />

Screens/Filters - A distinction should be made between<br />

conversion screens used in real-time radiography, which<br />

directly convert x-<strong>ray</strong>s to visible light, and intensifying<br />

screens, which filter low energy x-<strong>ray</strong>s and emit<br />

intensifying photoelectrons to increase light output.<br />

Real-time radiography uses several different types of<br />

conversion screens. For low energy, these screens can be<br />

used without intensifying filters. However, for higher<br />

energies, intensifying filters (screens) are used to provide<br />

better image contrast. The combination of conversion<br />

screen and filter depend upon the application.<br />

As higher energies are used, image degradation results from<br />

high energy photons passing through the conversion screen<br />

without sufficient interaction with the phosphors in the<br />

screen. By adding a heavy metal intensifying screen on the<br />

x-<strong>ray</strong> side of the fluorescent (conversion) screen, “knock<br />

out” electrons are emitted which interact with the<br />

phosphors of the screen. These intensifying screens are<br />

usually made from tungsten or tantalum. Their thickness<br />

requirement is a function of the x-<strong>ray</strong> energy, but in<br />

practice 0.020 inch (0.50 mm) thick tantalum is used for<br />

energies from 2 to 6 MV and 0.040 inch (1 mm) thick<br />

tantalum for higher energies.<br />

Fused scintillating fiber optic conversion screens are thicker<br />

than conventional fluoroscopic screens and do not<br />

generally need intensifying screens. Fiber optic screens<br />

exhibit excellent conversion efficiency, which is a function<br />

of the screen thickness, and low energy scatter rejection,<br />

which is a function of the collimating effect of the<br />

individual fibers. Fiber optic screens are especially effective<br />

in high scatter, high energy applications.<br />

Field of View - Real-time cameras generally provide more<br />

than one field of view by using two or more optical lenses<br />

to provide magnification. A magnified image results in<br />

higher resolution but with a smaller field of view and lower<br />

throughput. The application will determine which field of<br />

view is appropriate.<br />

Image Acquisition - There are generally three basic<br />

methods of image acquisition used in real-time<br />

radiography, real time, recursive averaging and integration<br />

(summation).<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Real-time image acquisition displays a new image at the<br />

basic frame rate. This is normally an image every thirtieth<br />

of a second. This mode of obtaining images is useful for<br />

observing the proper positioning of a part, collimator setup<br />

and screening applications where plenty of radiation<br />

output is available. Quantum fluctuation can have a large<br />

effect upon the detail that can be observed in an image.<br />

Recursive Averaging is a frame summing procedure that<br />

provides for a moving average image. The result of this<br />

procedure is to accumulate in memory an exponentially<br />

weighted sum of previously input frames. Because the<br />

memory is constantly being refreshed with a new image, it<br />

is possible to conduct motion imaging with an improved<br />

signal to noise ratio.<br />

The random noise will be reduced. However, as more<br />

frames are averaged, the time lag of the image also<br />

increases, making the use of this averaging technique less<br />

useful for motion imaging. Therefore, a balance must be<br />

found between noise improvement and image lag.<br />

Considering random noise only, integration (summation)<br />

increases the signal to noise ratio of the image by a factor<br />

of the square root of the number of integrated frames-<br />

(N) 1/2 . This method of image acquisition compares with<br />

film exposure methods and is widely used to improve<br />

image quality. Integration is used most often for static<br />

imaging rather than dynamic processes. For any given time<br />

of image acquisition, summation improves the image signal<br />

to noise ratio of the image more than recursive averaging.<br />

Image Processing - Real-time radiography provides several<br />

different types of image processing to improve the<br />

detectability of defects in the test object.<br />

page 58<br />

Contrast Enhancement or Stretching is the most common<br />

form of image processing. Often the important<br />

information in an image is contained in a small part of the<br />

contrast range available. Contrast enhancement allows<br />

using the total dynamic contrast range over a small<br />

statistical range. Contrast enhancement does not modifiy<br />

the original image data. It only modifies the way the data is<br />

displayed. Subtraction techniques subtract one image from<br />

another after moving either the x-<strong>ray</strong> source, the test object<br />

(or part of the test object) or the camera between images.<br />

Any data, such as systemic noise, that are common<br />

between the two images is subtracted out of the image.<br />

Several different subtraction methods can be used (shift<br />

subtract, mask subtract, etc.) depending upon the<br />

application. Care must be taken during subtract processes<br />

not to introduce false information into the resultant image.<br />

Additionally, the direction that the x-<strong>ray</strong> source, the object<br />

or the camera is moved is critical.<br />

Digital Filtering can remove high or low spatial frequency<br />

data from an image or Edge Enhancement can sharpen the<br />

representation of internal structure in a test object.<br />

Conclusion<br />

Real-time radiography is a nondestructive testing technique<br />

that is useful for dynamic imaging and automated highthroughput<br />

radiographic testing. Present real-time systems<br />

include an x-<strong>ray</strong> source, test-object manipulator, (partshandling<br />

system) and an imaging system for image<br />

acquisition, processing and archival.<br />

<strong>High</strong> energy applications of real-time radiography are<br />

rocket motor, ordnance and heavy casting inspection.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Glossary<br />

ABSORPTION<br />

Process in which X-<strong>ray</strong> photons, as they pass through a<br />

material, are absorbed in the material. (See<br />

PHOTOELECTRIC ABSORPTION and PAIR<br />

PRODUCTION).<br />

ATTENUATION<br />

Combination of absorption and scattering processes in<br />

which X-<strong>ray</strong>s, as they pass through material, are either<br />

stopped, or diverted from straight and forward travel. Total<br />

Attenuation, depending upon the X-<strong>ray</strong> energy, consists of:<br />

PHOTOELECTRIC ABSORPTION, COMPTON<br />

SCATTERING and PAIR PRODUCTION.<br />

BACKSCATTER<br />

Secondary radiation produced by scattering of X-<strong>ray</strong>s from<br />

their original (forward) direction through angles greater<br />

than 90 degrees.<br />

BEAM FLATTENER<br />

Cone shaped X-<strong>ray</strong> absorber placed centrally in the beam<br />

of a high-energy X-<strong>ray</strong> source, to absorb a relatively greater<br />

proportion of the high-intensity central <strong>ray</strong>s than of the<br />

<strong>ray</strong>s at the edges of the beam, to produce a more uniform<br />

X-<strong>ray</strong> intensity at the plane of the X-<strong>ray</strong> film. Also referred<br />

to as a BEAM COMPENSATOR.<br />

BEAMING<br />

The condition that higher radiation intensity occurs in the<br />

forward, central X-<strong>ray</strong>s from a high-energy X-<strong>ray</strong> source<br />

(target) than is emitted in all other directions. Caused by<br />

the large forward momentum of the accelerated electrons<br />

which strike the target to produce the X-<strong>ray</strong>s.<br />

BLOCKING<br />

Use of lead or other shielding material around the edges of<br />

the object being radiographed, to absorb scattered<br />

radiation that would otherwise expose and excessively<br />

darken areas of the X-<strong>ray</strong> film under the object.<br />

page 59<br />

BROAD BEAM<br />

Arrangement of the source, object and x-<strong>ray</strong> film (or other<br />

radiation detector) in which scattered radiation from the<br />

object contributes to the total exposure (at a given point)<br />

on the film; specifically, scattered radiation at solid angles<br />

greater than 0.01 steradian. The solid angle is formed by<br />

the point on the film and the perimeter of the exposed<br />

cross- sectioned area of the object. NARROW BEAM<br />

arrangements are those where scatter reaching the x-<strong>ray</strong><br />

film or detector is only that scatter radiation within angles<br />

less than 0.01 steradian.<br />

CENTRAL RAY<br />

Line within the x-<strong>ray</strong> beam, coincident with the direction<br />

of peak x-<strong>ray</strong> intensity, the (usually) central axis of the<br />

electron accelerator, and with the axis of the collimator. (It<br />

also coincides with the laser beam indicator in a <strong>Linatron</strong>.)<br />

COLLIMATOR<br />

<strong>High</strong>-density metal absorber with a conical (sometimes<br />

pyramid-shaped) opening for passage of x-<strong>ray</strong>s to produce<br />

a well-defined beam of x-<strong>ray</strong>s from the target.<br />

COMPENSATOR<br />

(See BEAM FLATTENER)<br />

COMPTON SCATIERING<br />

X-<strong>ray</strong> attenuation process in which a photon transfers<br />

energy and momentum to an orbital electron of the<br />

attenuating material, and continues to travel through the<br />

material at an angle to the original photon direction.<br />

CONTRAST<br />

RADIOGRAPHIC CONTRAST is the magnitude of the<br />

difference in density from one area to another on a<br />

radiograph resulting from variation in x-<strong>ray</strong> intensity<br />

transmitted through the corresponding sections<br />

(thicknesses) of the object being radiographed. SUBJECT<br />

CONTRAST refers to the ratio of radiation intensities<br />

transmitted through selected sections of the object, and is<br />

therefore a function of the thicknesses of those sections.<br />

(Also see: FILM CONTRAST)<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


D/T RATIO<br />

Ratio of the distance between the source (<strong>Linatron</strong> target)<br />

and the front surface of the object being radiographed to<br />

the distance from the front surface of the object to the film<br />

(usually the object thickness).<br />

DEFECTS<br />

Usually discontinuities and imperfections in the object<br />

being examined, considered deleterious to the service of the<br />

object, and which are revealed in <strong>Linatron</strong> radiography.<br />

Depending on the object and service requirements, Voids,<br />

Gaps, Separations, Cracks, Misassemblies, and other<br />

homogeneities may be identified as DEFECTS in a<br />

specification. (See Table 5-2, p. , also Table 5-3, p. )<br />

DEFINITION<br />

Fidelity in x-<strong>ray</strong> film images of sharp edges of the object,<br />

and the degree with which the detail of small defects and<br />

discontinuities are clearly shown. (See also:<br />

UNSHARPNESS)<br />

DENSITY (Film)<br />

Degree of blackening of the exposed and developed x-<strong>ray</strong><br />

film; DENSITY is usually expressed in terms of the H&D<br />

scale. (See H&D UNIT)<br />

DENSITY (Film) GRADIENT<br />

Amount of density change in the exposed and developed<br />

film per unit of change in the logarithm of the exposures.<br />

Film manufacturers also refer to density Gradient as the<br />

GAMMA ( y ) of the film at the particular density<br />

specified.<br />

DIFFERENTIAL ABSORPTION<br />

Differences in the x-<strong>ray</strong> absorption (and therefore the<br />

transmission through) various adjacent sections of an<br />

object being radiographed, which result in differences in<br />

the exposure to the film behind those areas.<br />

EDGE ENHANCEMENT<br />

TV scanning and electronic processing of radiographic<br />

(Real-Time or Film) images, that produce highlighting of<br />

edges of the object, defects, etc., in the final image. The<br />

resulting processed (edge-enhanced) images are displayed<br />

on a TV monitor.<br />

page 60<br />

ELECTRON EQUILIBRIUM<br />

Occurs in an x-<strong>ray</strong> measurement arrangement when, for<br />

electrons (set in motion by the x-<strong>ray</strong>s) leaving the<br />

measuring cavity, electrons of equal total energy enter.<br />

ELECTRON LINEAR ACCELERATOR<br />

A system containing an electron source, power supply,<br />

accelerator section, and metal target (when x-<strong>ray</strong>s are to be<br />

produced). The system generates high-energy x-<strong>ray</strong>s by<br />

accelerating the electrons to high energies and by directing<br />

the electrons in a linear path to collide with the metal target<br />

which results in producing x-<strong>ray</strong>s.<br />

ENERGY SPECTRUM (Photon)<br />

Distribution of x-<strong>ray</strong> intensity (or quantity of x-<strong>ray</strong><br />

photons) as a function of the x-<strong>ray</strong> energy in an x-<strong>ray</strong><br />

beam.<br />

EXPOSURE CURVE<br />

Plot of the exposure Rads vs material thickness, that gives<br />

the exposure conditions to obtain a radiograph with<br />

specific film density.<br />

FIELD COVERAGE<br />

Size of the area that can be exposed in a single radiographic<br />

exposure, for a particular source, collimator, and<br />

distance from the x-<strong>ray</strong> target.<br />

FIELD FLATNESS<br />

Degree of constancy of radiation intensity level across the<br />

field of an x-<strong>ray</strong> beam usually measured in a plane normal<br />

to the beam central axis.<br />

FIELD HALF-WIDTH<br />

Distance measured at the film plane outward from the<br />

central <strong>ray</strong> of the x-<strong>ray</strong> beam, to the outer edge of the x-<strong>ray</strong><br />

beam.<br />

FILM CHARACTERISTIC CURVE<br />

Plot of the relationship between exposure time and image<br />

density for a specific film and exposure strength. This term,<br />

in practice, is used only by the film manufacturer as one<br />

specification of the film’s properties. Film users who make<br />

measurements to determine this relationship with their x<strong>ray</strong><br />

source, exposure procedure, and film processing, refer<br />

to their results as: FILM RESPONSE CURVES.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


FILM CONTRAST<br />

Refers to the slope (steepness) of the FILM RESPONSE<br />

CURVE, and the resulting differences in film density<br />

achievable for a particular source, exposure technique, and<br />

processing; same as FILM GRADIENT. (See also<br />

CONTRAST)<br />

FILM GRADIENT<br />

(See FILM CONTRAST)<br />

FILM GRAIN<br />

The size, in general, of the original silver salt particles in<br />

the emulsion of the x-<strong>ray</strong> film. “Fine Grained Film” has<br />

very small silver salt particles. Finer film equates to smaller<br />

particle size and greater resolution. (Also see:<br />

GRAININESS)<br />

FILM RESPONSE CURVE<br />

(See FILM CHARACTERISTIC CURVE)<br />

FILM SPEED<br />

Sensitivity of the emulsion type to an x-<strong>ray</strong> exposure,<br />

expressed as the inverse of the amount of exposure needed<br />

to attain a specified FILM DENSITY.<br />

FILM SPEED INDEX<br />

As used in this Manual, it is a number assigned to each<br />

film type which is proportional to the rad exposure needed<br />

to attain a specified film density. (See Table 4.3, p.23)<br />

FLUORESCENTSCREEN<br />

A thin sheet of material, coated with a fluorescent salt<br />

(Calcium Tungstate, Gadolinium Oxysulfide, etc.), placed<br />

in contact with the front and back of the x-<strong>ray</strong> film in the<br />

film holder, to intensify the effect of the radiation arriving<br />

at the film holder.<br />

FOCAL SPOT SIZE<br />

Size of that area of the target in the electron accelerator<br />

from which x-<strong>ray</strong>s emanate for useful radiography.<br />

FORWARD SCATTER<br />

Secondary x-<strong>ray</strong>s emitted from the object being radiographed<br />

at small angles from the forward direction of the<br />

primary x-<strong>ray</strong> beam.<br />

page 61<br />

GRAININESS<br />

Refers to the “clumping” of the grains of silver that form in<br />

the exposed and developed emulsion of an x-<strong>ray</strong> film<br />

visible when viewing the film.<br />

H&D UNIT<br />

Unit for expressing FILM DENSITY and the scale for<br />

measuring film blackening; named after Hurter and<br />

Driffield who (in 1890) developed it. The film density at a<br />

point on an x-<strong>ray</strong>-exposed and developed film is<br />

determined from:<br />

DENSITY = Log 10 /lt H&D UNITS<br />

Where lo = Visible light intensity incident on the measured<br />

point of the film.<br />

L t = Visible light intensity transmitted through the<br />

measured point of the film.<br />

HALF-VALUE LAYER<br />

That thickness of material required to attenuate the x-<strong>ray</strong><br />

intensity by one-half.<br />

HARD PLATE X-RAY<br />

X-<strong>ray</strong> radiography which produces the radiographic image<br />

on an x-<strong>ray</strong> film.<br />

IMAGE SHARPNESS<br />

Fidelity attained in an x-<strong>ray</strong> image of a step or straight edge<br />

of the imaged object. (See UNSHARPNESS)<br />

INTENSIFYING SCREENS<br />

Thin sheet of lead or other material placed in contact with<br />

the x-<strong>ray</strong> film inside the film holder to increase the effect<br />

of the radiation resulting in a shorter exposure time. (See<br />

FLUORESCENT SCREEN)<br />

IQI<br />

An acronym for IMAGE QUALITY INDICATOR. A<br />

device, consisting of small wires, narrow slits, or a drilled<br />

hole strip of material with the same composition of the<br />

object being radiographed, and whose thickness or<br />

dimensions are a small percentage of the object’s thickness.<br />

When radiographed with the object, the device provides a<br />

measure of the contrast and resolution attained by the x<strong>ray</strong><br />

procedure.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


LINEAR ATTENUATION COEFFICIENT<br />

Constant used to describe the degree of x-<strong>ray</strong> attenuation<br />

per unit path length in a specified material. It is a function<br />

of x-<strong>ray</strong> energy and is usually expressed in units of<br />

reciprocal inch or centimeter.<br />

MAGNIFICATION<br />

Degree of projection and enlargement of regions of the<br />

object being radiographed in the developed film that result<br />

from the choice of distances between the source, object,<br />

and film in the radiography setup.<br />

NARROW BEAM<br />

(See BROAD BEAM)<br />

NDT<br />

An acronym of NONDESTRUCTIVE TESTING, and<br />

the name given to a test, inspection, or examination of<br />

materials to determine specific properties or characteristics,<br />

or to locate defects without causing damage to the object<br />

under test.<br />

PENETRAMETER<br />

Same as IQI.<br />

PAIR PRODUCTION<br />

An absorption process for photons of energies greater than<br />

1.02 MeV, in which the photon transforms into a pair of<br />

particles (an electron and a positron).<br />

PHOTOELECTRIC ABSORPTION<br />

An absorption process for photons of energies under<br />

1 MeV in which the photon loses all of its energy to an<br />

atomic electron. The electron leaves its atomic orbit and<br />

continues to move though the material.<br />

RAD<br />

Unit of radiation dose; 1 rad equals the absorption of 100<br />

ergs of (any form of) radiation per gram of absorbing<br />

material.<br />

RADIOGRAPHIC COVERAGE<br />

That section and area of the object that is radiographed,<br />

exposed and imaged on the x-<strong>ray</strong> film. The<br />

RADIOGRAPHIC COVERAGE is usually stated as part<br />

of the specifications for the radiography work.<br />

page 62<br />

REAL-TIME IMAGING<br />

X-<strong>ray</strong> radiography that produces instantaneous and<br />

continuous images on a TV monitor. The images obtained<br />

can be electronically processed to enhance their quality,<br />

and can be recorded (e.g., on videotape) for later playback.<br />

ROENTGEN<br />

Unit of radiation exposure (the ability of an x-<strong>ray</strong> beam to<br />

ionize air) corresponding to producing 1.610 x 1012 ion<br />

pairs per gram air.<br />

SCATTER mRADIATION<br />

Secondary x-<strong>ray</strong>s and electrons produced whenever a<br />

primary x-<strong>ray</strong> beam irradiates an object. Also includes<br />

objects not being examined such as the floor, walls, tables,<br />

etc. Secondary radiations are emitted in all directions, and<br />

are of lower energy than the primary <strong>ray</strong>s.<br />

SENSlTIVITY<br />

Refers to the degree to which images of wires (Wire<br />

Sensitivity), drilled holes in plaques (Plaque Sensitivity),<br />

steps (Contrast or Thickness Sensitivity), and actual defects<br />

in materials (Radiographic Sensitivity) are displayed and<br />

capable of being discerned in an x-<strong>ray</strong> film or other<br />

imaging device. Sensitivity is usually expressed as a<br />

percentage of the thickness of the object being examined.<br />

SOURCE-TO-FILM DISTANCE<br />

The actual distance between the focal spot of the x-<strong>ray</strong><br />

source and the plane of the x-<strong>ray</strong> film in the specific<br />

exposure. This distance affects the amount of exposure<br />

used in every application of radiography.<br />

22˚ PYRAMID<br />

Refers to the size and shape of the collimator used in the<br />

<strong>Linatron</strong> Model 200A, 400 and 1000. The collimator<br />

provides a cone (four-sided pyramid) of radiation with the<br />

focal spot as apex, the base a square, and with the sides<br />

forming a 22˚ interior angle.<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


UNSHARPNESS<br />

Degree of loss in image fidelity (in the x-<strong>ray</strong> film) of edges<br />

and other features of the object being examined. Appears<br />

as regions of fuzziness or of indefinite location in the image<br />

of the edge. Major contributor to unsharpness are the<br />

geometry of the setup (Geometric Unsharpness), and the<br />

inherent effect of the screens and film used (Film-Screen<br />

Unsharpness).<br />

WHITE RADIATION<br />

The presence and distribution of x-<strong>ray</strong> photons at all<br />

energies up to the maximum emitted by an x-<strong>ray</strong> source.<br />

X-RAY LEAKAGE<br />

Refers to x-<strong>ray</strong> radiation that originates within an x-<strong>ray</strong><br />

machine, and which penetrates the materials of the x-<strong>ray</strong><br />

head in directions other than the opening provided by the<br />

collimator.<br />

X-RAY OUTPUT<br />

The intensity of the useful x-<strong>ray</strong> beam, usually expressed as<br />

rads per minute at l-meter from the x-<strong>ray</strong> source on the<br />

beam CENTRAL <strong>ray</strong>.<br />

page 63<br />

<strong>Varian</strong> <strong>Linatron</strong> applications


Security & Inspection Products<br />

6883 Spencer Street, Las Vegas, NV 89119<br />

tel: 702.938.4859 www.varian.com/sip<br />

fax:702.938.4833 linatron@varian.com<br />

RAD 1936E © <strong>2007</strong> <strong>Varian</strong> Medical Systems, Inc. Printed in USA 7/07(1K)

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