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Infrared Thermal Testing<br />

Reading III- SGuide-IRT Part 1 <strong>of</strong> 2<br />

My ASNT Level III Pre-Exam Preparatory<br />

Self Study Notes 29th April 2015<br />

Charlie Chong/ Fion Zhang


Infrared Thermography<br />

Charlie Chong/ Fion Zhang


Infrared Thermography<br />

Charlie Chong/ Fion Zhang


Infrared Thermography<br />

Charlie Chong/ Fion Zhang


DEADLY French Military Mistral Anti Aircraft Missile System<br />

■ https://www.youtube.com/embed/_3c0NpYapM0<br />

Charlie Chong/ Fion Zhang<br />

https://www.youtube.com/watch?v=_3c0NpYapM0


See Through & Fun Thermal Camera Experiments<br />

■ https://www.youtube.com/embed/pXAzZoWLzSo<br />

Charlie Chong/ Fion Zhang<br />

https://www.youtube.com/watch?v=pXAzZoWLzSo


LEAKED Body Scan Images From The TSA!<br />

■ https://www.youtube.com/embed/QRkWmRVs-nk<br />

Charlie Chong/ Fion Zhang<br />

https://www.youtube.com/watch?v=QRkWmRVs-nk


How to see through clothing 2<br />

■ https://www.youtube.com/embed/0wQlyCNPw8M<br />

Charlie Chong/ Fion Zhang<br />

https://www.youtube.com/watch?v=0wQlyCNPw8M


Bf4 little bird ah-6j night vision <strong>infrared</strong> real combat footage helmet cam<br />

montage funker tactical. – 金 头 盔<br />

■ https://www.youtube.com/embed/dRra63kOwWE<br />

Charlie Chong/ Fion Zhang<br />

https://www.youtube.com/watch?v=XfXShaTzAhI&list=PL7D451B08CD9A119B


Apache IR Thermal Weaponry<br />

■<br />

https://www.youtube.com/embed/XfXShaTzAhI?list=PL7D451B08CD9A119B<br />

Charlie Chong/ Fion Zhang<br />

https://www.youtube.com/watch?v=XfXShaTzAhI&list=PL7D451B08CD9A119B


Infrared Electrical Testing<br />

■<br />

https://www.youtube.com/embed/DgXsmvv7Q9o<br />

Charlie Chong/ Fion Zhang<br />

https://www.youtube.com/watch?v=DgXsmvv7Q9o


Charlie Chong/ Fion Zhang


Fion Zhang at Shanghai<br />

29th May 2015<br />

http://meilishouxihu.blog.163.com/<br />

Charlie Chong/ Fion Zhang


Charlie Chong/ Fion Zhang


Charlie Chong/ Fion Zhang<br />

http://greekhouse<strong>of</strong>fonts.com/


Greek letter<br />

Charlie Chong/ Fion Zhang


IVONA TTS Capable.<br />

Charlie Chong/ Fion Zhang<br />

http://www.naturalreaders.com/


SGuide-IRT<br />

Content<br />

Part 1 <strong>of</strong> 2<br />

■ Chapter 1 - Introduction to Principles & Theory<br />

■ Chapter 2 - Materials and Their Properties<br />

■ Chapter 3 – Thermal Instrumentation<br />

Part 2 <strong>of</strong> 2<br />

■ Chapter 4 – Operating Equipment and <strong>Understanding</strong> Results<br />

■ Chapter 5 – Applications<br />

■ Appendices A, B, C<br />

Charlie Chong/ Fion Zhang


Chapter 1<br />

Principles & Theory<br />

Charlie Chong/ Fion Zhang


1.1 Introduction to Principles & Theory<br />

Infrared/thermal testing involves the use <strong>of</strong> (1) temperature and (2) heat flow<br />

measurement as a means to predict or diagnose failure.<br />

This may involve the use <strong>of</strong> contacting or noncontacting devices, or a<br />

combination <strong>of</strong> both. A fundamental knowledge <strong>of</strong> heat flow and the thermal<br />

behavior <strong>of</strong> materials is necessary to understand the significance <strong>of</strong> temperature<br />

and temperature changes on a test sample.<br />

Contacting devices include thermometers <strong>of</strong> various types, thermocouples,<br />

thermopiles and thermochromic coatings.<br />

Noncontacting devices include convection (heat flux) devices, optical pyrometers,<br />

<strong>infrared</strong> radiation thermometers, <strong>infrared</strong> Line scanners and <strong>infrared</strong> thermal<br />

imaging (thermographic) equipment.<br />

Infrared <strong>thermography</strong> is the nondestructive, non-intrusive. noncontact mapping<br />

<strong>of</strong> thermal patterns on the surface <strong>of</strong> objects. It is usually used to diagnose<br />

thermal behavior and, thereby, to assess the performance <strong>of</strong> equipment and the<br />

integrity <strong>of</strong> materials, products and processes.<br />

Charlie Chong/ Fion Zhang


Keywords:<br />

Principles:<br />

• temperature and<br />

• heat flow measurement as a means to predict or diagnose failure.<br />

Techniques:<br />

• contacting or<br />

• noncontacting devices,<br />

• or a combination <strong>of</strong> both.<br />

Contacting devices include:<br />

• thermometers <strong>of</strong> various types,<br />

• thermocouples,<br />

• thermopiles and<br />

• thermochromic coatings.<br />

Noncontacting devices include:<br />

• convection (heat flux) devices,<br />

• optical pyrometers,<br />

• <strong>infrared</strong> radiation thermometers,<br />

• <strong>infrared</strong> Line scanners and<br />

• <strong>infrared</strong> thermal imaging (thermographic) equipment.<br />

Charlie Chong/ Fion Zhang


The <strong>infrared</strong> thermal imaging equipment used in <strong>infrared</strong> <strong>thermography</strong> is<br />

available in numerous configurations and with varying degrees <strong>of</strong> complexity.<br />

The thermal maps produced by <strong>infrared</strong> thermal imaging instruments are<br />

called thermograms. To understand and interpret thermograms, the<br />

thermograpber must be familiar with the fundamentals <strong>of</strong> temperature and<br />

heat transfer, <strong>infrared</strong> radiative heat flow and the performance <strong>of</strong> <strong>infrared</strong><br />

thermal imaging instruments and other thermal instruments.<br />

An understanding <strong>of</strong> the equipment, materials and processes being observed<br />

is also important to effectively assess the full significance <strong>of</strong> <strong>infrared</strong>/thermal<br />

measurements. A more detailed discussion <strong>of</strong> the performance parameters <strong>of</strong><br />

<strong>infrared</strong> thermal imaging instruments is provided in Chapter 3.<br />

Keywords:<br />

■ <strong>infrared</strong> <strong>thermography</strong> - The thermal maps produced by <strong>infrared</strong> thermal<br />

imaging instruments are called thermograms.<br />

Charlie Chong/ Fion Zhang


1.2 Fundamentals <strong>of</strong> Temperature and Heat<br />

Transfer<br />

Heat is a transient form <strong>of</strong> energy in which thermal energy is transient. What<br />

is <strong>of</strong>ten referred to as a heat source (such as an oil furnace or an electric<br />

heater) is really one form or another <strong>of</strong> energy conversion – the energy stored<br />

in one object being converted to heat and nowing to another object.<br />

Heat flow is thermal energy in transit and heat always flows from warmer<br />

objects to cooler objects. (transient<br />

Temperature is a measure <strong>of</strong> the thermal energy contained in an object - the<br />

degree <strong>of</strong> hotness or coldness <strong>of</strong> an object that is measurable by any <strong>of</strong> a<br />

number <strong>of</strong> relative scales.<br />

Comments:<br />

“HBNDEv C9 -Transfer <strong>of</strong> heat energy can be described as either steady-state or transient 暂 态 .<br />

In the steady-state condition, heat transfer is constant and in the same direction over time.” –<br />

However, In this PPT, both steady state and transient are both transient form <strong>of</strong> energy.<br />

Charlie Chong/ Fion Zhang


The three modes <strong>of</strong> heat transfer are:<br />

■ conductive,<br />

■ convective and<br />

■ radiative.<br />

All heat is transferred by one <strong>of</strong> these three modes. In most situations, beat is<br />

transferred by a combination <strong>of</strong> two or all three modes. Of these three modes<br />

<strong>of</strong> heat transfer, <strong>infrared</strong> <strong>thermography</strong> is most closely associated with the<br />

radiative process, but it is essential to study all three to understand the<br />

meaning <strong>of</strong> thermograms and to pursue a successful program <strong>of</strong><br />

<strong>thermography</strong>. As a result <strong>of</strong> heat transfer, objects tend to increase or<br />

decrease their temperature until they come to thermal equilibrium with their<br />

surroundings. To maintain a steadystate heat flow condition, energy must be<br />

continuously supplied by some means <strong>of</strong> energy conversion so that the<br />

temperature differential, and hence the heat flow remains constant.<br />

Charlie Chong/ Fion Zhang


The three modes <strong>of</strong> heat transfer are:<br />

■ conductive,<br />

■ convective and<br />

■ radiative.<br />

Charlie Chong/ Fion Zhang<br />

http://www.chem.purdue.edu/gchelp/liquids/character.html


The three modes <strong>of</strong> heat transfer are: Water in 3 phases.<br />

http://dli.taftcollege.edu/streams/Geography/Animations/WaterPhases.swf<br />

Charlie Chong/ Fion Zhang<br />

http://dli.taftcollege.edu/streams/Geography/Animations/WaterPhases.html


Temperature and Temperature Scales<br />

Temperature is expressed in either absolute or relative terms. There are two<br />

absolute scales called Rankine (English system) and Kelvin (metric system).<br />

There are two corresponding relative scales called Fahrenheit (English<br />

system) and Celsius or centigrade (metric system). Absolute zero is the<br />

temperature at which no molecular action takes place. This is expressed as<br />

zero Kelvin or zero degrees Rankin (0 K or 0° R). Relative temperature is<br />

expressed as degrees Celsius or degrees Fahrenheit (°C or °F). The<br />

numerical relations among the four scales are as follows:<br />

converting ºC to ºF, (9/5 x ºC +32) ºF<br />

converting ºF to ºC, (5/9 x ºF -32) ºC<br />

T Rankine = T Fahrenheit+ 459.7<br />

T Kelvin = T Celsius + 273.16<br />

Exercise: Temperature (not temperature interval)<br />

0 ºC = 32 ºF<br />

thus -273.16 ºC = (-273.16 x 9/5 + 32) ºF = 459.7 ºF<br />

Charlie Chong/ Fion Zhang


Temperature and Temperature Scales<br />

■<br />

http://www.mathsisfun.com/temperature-conversion.html<br />

Charlie Chong/ Fion Zhang


Temperature and Temperature Scales<br />

REMEMBER<br />

0ºC = 32ºF<br />

for my ASNT exam<br />

converting ºC to ºF, (9/5 x ºC +32) ºF<br />

Charlie Chong/ Fion Zhang


Boston Tea Party – New governances not the Old Fahrenheit & ⅝”.<br />

Charlie Chong/ Fion Zhang


Boston Tea Party – New governances not the Old Fahrenheit & ⅝”.<br />

Charlie Chong/ Fion Zhang


The Mighty Fahrenheit & ⅝”,<br />

English System.<br />

Charlie Chong/ Fion Zhang


The Mighty Fahrenheit & ⅝”, English System.<br />

Charlie Chong/ Fion Zhang


Absolute zero is equal to - 273.16 °C and also equal to approximately - 459.7<br />

°F. To conveIt, a change in temperature or delta T (∆T) between the English<br />

and metric systems, the simple 9/5 (1.8 to 1) relationship is used:<br />

∆T Fahrenheit (or º Rankine) = 9/5 x ∆T Celsius (or Kelvin)<br />

or simply;<br />

∆T Fahrenheit (or º Rankine) = 1.8 x ∆T Celsius (or Kelvin)<br />

Table 1.1 (pages 12 to 14) is a conversion table that will assist in the rapid<br />

conversion <strong>of</strong> temperature between fabrenheit and celsius values.<br />

Instructions for the use <strong>of</strong> the table are shown at the top <strong>of</strong> the table. (not in<br />

this PPT)<br />

Charlie Chong/ Fion Zhang


Conductive Heat Transfer<br />

Conductive beat transfer is probably the simplest form to understand. lt is the<br />

transfer <strong>of</strong> beat in stationary media. It is the only mode <strong>of</strong> heat flow in solids,<br />

but it can also take place in liquids and gases.<br />

Conductive heat transfer occurs as the result <strong>of</strong> atomic vibrations (in solids)<br />

and molecular collisions (in liquids) whereby energy is moved, one molecule<br />

at a time, from higher temperature sites to lower temperature sites. An<br />

example <strong>of</strong> conductive heat transfer is when one end <strong>of</strong> a section <strong>of</strong> metal<br />

pipe warms up after a flame is applied to the other end. There are physical<br />

laws that allow the amount <strong>of</strong> conductive heat flow to be calculated, and they<br />

are presented here to show the factors on which conductive heat flow<br />

depends.<br />

Keywords:<br />

■ atomic vibrations<br />

■ molecular collisions (atomic collisions in inert gas)<br />

Charlie Chong/ Fion Zhang


The Fourier conduction Law expresses the conductive heat flow, Q per unit<br />

area A, through a slab <strong>of</strong> solid material <strong>of</strong> thickness L as illustrated in Figure<br />

1.1. Thermal resistance R t is defined as:<br />

Thermal conductivity is defined as:<br />

Heat flow per unit area is defined as:<br />

Charlie Chong/ Fion Zhang


Where:<br />

• Q/A = the rate <strong>of</strong> heat transfer through the slab per unit area (BTU/h∙ft 2 ) or<br />

(W/m 2 ) perpendicular to the flow,<br />

• L = the thickness <strong>of</strong> the slab (ft or m),<br />

• T 1 =(°F) or (ºC) is the higher temperature (at the left),<br />

• T 2 = the lower temperature (at the right)<br />

• k = the thermal conductivity <strong>of</strong> the slab material (BTU/h∙ft∙ºF) or (W/m∙K)<br />

• R t = the thermal resistance <strong>of</strong> the slab material (°F∙h∙ft 2 fBTU) or (m 2 ∙K/W)<br />

Charlie Chong/ Fion Zhang


The Fourier conduction Law ( One dimension heat flow)<br />

The mathematical relationship that describes heat transfer as a function <strong>of</strong> the<br />

material that heat is conducting through is known as Fourier's law and is<br />

given below.<br />

Fourier’s Law: q = k ∙ A ∙ (T H -T C ) ∙ L -1<br />

Where:<br />

q = heat transfer per unit time (W)<br />

A = heat transfer area (m 2 )<br />

k = thermal conductivity <strong>of</strong> material (W/m∙K)<br />

L = material thickness (m)<br />

Charlie Chong/ Fion Zhang


Thermal conductivity is highest for metals such as aluminum and lower for<br />

porous materials such as brick. It is inversely proportional to thermal<br />

resistance.<br />

K= 1/R t<br />

Comment:<br />

k α 1/R, R= thermal resistivity and the thermal resistance R t = L∙R<br />

Thermal conductivity is highest for metals such as aluminum and lower for<br />

porous materials such as brick. It is inversely proportional to thermal<br />

resistance. In real terms, the Fourier expression means that the rate <strong>of</strong> heat<br />

flow increases with increasing temperature difference. increases with<br />

increasing thermal conductivity and decreases with increasing slab thickness.<br />

Heat flow may be expressed in English units or metric units.<br />

Charlie Chong/ Fion Zhang


Convective Heat Transfer<br />

Convective heat transfer takes place in a moving medium and is almost<br />

always associated with heat transfer between a solid and a moving fluid (such<br />

as air). Forced convection takes place when an external driving force, such as<br />

a wind or an air pump, moves the fluid. Free convection takes place when<br />

there is no external driving force - the temperature differences necessary for<br />

heat transfer produce density changes in the fluid. The warmer fluid rises as a<br />

result <strong>of</strong> increased buoyancy. In convective heat flow, heat transfer takes<br />

effect by direct conduction through the fluid and the mixing motion <strong>of</strong> the fluid<br />

itself. Figure 1.2 illustrates convective heat transfer between a flat plate and a<br />

moving fluid.<br />

Charlie Chong/ Fion Zhang


Figure 1.2: Convective heat flow<br />

Charlie Chong/ Fion Zhang


Figure 1.2: Convective heat flow<br />

T ∞<br />

Distance from<br />

boundary layer<br />

Thermal Boundary layer<br />

T surface<br />

fluid velocity<br />

Charlie Chong/ Fion Zhang


The presence <strong>of</strong> the plate causes the velocity <strong>of</strong> the fluid to decrease to zero<br />

at the surface and influences its velocity throughout the thickness <strong>of</strong> a<br />

boundary layer. The thickness <strong>of</strong> the boundary layer depends on the free fluid<br />

velocity V ∞ - the higher the free fluid velocity, the thinner the boundary layer.<br />

It is greatest for free convection where V ∞ = 0. The rate <strong>of</strong> heat flow depends,<br />

in turn, on the thickness <strong>of</strong> the boundary layer as well as the temperature<br />

difference between T s and T ∞ , T s being the surface temperature and T ∞<br />

being the free field fluid temperature outside the boundary layer.<br />

Charlie Chong/ Fion Zhang


Newton's cooling law defines the convective heat transfer coefficient as:<br />

where: h = (BTU/b-ft2-°F) or (W/m2-K)<br />

This is rearranged to obtain an expression for convective heat flow per unit<br />

area:<br />

If R c = 1/h is the resistance to convective heat flow, then:<br />

Charlie Chong/ Fion Zhang


R c is easier to use than h when determining combined conductive and<br />

convective heat transfer because then they are additive terms.<br />

In real terms, this expression means that the rate <strong>of</strong> convective heat flow<br />

increases with increasing temperature difference, increases with higher<br />

convective heat flow coefficient and decreases with increasing convective<br />

thermal resistance.<br />

Conductive and convective heat transfer are very similar. In both, the heat<br />

transfer is directly proportional to the temperature difference and the speed at<br />

which th is energy is transferred (rate <strong>of</strong> heat flow) depends on the transfer<br />

coefficient <strong>of</strong> the media or material through which the heat energy flows. By<br />

comparison, radiative heat transfer takes place in accordance with a different<br />

set <strong>of</strong> rules.<br />

Charlie Chong/ Fion Zhang


Radiative Heat Transfer<br />

Radiative heat transfer is unlike the other two modes because:<br />

1. it occurs by electromagnetic emission and absorption in a manner similar<br />

to light;<br />

2. it propagates at the speed <strong>of</strong> light;<br />

3. like light, it requires a direct line <strong>of</strong> sight;<br />

4. the heat energy transferred is proportional to the fourth power T 4 <strong>of</strong> the<br />

temperature <strong>of</strong> the objects; and<br />

5. it can take place across a vacuum – in fact, a vacuum is the most efficient<br />

medium for radiative heat transfer.<br />

The electromagnetic spectrum is illustrated in Figure 1.3 and shows that X-<br />

rays. radio waves. light waves (ultraviolet and visible) and <strong>infrared</strong> radiation<br />

are all related. Radioactive heat transfer takes place in the <strong>infrared</strong> portion <strong>of</strong><br />

the spectrum, from 0.75μm to about 100μm, although most practical<br />

measurements can be calculated to about 20μm . The symbols μm (μm is<br />

preferred) stand for micrometers or microns. A micron is one-millionth <strong>of</strong> a<br />

meter and the measurement unit for radiant energy wavelength. Wavelength<br />

is inversely related to frequency (longer wavelengths have lower frequencies).<br />

Charlie Chong/ Fion Zhang


Figure 1.3: Infrared in the electromagnetic spectrum<br />

Practical Infrared Thermography λ; 2μm to 6μm and 8μm to 14μm<br />

Charlie Chong/ Fion Zhang


Figure 1.4: Infrared radiation leaving a target surface (ρετσ)<br />

Ɛ<br />

ρ<br />

τ<br />

Charlie Chong/ Fion Zhang


1.3 Fundamentals <strong>of</strong> Radiative Heat Flow<br />

Radiation Exchange at the Target Surface<br />

The measurement <strong>of</strong> <strong>infrared</strong>/thermal radiation is the basis for non-contact<br />

temperature measurement and <strong>infrared</strong> <strong>thermography</strong>. The surface to be<br />

evaluated is called the target surface. Thermal <strong>infrared</strong> radiation leaving a<br />

surface is called exitance or radiosity. It can be emitted from the surface,<br />

reflected by the surface, or transmitted through the surface. This is illustrated<br />

in Figure 1.4.<br />

The total radiosity is equal to the sum <strong>of</strong> the emitted component (W e ), the<br />

reflected component (W r ) and the transmitted component (W t ).<br />

It is important to note that the surface temperature T e is related to the emitted<br />

component W e only.<br />

Keywords:<br />

■ Exitance<br />

■ Radiosity<br />

Charlie Chong/ Fion Zhang


Thermal <strong>infrared</strong> radiation impinging on a surface can be absorbed, reflected,<br />

or transmitted as illustrated in Figure 1.5. Kirchh<strong>of</strong>f's law states that the sum<br />

<strong>of</strong> the three components is always equal to the total received radiation, E t The<br />

fractional sum <strong>of</strong> the three components equals unity or 100 percent:<br />

E t = E α + E ρ + E τ , (for blackbody E Ɛ = E α )<br />

where:<br />

E t = total energy<br />

Likewise, the sum <strong>of</strong> the three material properties, transmissivity, reflectivity<br />

and emissivity, also always equals unity:<br />

τ + ρ + Ɛ =1<br />

Charlie Chong/ Fion Zhang


Figure 1.5: Infrared radiation impinging on a target surface<br />

Kirchh<strong>of</strong>f's law<br />

Charlie Chong/ Fion Zhang


Reflections <strong>of</strong>f Specular and Diffuse Surfaces<br />

A perfectly smooth surface will reflect incident energy at an angle<br />

complementary to the angle <strong>of</strong> incidence as shown in Figure 1.5. This is<br />

called a specular reflector. A completely rough or structured surface will<br />

scatter or disperse all <strong>of</strong> the incident radiation. This is called a diffuse reflector.<br />

No perfectly specular or perfectly diffuse surface can exist in nature, and all<br />

real surfaces have some diffusivity and some specularity. These surface<br />

characteristics will determine the type and direction <strong>of</strong> the reflected<br />

component <strong>of</strong> incident radiation. When making practical measurements, the<br />

specularity or diffusivity <strong>of</strong> a target surface are taken into account by<br />

compensating for the effective emissivity (Ɛ*) <strong>of</strong> the surface. The<br />

thermographer's use <strong>of</strong> effective emissivity is reviewed as <strong>part</strong> <strong>of</strong> the detailed<br />

discussion <strong>of</strong> equipment operation in Chapter 5.<br />

Keywords:<br />

■ Specular reflector<br />

■ Diffuse reflector<br />

Charlie Chong/ Fion Zhang


Reflections <strong>of</strong>f Specular and Diffuse Surfaces<br />

Charlie Chong/ Fion Zhang


Reflections <strong>of</strong>f Specular and Diffuse Surfaces<br />

Charlie Chong/ Fion Zhang


Transient Heat Exchange<br />

The previous discussions <strong>of</strong> the three types <strong>of</strong> heat transfer deal with steady<br />

state heat exchange for reasons <strong>of</strong> simplicity and comprehension. Heat<br />

transfer is assumed to take place between two points, each <strong>of</strong> which is at a<br />

fixed temperature. However, in many applications, temperatures are in<br />

transition so that the values shown for energy radiated from a target surface<br />

are the instantaneous values at the moment measurements are made. In<br />

many instances, existing transient thermal conditions are exploited to use<br />

<strong>thermography</strong> to reveal material or structural characteristics in test articles. In<br />

<strong>infrared</strong> nondestructive testing <strong>of</strong> materials, thermal injection or active<br />

<strong>thermography</strong> techniques are used to generate controlled thermal transient<br />

flow based on the fact that uniform structural continuity results in predictable<br />

thermal continuity. These techniques will be discussed in greater detail in<br />

Chapter 5.<br />

Charlie Chong/ Fion Zhang


Radiant Energy Related to Target Surface Temperature<br />

All target surfaces warmer than absolute zero radiate energy in the <strong>infrared</strong><br />

spectrum. Figure 1.6 shows the spectral distribution <strong>of</strong> energy radiating from<br />

various idealized target surfaces as a function <strong>of</strong> surface temperature (T) and<br />

wavelength (A.). Very hot targets radiate in the visible as well, and our eyes<br />

can see this because they are sensitive to light. The sun, for example, is at a<br />

temperature <strong>of</strong> about 6000 K and appears to glow white bot. The heating<br />

element <strong>of</strong> an electric stove at 800 K glows a cherry red and, as it cools, it<br />

loses its visible glow but continues to radiate. This radiant energy can be felt<br />

with a hand placed near the surface even though the glow is invisible. The<br />

idealized curves shown in Figure 1.6 are for perfect radiators known as<br />

blackbodies. Blackbodies are defined and discussed in greater detail later in<br />

this chapter. Figure 1.6 also shows two key physical laws regarding <strong>infrared</strong><br />

energy emitted from surfaces.<br />

Charlie Chong/ Fion Zhang


Radiant Energy Related to Target Surface Temperature<br />

All target surfaces warmer than absolute zero radiate energy in the <strong>infrared</strong><br />

spectrum.<br />

Charlie Chong/ Fion Zhang


The Stefan-Boltzmann law: W= σƐT 4<br />

Where:<br />

W = radiant flux emitted per unit area (W/m 2 )<br />

Ɛ = emissivity (unity for a blackbody target)<br />

σ = Stefan-Boltzmann constant= 5.673 x I0 -8 W/m -2 ∙K -4<br />

T = absolute temperature <strong>of</strong> target (K)<br />

(Comments: for blackbody Ɛ=1, α=Ɛ.)<br />

illustrates that W, the total radiant flux emitted per unit area <strong>of</strong> surface, (the<br />

area under the curve) is proportional to the fourth power <strong>of</strong> the absolute<br />

surface temperature T 4 . It is also proportional to a numerical constant σ, and<br />

the emissivity <strong>of</strong> the surface, Ɛ.<br />

Charlie Chong/ Fion Zhang


Figure 1.6: Typical blackbody distribution<br />

curves and basic radiation laws<br />

Stefan-Boltzmann Law<br />

Radiant Flux per Unit Area In W/cm 2<br />

W= σƐT 4<br />

Ɛ = emissivity (unity for a blackbody target)<br />

σ = Stefan-Boltzmann constant<br />

= 5.673 x I0 -8 W/m -2 ∙K -4<br />

T = absolute temperature <strong>of</strong> target (K)<br />

Wien's Displacement Law<br />

λ max = b/T<br />

where: λ max = peak wavelength (μm)<br />

b = Wien's displacement constant<br />

(2897 or 3000 approximately)<br />

Charlie Chong/ Fion Zhang


Figure 1.6: Typical blackbody distribution curves and basic radiation laws<br />

Charlie Chong/ Fion Zhang


Wien's displacement law:<br />

λ max = b/T<br />

Where:<br />

λ max wavelength <strong>of</strong> maximum radiation (μm)<br />

b Wien's displacement constant or 2897 (μm∙K)<br />

illustrates that the peak wavelength, λ max (μm) at which a surface radiates, is<br />

easily determined by dividing a constant b (approximately 3000) by the<br />

absolute temperature T (Kelvin) <strong>of</strong> the surface.<br />

Charlie Chong/ Fion Zhang


1.4 Practical Infrared Measurements<br />

ln practical measurement applications, the radiant energy leaves a target<br />

surface, passes through some transmitting medium. usually an atmospheric<br />

path, and reaches a measuring instrument.<br />

Therefore, when making measurements or producing a thermogram, three<br />

sets <strong>of</strong> characteristics must be considered:<br />

1. characteristics <strong>of</strong> the target surface,<br />

2. characteristics <strong>of</strong> the transmitting medium and<br />

3. characteristics <strong>of</strong> the measuring instrument.<br />

This is illustrated in Figure 1.7.<br />

Charlie Chong/ Fion Zhang


Figure 1.7: Three sets <strong>of</strong> characteristics <strong>of</strong> the <strong>infrared</strong> measurement<br />

problem<br />

Ɛ obj<br />

ρ amb<br />

τ assumed = 0<br />

Ɛ atm<br />

τ atm<br />

Charlie Chong/ Fion Zhang


Characteristics <strong>of</strong> the Target Surface<br />

Target surfaces are separated into three categories; blackbodies, graybodies<br />

and nongraybodies (also called real bodies, selective radiators or spectral<br />

bodies).<br />

The target surfaces shown in Figure 1.6 are all perfect radiators (or<br />

blackbodies). A blackbody radiator is defined as a theoretical surface having<br />

unity emissivity at all wavelengths and absorbing all <strong>of</strong> the radiant energy<br />

impinging upon it.<br />

Emissivity, in turn, is defined as the ratio <strong>of</strong> the radiant energy emitted from a<br />

surface to the energy emitted from a blackbody surface at the same<br />

temperature. Blackbody radiators are theoretical and do not exist in practice.<br />

The surface <strong>of</strong> most solids are graybodies, that is, surfaces with high<br />

emissivities that are fairly constant with wavelength. Figure 1.8 shows the<br />

comparative spectral distribution <strong>of</strong> energy emitted by a blackbody, a<br />

graybody and a nongraybody, all at the same temperature (300 K).<br />

Charlie Chong/ Fion Zhang


Figure 1.8: Spectral distribution <strong>of</strong> a blackbody, graybody and nongraybody<br />

Charlie Chong/ Fion Zhang


Referring back to Figure 1.5, the total exitance available to the measuring<br />

instrument has three components:<br />

• emitted energy (We),<br />

• reflected energy (Wr) from the environment and other reflecting sources,<br />

and<br />

• for nonopaque targets, energy transmitted through the target (Wt) from<br />

sources behind the target.<br />

Because a theoretical blackbody has an emissivity Ɛ <strong>of</strong> 1.00, it will reflect and<br />

transmit no energy ρ = 0, τ = 0.<br />

Real targets, however, are not blackbodies. and figure 1.9 shows the three<br />

components that comprise Wx, the total exitance that an instrument sees<br />

when aimed at a real Ufe target surface. Because only the emitted<br />

component, We, is related to the temperature <strong>of</strong> the target surface, it<br />

becomes apparent that a significant <strong>part</strong> <strong>of</strong> the measurement problem is<br />

eliminating or compensating for the other two components. This is discussed<br />

in greater detail in Chapter 4.<br />

Charlie Chong/ Fion Zhang


Figure 1.9: Components <strong>of</strong> energy reaching the measuring instrument<br />

Charlie Chong/ Fion Zhang


Characteristics <strong>of</strong> the Transmitting Medium<br />

Because lhe <strong>infrared</strong> radiation from the target passes through some<br />

transmitting medium on its way to the target, the transmission and emission<br />

characteristics <strong>of</strong> the medium in the measurement path must be considered<br />

when making non contact thermal measurement. No loss <strong>of</strong> energy or self<br />

emission (Ɛ atm ) is encountered when measuring through a vacuum. However.<br />

most measurements are made through air. For short path length (a few<br />

meters, for example), most gases (including the atmosphere) absorb and emit<br />

very little energy and can be ignored. However. when highly accurate<br />

temperature measurements are required, the effects <strong>of</strong> atmospheric<br />

absorption must be taken into account. (τ atm , Ɛ atm ).<br />

Charlie Chong/ Fion Zhang


As the path length increases to more than a few meters, or as the air<br />

becomes heavy with water vapor, atmospheric absorption may become a<br />

significant factor. Therefore, it is necessary to understand the <strong>infrared</strong><br />

transmission characteristics <strong>of</strong> the atmosphere. Figure 1.10 illustrates the<br />

spectral transmission characteristics <strong>of</strong> a 10 m (33 ft) path <strong>of</strong> ground level<br />

atmosphere at a temperature <strong>of</strong> 25 °C (77 °F) and 50 percent humidity.<br />

It is immediately apparent that the atmosphere is not as transparent in the<br />

<strong>infrared</strong> ponion <strong>of</strong> the spectrum as it is in the visible ponion. Two spectral<br />

intervals have very high transmission. These are known as the 3 to 5 μm and<br />

the 8 to 14μm atmospheric windows, and almost all <strong>infrared</strong> sensing and<br />

imaging instruments are designed to operate in one <strong>of</strong> these two windows.<br />

The absorption segments shown in Figure 1.10 were formed by carbon<br />

dioxide and water vapor, which are two <strong>of</strong> the major constituents in air. For<br />

measurements through gaseous media other than atmosphere, it is<br />

necessary to investigate the transmission spectra <strong>of</strong> the medium before<br />

validating the measurements, which is explained in greater detail in Chapter 2.<br />

Charlie Chong/ Fion Zhang


Figure 1.10; Transmission <strong>of</strong> 10m (33ft) <strong>of</strong> ground level atmosphere at 50<br />

percent humidity and 25 °C (77ºF)<br />

Percentage Transmission<br />

Wave Length μm<br />

Charlie Chong/ Fion Zhang


When there is a solid material, such as a glass or quartz viewing port,<br />

between the target and the instrument, the spectral characteristics <strong>of</strong> the solid<br />

media must be known and considered. Figure 1.11 shows transmission<br />

curves for various samples <strong>of</strong> glass. Most significant is the fact that glass<br />

does not transmit <strong>infrared</strong> energy at 10μm where ambient (30 °C, 86 °F)<br />

surfaces radiate their peak energy. In practice, <strong>infrared</strong> thermal<br />

measurements <strong>of</strong> ambient targets can never be made through glass. One<br />

practical approach to this problem is to eliminate the glass, or at least a<br />

portion through which the instrument can be aimed at the target. If a window<br />

must be present for personal safety, vacuum, or product safety, a material<br />

might be substituted that transmits in the longer wavelengths. Figure 1.12<br />

shows the spectral transmission characteristics <strong>of</strong> several <strong>infrared</strong><br />

transmitting materials, many <strong>of</strong> which transmit energy past 10μm. In addition<br />

to being used as transmitting windows, these materials are <strong>of</strong>ten used as<br />

lenses and optical elements in <strong>infrared</strong> sensors and imagers. Of course, as<br />

targets become hotter, and the emitted energy shifts to the shorter<br />

wavelengths, glass and quartz windows pose less <strong>of</strong> a problem and are even<br />

used as elements and lenses in high temperature sensing instruments.<br />

Characteristics <strong>of</strong> the measuring instrument are addressed in Chapter 4.<br />

Charlie Chong/ Fion Zhang


Figure 1.11: Transmission, absorption and reflectance characteristics <strong>of</strong><br />

glass<br />

Charlie Chong/ Fion Zhang


Figure 1.12: Transmission curves <strong>of</strong> various <strong>infrared</strong> transmitting material<br />

Charlie Chong/ Fion Zhang


Figure 1.12: Transmission curves <strong>of</strong> various <strong>infrared</strong> transmitting material<br />

Charlie Chong/ Fion Zhang


Convective Heat Transfer<br />

Convective heat transfer, <strong>of</strong>ten referred to simply as convection, is the transfer <strong>of</strong> heat from one place to<br />

another by the movement <strong>of</strong> fluids. Convection is usually the dominant form <strong>of</strong> heat transfer in liquids and<br />

gases. Although <strong>of</strong>ten discussed as a distinct method <strong>of</strong> heat transfer, convective heat transfer involves the<br />

combined processes <strong>of</strong> conduction (heat diffusion) and advection (heat transfer by bulk fluid flow). The term<br />

convection can sometimes refer to transfer <strong>of</strong> heat with any fluid movement, but advection is the more precise<br />

term for the transfer due only to bulk fluid flow. The process <strong>of</strong> transfer <strong>of</strong> heat from a solid to a fluid, or the<br />

reverse, is not only transfer <strong>of</strong> heat by bulk motion <strong>of</strong> the fluid, but diffusion and conduction <strong>of</strong> heat through the<br />

still boundary layer next to the solid. Thus, this process without a moving fluid requires both diffusion and<br />

advection <strong>of</strong> heat, a process that is usually referred to as convection. Convection that occurs in the earth's<br />

mantle causes tectonic plates to move. Convection can be "forced" by movement <strong>of</strong> a fluid by means other than<br />

buoyancy forces (for example, a water pump in an automobile engine). Thermal expansion <strong>of</strong> fluids may also<br />

force convection. In other cases, natural buoyancy forces alone are entirely responsible for fluid motion when<br />

the fluid is heated, and this process is called "natural convection". An example is the draft in a chimney or<br />

around any fire. In natural convection, an increase in temperature produces a reduction in density, which in turn<br />

causes fluid motion due to pressures and forces when fluids <strong>of</strong> different densities are affected by gravity (or any<br />

g-force). For example, when water is heated on a stove, hot water from the bottom <strong>of</strong> the pan rises, displacing<br />

the colder denser liquid, which falls. After heating has stopped, mixing and conduction from this natural<br />

convection eventually result in a nearly homogeneous density, and even temperature. Without the presence <strong>of</strong><br />

gravity (or conditions that cause a g-force <strong>of</strong> any type), natural convection does not occur, and only forcedconvection<br />

modes operate. The convection heat transfer mode comprises one mechanism. In addition to<br />

energy transfer due to specific molecular motion (diffusion), energy is transferred by bulk, or macroscopic,<br />

motion <strong>of</strong> the fluid. This motion is associated with the fact that, at any instant, large numbers <strong>of</strong> molecules are<br />

moving collectively or as aggregates. Such motion, in the presence <strong>of</strong> a temperature gradient, contributes to<br />

heat transfer. Because the molecules in aggregate retain their random motion, the total heat transfer is then<br />

due to the superposition <strong>of</strong> energy transport by random motion <strong>of</strong> the molecules and by the bulk motion <strong>of</strong> the<br />

fluid. It is customary to use the term convection when referring to this cumulative transport and the term<br />

advection when referring to the transport due to bulk fluid motion.<br />

Charlie Chong/ Fion Zhang<br />

http://en.wikipedia.org/wiki/Convective_heat_transfer


Chapter 1<br />

Review Questions<br />

Q&A<br />

1. b<br />

2. d<br />

3. c<br />

4. a<br />

5. c<br />

6. d<br />

7. b<br />

8. b<br />

9. d<br />

10. d<br />

11. a<br />

12. a<br />

13. d<br />

14. e<br />

I5. d<br />

16. e<br />

17. b<br />

18. d<br />

19. a<br />

20. d<br />

21. b<br />

22. e<br />

Charlie Chong/ Fion Zhang


Q1. At a temperature <strong>of</strong> absolute zero:<br />

a. hydrogen becomes a liquid.<br />

b. all molecular motion ceases.<br />

c. salt water is <strong>part</strong> solid and <strong>part</strong> liquid.<br />

d. fahrenheit and celsius <strong>reading</strong>s are the same.<br />

Q2. Conductive heat transfer cannot take place:<br />

a. within organic materials such as wood.<br />

b. between two solid materials in contact.<br />

c. between dissimilar metals.<br />

d. across a vacuum.<br />

Q3. The only three modes <strong>of</strong> heat transfer are:<br />

a. resistive, capacitive and inductive.<br />

b. steady state, transient and reversible.<br />

c. conduction, convection and radiation.<br />

d. conduction. convection and absorption.<br />

Charlie Chong/ Fion Zhang


Q4. Heat can only flow in the direction from:<br />

a. hotter objects to colder objects.<br />

b. colder objects to houer objects.<br />

c. more dense objects to less dense objects.<br />

d. larger object to smaller objects.<br />

Q5. Thermal resistance is:<br />

a. analogous to electrical current.<br />

b. proportional to the fourth power <strong>of</strong> emissivity.<br />

c. inversely proportional to the rate <strong>of</strong> heat flow by conduction.<br />

d. a measure <strong>of</strong> material stiffness.<br />

Q6. The radiation <strong>of</strong> thermal <strong>infrared</strong> energy from a target surface:<br />

a. occurs most efficiently in a vacuum.<br />

b. is proportional to the fourth power <strong>of</strong> the absolute surface temperature.<br />

c. is directly proportional to surface emissivity.<br />

d. is all <strong>of</strong> the above.<br />

Charlie Chong/ Fion Zhang


Q7. The mode <strong>of</strong> heat transfer most closely associated with <strong>infrared</strong><br />

<strong>thermography</strong> is:<br />

a. induction.<br />

b. radiation.<br />

c. convection.<br />

d. conduction.<br />

Q8. To convert a fahrenheit <strong>reading</strong> to celsius:<br />

a. divide by 1.8.<br />

b. subtract 32 and divide by 1.8.<br />

c. multiply by 1.8 and add 32.<br />

d. add 273.<br />

Q9. Thermal radiation reaching the surface <strong>of</strong> an object can be:<br />

a. absorbed only in the presence <strong>of</strong> atmosphere.<br />

b. reflection and absorbed only in a vacuum.<br />

c. transmitted only if the surface is organic.<br />

d. absorbed, reflected and transmitted.<br />

Charlie Chong/ Fion Zhang


Q10. The follow ing spectral band is included in the <strong>infrared</strong> spectrum:<br />

a. 0.1 to 5.5 μm.<br />

b. 0.3 to 10.6 μm.<br />

c. 0.4 to 20.0 μm.<br />

d. 0.75 to 100 μm.<br />

Q11. Mosl instruments used in <strong>infrared</strong> <strong>thermography</strong> operate somewhere<br />

within the;<br />

a. 2 to 14 μm spectral region.<br />

b. 5 to 10 μm spectral region.<br />

c. 10 to 20 μm spectral region.<br />

d. 20 to 100 J μm spectral region.<br />

Q12. As a surface cools, the peak <strong>of</strong> its radiated <strong>infrared</strong> energy:<br />

a. shifts to longer wavelengths.<br />

b. shifts to shorter wavelengths.<br />

c. remains constant if emissivity remains constant.<br />

d. remains constant even if emissivity varies.<br />

Charlie Chong/ Fion Zhang


Q13. The peak emitting wavelength <strong>of</strong> a 300 °C (572 ° F) blackbody is<br />

approximately:<br />

a. 1.5 μm.<br />

b. 3 μm.<br />

λ max = b/T( in K) = 2897/573 μm<br />

0. 10 μm.<br />

d. 5 μm.<br />

Q14. An opaque surface with an emissivity <strong>of</strong> 0.04 would be:<br />

a. transparent to <strong>infrared</strong> radiation.<br />

b. a fairly good emitter.<br />

c. almost a perfect reflector. (τ=0, Ɛ=0.04, ρ = 0.96)<br />

d. almost a perfect emitter.<br />

Q15. If a surface has an emissivity <strong>of</strong> 0.35 and a reflectivity <strong>of</strong> 0.45. its<br />

transmissivity would be:<br />

a. impossible to detennine without additional information.<br />

b. 0.80.<br />

c. 0.10.<br />

d. 0.20. [1-(0.35+0.45)]<br />

Charlie Chong/ Fion Zhang


Q16. In forced convection, the boundary layer:<br />

a. increases as the fluid velocity increases.<br />

b. remains the same as the fluid velocity increases.<br />

c. decreases as the fluid velocity increases.<br />

d. increases in proportion to the fourth power <strong>of</strong> the fluid velocity.<br />

Q17. When heating one end <strong>of</strong> a car key to thaw a frozen automobile door<br />

lock, heat transfer from the key to the lock is an example <strong>of</strong>:<br />

a. forced convection.<br />

b. conductive heat transfer.<br />

c. free convection.<br />

d. radiative heat transfer.<br />

Q18. The <strong>infrared</strong> atmospheric window that transmits <strong>infrared</strong> radiation best is<br />

the:<br />

a. 2.0 to 3.0 μm region.<br />

b. 3.0 to 6.0 μm region.<br />

c. 6.0 to 9.0 μm region.<br />

d. 9.0 to 11.0 μm region.<br />

Charlie Chong/ Fion Zhang


Q19. The spectral band in which glass transmits <strong>infrared</strong> radiation best is the:<br />

a. 2.0 to 3.0 μm region.<br />

b. 3.0 to 6.0 μm region.<br />

c. 6.0 to 9.0 μm region.<br />

d. 9.0 to 11.0 μm region.<br />

Q20. Reflectance <strong>of</strong> <strong>infrared</strong> radiation by a glass surface is greatest in the:<br />

a. 2.0 to 3.0 μm region.<br />

h. 3.0 to 6.0 μm region.<br />

c. 6.0 to 9.0 μm region.<br />

d. 9.0 to 11.0 μm region.<br />

Q21. A diffuse reflecting surface is:<br />

a. a polished surface that reflects incoming energy at a complementary angle.<br />

b. a surface that scatters reflected energy in many directions.<br />

c. also called a specular reflecting surface.<br />

d. usually transparent to <strong>infrared</strong> radiation.<br />

Charlie Chong/ Fion Zhang


Q22. In the 8 to 14 μm spectral region:<br />

a. the atmosphere absorbs <strong>infrared</strong> radiant energy almost completely.<br />

b. the atmosphere reflects <strong>infrared</strong> radiant energy almost completely.<br />

c. the atmosphere transmits <strong>infrared</strong> energy very efficiently.<br />

d. <strong>infrared</strong> instruments do not operate very accurately.<br />

Charlie Chong/ Fion Zhang


Chapter 2<br />

Materials and Their Properties<br />

Charlie Chong/ Fion Zhang


2.1 Materials Characteristics<br />

A knowledge <strong>of</strong> the characteristics <strong>of</strong> materials is important to the<br />

thermographer for numerous reasons, but the two most important arc the<br />

need to know how a <strong>part</strong>icular target surface e mits. transmits and refl ects<br />

<strong>infrared</strong> radiant energy. and the need 10 know how heat flows within a<br />

<strong>part</strong>icular material.<br />

2.2 Surface Properties <strong>of</strong> Materials<br />

The surface properties <strong>of</strong> materials include emissivity. reflectivity and<br />

transmissivity.<br />

Charlie Chong/ Fion Zhang


Emissivity Ɛ<br />

When using <strong>infrared</strong> <strong>thermography</strong> to measure surface temperature <strong>of</strong> a<br />

target. it is essential to know the effective emissivity (Ɛ*) <strong>of</strong> the surface<br />

material. This is the value that must be set into the instrument's menu under<br />

the specific conditions <strong>of</strong> measurement for the instrument to display an<br />

accurate surface temperature value. When attempting to make temperature<br />

measurements on a target <strong>of</strong> unknown emissivity. an estimate <strong>of</strong> emissivity<br />

may be the only available alternative. There are numerous reference tables<br />

available that list generic values <strong>of</strong> emissivity for common materials and these<br />

can be used as guides. Table 2.2 is an example <strong>of</strong> a reference table. As<br />

previously noted. emissivity depends on the material and the surface texture.<br />

It may also vary with surface temperature and with the spectral interval over<br />

which the measurement is made. These variations, though usually small ,<br />

cannot always be ignored.<br />

Charlie Chong/ Fion Zhang


For an emissivity reference table to be useful. conditions <strong>of</strong> target<br />

temperature and spectral interval (wavelength) must also be presented. If the<br />

temperature and wavelength listed do not correspond to the actual<br />

measurement conditions. the emissivity listed must be considered to be a<br />

rough estimate. Even if there is an exact match to the measurement<br />

conditions, the lookup method is not the best approach for accurate<br />

temperature measurement. Ideally. the way to determine effective<br />

emissivity is to measure it with one <strong>of</strong> the several established protocols. using<br />

a sample <strong>of</strong> the actual target surface material and the actual instrument to be<br />

used for the measurement mission. The protocols for measuring effective<br />

emissivity <strong>of</strong> material samples are discussed in Chapter 4.<br />

Charlie Chong/ Fion Zhang


Reflectivity ρ<br />

Reflectivity <strong>of</strong> a surface generally increases as emissivity decreases. For<br />

opaque graybody surfaces τ=0. the sum <strong>of</strong> emissivity and reflectivity is unity<br />

(1.0). Therefore. an opaque graybody surface with a low effective cmissivity<br />

will be highly reflective, which can result in erroneous temperature <strong>reading</strong>s<br />

even if the correct emissivity is set into the instrument. These errors can be<br />

the result <strong>of</strong> either point source reflections, background reflections or both<br />

entering the instrument . There are two components <strong>of</strong> reflected energy the<br />

diffuse componenl and the specular component. If the surface is relatively<br />

specular (smooth). most <strong>of</strong> the reflected energy is specular, that is. it reflects<br />

<strong>of</strong>f the surface at an angle complementary to the angle <strong>of</strong> incidenct. If the<br />

surface is relatively diffuse (textured) most <strong>of</strong> the renected energy is scattered<br />

uniformly (haphazardly?) in all directions regardless <strong>of</strong> the angle <strong>of</strong> incidence.<br />

Keywords:<br />

Therefore. an opaque graybody surface with a low effective cmissivity will be<br />

highly reflective<br />

Charlie Chong/ Fion Zhang


Errors because <strong>of</strong> point source reflections are usually larger when the target<br />

surfaces are specular, and errors because <strong>of</strong> background reflections are not<br />

affected by the specularity or diffusivity <strong>of</strong> the target surface. Both types <strong>of</strong><br />

reflective errors are more serious when the target surface is cool compared to<br />

the temperature <strong>of</strong> the point source or the background because the point<br />

source makes a greater contribution to the total radiant exitance than the<br />

target does. In practice, the thermographer can learn to recognize and avoid<br />

errors due to point source reflections. The thermographer also can learn to<br />

measure and compensate for errors due to background reflection. This is<br />

discussed in Chapter 4.<br />

Charlie Chong/ Fion Zhang


Transmissivity τ<br />

When the target surface is a non-graybody, the target material may be <strong>part</strong>ly<br />

transparent to <strong>infrared</strong> radiation. This means the target material has a<br />

transmissivity greater than 0. Due to this transparency. radiant thermal energy<br />

may be transmitted through the target from sources behind the target. This<br />

energy may enter the instrument and cause temperature measurement errors<br />

even if the correct emissivity is set into the instrument and reflective errors<br />

are eliminated. Although errors due to transmission are the least common in<br />

practice. errors due to energy transmiued through the target usually require<br />

the most sophisticated procedures to correct them. In most cases, spectral<br />

filtering is the best solution. Methods for correcting these errors are discussed<br />

in Chapters 4 and 5.<br />

Keywords:<br />

■ spectral filtering<br />

■ non-graybody (could be any others like black body, selective emitter, could<br />

be a body with τ > 0)<br />

Charlie Chong/ Fion Zhang


View Angle<br />

The angle between the instrument's line <strong>of</strong> sight and the surface material will<br />

have a minimal effect on the material properties described above, providing<br />

this angle is kepi as close as possible to normal (perpendicul ar) and no<br />

greater than ±30 degrees from normal (for many nonmetallic surfaces this<br />

may be increased 10 as large as ±60 degrees from normal. if unavoidable).<br />

If it is not possible to view a target at an angle within this range, the effective<br />

emissivity may Change. <strong>part</strong>icularly if it is low to begin with. This will most<br />

likely compromise the accuracy <strong>of</strong> temperature measurements. Note that the<br />

emissivities listed in Table 2.2 are normal emissivities and are not valid at<br />

acute viewing angles. On curved (nonflat) surfaces. view angle can be even<br />

more critical and measurements should be made cautiously.<br />

Note:<br />

An acute angle is an angle whose degree measure is greater than 0 but less<br />

than 90.<br />

Charlie Chong/ Fion Zhang


2.3 Heat Conducting Properties <strong>of</strong> Materials<br />

The use <strong>of</strong> <strong>infrared</strong> themlography for nondestructive material testing is<br />

generally based on the assumption that uniform structural continuity provides<br />

uniform thermal continuity. Both unstimulated and stimulated approaches to<br />

thermographic material testing depend on this assumption. as will be<br />

discussed in greater detail in Chapters 4 and 5. It is necessary. therefore, that<br />

the thermographer have a clear basic understanding <strong>of</strong> the manner in which<br />

heat flows within a material and the material properties that affect this flow.<br />

Keywords:<br />

The use <strong>of</strong> <strong>infrared</strong> themlography for nondestructive material testing is<br />

generally based on the assumption that uniform structural continuity provides<br />

uniform thermal continuity.<br />

Charlie Chong/ Fion Zhang


Thermal Conductivity<br />

Thermal conductivity k is the relative one dimensional capability <strong>of</strong> a material<br />

to transfer heat. It affects the speed (thus time, t) that a given quantity <strong>of</strong> heat<br />

applied to one point in a slab <strong>of</strong> material will travel a given distance within that<br />

material to another point cooler than the first. Thermal conductivity is high for<br />

metals and low for porous materials. It is logical. therefore. that heat will be<br />

conducted more rapidly in metals than in more porous materials. Although<br />

thermal conductivity varies slightly with temperature in solids and liquids and<br />

with temperature and pressure in gases, for practical purposes it can be<br />

considered a constant for a <strong>part</strong>icular material. Table 2.1 is a list <strong>of</strong> thermal<br />

properties for several conunon materials.<br />

Charlie Chong/ Fion Zhang


Heat Capacity<br />

The heat capacity <strong>of</strong> a malerial or a structure describes its ability to store heat.<br />

It is the product <strong>of</strong> the specific thermal energy C p and the density ρ <strong>of</strong> the<br />

material. When thermal energy is stored in a structure and then the structure<br />

is placed in a cooler environment, the sections <strong>of</strong> the structure that have low<br />

heat capacity will change temperature more rapidly because less thermal<br />

energy is stored in them. Consequently, these sections will reach thermal<br />

equilibrium with their surroundings sooner than those sections with higher<br />

heat capacity, The term thermal capacitance is used to describe heat capacity<br />

in terms <strong>of</strong> an electrical analog. where loss <strong>of</strong> heat is analogous to loss <strong>of</strong><br />

charge on a capacitor. Structures with low thermal capacitance reach<br />

equilibrium sooner when placed in a cooler environmcnt than those with high<br />

thermal capacitance. This phenomenon is exploited when performing<br />

unstimulated nondestructive testing <strong>of</strong> structures, specifically when locating<br />

water saturated sections on flat ro<strong>of</strong>s. This is discussed in greater detail in<br />

Chapter 5,<br />

Charlie Chong/ Fion Zhang


Thermal Diffusivity<br />

As in emissivity Ɛ. the heat conducting properties <strong>of</strong> materials may vary from sample<br />

to sample. depending on variables in the fabrication process and other factors.<br />

Thermal diffusivity α is the 3D expansion <strong>of</strong> thermal conductivity in any given material<br />

sample. Diffusivily relates more to transient heat flow, whereas conductivity relates to<br />

steady state heat flow. It takes into account the thermal conductivity k <strong>of</strong> the sample,<br />

its specific heat C p<br />

, and its density ρ. Its equation is<br />

α = k/ρ C p cm 2 s -1 .<br />

Because thermal diffusivity <strong>of</strong> a sample can be measured directly using <strong>infrared</strong><br />

<strong>thermography</strong>, it is used extensively by the materials flaw evaluation community as an<br />

assessment <strong>of</strong> a test sample's ability to carry heat away, in all directions, from a heat<br />

injection site. Table 2.1 lists thermal diffusivities for several common materials in<br />

increasing order <strong>of</strong> thermal diffusivity. Several protocols for measuring the thermal<br />

diffusivity <strong>of</strong> a test sample are described by Maldague.<br />

Charlie Chong/ Fion Zhang


Thermal Diffusivity<br />

Diffusivily relates more to transient heat<br />

flow, whereas conductivity relates to<br />

steady state heat flow.<br />

Charlie Chong/ Fion Zhang


Partial 2.1<br />

Charlie Chong/ Fion Zhang


Partial Table 2.1<br />

Charlie Chong/ Fion Zhang


Partial Table 2.2<br />

Charlie Chong/ Fion Zhang


Thermal Diffusivity<br />

As in emissivity Ɛ. the heat conducting properties <strong>of</strong> materials may vary from sample to sample. depending on<br />

variables in the fabrication process and other factors. Thermal diffusivity α is the 3D expansion <strong>of</strong> thermal<br />

conductivity in any given material sample. Diffusivily relates more to transient heat flow, whereas conductivity<br />

relates to steady state heat flow. It takes into account the thermal conductivity k <strong>of</strong> the sample, its specific heat<br />

Cp, and its density ρ. Its equation is<br />

α = k/ρ ∙ C p cm 2 s -1 .<br />

for my ASNT exam<br />

Charlie Chong/ Fion Zhang


Chapter 2<br />

Review Questions<br />

Q&A<br />

1. c<br />

2. b<br />

3. a<br />

4. d<br />

5. a<br />

6. b<br />

7. a<br />

8. b<br />

9. b<br />

10. b<br />

Charlie Chong/ Fion Zhang


1. The best way to determine the effective emissivity <strong>of</strong> a target surface is:<br />

a. to look it up in a table.<br />

b. to calcu late it.<br />

c. to measure the effective emissivity <strong>of</strong> the material itself or a similar<br />

sample.<br />

d. all <strong>of</strong> the above.<br />

2. For an opaque graybody target surface, emissivity equals:<br />

a. 1/refleclivity.<br />

b. 1-reflectivity.<br />

c. 1.0.<br />

d. reflectivity to the fourth power.<br />

3. The effective emissivity <strong>of</strong> a surface is always affected by:<br />

a. the material, its surface texture and the viewing angle.<br />

b. the material, its thermal conductivity and humidity.<br />

c. the material, its surface texture and its thermal diffusivity.<br />

d. the material, its visible color and its thermal conductivity.<br />

Charlie Chong/ Fion Zhang


4. When measuring the temperature <strong>of</strong> a nongraybody target:<br />

a, the viewing angle is not critical.<br />

b. always assume an emissivity <strong>of</strong> 1.0.<br />

c. reflections <strong>of</strong>f the near surface may be ignored.<br />

d. errors may be caused by hot sources behind the target.<br />

5. The effective emissivity <strong>of</strong> a target surface:<br />

a, can vary at different wavelengths.<br />

b. is the same for all wavelengths if the viewing angle is kept constant.<br />

c. is always higher at longer wavelengths.<br />

d. is always lower at longer wavelengths.<br />

6. Unfinished, unoxidized metal surfaces usually have:<br />

a. high and uniform emissivities.<br />

b. low and uniform emissivities.<br />

c. non-graybody characteristics.<br />

d. low specular reflectivity.<br />

Charlie Chong/ Fion Zhang


7. Thermal diffusivity is:<br />

a. high for metals and low for porous materials.<br />

b. the same for all metals.<br />

c, low for metals and high for porous materials.<br />

d. the same for all porous materials.<br />

8. Thermal diffusivity is:<br />

a, the same as diffuse reflectivity.<br />

b. related more to transient heat flow than to steady Slale heat flow.<br />

c. related more 10 steady stale heat flow than to transient heat flow.<br />

d. the same as spectral transmittance.<br />

9. Thermal capacitance:<br />

a. describes the heating <strong>of</strong> a condenser.<br />

b. expresses the heat capacity <strong>of</strong> a material in a form analogous to<br />

electrical capacitance.<br />

c. is zero for a blackbody radiator.<br />

d. describes the maximum temperature rating <strong>of</strong> a capacitor.<br />

Charlie Chong/ Fion Zhang


10. A highly textured surface is said to be diffuse. A smooth surface is said to<br />

be:<br />

a. opaque.<br />

b. specular.<br />

c. convex.<br />

d. transparent.<br />

Charlie Chong/ Fion Zhang


Chapter 3<br />

Thermal Instrumentation<br />

Charlie Chong/ Fion Zhang


3.1 Thermal Instrumentation Overview<br />

Equipment for temperature measurement and <strong>thermography</strong> includes<br />

contacting as well as noncontacting devices. Contacting devices for<br />

temperature measurement include thermopiles. thermocouples, liquid<br />

thermometers, gas expansion devices (bourdon gas thermometers), liquid<br />

crystals (cholesterol crystals ?), heat flux indicators and fiber optic sensors.<br />

Aside from some specialized instruments, the vast majority <strong>of</strong> noncontacting<br />

temperature measurement devices are <strong>infrared</strong> sensing instruments and<br />

systems. Infrared sensing instruments and systems are divided into (1) point<br />

sensors (radiation thermometers), (2) line scanners and (3) thermal imagers.<br />

This chapter begins with a review <strong>of</strong> contacting thermal measurement<br />

instruments and a discussion <strong>of</strong> the basic configurations <strong>of</strong> <strong>infrared</strong> sensing<br />

and imaging instruments. This is followed by a discussion <strong>of</strong> performance<br />

parameters and, finally, descriptions <strong>of</strong> commercial thermal sensing and<br />

imaging equipment, thermographic image processing s<strong>of</strong>tware and image<br />

hard copy recording accessories.<br />

Charlie Chong/ Fion Zhang


What is Thermopile<br />

A thermopile is an electronic device that converts thermal energy into electrical energy.<br />

It is composed <strong>of</strong> several thermocouples connected usually in series or, less<br />

commonly, in parallel. Thermopiles do not respond to absolute temperature, but<br />

generate an output voltage proportional to a local temperature difference or<br />

temperature gradient.<br />

Thermopiles are used to provide an output in response to temperature as <strong>part</strong> <strong>of</strong> a<br />

temperature measuring device, such as the <strong>infrared</strong> thermometers widely used by<br />

medical pr<strong>of</strong>essionals to measure body temperature. They are also used widely in<br />

heat flux sensors (such as the Moll thermopile and Eppley pyrheliometer) and gas<br />

burner safety controls. The output <strong>of</strong> a thermopile is usually in the range <strong>of</strong> tens or<br />

hundreds <strong>of</strong> millivolts. As well as increasing the signal level, the device may be used<br />

to provide spatial temperature averaging. Thermopiles are also used to generate<br />

electrical energy from, for instance, heat from electrical components, solar wind,<br />

radioactive materials, or combustion. The process is also an example <strong>of</strong> the Peltier<br />

Effect (electric current transferring heat energy) as the process transfers heat from the<br />

hot to the cold junctions.<br />

Charlie Chong/ Fion Zhang<br />

http://en.wikipedia.org/wiki/Thermopile


Thermopile- Thermoelectric Seebeck module<br />

Charlie Chong/ Fion Zhang<br />

http://en.wikipedia.org/wiki/Thermopile


The Working Principle: Thermopile, composed <strong>of</strong> multiple thermocouples in<br />

series. If both the right and left junctions are the same temperature, voltages<br />

cancel out to zero. However if one side is heated and other side cooled,<br />

resulting total output voltage is equal to the sum <strong>of</strong> junction voltage<br />

differentials.<br />

Charlie Chong/ Fion Zhang


What is a IR Thermopile? (non-contact)<br />

A thermopile is a serially-interconnected array <strong>of</strong> thermocouples, each <strong>of</strong><br />

which consists <strong>of</strong> two dissimilar materials with a large thermoelectric power<br />

and opposite polarities. The thermocouples are placed across the hot and<br />

cold regions <strong>of</strong> a structure and the hot junctions are thermally isolated from<br />

the cold junctions. The cold junctions are typically placed on the silicon<br />

substrate to provide effective heat sink. In the hot regions, there is a black<br />

body for absorbing the <strong>infrared</strong>, which raises the temperature according to the<br />

intensity <strong>of</strong> the incident <strong>infrared</strong>. These thermopiles employ two different<br />

thermoelectric materials which are placed on a thin diaphragm having a low<br />

thermal conductance and capacitance.<br />

Charlie Chong/ Fion Zhang<br />

http://www.ge-mcs.com/download/temperature/930-164A-LR.PDF


IR Thermopiles Sensor (non-contact)<br />

Charlie Chong/ Fion Zhang


IR Thermopile Quad Sensor (non-contact)<br />

Charlie Chong/ Fion Zhang


Thermocouple<br />

General description: Thomas Seebeck discovered in 1821 that when two wires composed <strong>of</strong><br />

dissimilar metals are joined at both ends and one <strong>of</strong> the ends is heated, there is a continuous<br />

current which flows in the thermoelectric circuit. (Seebeck effect). The junctions can be exposed,<br />

grounded or ungrounded. The thermocouple is normally directly connected to a standard<br />

temperature controller. Thermocouples are among the easiest temperature sensors used in<br />

science and industry and very cost effective. (usually less than $50.00)<br />

thermocouple embedded in<br />

Dalton cartridge heater<br />

Charlie Chong/ Fion Zhang<br />

http://www.deltat.com/thermocouple.html


Thermocouple<br />

A thermocouple is a temperature-measuring device consisting <strong>of</strong> two dissimilar conductors that contact each other at one or more spots, where a temperature differential is experienced by the<br />

different conductors (or semiconductors). It produces a voltage when the temperature <strong>of</strong> one <strong>of</strong> the spots differs from the reference temperature at other <strong>part</strong>s <strong>of</strong> the circuit. Thermocouples are a<br />

widely used type <strong>of</strong> temperature sensor for measurement and control, and can also convert a temperature gradient into electricity. Commercial thermocouples are inexpensive, interchangeable,<br />

are supplied with standard connectors, and can measure a wide range <strong>of</strong> temperatures. In contrast to most other methods <strong>of</strong> temperature measurement, thermocouples are self powered and<br />

require no external form <strong>of</strong> excitation. The main limitation with thermocouples is accuracy; system errors <strong>of</strong> less than one degree Celsius (°C) can be difficult to achieve.<br />

Any junction <strong>of</strong> dissimilar metals will produce an electric potential related to temperature. Thermocouples for practical measurement <strong>of</strong> temperature are junctions <strong>of</strong> specific alloys which have a<br />

predictable and repeatable relationship between temperature and voltage. Different alloys are used for different temperature ranges. Properties such as resistance to corrosion may also be<br />

important when choosing a type <strong>of</strong> thermocouple. Where the measurement point is far from the measuring instrument, the intermediate connection can be made by extension wires which are<br />

less costly than the materials used to make the sensor. Thermocouples are usually standardized against a reference temperature <strong>of</strong> 0 degrees Celsius; practical instruments use electronic<br />

methods <strong>of</strong> cold-junction compensation to adjust for varying temperature at the instrument terminals. Electronic instruments can also compensate for the varying characteristics <strong>of</strong> the<br />

thermocouple, and so improve the precision and accuracy <strong>of</strong> measurements. Thermocouples are widely used in science and industry; applications include temperature measurement for kilns,<br />

gas turbine exhaust, diesel engines, and other industrial processes. Thermocouples are also used in homes, <strong>of</strong>fices and businesses as the temperature sensors in thermostats, and also as<br />

flame sensors in safety devices for gas-powered major appliances.<br />

Charlie Chong/ Fion Zhang<br />

http://en.wikipedia.org/wiki/Thermocouple


Liquid or Gas Expansion Devices<br />

Many physical properties change with temperature, such as the volume <strong>of</strong> a liquid, the length <strong>of</strong> a metal rod,<br />

the electrical resistance <strong>of</strong> a wire, the pressure <strong>of</strong> a gas kept at constant volume, and the volume <strong>of</strong> a gas kept<br />

at constant pressure. Filled-system thermometers use the phenomenon <strong>of</strong> thermal expansion <strong>of</strong> matter to<br />

measure temperature change.<br />

The filled thermal device consists <strong>of</strong> a primary element that takes the form <strong>of</strong> a reservoir or bulb, a flexible<br />

capillary tube, and a hollow Bourdon tube that actuates a signal-transmitting device and/or a local indicating<br />

temperature dial. A typical filled-system thermometer is shown in Figure 7-1. In this system, the filling fluid,<br />

either liquid or gas, expands as temperature increases. This causes the Bourdon tube to uncoil and indicate the<br />

temperature on a calibrated dial.<br />

Charlie Chong/ Fion Zhang


Bourdon Gas Thermometers<br />

Charlie Chong/ Fion Zhang


Liquid Crystal Thermometer<br />

A liquid crystal thermometer or plastic strip thermometer is a type <strong>of</strong> thermometer that contains heat-sensitive<br />

(thermochromic) liquid crystals in a plastic strip that change color to indicate different temperatures. Liquid<br />

crystals possess the mechanical properties <strong>of</strong> a liquid, but have the optical properties <strong>of</strong> a single crystal.<br />

Temperature changes can affect the color <strong>of</strong> a liquid crystal, which makes them useful for temperature<br />

measurement. The resolution <strong>of</strong> liquid crystal sensors is in the 0.1°C range. Disposable liquid crystal<br />

thermometers have been developed for home and medical use. For example if the thermometer is black and it<br />

is put onto someone's forehead it will change colour depending on the temperature <strong>of</strong> the person.<br />

There are two stages in the liquid crystals: 1. the hot nematic stage is the closest to the liquid phase where the<br />

molecules are freely moving around and only <strong>part</strong>ly ordered. 2. the cold smectic stage is closest to a solid<br />

phase where the molecules align themselves into tightly wound chiral matrixes.<br />

Liquid crystal thermometers portray temperatures as colors and can be used to follow temperature changes<br />

caused by heat flow. They can be used to observe that heat flows by conduction, convection, and radiation. In<br />

medical applications, liquid crystal thermometers may be used to read body temperature by placing against the<br />

forehead. These are safer than a mercury-in-glass thermometer, and may be advantageous in some patients,<br />

but do not always give an exact result, except the analytic liquid crystal thermometer which show the exact<br />

temperature between 35.5 to 40.5° Celsius.<br />

Charlie Chong/ Fion Zhang<br />

http://en.wikipedia.org/wiki/Liquid_crystal_thermometer


Liquid Crystal Thermometer<br />

A liquid crystal thermometer or plastic strip thermometer is a type <strong>of</strong><br />

thermometer that contains heat-sensitive (thermochromic) liquid crystals in a<br />

plastic strip that change color to indicate different temperatures. Liquid<br />

crystals possess the mechanical properties <strong>of</strong> a liquid, but have the optical<br />

properties <strong>of</strong> a single crystal.<br />

Charlie Chong/ Fion Zhang


Thermocouple<br />

Thermocouple grade wires<br />

Stainless steel sheath<br />

Flexible SS sheath<br />

Adjustable nut<br />

Wire junction<br />

Charlie Chong/ Fion Zhang<br />

http://www.omega.com/temperature/z/pdf/z021-032.pdf


Bimetallic Thermometers<br />

Charlie Chong/ Fion Zhang<br />

http://www.omega.com/temperature/z/pdf/z021-032.pdf


Resistance Thermometers - Resistance thermometers, also called resistance<br />

temperature detectors (RTDs), are sensors used to measure temperature by correlating the<br />

resistance <strong>of</strong> the RTD element with temperature. Most RTD elements consist <strong>of</strong> a length <strong>of</strong> fine<br />

coiled wire wrapped around a ceramic or glass core. The element is usually quite fragile, so it is<br />

<strong>of</strong>ten placed inside a sheathed probe to protect it. The RTD element is made from a pure<br />

material, typically platinum, nickel or copper. The material has a predictable change in resistance<br />

as the temperature changes and it is this predictable change that is used to determine<br />

temperature. They are slowly replacing the use <strong>of</strong> thermocouples in many industrial applications<br />

below 600 °C, due to higher accuracy and repeatability.<br />

http://www.npl.co.uk/content/ConMediaFile/113<br />

Charlie Chong/ Fion Zhang<br />

http://en.wikipedia.org/wiki/Resistance_thermometer


In RTD devices; Copper, Nickel and Platinum<br />

are widely used metals. These three metals are<br />

having different resistance variations with<br />

respective to the temperature variations. That is<br />

called resistance-temperature characteristics.<br />

Platinum has the temperature range <strong>of</strong> 650°C,<br />

and then the Copper and Nickel have 120°C<br />

and 300°C respectively. The figure-1 shows the<br />

resistance-temperature characteristics curve <strong>of</strong><br />

the three different metals. For Platinum, its<br />

resistance changes by approximately 0.4 ohms<br />

per degree Celsius <strong>of</strong> temperature.<br />

The purity <strong>of</strong> the platinum is checked by<br />

measuring R100 / R0. Because, whatever the<br />

materials actually we are using for making the<br />

RTD that should be pure. If it will not pure, it will<br />

deviate from the conventional resistancetemperature<br />

graph. So, α and β values will<br />

change depending upon the metals.<br />

Charlie Chong/ Fion Zhang<br />

http://en.wikipedia.org/wiki/Resistance_thermometer


Platinum Resistance Thermometer<br />

http://www.aoip.com/product/670-standard-platinum-resistance-thermometers/<br />

Charlie Chong/ Fion Zhang


Platinum Resistance Thermometer<br />

Charlie Chong/ Fion Zhang


Resistance Temperature Detector (RTD) - Principle <strong>of</strong> Operation,<br />

Materials, Configuration and Benefits by Innovative Sensor Technology<br />

Overview<br />

Innovative Sensor Technology is a world-class manufacturer <strong>of</strong> thin-film RTD<br />

temperature sensors, capacitive humidity sensors, and mass flow sensors at the<br />

component level. With our state-<strong>of</strong>-the-art manufacturing technology, Innovative<br />

Sensor Technology <strong>of</strong>fers both standard and custom sensors to satisfy unique<br />

applications. Additionally, our highly qualified staff is now <strong>of</strong>fering R&D consulting<br />

services for industrial applications. Our sensors have applications in the automotive,<br />

HVAC, appliance, controls, and test & measurement industries.<br />

Resistance Temperature Detector (RTD) - Principle <strong>of</strong> Operation<br />

An RTD (resistance temperature detector) is a temperature sensor that operates on<br />

the measurement principle that a material’s electrical resistance changes with<br />

temperature. The relationship between an RTD resistance and the surrounding<br />

temperature is highly predictable, allowing for accurate and consistent temperature<br />

measurement. By supplying an RTD with a constant current and measuring the<br />

resulting voltage drop across the resistor, the RTD resistance can be calculated, and<br />

the temperature can be determined.<br />

Charlie Chong/ Fion Zhang<br />

http://www.azom.com/article.aspx?ArticleID=5573


RTD Materials<br />

Different materials used in the construction <strong>of</strong> RTD <strong>of</strong>fer a different relationship<br />

between resistance and temperature. Temperature sensitive materials used in the<br />

construction <strong>of</strong> RTD include platinum, nickel, and copper; platinum being the most<br />

commonly used. Important characteristics <strong>of</strong> an RTD include the temperature<br />

coefficient <strong>of</strong> resistance (TCR), the nominal resistance at 0 degrees Celsius, and the<br />

tolerance classes. The TCR determines the relationship between the resistance and<br />

the temperature. There are no limits to the TCR that is achievable, but the most<br />

common industry standard is the platinum 3850 ppm/K. This means that the<br />

resistance <strong>of</strong> the sensor will increase 0.385 ohms per one degree Celsius increase in<br />

temperature. The nominal resistance <strong>of</strong> the sensor is the resistance that the sensor<br />

will have at 0 degrees Celsius. Although almost any value can be achieved for<br />

nominal resistance, the most common is the platinum 100 ohm (pt100). Finally, the<br />

tolerance class determines the accuracy <strong>of</strong> the sensor, usually specified at the<br />

nominal point <strong>of</strong> 0 degrees Celsius. There are different industry standards that have<br />

been set for accuracy including the ASTM and the European DIN. Using the values <strong>of</strong><br />

TCR, nominal resistance, and tolerance, the functional characteristics <strong>of</strong> the sensor<br />

are defined.<br />

Charlie Chong/ Fion Zhang<br />

http://www.azom.com/article.aspx?ArticleID=5573


RTD Configurations<br />

In addition to different materials, RTD are also <strong>of</strong>fered in two major configurations:<br />

wire wound and thin film. Wire wound configurations feature either an inner coil RTD<br />

or an outer wound RTD. An inner coil construction consists <strong>of</strong> a resistive coil running<br />

through a hole in a ceramic insulator, whereas the outer wound construction involves<br />

the winding <strong>of</strong> the resistive material around a ceramic or glass cylinder, which is then<br />

insulated.<br />

The thin film RTD construction features a thin layer <strong>of</strong> resistive material deposited onto<br />

a ceramic substrate through a process called deposition. A resistive meander is then<br />

etched onto the sensor, and laser trimming is used to achieve the appropriate nominal<br />

values <strong>of</strong> the sensor. The resistive material is then protected with a thin layer <strong>of</strong> glass,<br />

and lead wires are welded to pads on the sensor and covered with a glass dollop.<br />

Thin film RTD have advantages over the wire wound configurations. The main<br />

advantages include that they are less expensive, are more rugged and vibration<br />

resistant, and have smaller dimensions that lead to better response times and<br />

packaging capabilities. For a long time wire wound sensors featured much better<br />

accuracy. Thanks to recent developments, however, there is now thin film technology<br />

capable <strong>of</strong> achieving the same level <strong>of</strong> accuracy.<br />

Charlie Chong/ Fion Zhang<br />

http://www.azom.com/article.aspx?ArticleID=5573


Operations <strong>of</strong> RTD<br />

An RTD takes a measurement when a small DC current is supplied to the sensor. The<br />

current experiences the impedance <strong>of</strong> the resistor, and a voltage drop is experienced<br />

over the resistor. Depending on the nominal resistance <strong>of</strong> the RTD, different supply<br />

currents can be used. To reduce self-heating on the sensor the supply current should<br />

be kept low. In general, around 1mA or less <strong>of</strong> current is used. An RTD can be<br />

connected in a two, three, or four-wire configuration. The two-wire configuration is the<br />

simplest and also the most error prone. In this setup, the RTD is connected by two<br />

wires to a Wheatstone bridge circuit and the output voltage is measured. The<br />

disadvantage <strong>of</strong> this circuit is that the two connecting lead wire resistances add<br />

directly two the RTD resistance and an error is incurred.<br />

2-Wire Configuration<br />

Charlie Chong/ Fion Zhang<br />

http://www.azom.com/article.aspx?ArticleID=5573


The four-wire configuration consists <strong>of</strong> two current leads and two potential leads that<br />

measure the voltage drop across the RTD. The two potential leads are high resistance<br />

to negate the effect <strong>of</strong> the voltage drop due to current flowing during the measurement.<br />

This configuration is ideal for canceling the lead wire resistances in the circuit as well<br />

as eliminating the effects <strong>of</strong> different lead resistances, which was a possible problem<br />

with the three-wire configuration. The four-wire configuration is commonly used when<br />

a highly accurate measurement is required for the application.<br />

4-Wire Configuration<br />

Charlie Chong/ Fion Zhang<br />

http://www.azom.com/article.aspx?ArticleID=5573


Benefits <strong>of</strong> Thin Film RTD<br />

There are many options when considering contact temperature measurement,<br />

including thermocouples, thermistors, and RTD (wire wound and thin film).<br />

While thermocouples can handle very high temperatures and thermistors are<br />

inexpensive, there are many advantages <strong>of</strong> RTD. Some <strong>of</strong> these advantages<br />

include their accuracy, precision, long-term stability, and good hysteresis<br />

characteristics. Even beyond these, there are advantages <strong>of</strong> thin film RTD<br />

over wire wound, including smaller dimensions, better response times,<br />

vibration resistance, and relative inexpensiveness. New advancements has<br />

even made thin film technology just as accurate as wire wound at higher<br />

temperatures ranges.<br />

Charlie Chong/ Fion Zhang<br />

http://www.azom.com/article.aspx?ArticleID=5573


Thermistor<br />

A thermistor is a type <strong>of</strong> resistor whose resistance varies significantly with temperature,<br />

more so than in standard resistors. The word is a portmanteau <strong>of</strong> thermal and resistor.<br />

Thermistors are widely used as inrush current limiter, temperature sensors (NTC type<br />

typically), self-resetting overcurrent protectors, and self-regulating heating elements.<br />

Thermistors differ from resistance temperature detectors (RTDs) in that the material<br />

used in a thermistor is generally a ceramic or polymer, while RTDs use pure metals.<br />

The temperature response is also different; RTDs are useful over larger temperature<br />

ranges, while thermistors typically achieve a higher precision within a limited<br />

temperature range, typically −90 °C to 130 °C<br />

Charlie Chong/ Fion Zhang<br />

http://en.wikipedia.org/wiki/Thermistor


Thermistor<br />

Charlie Chong/ Fion Zhang<br />

http://swordrock.wordpress.com/category/robotic-2/


Thermistor<br />

Charlie Chong/ Fion Zhang<br />

http://en.wikipedia.org/wiki/Thermistor


3.2 Contacting Thermal Measuring Devices<br />

The most commonly used contacting devices include bimetallic thermometers,<br />

thermochromic liquid crystals, thermocouples, resistance thermometer,<br />

thermistors and heat flux indicators. These devices are discussed briefly here.<br />

For more detailed information, refer to ASNT Nondestructive Testing<br />

Handbook. third edition: Volume 3. Infrared and Thermal Testing.<br />

■ Bimetallic Thermometers<br />

Bimetallic thermometers are sensors constructed <strong>of</strong> dissimilar metallic strips<br />

bonded together. Typically. different iron nickel alloys are used. The strips<br />

differ in temperature coefficient <strong>of</strong> expansion such that temperature changes<br />

result in predictable bending <strong>of</strong> the assembly. Arranged in a spiral or helical<br />

configuration. one end <strong>of</strong> the bimetallic element is fixed and the other end is<br />

attached to a pointer. Properly calibrated, the angular position <strong>of</strong> the pointer<br />

can be made to indicate temperature on a scale.<br />

Charlie Chong/ Fion Zhang


■ Thermochromic Liquid Crystals<br />

Thermochromic liquid crystals (also called cholesterol crystals) change color<br />

with temperature. Coatings made <strong>of</strong> liquid crystals are commonly used as<br />

temperature threshold indicators. Depending on the mixture. a coating<br />

applied to a surface will change color predictably when the surface exceeds a<br />

threshold temperature. The color change may be reversible or irreversible.<br />

and the sensing range for most mixtures is limited to a narrow temperature<br />

span. Typically. a set <strong>of</strong> liquid crystal markers provides a selection <strong>of</strong><br />

transition temperatures. This allows the user to select the appropriate marker<br />

for the desired temperature.<br />

Keywords:<br />

Threshold temperature<br />

Charlie Chong/ Fion Zhang


■ Thermocouple<br />

Thermocouples are contact temperature sensors based on the thermoelectric<br />

effect. or Seebeck effect. Thomas Seebeck discovered that, when two<br />

dissimilar metals arc joined at both ends and these ends are at different<br />

temperatures, a predictable direct current will flow through the circuit. The<br />

thermoelectric coefficient determines the relationship between this current<br />

and the temperature difference between the two junctions. This coefficient is<br />

known for each type <strong>of</strong> thermocouple. To configure a thermometer. the circuit<br />

is broken and the open-circuit voltage is measured by a volt meter. One <strong>of</strong> the<br />

two junctions is then held al a reference temperature. such as an ice bath,<br />

and the voltage is calibrated to indicate the temperature <strong>of</strong> the other junction.<br />

which then becomes the temperature sensing junction. Thermopiles arc<br />

banks <strong>of</strong> thermocouples connected in parallel or in series to increase output<br />

gradient. The reference temperature is important because <strong>of</strong> the<br />

thermocouples' non linear response.<br />

Keywords:<br />

thermoelectric coefficient<br />

Charlie Chong/ Fion Zhang


■ Resistance Thermometers<br />

Resistance temperature detector (RTDs) arc contact sensors thaI measure<br />

tcmpcralUrc by a predictable change in resistance as a function <strong>of</strong><br />

temperature. Platinum is the most popular resistance temperature detector<br />

material because <strong>of</strong> its excellent stability and its linear response to<br />

temperature change. Other materials used include nickel. copper. tungsten<br />

and iridium. In operation. the resistance temperature detector may be placed<br />

in a bridge circuit such that the bridge output voltage is a measure <strong>of</strong> the<br />

resistance and hence the temperature at the resistance temperature detector.<br />

A more accurate measurement may be achieved by using a constant current<br />

source and a digital volt meter (DVM). such that the digital volt meter <strong>reading</strong><br />

is proportional to the resistance temperature detector resistance and hence<br />

the temperature at the resistance temperature detector.<br />

Charlie Chong/ Fion Zhang


■ Thermistors<br />

Thermistors arc also sensors that measure temperature by a predictable<br />

change in resistance as a fun ction <strong>of</strong> temperature. Thermistors are made <strong>of</strong><br />

semiconductor materials. Whereas resistance temperature detectors are low<br />

impedance devices. thennistors are high impedance devices. Thermistors<br />

typically are more sensitive to temperature changes than resistance<br />

temperature detectors but thermistors are not as stable.<br />

Keywords:<br />

Thermistors typically are more sensitive to temperature changes than<br />

resistance temperature detectors<br />

Charlie Chong/ Fion Zhang


■ Heat Flux Indicators<br />

Heat flux indicators are heat flow meters and are used to measure rates in<br />

conduction, convection, radiation and phase change systems such as<br />

building walls, boiler tubes and air conditioning ducts. A typical heat flux<br />

indicator consists <strong>of</strong> a sensitive thermopile, composed <strong>of</strong> many fine gage<br />

thermocouples connected in series on opposite sides <strong>of</strong> a nat core wilh<br />

known and stable thermal resistance. The entire assembly is covered with<br />

protective material.<br />

The voltage generated across the thermopile is calibrated to be a measure <strong>of</strong><br />

the steady state heat flux through the device. Transient heat flux can be<br />

related to the transient thermopile output and the geometry <strong>of</strong> the device.<br />

Charlie Chong/ Fion Zhang


3.3 Optical Pyrometers<br />

Optical pyrometers include brightness pyrometers and <strong>infrared</strong> pyrometers.<br />

Infrared pyrometers are also called <strong>infrared</strong> radiation themlometers. Various<br />

types are discussed in the next section. Brightness pyrometers are also called<br />

matching pyrometers. They incorporate a calibrated light source (lamp)<br />

powered by a calibrated current supply. Looking through a viewer. the<br />

operator matches the brightness <strong>of</strong> the target to be measured with the<br />

brightness <strong>of</strong> the calibrated lamp. The adjustment control is cal ibrated in<br />

temperature units. such that when the brightnesses arc matched, the control<br />

indicates the temperature <strong>of</strong> the target to be measured.<br />

Charlie Chong/ Fion Zhang


Pyrometer<br />

A pyrometer is a device that is used for the temperature measurement <strong>of</strong> an object.<br />

The device actually tracks and measures the amount <strong>of</strong> heat that is radiated from an<br />

object. The thermal heat radiates from the object to the optical system present inside<br />

the pyrometer. The optical system makes the thermal radiation into a better focus and<br />

passes it to the detector. The output <strong>of</strong> the detector will be related to the input thermal<br />

radiation. The biggest advantage <strong>of</strong> this device is that, unlike a Resistance<br />

Temperature Detector (RTD) and Thermocouple, there is no direct contact between<br />

the pyrometer and the object whose temperature is to be found out.<br />

Optical (brightness) Pyrometer<br />

In an optical pyrometer, a brightness comparison is made to measure the temperature.<br />

As a measure <strong>of</strong> the reference temperature, a color change with the growth in<br />

temperature is taken. The device compares the brightness produced by the radiation<br />

<strong>of</strong> the object whose temperature is to be measured, with that <strong>of</strong> a reference<br />

temperature. The reference temperature is produced by a lamp whose brightness can<br />

be adjusted till its intensity becomes equal to the brightness <strong>of</strong> the source object. For<br />

an object, its light intensity always depends on the temperature <strong>of</strong> the object, whatever<br />

may be its wavelength. After adjusting the temperature, the current passing through it<br />

is measured using a multimeter, as its value will be proportional to the temperature <strong>of</strong><br />

the source when calibrated. The working <strong>of</strong> an optical pyrometer is shown in the figure<br />

below.<br />

Charlie Chong/ Fion Zhang<br />

http://www.instrumentationtoday.com/optical-pyrometer/2011/08/


Pyrometer<br />

A pyrometer is a type <strong>of</strong> remote sensing thermometer used to measure temperature. Various<br />

forms <strong>of</strong> pyrometers have historically existed. In the modern usage, it is a non-contacting device<br />

that intercepts and measures thermal radiation, a process known as pyrometry and sometimes<br />

radiometry. The thermal radiation can be used to determine the temperature <strong>of</strong> an object's<br />

surface.<br />

The word pyrometer comes from the Greek word for fire, "πυρ" (pyro), and meter, meaning to<br />

measure. The word pyrometer was originally coined to denote a device capable <strong>of</strong> measuring the<br />

temperature <strong>of</strong> an object by its incandescence, or the light that is emitted by the body as caused<br />

by its high temperature. Modern pyrometers are capable <strong>of</strong> interpreting temperatures <strong>of</strong> room<br />

temperature objects by measuring radiation flux in the <strong>infrared</strong> spectrum.<br />

A modern pyrometer has an optical system and a detector. The optical system focuses the<br />

thermal radiation onto the detector. The output signal <strong>of</strong> the detector (temperature T) is related to<br />

the thermal radiation or irradiance j* <strong>of</strong> the target object through the Stefan–Boltzmann law, the<br />

constant <strong>of</strong> proportionality σ, called the Stefan-Boltzmann constant and the emissivity ε <strong>of</strong> the<br />

object.<br />

J* = εσT 4<br />

This output is used to infer the object's temperature. Thus, there is no need for direct contact<br />

between the pyrometer and the object, as there is with thermocouples and resistance<br />

temperature detectors (RTDs).<br />

Charlie Chong/ Fion Zhang<br />

http://en.wikipedia.org/wiki/Pyrometer


Brightness Pyrometers<br />

Charlie Chong/ Fion Zhang<br />

http://www.instrumentationtoday.com/optical-pyrometer/2011/08/


Brightness Pyrometers –Wien’s Law<br />

Charlie Chong/ Fion Zhang<br />

http://www.instrumentationtoday.com/optical-pyrometer/2011/08/


3.4 Basic Configurations <strong>of</strong> Infrared Radiation<br />

Sensing and Imaging Instruments<br />

In terms <strong>of</strong> configuration and operation. most thermal imagers are considered<br />

to be extensions <strong>of</strong> radiation thermometers or radiation thermometers plus<br />

scanning optics. The performance parameters <strong>of</strong> thermal imagers are<br />

extensions <strong>of</strong> the performance parameters <strong>of</strong> radiation thermometers. To aid<br />

comprehension. the basic measurement problem is discussed in this chapter<br />

in terms <strong>of</strong> the measurement <strong>of</strong> a single point. It is then expanded to cover<br />

thermal scanning and imaging. Figure 3.1 illustrates the basic configuration <strong>of</strong><br />

an <strong>infrared</strong> sensing instrument (<strong>infrared</strong> radiation thermometer), showing the<br />

components necessary to make measurements. Collecting optics (an <strong>infrared</strong><br />

lens, for example) arc necessary for gathering the energy emitted by the<br />

target spot and focusing this energy onto the sensitive surface <strong>of</strong> an <strong>infrared</strong><br />

detector.<br />

Charlie Chong/ Fion Zhang


The processing electronics unit amplifies and conditions the signal from the<br />

<strong>infrared</strong> detector and introduces corrections for such factors as detector<br />

ambient temperature drift and target effective surface emissivity. Generally. a<br />

readout. such as a meter. indicates the target temperature and an analog<br />

output is provided. The output signal is used to record, display. alarm, control,<br />

correct or any combination <strong>of</strong> these.<br />

Charlie Chong/ Fion Zhang


Figure 3.1: Basic configuration <strong>of</strong> an <strong>infrared</strong> radiation thermometer<br />

Charlie Chong/ Fion Zhang


Infrared Detector<br />

An <strong>infrared</strong> detector is at the heart <strong>of</strong> every <strong>infrared</strong> sensing and imaging<br />

instrument. whatever its configuration. Infrared detectors can sense <strong>infrared</strong><br />

radiant energy and produce useful electrical signals proportional to the<br />

temperature <strong>of</strong> target surfaces. Instruments using <strong>infrared</strong> detectors and<br />

optics to gather and focus energy from the targets onto these detectors are<br />

capable <strong>of</strong> measuring target surface temperatures with sensitivities better<br />

than 0.10 °C (0.18 ºF). and with response limes in the microsecond (μs)<br />

range. An instrument that measures the temperature <strong>of</strong> a spot on a target in<br />

this manner is called an infra red radiation thermometer. An instrument that<br />

combines this measurement capability with a means or mechanism for<br />

scanning the target surface is called an <strong>infrared</strong> thermal imager. It can<br />

produce thermal maps, or thermograms, where the brightness intensity or<br />

color hue <strong>of</strong> any spot on the map represents the apparent temperature <strong>of</strong> the<br />

surface at that point.<br />

Charlie Chong/ Fion Zhang


Figure 3.2 illustrates the spectral responses <strong>of</strong> various <strong>infrared</strong> radiation<br />

detectors. Radiant energy impinging on their sensitive surfaces causes all<br />

<strong>infrared</strong> detectors to respond with some kind <strong>of</strong> electrical change. This may<br />

be an impedance change. a capacitance change, the generation <strong>of</strong> an<br />

electromotive force (emf) known as Voltage, or the release <strong>of</strong> photons,<br />

depending on the type <strong>of</strong> detector.<br />

Infrared detectors are divided into (1) thermal detectors and (2) photon<br />

detectors. Thermal detectors have broad uniform spectral responses,<br />

somewhat lower sensitivities and slower response times (measured in<br />

millisecond): photon detectors (also called photo detectors) have limited<br />

spectral responses. higher peak sensitivities and faster response times<br />

(measured in microsecond). Thermal detectors usually operate at or near<br />

room temperature. whereas photon detectors are usually cooled to optimize<br />

performance.<br />

Keywords:<br />

■ Thermal Detector- broad uniform spectral responses/ slower<br />

■ Photon Detector- limited spectral responses/ faster<br />

Charlie Chong/ Fion Zhang


Figure 3.2: Response Curves <strong>of</strong> Various Infrared Detectors<br />

Charlie Chong/ Fion Zhang


Discussion<br />

Subject: Why (or How) there are 2 MCT; MCT(215K), MCT(77K)?<br />

Charlie Chong/ Fion Zhang


The mercury cadmium telluride (HgCdTe) detectors shown in Figure 3.2 are<br />

photon detectors cooled to 77 K (-321° F) for operation from 8 to 12 μm and<br />

to 195 K (-109 ° F) for operation from 3 to 5 μm. Because <strong>of</strong> their fast<br />

response, these detectors are used extensively in high speed scanning and<br />

imaging applications. In contrast to the mercury cadmium telluride detector,<br />

the radiation thermopile shown in Figure 3.2, is a broad band thermal detector<br />

operating uncooled. It is used extensively for spot measurements. Because it<br />

generates a direct current electromotive force proportional to the radiant<br />

energy reaching its surface. it is ideal for use in portable, battery powered<br />

instruments. The lead sulfide (PbS) detector is typical <strong>of</strong> those used in<br />

radiation thermometers that measure and control the temperature <strong>of</strong> very hot<br />

targets. Its peak sensitivity at 3μm matches the peak energy emitted by a<br />

1000K (727 °C = 1340 ° F) graybody.<br />

Because <strong>of</strong> the atmospheric absorption considerations previously discussed.<br />

most <strong>infrared</strong> thermal imagers operate in either the 3 to 5 μm or the 8 to 12<br />

μm spectral region.<br />

Note: 195K = [(-273+195) x 9/5] + 32 = -108 ° F<br />

Charlie Chong/ Fion Zhang


Figure 3.2: Response Curves <strong>of</strong> Various Infrared Detectors<br />

Indium Antimony<br />

Photon Detectors<br />

Charlie Chong/ Fion Zhang


Infrared Optics - Lenses, Mirrors and Filters<br />

There are two types <strong>of</strong> <strong>infrared</strong> optics; (1) refractive (lenses. filters, windows)<br />

and (3) reflective (mirrors). Refractive optics transmit <strong>infrared</strong> wavelengths <strong>of</strong><br />

interest. When used for higher temperature applications. their throughput<br />

losses can usually be ignored. When used in low temperature measurement<br />

instruments and imagers, absorption is <strong>of</strong>ten substantial and must be<br />

considered when making accurate measurements.<br />

Reflective optics. which are more efficient are not spectrally selective and<br />

somewhat complicate the optical path. Reflective optics are used more <strong>of</strong>ten<br />

for low temperature applications. where the energy levels cannot warrant<br />

throughput energy losses. When an <strong>infrared</strong> radiation thermometer is aimed<br />

at a target, energy is collected by the optics in the shape <strong>of</strong> a solid angle<br />

determined by the configuration <strong>of</strong> the optics and the detector.<br />

Charlie Chong/ Fion Zhang


The cross section <strong>of</strong> this collecting beam is called the field <strong>of</strong> view (FOV) <strong>of</strong><br />

the instrument and it detennines the size <strong>of</strong> the area (spot size) on the target<br />

surface that is measured by the instrument at any given working distance. On<br />

scanning and imaging instruments this is called the instantaneous field <strong>of</strong><br />

view (lFOV) and becomes one picture element on the thermogram. An<br />

<strong>infrared</strong> interference filter is <strong>of</strong>ten placed in front <strong>of</strong> the detector to limit the<br />

spectral range <strong>of</strong> the energy reaching the detector. The reasons for spectral<br />

selectivity will be discussed later in this chapter.<br />

Processing Electronics<br />

The processing electronics unit amplifies and conditions the signal from the<br />

<strong>infrared</strong> detector and introduces corrections for factors such as detector<br />

ambient temperature drift and effective target surface emissivity.<br />

In radiation thermometers, a meter is usually provided to indicate the target’s<br />

apparent temperature. An analog or digital output signal is provided to record,<br />

display, alarm, control, correct or any combination <strong>of</strong> these.<br />

Charlie Chong/ Fion Zhang


Field <strong>of</strong> View (FOV)<br />

A field <strong>of</strong> view (FOV) is a specification that defines the size <strong>of</strong> what is seen in<br />

the thermal image. The lens has the greatest influence on what the FOV will<br />

be, regardless <strong>of</strong> the size <strong>of</strong> the array. Large arrays, however, provide greater<br />

detail, regardless <strong>of</strong> the lens used, compared to narrow arrays. For some<br />

applications, such as work in outdoor substations or inside a building, a large<br />

FOV is useful. While smaller arrays may provide sufficient detail in a building,<br />

more detail is important in substation work. See Figure 4-7.<br />

Charlie Chong/ Fion Zhang


Figure 4-7. The field <strong>of</strong> view<br />

(FOV) is a specification that<br />

defines the area that is seen in<br />

the thermal image when using a<br />

specific lens.<br />

Charlie Chong/ Fion Zhang


What is IFOV?<br />

A measure <strong>of</strong> the spatial resolution <strong>of</strong> a remote sensing imaging system.<br />

Defined as the angle subtended by a single detector element on the axis <strong>of</strong><br />

the optical system. IFOV has the following attributes:<br />

■<br />

■<br />

Solid angle through which a detector is sensitive to radiation.<br />

The IFOV and the distance from the target determines the spatial<br />

resolution.<br />

A low altitude imaging instrument will have a higher spatial resolution than a<br />

higher altitude instrument with the same IFOV<br />

Charlie Chong/ Fion Zhang<br />

http://www.ssec.wisc.edu/sose/tutor/ifov/define.html


What is IFOV?<br />

IFOV (instantaneous field <strong>of</strong> view) – smallest object detectable<br />

The IFOV (instantaneous field <strong>of</strong> view), also known as IFOV geo (geometric<br />

resolution), is the measure <strong>of</strong> the ability <strong>of</strong> the detector to resolve detail in<br />

conjunction with the objective. Geometric resolution is represented by mrad<br />

and defines the smallest object that can be represented in the image <strong>of</strong> the<br />

display, depending on the measuring distance. The <strong>thermography</strong>, the size <strong>of</strong><br />

this object corresponds to a pixel. The value represented by mrad<br />

corresponds to the size <strong>of</strong> the visible point [mm] a pixel at a distance <strong>of</strong> 1 m.<br />

Charlie Chong/ Fion Zhang<br />

http://www.academiatesto.com.ar/cms/?q=ifov


Instantaneous Field <strong>of</strong> View (IFOV)<br />

An instantaneous field <strong>of</strong> view (IFOV) is a specification used to describe the<br />

capability <strong>of</strong> a thermal imager to resolve spatial detail (spatial resolution). The<br />

IFOV is typically specified as an angle in milliradians (mRad). When projected<br />

from the detector through the lens, the IFOV gives the size <strong>of</strong> an object that<br />

can be seen at a given distance. An IFOV measurement is the measurement<br />

resolution <strong>of</strong> a thermal imager that describes the smallest size object that can<br />

be measured at a given distance. See Figure 4-8. It is specified as an angle<br />

(in mRad) but is typically larger by a factor <strong>of</strong> three than the IFOV. This is due<br />

to the fact that the imager requires more information about the radiation <strong>of</strong> a<br />

target to measure it than it does to detect it. It is vital to understand and work<br />

within the spatial and measurement resolution specific to each system.<br />

Failure to do so can lead to inaccurate data or overlooked findings.<br />

IFOV, θ in milli-radian<br />

H<br />

H in mm = D∙ θ<br />

D in meter<br />

Charlie Chong/ Fion Zhang


Figure 4-8. An IFOV measurement is the measurement resolution <strong>of</strong> a thermal imager that describes the<br />

smallest size object that can be measured at a given distance. IFOV is similar to seeing a sign in the distance<br />

while IFOV measurement is similar to <strong>reading</strong> the sign, either because it is closer or larger.<br />

Instantaneous field <strong>of</strong> view (spatial resolution)/ IFOV measurement (measurement <strong>of</strong> resolution)<br />

Charlie Chong/ Fion Zhang


3.5 Scanning and Imaging<br />

When problems in temperature monitoring and control cannot be solved by<br />

the measurement <strong>of</strong> one or several discrete points on a target surface. it<br />

becomes necessary to spatially scan - that is to move the collecting beam or<br />

the instrument's field <strong>of</strong> view relative to the target. This is usually done by<br />

inserting a movable optical element into the collecting beam as illustrated in<br />

Figure 3.3.<br />

Charlie Chong/ Fion Zhang


Figure 3.3: Adding the scanning element(s) for imaging<br />

Charlie Chong/ Fion Zhang


Line Scanning<br />

When the measurement <strong>of</strong> a single spot on a target surface is not sufficient.<br />

<strong>infrared</strong> line scanners can be used to assemble infonnalion concerning the<br />

distribution <strong>of</strong> radiant energy along a single straight line. Quite <strong>of</strong>ten, this is all<br />

that is necessary to locate a critical thermal anomaly. The instantaneous<br />

position <strong>of</strong> the scanning element is usually controlled or sensed by an<br />

encoder or potentiometer so that the radiometric output signal can be<br />

accompanied by a position signal output and be displayed on a recording<br />

device and/or fed out to a computer based process control system. A typical<br />

high speed commercial line scanner develops a high resolution thermal map<br />

by scanning normal to the motion <strong>of</strong> a moving target such as a paper web or<br />

a strip steel process. The resulting output is a thermal strip map <strong>of</strong> the<br />

process as it moves normal to the scan line. The scanning configuration is<br />

illustrated in Figure 3.4. The output signal information is in a real time<br />

computer compatible format and can be used to monitor, control or predict the<br />

behavior <strong>of</strong> the target.<br />

Charlie Chong/ Fion Zhang


Figure 3.4: Line scanner scanning configuration<br />

Charlie Chong/ Fion Zhang


Two-dimensional Scanning - Thermal Imaging<br />

The three common imaging configurations that produce <strong>infrared</strong> thermograms<br />

are (1) optomechanical scanning, (2) electronic scanning and (3) focal plane<br />

array imaging.<br />

Of the three, optomechanical scanning was the most common until the mid-<br />

I990s. Focal plane array imagers have replaced scanning imagers in most<br />

applications.<br />

Charlie Chong/ Fion Zhang


Optomechanical Scanning<br />

To scan optomechanically in two dimensions generally requires two scanning<br />

elements. Although an almost infinite variety <strong>of</strong> scanning patterns can be<br />

generated using two moving elements. the most common pattern is rectilinear.<br />

This scanning pattern is most <strong>of</strong>ten accomplished by two elements, each<br />

scanning a line normal to the other. A representative rectilinear scanner is<br />

illustrated in the schematic <strong>of</strong> Figure 3.5. Its scanning mechanism comprises<br />

two oscillating mirrors behind the primary lens, a high speed horizontal<br />

scanning mirror and a slower speed vertical scanning mirror. One<br />

performance limitation <strong>of</strong> single-detector optomechanical scanners is a trade<br />

<strong>of</strong>f between speed <strong>of</strong> response and signal-to-noise ratio <strong>of</strong> the detector.<br />

These instruments require high speed cooled photodetectors that are pushed<br />

to their performance limits as the desired real time scanning rate is increased.<br />

Multidetector scanners reduce the constraints on detector performance by<br />

adding detector elements that share the temporal spatial burden, allowing for<br />

faster frame rales with no reduction in signal-to-noise ratio or improving the<br />

signal-to-noise ratio with no decrease in frame rate.<br />

Charlie Chong/ Fion Zhang


Figure 3.5: Optomechanlcally scanned <strong>infrared</strong> imager<br />

Charlie Chong/ Fion Zhang


Electronic Scanning – Pyroelectric Vidicon Thermal Imagers<br />

Electronically scanned thermal imaging systems based on pyrovidicons and<br />

operating primarily in the 8 to 14 μm atmospheric window are commonly used.<br />

They provide qualitative thermal images and are classified as thermal viewers.<br />

A pyroelectric vidicon or pyrovidicon is configured the same as a conventional<br />

video camera tube except that it operates in the <strong>infrared</strong> (2 to 20 μm) region<br />

instead <strong>of</strong> the visible spectrum. Image scanning is accomplished<br />

electronically in the same manner as in a video camera tube.<br />

Charlie Chong/ Fion Zhang


Pyroelectric Vidicon Thermal Imagers<br />

Charlie Chong/ Fion Zhang


Focal Plane Array Imaging<br />

First introduced to the commercial market in 1987. cooled <strong>infrared</strong> focal plane<br />

array (IRFPA) imagers have evolved into compact, qualitative and<br />

quantitative thermal imagers without scanning optics. These devices have<br />

been replacing optomechanically scanned imagers for many applications.<br />

The first uncooled <strong>infrared</strong> focal plane array imagers have been used by the<br />

military for several years and became available to thermographers in 1997.<br />

Figure 3.6 is a schematic <strong>of</strong> a typical. uncooled <strong>infrared</strong> focal plane array<br />

imager. Microbolometer arrays are also available.<br />

Charlie Chong/ Fion Zhang


Figure 3.6: Typical uncooled <strong>infrared</strong> focal plane array imager<br />

Charlie Chong/ Fion Zhang


IRFPA - Large IR mosaic prototype array with 35 H2RG arrays. The array has<br />

a total <strong>of</strong> nearly 147 million pixels. Each <strong>of</strong> the H2RG arrays has 2,048×2,048<br />

pixels.<br />

Charlie Chong/ Fion Zhang<br />

http://www.osa-opn.org/home/articles/volume_19/issue_6/features/high-performance_<strong>infrared</strong>_focal_plane_arrays_for_s/


IRFPA<br />

Charlie Chong/ Fion Zhang<br />

http://ececavusoglu.girlshopes.com/cmoslineararraysirsensor/


Infrared sensors with 3D ROIC for cooled dual-band IR arrays<br />

Charlie Chong/ Fion Zhang<br />

http://www.militaryaerospace.com/articles/2013/07/army-irfpa-roic.html


3.6 Performance Parameters <strong>of</strong> Infrared<br />

Sensing and Imaging Instruments<br />

To select an appropriate instrument for an application, or to determine<br />

whether an available instrument will perform adequately. it is necessary for<br />

the thermographer to understand its performance parameters. The<br />

performance parameters for point sensing instruments (<strong>infrared</strong> radiation<br />

thermometers) are temperature range, absolute accuracy, repeatability,<br />

temperature sensitivity, speed <strong>of</strong> response, target spot size and working<br />

distance (field-<strong>of</strong>-view-spatial resolution), output requirements. sensor<br />

environment and spectral range.<br />

For scanners and imagers the performance parameters include temperature<br />

range. absolute accuracy, repeatability, temperature sensitivity, total field <strong>of</strong><br />

view (TFOV), instantaneous field <strong>of</strong> view (lFOV), measurement spatial<br />

resolution (IFOVmeas), frame repetition rate, minimum resolvable<br />

temperature (MRT), temperature sensitivity, image processing s<strong>of</strong>tware,<br />

sensor environment and spectral range.<br />

Charlie Chong/ Fion Zhang


Qualitative Versus Quantitative Thermography<br />

For scanners and imagers. one distinction based on instrument performance<br />

limitations is that between qualitative and quantitative <strong>thermography</strong>.<br />

A qualitative thermogram displays the distribution <strong>of</strong> <strong>infrared</strong> radiance over<br />

the target surface, uncorrected for target, instrument and media<br />

characteristics.<br />

A quantitative thermogram displays the distribution <strong>of</strong> <strong>infrared</strong> radiosity over<br />

the surface <strong>of</strong> the target. corrected for target, instrument and media<br />

charactcristics so as to approach a graphic representation <strong>of</strong> true surface<br />

temperature distribution.<br />

Charlie Chong/ Fion Zhang


Performance parameters <strong>of</strong> qualitative thermographic instruments. therefore,<br />

do not include temperature accuracy, temperature repeatability and<br />

measurement spatial resolution.<br />

Generally, instruments that include the capability to produce quantitative<br />

thermograms are more costly than qualitative instruments and require<br />

periodic recalibration. Many applications can be solved without the time and<br />

expense <strong>of</strong> quantitative <strong>thermography</strong>, but others require true temperature<br />

mapping. A discussion <strong>of</strong> the most appropriate applications for quantitative<br />

and qualitative thermal imagers is included in Chapter 5.<br />

Keywords:<br />

Performance parameters <strong>of</strong> qualitative thermographic instruments. therefore,<br />

do not include temperature accuracy, temperature repeatability and<br />

measurement spatial resolution.<br />

Charlie Chong/ Fion Zhang


Performance Characteristics <strong>of</strong> Point Sensing Instruments (Radiation<br />

Thermometers)<br />

The American Society for Testing and Materials defines <strong>infrared</strong> point sensing<br />

instruments as <strong>infrared</strong> radiation thermometers even though they do not<br />

always read out in temperature units. Some read out directly in apparent<br />

radiant power units such as W·m -2· s -1 (or BTU· ft -2 ∙ h -1 ), some provide a<br />

closure or alarm signal at a selectable temperature and some others provide<br />

only difference indications on a light emitting diode display.<br />

Charlie Chong/ Fion Zhang


Temperature Range<br />

Temperature range is a statement <strong>of</strong> the high and low limits over which the<br />

target temperature can be measured by the instrument. A typical specification<br />

would be. for example. "temperature range 0 to 1000 °C (32 to 1832 ºF).“<br />

Absolute Accuracy<br />

Absolute accuracy, as defined by the National Lnstitute <strong>of</strong> Standards and<br />

Technology (NIST) standard, entails the maximum error. over the full range,<br />

that the measurement will have when compared to this standard blackbody<br />

reference. A typical specification would be, for example. "absolute accuracy<br />

±0.5 °C (±0.9 ºF) ± 1 percent <strong>of</strong> full scale.“<br />

Charlie Chong/ Fion Zhang


Repeatability<br />

Repeatability describes how faithfully a <strong>reading</strong> is repeated for the same<br />

target over the short and long term. A typical specification would be, for<br />

example, "repeatability (short and long term) <strong>of</strong> ±0.25 °C (±0.45ºF) “.<br />

Temperature range and absolute accuracy will always be interrelated; for<br />

example, the instrument might be expected to measure a range <strong>of</strong><br />

temperatures from 0 to 200 °C (32 to 392 OF) with an absolute accuracy ±2<br />

°C (±3.6ºF) over the entire range. This could alternately be specified as ±1<br />

percent absolute accuracy over full scale. On the other hand, the best<br />

accuracy might be required at some specific temperature, say 100 °C<br />

(212 ° F). In this case, the manufacturer should be informed and the<br />

instrument could be calibrated to exactly match the manufacturer's laboratory<br />

calibration standard at that temperature. Because absolute accuracy is based<br />

on traceability to the NIST standard. it is difficult for a manufacturer to comply<br />

with a tight specification for absolute accuracy. An absolute accuracy <strong>of</strong> ±0.5<br />

°C (±0.9 ° F) or ±1 percent <strong>of</strong> full scale is about as tight as can be<br />

reasonably specified. Repeatability, on the other hand, can be more easily<br />

ensured by the manufacturer and is usually more important to the user.<br />

Charlie Chong/ Fion Zhang


Temperature Sensitivity<br />

Temperature sensitivity defines the smallest target temperature change the<br />

instrument will dctect. Temperature sensitivity is also called thermal resolution<br />

or noise equivalent temperature difference (NETD). It is the smallest<br />

temperature change at the target surface that can be clearly sensed at the<br />

output <strong>of</strong> the instrument. This is almost always closely associated with the<br />

cost <strong>of</strong> the instrument. so unnecessarily fine temperature sensitivity should<br />

not be specified. An important rule to remember is that. for any given<br />

instrument. target sensitivity will improve for hotter targets where there is<br />

more energy available for the instrument to measure. Temperature sensitivity<br />

should be specified, therefore, at a <strong>part</strong>icular target temperature near the low<br />

end <strong>of</strong> the range <strong>of</strong> interest. A typical specification for temperature sensitivity<br />

would be, for example, “temperature sensitivity <strong>of</strong> 0.25 °C (0.45 ºF) at a target<br />

temperature <strong>of</strong> 25 °C (77 ºF)." In this case, the sensitivity <strong>of</strong> the instrument<br />

would improve for targets hotter than 2 °C (36 °F).<br />

Keywords:<br />

Temperature sensitivity is also called thermal resolution or noise equivalent<br />

temperature difference (NETD).<br />

Charlie Chong/ Fion Zhang


Temperature sensitivity is<br />

also called: thermal resolution<br />

or<br />

noise equivalent temperature<br />

difference (NETD).<br />

for my ASNT exam<br />

Charlie Chong/ Fion Zhang


Speed <strong>of</strong> Response<br />

Speed <strong>of</strong> response is how long it takes for an instrument to update a<br />

measurement. It is defined as the time it takes the instrument output to<br />

respond to a step change in temperature at the target surface.<br />

Figure 3.7 shows this graphically. The sensor time constant is defined by<br />

convention to be the time required for the output signal to reach 63 percent <strong>of</strong><br />

a step change in temperature at the target surface. Instrument speed <strong>of</strong><br />

response is usually specified in terms <strong>of</strong> a large percentage <strong>of</strong> the full <strong>reading</strong>,<br />

such as 95 percent. As illustrated in Figure 3.7, this takes about five time<br />

constants, and is generally limited by the detector used (on the order <strong>of</strong><br />

microseconds for photodctcetors and milliseconds for thermal detectors).<br />

Charlie Chong/ Fion Zhang


A typical speed <strong>of</strong> response specification would be, for example. "speed <strong>of</strong><br />

response (to 95 percent) = 0.05 s.“ It should be understood that there is<br />

always a trade<strong>of</strong>f between speed <strong>of</strong> response and temperature sensitivity.<br />

As in all instrumentation systems, as the speed <strong>of</strong> response for a <strong>part</strong>icular<br />

device becomes faster (instrumentation engineers call this a wider<br />

information bandwidth) the sensitivity becomes poorer (lower signal- to-noise<br />

ratio). If the speed <strong>of</strong> response is specified to be faster than is necessary for<br />

the application, the instrument may not have as good a temperature<br />

sensitivity as might be possible otherwise.<br />

Charlie Chong/ Fion Zhang


Figure 3.7: Instrument speed to response and time constant<br />

Charlie Chong/ Fion Zhang


Target Spot Size and Working Distance<br />

Targct spot size D and working distance d define the spalial resolution <strong>of</strong> the<br />

instrument. In a radiation thermometer, spot size is the projcction <strong>of</strong> the<br />

sensitive area <strong>of</strong> the detector at the target plane. It may be specified directly,<br />

“1 cm at I m (0.4 in. at 3 ft)," for example, but it is usually expressed in more<br />

general terms such as a field <strong>of</strong> view solid angle ( 10 mrad, 1 degree, 2<br />

degree) or a field-<strong>of</strong>-view ratio (ratio <strong>of</strong> spot size to working distance - for<br />

example, d/15, d/30, d/75.<br />

A milliradian (mrad) is an angle with a tangent <strong>of</strong> 0.001. A d/15 ratio means<br />

that the instrument measures the emitted energy <strong>of</strong> a spot one-fifteenth the<br />

size <strong>of</strong> the working distance: 3 cm at 45 cm (1.2 in. at 18 in .) f<br />

or example. Figure 3.8 illustrates these relationships and also shows how<br />

spot size can be approximated quickly based on working distance and field<strong>of</strong>-view<br />

information furnished by the manufacturer. A typical specification for<br />

spot size would be. for example. "target spot size = 2 degrees from 1 m (39<br />

in.) to ∞.“<br />

Charlie Chong/ Fion Zhang


Figure 3.8: Instrument field-<strong>of</strong>-view determination<br />

Charlie Chong/ Fion Zhang


This would take into account the shortest working distance at which the<br />

instrument could be focused (1 m or 39 in.). For some instruments designed<br />

for very close workiing distances, the simple d∙D -1 ratio does not always apply.<br />

If closeup information is not clearly provided in the product literature, the<br />

instrument manufacturer should be consulted. For most applications and for<br />

middle and long working distance (greater than 1m or 3 ft), the following<br />

simple calculation (illustrated in Figure 3.8) will closely approximate target<br />

spot size: where:<br />

D ≡ αd<br />

D = spot size (approximate),<br />

α = field-or-view plane angle in radians,<br />

d = distance to the target.<br />

A 17.5 mrad (1 degree) field <strong>of</strong> view means a d∙D -1 ratio <strong>of</strong> 60 to1 and a 35<br />

mrad (2 degree) field <strong>of</strong> view means a d∙D -1 ratio <strong>of</strong> 30 to 1. (?)<br />

Charlie Chong/ Fion Zhang


D ≡ αd<br />

D = spot size (approximate),<br />

α = field-or-view plane angle in radians,<br />

d = distance to the target.<br />

A 17.5 mrad (1 degree) field <strong>of</strong> view means a d∙D -1 ratio <strong>of</strong> 60 to1 and a 35<br />

mrad (2 degree) field <strong>of</strong> view means a d∙D -1 ratio <strong>of</strong> 30 to 1. (?)<br />

for D ≡ α∙d<br />

given that α = 17.5mrad, D=17.5mm if d=1000mm, thus<br />

d/D = 1000/17.5 = 57.296 ≈ 60<br />

This is to say the IFOV measurement ration = 1000 ∙ 1/α where α in mRad.<br />

Charlie Chong/ Fion Zhang


EXAM score!<br />

D=σ∙d<br />

IFOV ratio = d/D or 1/σ<br />

(care on unit used!)<br />

for my ASNT exam<br />

Charlie Chong/ Fion Zhang


Output Requirements<br />

Output requirements for radiation thermometers can vary widely - from a<br />

simple digital indicator and an analog signal to a broad selection <strong>of</strong> output<br />

functions, including digital output (binary coded decimal); high, low and<br />

proportional set points; signal peak or valley sensors; sample and hold<br />

circuits; and even closed loop controls for specific applications. On board<br />

microprocessors provide many <strong>of</strong> the above functions on even inexpensive<br />

standard portable models <strong>of</strong> radiation thermometers.<br />

Charlie Chong/ Fion Zhang


Sensor Environment<br />

Sensor environment includes the ambient extremes under which the<br />

instrument will perform within specifications and the extremes under which it<br />

can be stored without damage when not in operation. For a portable radiation<br />

thermometer. a typical specifi cation for sensor environment would be as<br />

followas.<br />

1. Operating temperature is 0 to 37°C (32 to 100 °F)<br />

2. Humidity is at 20 to 80 percent relative (not condensing).<br />

3. Atmospheric pressure is at -610 m to +2440 m (-2000 to +8000 ft) above<br />

sea level.<br />

4. Storage temperature (nonoperating) ranges from -15 to +60 °C (5 to 140<br />

°F).<br />

Frequently in process control applications, the sensor must be permanently<br />

installed in a somewhat more extreme environment involving smoke, soot.<br />

high temperature and even radioactivity. For these applications,<br />

manufacturers provide a wide range <strong>of</strong> enclosures that <strong>of</strong>fer special protective<br />

featu res such as air cooling, water cooling, pressurization, purge gases and<br />

shielding.<br />

Charlie Chong/ Fion Zhang


Spectral Range<br />

Spectral range denotes the portion <strong>of</strong> the <strong>infrared</strong> spectrum over which the<br />

instrument will operate. The operating spectral range <strong>of</strong> the instrument is<br />

<strong>of</strong>ten critical to its performance and, in many applications. can be exploited to<br />

solve difficult measurement problems. The spectral range is determined by<br />

the detector and the instrument optics. as shown in Figure 3.9. Here, the fiat<br />

spectral response <strong>of</strong> a radiation thermopile detector is combined with that <strong>of</strong> a<br />

germanium lens and an 8 to 14 μm band pass filter. The instrument<br />

characterized is suitable for general purpose temperature measurement <strong>of</strong><br />

cool targets through atmosphere. The transmission spectrum <strong>of</strong> a 0.3 km (0.<br />

19 mil) atmospheric ground level is also shown. An <strong>infrared</strong> interference filter<br />

is <strong>of</strong>ten placed in front <strong>of</strong> the detector to limit the spectral range <strong>of</strong> the energy<br />

reaching the detector.<br />

Charlie Chong/ Fion Zhang


the following three classes <strong>of</strong> filters are common:<br />

1. High pass ti lters pass energy only at wavelengths longer than a<br />

designated wavelength.<br />

2. Low pass filters pass energy only at wavelengths shorter than a<br />

designated wavelength.<br />

3. Band pass filters similar to the one shown in Figure 3.9. pass radiation<br />

within a designated spectral band (8 to 14 μm. for example).<br />

Charlie Chong/ Fion Zhang


Spectrall y selective instrumems use band pass filters to allow only a very<br />

specific broad or narrow band <strong>of</strong> wavelengths to reach the detector. (A<br />

combination <strong>of</strong> a spectrally selective detector and a filter can also be used.)<br />

This can make the instrument highl y selective to a specific material whose<br />

temperature is to be measured in the presence <strong>of</strong> an intervening medium or<br />

an interfering background. Solving measurement problems by means <strong>of</strong><br />

spectrally selective instruments is discussed in greater detail in Chapter 4.<br />

For general purpose use and for measuring cooler targets cooler than about<br />

500 °C (932 °F). most manufacturers <strong>of</strong> radiation thermometers <strong>of</strong>fer<br />

instruments operating in the 8 to 14 μm atmospheric window. For dedicated<br />

use on hotter targets. shorter operating wavelengths are selected. usually<br />

shorter than 3 μm. One reason for choosing shorter wavelengths is that this<br />

enables manufacturers to use commonly available and less expensive quartz<br />

and glass optics, which have the added benefit <strong>of</strong> being visibly transparent for<br />

more convenient aiming and sighting. Another reason is that estimating<br />

emissivity incorrectly will result in smaller temperature errors when<br />

measurements are made at shorter wavelengths.<br />

Charlie Chong/ Fion Zhang


Thermographers have learned that a good general rule to follow, <strong>part</strong>icularly<br />

when dealing with targets <strong>of</strong> low or uncertain emissivities, is to work at the<br />

shortest wavelengths possible without compromising sensitivity or risking<br />

susceptibility to reflections from visible energy sources.<br />

Charlie Chong/ Fion Zhang


Figure 3.9: Spectral response <strong>of</strong> an instrument determined by detector and<br />

optics spectra<br />

Charlie Chong/ Fion Zhang


MWIR OR LWIR?<br />

For general purpose use and for measuring cooler targets cooler than about<br />

500 °C (932 °F). most manufacturers <strong>of</strong> radiation thermometers <strong>of</strong>fer<br />

instruments operating in the 8 to 14 μm atmospheric window. For dedicated<br />

use on hotter targets. shorter operating wavelengths are selected. usually<br />

shorter than 3 μm. One reason for choosing shorter wavelengths is that this<br />

enables manufacturers to use commonly available and less expensive quartz<br />

and glass optics, which have the added benefit <strong>of</strong> being visibly transparent for<br />

more convenient aiming and sighting. Another reason is that estimating<br />

emissivity incorrectly will result in smaller temperature errors when<br />

measurements are made at shorter wavelengths.<br />

Thermographers have learned that a good general rule to follow, <strong>part</strong>icularly<br />

when dealing with targets <strong>of</strong> low or uncertain emissivities, is to work at the<br />

shortest wavelengths possible without compromising sensitivity or risking<br />

susceptibility to reflections from visible energy sources.<br />

Charlie Chong/ Fion Zhang


3.7 Performance Characteristics <strong>of</strong> Scanners and<br />

Imagers<br />

Because an <strong>infrared</strong> thermogram consists <strong>of</strong> a matrix <strong>of</strong> discrete point<br />

measurements, many <strong>of</strong> fhe performance parameters <strong>of</strong> <strong>infrared</strong> thermal<br />

imager are the same as those <strong>of</strong> radiation thermometers. The output <strong>of</strong> an<br />

<strong>infrared</strong> line scanner can be considered as one line <strong>of</strong> discrete point<br />

measurements. The parameters <strong>of</strong> temperature range, absolute accuracy.<br />

repeatability, sensor environment and spectral range are esscntially the same<br />

for radiation thermometers, line scanners and imagers. Others are derived<br />

from or are extensions <strong>of</strong> radiation thermometer performance parameters.<br />

Qualitative thermal imagers (also called thermal viewers) differ from<br />

quantitative thermal imagers (also called imaging radiometers) in that thermal<br />

viewers do not provide temperature or thermal energy measurements. For<br />

thermographers requiring qualitative rather than quantitative thermal images,<br />

therefore, some performance parameters are unimportant.<br />

Charlie Chong/ Fion Zhang


Total Field <strong>of</strong> View (FOV total )<br />

For scanners and imagers. total field <strong>of</strong> view denotes the image size in terms<br />

<strong>of</strong> total scanning angles for any given lens. An example <strong>of</strong> a typical total field<br />

<strong>of</strong> view specifi cation would be "TFOV = 20 degrees vertical x 30 degrees<br />

horizontal" (with standard Ix lens) and would define the thermogram total<br />

target size by a simple trigonometric relationship:<br />

tan θ/2 = V/2∙d -1<br />

V = 2 ∙ tan (y/2) ∙ d, for θ = y<br />

d = working distance,<br />

H = total horizontal image size,<br />

V = total vertical image size,<br />

x = horizontal scanning angle,<br />

y = vertical scanning angle.<br />

θ = y or x<br />

This is illustrated in Figure 3. 10.<br />

Charlie Chong/ Fion Zhang


The total field <strong>of</strong> view for a line scanner consists <strong>of</strong> one scan line as shown in<br />

Figure 3.4 and Figure 3.10. The horizontal image size H is equal to the scan<br />

sector. The vertical image size V is equal to the instantaneous field <strong>of</strong> view.<br />

All other parameters are the same as for an imager.<br />

Figure 3.4: Line scanner scanning configuration<br />

Charlie Chong/ Fion Zhang


Figure 3.10: Total field <strong>of</strong> view (TFOV) determination for an <strong>infrared</strong> imager<br />

Charlie Chong/ Fion Zhang


Instantaneous Field <strong>of</strong> View IFOV<br />

Instantaneous field <strong>of</strong> view in an imager is very similar to that for a point<br />

sensing instrument: it is the angular projection <strong>of</strong> the detector element at the<br />

target plane. (resolution?)<br />

In an imager, however, it is also called imaging spatial resolution and<br />

represents the size <strong>of</strong> the smallest picture element that ean be imaged. An<br />

example <strong>of</strong> a typical instantaneous field <strong>of</strong> view specification would be "IFOV<br />

= 1.7 mRad at 0.35 MTF." The 0.35 MTF refers to 35 percent <strong>of</strong> the<br />

modulation transfer function test used to check imaging spatial resolution.<br />

This is described in detail in Chapter 4. The simple expression. D = αd, can<br />

be used to estimate imaging spot size at the target plane from manufacturer's<br />

published data by substituting the published instantaneous field <strong>of</strong> view for α.<br />

Keywords:<br />

IFOV, image spatial resolution,<br />

MTF-modulated transfer function<br />

Charlie Chong/ Fion Zhang


EXAM score!<br />

IFOV<br />

is also called;<br />

image spatial resolution<br />

for my ASNT exam<br />

Charlie Chong/ Fion Zhang


Recalling!<br />

Temperature sensitivity is<br />

also called: thermal resolution<br />

or<br />

noise equivalent temperature<br />

difference (NETD).<br />

for my ASNT exam<br />

Charlie Chong/ Fion Zhang


Measurement Spatial Resolution<br />

Measurement spatial resolution (IFOVmeas) is the spatial resolution <strong>of</strong> the<br />

minimum target spot size on which an accurate measurement can be made in<br />

lenns <strong>of</strong> its distance from the instrument. An example <strong>of</strong> a typical<br />

measurement spatial resolution specification would be "IFOVmeas = 3.5 mrad<br />

at 0.95 SRF.“ The 0.95 SRF refers to 95 percent slit response function test<br />

used to check measurement spatial resolution. This is described in detail in<br />

Chapter 4. The simple ex pression, D = αd, can again be used to estimate<br />

measurement spot size at the target plane from manufacturer's published<br />

data by substituting published measurement spatial resolution for α.<br />

Keywords:<br />

SRF refers to 95 percent slit response function test used to check<br />

measurement spatial resolution.<br />

Comments:<br />

IFOVmeas – IFOV measurement<br />

Charlie Chong/ Fion Zhang


IFOV - MTF<br />

The 0.35 MTF refers to:<br />

0.35 percent <strong>of</strong> the modulation transfer<br />

function test used to check imaging<br />

spatial resolution.<br />

for my ASNT exam<br />

Charlie Chong/ Fion Zhang


IFOV meas -SRF<br />

95 SRF refers to:<br />

95 percent slit response function test<br />

used to check measurement spatial<br />

resolution<br />

for my ASNT exam<br />

Charlie Chong/ Fion Zhang


Fig. 2a. Slit Response Function. Camera sees slit lips <strong>of</strong> radiometric temperature T0<br />

(back side radiometric temperature) and The body behind the slit <strong>of</strong> radiometric<br />

temperature T1 (“slit “ temperature). Slit width is d and D is the distance slit-camera<br />

(Figure is issue from reference 4)<br />

Charlie Chong/ Fion Zhang<br />

http://qirt.gel.ulaval.ca/archives/qirt2006/papers/025.pdf


Frame Repetition Rate<br />

Frame repetition rate replaces speed <strong>of</strong> response and is defined as the<br />

number <strong>of</strong> times every point on the target is scanned in one second. This<br />

should not be confused with field rate. Some imagers are designed to<br />

interlace consecutive fields. each consisting <strong>of</strong> alternate image lines. This<br />

results in images less disconcerting 令 人 不 安 的 to the human eye. The frame<br />

rate in this case would be one half the field rate. An example <strong>of</strong> a typical<br />

frame repetition rate specification for an imager would be "frame repetition<br />

rate = 30 frames per second." For a line scanner. the term line scan rate is<br />

used and it is expressed in lines per second.<br />

Comments:<br />

For interlace field rate scanning; The frame rate in this case would be one half<br />

the field rate.<br />

Charlie Chong/ Fion Zhang


Minimum Resolvable Temperature Difference<br />

Minimum resolvable temperature (MRT) or minimum resolvable temperature<br />

difference (MRTD) replaces temperature sensitivity and is defined as the<br />

smallest blackbody equivalent larget lemperature difference Ihat can be<br />

observed OUI <strong>of</strong> system noise on a thermogram. As in radiation thennometry.<br />

this difference improves (becomes smaller) with increasing target temperature<br />

and is expressed in those terms. An example <strong>of</strong> a typical minimum resolvable<br />

temperature diffe rence speci fi cation for a line scanner or an imager would<br />

be "MRTD = 0.05 °C at 25 °C target temperature (0.09 OF at 77<br />

OF),“ Minimum resolvable temperature difference may also depend on the<br />

spatial frequency imposed by the test discipline. The test techniques for<br />

checking minimum resolvable temperature difference is described in Chapter<br />

4,<br />

Comments: Temperature sensitivity is also called: thermal resolution or<br />

noise equivalent temperature difference (NETD).<br />

Charlie Chong/ Fion Zhang


Thermal Imaging Display and Diagnostic S<strong>of</strong>tware Overview<br />

Thermography applications <strong>of</strong>ten req uire extensive thermal imaging display<br />

and diagnostic s<strong>of</strong>tware. Thermal imagers feature image processing<br />

capabilities that may be divided into five categories. one or more <strong>of</strong> which<br />

may be used in the same application. These categories are quantitativc<br />

thermal measurements <strong>of</strong> targets; detailed processing and image diagnostics;<br />

image recording. storage and recovery; image comparison (differential or<br />

multispectral<strong>thermography</strong>); and database and documenlalion. Applications<br />

using s<strong>of</strong>tware capabilities, singly and in combination. will also be described<br />

in Chapter 5.<br />

Charlie Chong/ Fion Zhang


EXAM score!<br />

D=σ∙d<br />

IFOV ratio = d/D or 1/σ<br />

(when calculation IFOV ratio<br />

care on unit used!)<br />

for my ASNT exam<br />

Charlie Chong/ Fion Zhang


FOV - Animation<br />

Charlie Chong/ Fion Zhang<br />

http://www.imagerchina.com.cn/fov_calculator.html


Charlie Chong/ Fion Zhang


Questions & Answers<br />

Subject: Answer this web queries from: http://www.thesnellgroup.com/community/ir-talk/f/9/p/1402/5433.aspx<br />

wonder if anyone can help me here. I am studying for my employer's Level 2 certification exam and I am using<br />

the ASNT supplement booklet to help. They ask a few question about IFOV and spot size calculation and I do<br />

not quite understand how they get the answers. basically it is not the answer I want but how they got to the<br />

answers.<br />

Question #1: A camera has an IFOV <strong>of</strong> 1.9 mRad. What is it's theoretical minimum spot size at a distance <strong>of</strong><br />

100 cm? Answer is: 0.19 cm (What formula is used for this and are there any units conversion like mm to cm or<br />

mRad to something else?)<br />

Question #2: The IFOV measurement <strong>of</strong> a radiometric system is 1.2 mRad. What is the maximum size object<br />

this system can accurately measure at a distance <strong>of</strong> 25 m? Answer is: 3 cm (now clearly there are unit<br />

conversions going on here from meters to cm. So how is it done?)<br />

Question #3: You are looking at an electrical connection 20 m in the air. What IFOV measurement is required to<br />

accurately measure the temperature on the 2.54 cm (1 in.) head <strong>of</strong> a bolt? Answer is: 1.25 mRad (I know it's<br />

just a matter <strong>of</strong> transposing the formula, but again there is units changes and I do not know the formula to apply)<br />

Last question: Using an IR system with an IFOV measurement ratio <strong>of</strong> 180:1. What is the smallest size object<br />

you can accurately measure at a distance <strong>of</strong> 3m (3.3 ft)? Answer is: 16.6 mm or (0.65 in).<br />

NOW this one I kind <strong>of</strong> figured out using: 1/180 = 0.0055 & 3 m = 3000mm therefore 0.0055 x 3000 = 16.5<br />

Let me know if you all know how to do these problems. I think all I need is the formula and an understanding<br />

when and which units to convert.<br />

Charlie Chong/ Fion Zhang


Answer: D= σ•d, IFOV ration= 1/σ = d/D<br />

Question #1: A camera has an IFOV <strong>of</strong> 1.9 mRad. What is it's theoretical minimum spot size at a distance <strong>of</strong><br />

100 cm? Answer is: 0.19 cm (What formula is used for this and are there any units conversion like mm to cm or<br />

mRad to something else?)<br />

Calculation: D= 1.9 x 1 = 1.9mm or 0.19cm, (100cm = 1m)<br />

Question #2: The IFOV measurement <strong>of</strong> a radiometric system is 1.2 mRad. What is the maximum size object<br />

this system can accurately measure at a distance <strong>of</strong> 25 m? Answer is: 3 cm (now clearly there are unit<br />

conversions going on here from meters to cm. So how is it done?)<br />

Calculation: D= 1.2 x 25m = 30mm = 3cm<br />

Question #3: You are looking at an electrical connection 20 m in the air. What IFOV measurement is required to<br />

accurately measure the temperature on the 2.54 cm (1 in.) head <strong>of</strong> a bolt? Answer is: 1.25 mRad (I know it's<br />

just a matter <strong>of</strong> transposing the formula, but again there is units changes and I do not know the formula to apply)<br />

Calculation: 25.4 = σ x 20, σ = 1.27mRad<br />

Last question: Using an IR system with an IFOV measurement ratio <strong>of</strong> 180:1. What is the smallest size object<br />

you can accurately measure at a distance <strong>of</strong> 3m (3.3 ft)? Answer is: 16.6 mm or (0.65 in).<br />

Calculation: 1/ σ = d/D = 180, σ = 1/180,<br />

D = σ∙d, D = 1/180 x 3 = 0.01667m = 16.7mm<br />

(when calculating IFOV ratio, good to use the same unit for all inputs)<br />

Charlie Chong/ Fion Zhang


Charlie Chong/ Fion Zhang


Break Time<br />

– Kenya C<strong>of</strong>fee Picker<br />

Charlie Chong/ Fion Zhang<br />

http://www.kickstartcafe.com/journal/kenyan-c<strong>of</strong>fee#.VWuZY52S3IU


3.8 Descriptions <strong>of</strong> Thermal Sensing and Imaging<br />

Equipment<br />

Point Sensors (Radiation Thermometers)<br />

Point sensors (radiation thermometers) can be further divided into<br />

temperature probes. portable hand held devices. online process control<br />

devices and specially configured devices.<br />

■ Temperature Probes<br />

Temperature probes are low priced, pocket portable, battery powered devices<br />

that usually feature a pencil shaped sensor connected to a small basic<br />

readout unit. Generally, they are optically pre-adjusted for minimum spot size<br />

at a short working distance. A 0.5cm (0.2 in.) spot al a 2 cm (0.8 in.) working<br />

distance is typical. Temperature usually ranges from about - 20 °C to 300 °C<br />

(- 4 ° F to 570 ° F) and a sensitivity <strong>of</strong> ±1°C (1.8 ° F) is achieved easily.<br />

Probes are designed for close-up measurements such as circuit board<br />

analysis. troubleshooting <strong>of</strong> electrical connections. inspect ion <strong>of</strong> plumbing<br />

systems and biological and medical studies.<br />

Charlie Chong/ Fion Zhang


Portable Handheld Devices<br />

Charlie Chong/ Fion Zhang


■ Portable Handheld Devices<br />

Portable handheld radiation thermometers are designed for middle distance<br />

measurements and, with few exceptions, operate in the 8 to 14 μm spectral<br />

region and are configured like a pistol for one-handcd operation and aiming.<br />

They are usually optically preadjusted for infinity focus.<br />

A typical 2 degree field <strong>of</strong> view resolves a 7.5 cm (3 in.) spot at a 150 cm (60<br />

in.) working distance and a 30 cm (1 ft) spot at a 9 m (30 ft) working distance.<br />

(9 x tan(2º) = 0.314m=31cm)<br />

Most instruments in this group incorporate microcomputers with limited<br />

memory and some have data logging capabilities. An open or enclosed<br />

aiming sight is provided and in some models a projected laser beam is used<br />

to facilitate aiming <strong>of</strong> the instrument as shown in Figure 3. 11. Note that the<br />

laser beam docs not represent the field <strong>of</strong> view. A measurement readout is<br />

always provided and usually the temperature is shown on a digital liquid<br />

crystal display. These instruments are powered with disposable batteries and<br />

have low power drain.Temperature ranges are typically from 0 to 1000 °C (30<br />

to 1800 ºF).<br />

Charlie Chong/ Fion Zhang


Temperature sensitivity and readability are usually 1 percent <strong>of</strong> scale 1°C (2<br />

ºF) although sensitivities on the order <strong>of</strong> 0.1 °C (0.2 ° F) arc achievable.<br />

Response times are on the order <strong>of</strong> fractions <strong>of</strong> a second, usually limited by<br />

the response <strong>of</strong> the readout.<br />

Hand held radiation thermometers are used extensively in applications where<br />

spot checking <strong>of</strong> target temperatures is sufficient and continuous monitoring is<br />

not required. Handheld radiation thermometers have become an important<br />

<strong>part</strong> <strong>of</strong> many plant energy conservation programs. Process applications<br />

include monitoring mixing temperatures <strong>of</strong> food products. cosmetics and<br />

industrial solvents. Microcomputers enable handheld instruments to<br />

incorporate special features such as the ability to store sixty <strong>reading</strong>s for<br />

future retrievals and printout.<br />

Charlie Chong/ Fion Zhang


Figure 3.11: Hand held <strong>infrared</strong> radiation thermometer with laser aiming<br />

Charlie Chong/ Fion Zhang


Hand Held Infrared Module<br />

Charlie Chong/ Fion Zhang


Note that the laser beam docs not represent the field <strong>of</strong> view.<br />

Figure 1. Use the Fluke 66 within 5 m (15 ft.) <strong>of</strong> the intended target.<br />

At greater distances, the measured area will be larger (approximately<br />

the distance divided by 30). Field <strong>of</strong> view θ= tan -1 (1/30) = 1.91º<br />

Charlie Chong/ Fion Zhang<br />

http://www.fluke.com/fluke/m3en/products/thermometers


Note that the laser beam docs not represent the field <strong>of</strong> view.<br />

Figure 2. Use the Fluke 68 within 8 m (25 ft.) <strong>of</strong> the intended target.<br />

At greater distances, the measured area will be larger (approximately<br />

the distance divided by 50). Filed <strong>of</strong> view θ= tan -1 (1/50) = 1.14º<br />

Charlie Chong/ Fion Zhang<br />

http://www.fluke.com/fluke/m3en/products/thermometers


■ Online Process Monitoring and Control Devices<br />

Online monitoring and control sensors are for dedicated use on a product or a<br />

process. Permanently installed where it can measure the temperature <strong>of</strong> one<br />

specific target. this type <strong>of</strong> instrument remains there for the life <strong>of</strong> the<br />

instrument or the process. With few exceptions. these instruments operate on<br />

line power. The measurement value can be observed on a meter. but it is<br />

more <strong>of</strong>ten used to trigger a switch or relay or to feed a simple or<br />

sophisticated process control loop. Most <strong>of</strong> the online monitoring and control<br />

sensors send signals to universal indicator control units that accept inputs<br />

from various types <strong>of</strong> industrial sensors. Because this instrument group is<br />

selected to perform a specific task, a shopping list format is provided to the<br />

customer by the manufacturer so that all required features can be purchased.<br />

including environmental features such as water cooled housings. air purge<br />

fittings and air curtain devices.<br />

Charlie Chong/ Fion Zhang


Emissivity set controls, located in a prominent place on a general purpose<br />

instrument are more likely to be located behind a bezel 嵌 槽 / 柜 on the<br />

sensor on these dedicated units. where they are set once and locked. The<br />

spectral interval over which the sensing head operates is selected to optimize<br />

the signal from the target, to reduce or eliminate the effect <strong>of</strong> an interfering<br />

energy source or to enable the instrument to measure the surface<br />

temperature <strong>of</strong> thin films <strong>of</strong> material that are largely transparent to <strong>infrared</strong><br />

radiation. The capability for spectral selectivity has made these instruments<br />

important in the manufacture <strong>of</strong> glass and thin film plastics. Applications in<br />

these atres are discussed in Chapters 4 and 5.<br />

Charlie Chong/ Fion Zhang


IR Sensor Module<br />

Charlie Chong/ Fion Zhang


IR Sensor Module<br />

Charlie Chong/ Fion Zhang


IR Sensor Module<br />

Charlie Chong/ Fion Zhang


IR Sensor Module<br />

Charlie Chong/ Fion Zhang


■ Devices with Special Configurations<br />

Special configurations <strong>of</strong> <strong>infrared</strong> radiation thermometers include ratio<br />

pyrometers (also called two color pyrometers), <strong>infrared</strong> radiometric<br />

microscopes, laser reflection pyrometers and fiber-optic coupled pyrometers.<br />

1. Two-color pyrometers or ratio pyrometers, are a special case <strong>of</strong> the online<br />

instrument. Ratio pyrometers are <strong>part</strong>icularly useful in high temperature<br />

applications above 300 °C (572 ° F) and in measuring small targets <strong>of</strong><br />

unknown emissivity, provided the background is cool. constant and uniform.<br />

The emissivity <strong>of</strong> the target need not be known if it is constant and relections<br />

are controlled. The target does not need to fill the field <strong>of</strong> view. provided the<br />

background is cool, constant and uniform. The measurement is based on the<br />

ratio <strong>of</strong> energy in two spectral bands. so impurities in the optical path resulting<br />

in broad band absorption do not affect the measurement. Ratio pyrometers<br />

are usually, not applicable to measurements below 300 °C (572 °F).<br />

Charlie Chong/ Fion Zhang


Two-color Pyrometers or Ratio Pyrometers<br />

Charlie Chong/ Fion Zhang


Two-color Pyrometers or Ratio Pyrometers<br />

Charlie Chong/ Fion Zhang


Two-color Pyrometers or Ratio Pyrometers<br />

Charlie Chong/ Fion Zhang<br />

https://www.eutech-scientific.de/products-services/power-generation/euflame.html


Two-color Pyrometers or Ratio Pyrometers<br />

Charlie Chong/ Fion Zhang<br />

https://www.eutech-scientific.de/products-services/power-generation/euflame.html


Two-color Pyrometers or Ratio Pyrometers<br />

Ratio Radiation - Also called two-color radiation thermometers, these devices measure the<br />

radiated energy <strong>of</strong> an object between two narrow wavelength bands, and calculates the ratio <strong>of</strong><br />

the two energies, which is a function <strong>of</strong> the temperature <strong>of</strong> the object. Originally, these were<br />

called two color pyrometers, because the two wavelengths corresponded to different colors in the<br />

visible spectrum (for example, red and green). Many people still use the term two-color<br />

pyrometers today, broadening the term to include wavelengths in the <strong>infrared</strong>.<br />

The temperature measurement is dependent only on the ratio <strong>of</strong> the two energies measured, and<br />

not their absolute values as shown in Figure 3-4.<br />

Any parameter, such as target size, which affects the amount <strong>of</strong> energy in each band by an equal<br />

percentage, has no effect on the temperature indication. This makes a ratio thermometer<br />

inherently more accurate. (However, some accuracy is lost when you're measuring small<br />

differences in large signals). The ratio technique may eliminate, or reduce, errors in temperature<br />

measurement caused by changes in emissivity, surface finish, and energy absorbing materials,<br />

such as water vapor, between the thermometer and the target. These dynamic changes must be<br />

seen identically by the detector at the two wavelengths being used.<br />

Emissivity <strong>of</strong> all materials does not change equally at different wavelengths. Materials for which<br />

emissivity does change equally at different wavelengths are called gray bodies. Materials for<br />

which this is not true are called non-gray bodies. In addition, not all forms <strong>of</strong> sight path<br />

obstruction attenuate the ratio wavelengths equally. For example, if there are <strong>part</strong>icles in the<br />

sight path that have the same size as one <strong>of</strong> the wavelengths, the ratio can become unbalanced.<br />

Charlie Chong/ Fion Zhang<br />

http://www.omega.com/literature/transactions/volume1/thermometers2.html


Figure 3-4: The “Two-Color” IR Thermometer<br />

E 1<br />

T1<br />

E 1<br />

E 2<br />

T2<br />

E 2<br />

Charlie Chong/ Fion Zhang<br />

http://www.omega.com/literature/transactions/volume1/thermometers2.html


Phenomena which are non-dynamic in nature, such as the non-gray bodiness<br />

<strong>of</strong> materials, can be dealt with by biasing the ratio <strong>of</strong> the wavelengths<br />

accordingly. This adjustment is called slope. The appropriate slope setting<br />

must be determined experimentally. Figure 3-5 shows a schematic diagram <strong>of</strong><br />

a simple ratio radiation thermometer. Figure 3-6 shows a ratio thermometer<br />

where the wavelengths are alternately selected by a rotating filter wheel.<br />

Figure 3-5: Beam Splitting in the Ratio IR Thermometer<br />

Charlie Chong/ Fion Zhang<br />

http://www.omega.com/literature/transactions/volume1/thermometers2.html


Figure 3-6: Radio Pyometry Via a Filter wheel<br />

Figure 3-7: Schematic <strong>of</strong> a Multispectral IR Thermometer.<br />

Charlie Chong/ Fion Zhang<br />

http://www.omega.com/literature/transactions/volume1/thermometers2.html


Some ratio thermometers use more than two wavelengths. A multi-wavelength device<br />

is schematically represented in Figure 3-7.<br />

These devices employ a detailed analysis <strong>of</strong> the target's surface characteristics<br />

regarding emissivity with regard to wavelength, temperature, and surface chemistry.<br />

With such data, a computer can use complex algorithms to relate and compensate for<br />

emissivity changes at various conditions. The system described in Figure 3-7 makes<br />

parallel measurement possible in four spectral channels in the range from 1 to 25<br />

microns. The detector in this device consists <strong>of</strong> an optical system with a beam splitter,<br />

and interference filters for the spectral dispersion <strong>of</strong> the incident radiation. This<br />

uncooled thermometer was developed for gas analysis. Another experimental system,<br />

using seven different wavelengths demonstrated a resolution <strong>of</strong> +/-1°C measuring a<br />

blackbody source in the range from 600 to 900°C. The same system demonstrated a<br />

resolution <strong>of</strong> +/- 4°C measuring an object with varying emittance over the temperature<br />

range from 500 to 950°C<br />

Two color or multi-wavelength thermometers should be seriously considered for<br />

applications where accuracy, and not just repeatability, is critical, or if the target object<br />

is undergoing a physical or chemical change. Ratio thermometers cover wide<br />

temperature ranges. Typical commercially available ranges are 1652 to 5432° F (900<br />

to 3000°C) and 120 to 6692°F (50 to 3700°C). Typical accuracy is 0.5% <strong>of</strong> <strong>reading</strong> on<br />

narrow spans, to 2% <strong>of</strong> full scale.<br />

Charlie Chong/ Fion Zhang<br />

http://www.omega.com/literature/transactions/volume1/thermometers2.html


2. Infrared radiometric microscopes are configured like a conventional<br />

microscope and by using reflective microscope objectives and beam<br />

splitters, the operator can simultaneously view and measure targets down<br />

to 10 μm in diameter with accuracy and resolution <strong>of</strong> about 0,5 °C (1 °F).<br />

3. Laser reflection pyrometers use the reflected energy <strong>of</strong> an active laser to<br />

measure target reflectance. A built-in microcomputer calculates target<br />

effective emissivity and uses this figure to provide a corrected true<br />

temperature <strong>reading</strong>. This instrument. though expensive, is useful for<br />

measurement <strong>of</strong> high temperature specular target surfaces in adverse<br />

environments.<br />

4. Fiberoptic coupled pyrometers make possible the measurement <strong>of</strong><br />

normally inaccessible targets by replacing the optic with a flexible or rigid<br />

fiberoptic bundle. This limits the spectral performance and hence the<br />

temperature range to the higher values, but has allowed temperature<br />

measurements to be made when previously none were possible.<br />

Charlie Chong/ Fion Zhang


Infrared Radiometric Microscopes<br />

Charlie Chong/ Fion Zhang


Fiberoptic Coupled Pyrometers<br />

Charlie Chong/ Fion Zhang<br />

http://www.omega.com/temperature/pdf/4121_ir.pdf


Line Scanners<br />

Line scanners are divided into online process control devices and special<br />

purpose scanners.<br />

■ Online Process Control Devices<br />

Online (monitoring and control) line scanners are high speed online<br />

commercial line scanners that develop high resolution thermal maps by<br />

scanning normal to the motion <strong>of</strong> a moving target such as paper web or a<br />

strip steel process. The vast majority <strong>of</strong> commercial <strong>infrared</strong> line scanners are<br />

in this configuration. The output signal information is in a real time computer<br />

compatible format and can be used to monitor, control or predict the behavior<br />

<strong>of</strong> the target. Like the online point sensor, these line scanners are usually<br />

permanently installed where they monitor the temperature pr<strong>of</strong>ile at one site<br />

<strong>of</strong> the process, remaining there for the life <strong>of</strong> the instrument or the process.<br />

Likewise they are usually fitted with environmental housings and preset<br />

emissivity compensation sets. The best applications for this scanner are in<br />

online, real time process monitoring and control applications where they are<br />

integrated with the process host computer system.<br />

Charlie Chong/ Fion Zhang


It is not unusual to find line scanners at multiple locations in a process with all<br />

<strong>of</strong> them linked to the host computer. In the 1990s, <strong>infrared</strong> line scanners<br />

based on a linear focal plane array came into use. This type <strong>of</strong> instrument<br />

frequently uses an un-cooled array <strong>of</strong> thermal detectors radiation thermopiles.<br />

This scanner has no moving <strong>part</strong>s. The linear array is oriented perpendicular<br />

to a process or a target moving at a uniform rate. The scanner output may be<br />

used to develop a thermograms or the data for each pixel can be fed directly<br />

to a host computer and used to monitor and control the process. Instruments<br />

<strong>of</strong> this type have been used to monitor moving railroad cars for overheated<br />

wheels and brake assemblies.<br />

Charlie Chong/ Fion Zhang


Special Purpose Devices<br />

Special purpose configurations <strong>of</strong> line scanners include one type <strong>of</strong> portable<br />

line scanner and a number <strong>of</strong> aerial mappers that scan a line normal to the<br />

motion <strong>of</strong> the aircraft and develop a thermal strip map. Many <strong>of</strong> these<br />

mappers have been replaced by low cost forward looking <strong>infrared</strong> scanners<br />

(FLIRs) based on staring focal plane arrays.<br />

Charlie Chong/ Fion Zhang


FLIR- Forward Looking Infrared<br />

Charlie Chong/ Fion Zhang


FLIR- Forward Looking Infrared<br />

Charlie Chong/ Fion Zhang


Imagers (Thermographic Instruments)<br />

Imagers (thermographic instruments) consist <strong>of</strong> both qualitative and<br />

quantitative imagers.<br />

■ Qualitative Thermal Imagers<br />

Qualitative thermal imagers arc also called thermal viewers. They include<br />

mechanically scanned, electronically scanned (pyrovidicon) and staring focal<br />

plane array FPA imagers.<br />

● Mechanically Scanned Thermal Viewers<br />

Mechanically scanned thermal viewers are moderately priced battery<br />

powered scanning instruments that produce a qualitative image <strong>of</strong> the<br />

radiosity over the surface <strong>of</strong> a targct. The battery packs are rechargeable and<br />

usually provide 2 to 3 h <strong>of</strong> continuous operation. These one-piece, lightweight<br />

instruments, designed to be simple to operate, feature thermoelectric detector,<br />

cooling provided by a battery powered cooler. Although not designed for<br />

absolute temperature measurements, they can demonstrably sense<br />

temperature differences <strong>of</strong> tenths <strong>of</strong> degrees and can be used for targets from<br />

below 0 °C up to 1500 °C (32 <strong>of</strong> up to 2372 °F).<br />

Charlie Chong/ Fion Zhang


Typically, the total field <strong>of</strong> view is from 6 to 8 degrees high and from 12 to 18<br />

degrees wide, with spatial resolution <strong>of</strong> 2 mRad 10 mm at 2.0 m (0.4 in. at 7<br />

ft). Images are video recorded by means <strong>of</strong> a conventional video tape<br />

recorder output jack and video recorder accessories. The broad applications<br />

for thermal viewers are generally limited only to those in which the<br />

temperature measurements are not critical and recording quality does not<br />

need to be optimum. The combination <strong>of</strong> a thermal viewer (to locate thermal<br />

anomalies) and a hand held thermometer (to quantify them) can be a<br />

powerful and cost effective ombination.<br />

Charlie Chong/ Fion Zhang


● Electronically Scanned Viewers (Pyrovidcon Imagers)<br />

Pyrovidicon imagers arc electronically scanned video cameras. The camera<br />

tube is sensitive to target radiation in the <strong>infrared</strong> rather than the visible<br />

spectrum. Aside from the tube and germanium lens, which are expensive,<br />

these systems use television recording accessories, in comparison with other<br />

<strong>infrared</strong> imaging systems, the picture quality and resolution are good,<br />

approaching conventional television format.<br />

The thermal image can be viewed or videotaped with equal convenience and<br />

no cooling is required. Pyrovidicon systems do not intrinsically <strong>of</strong>fer<br />

quantitative measurement capability, but some manufacturers <strong>of</strong>fer models in<br />

which an integrated radiation thermometer is bore sighted with the scanner<br />

and its measurement is superimposed on the video display along with a<br />

defining reticle in the center <strong>of</strong> the display thermal resolution <strong>of</strong> flicker free<br />

pyrovidicon instruments is between 0.2 and 0.4 °C (0.4 and 0.7 °F).<br />

Charlie Chong/ Fion Zhang


Pyroelectric devices have no direct current response, and a basic pyrovidicon<br />

imager 's display will fade when the device is aimed at an unchanging thermal<br />

scene. Early pyrovidicon imagers needed to be panned to retain image<br />

definition.<br />

To enable fixed monitoring, crude, flag type choppers were devised to<br />

interrupt the image at adjustable chop rates. However, this resulted in a<br />

blinking image that was disconcerting to the eye. These choppers have been<br />

replaced by synchronous choppers that chop the image in synchronism with<br />

the electronic scan rate and produce flicker free images on the display.<br />

Pyrovidicon viewers operate well in the 8 to 14 μm atmospheric transmission<br />

window. Operating costs are very low because no cooler or coolant is<br />

required.<br />

Charlie Chong/ Fion Zhang


● Staring Infrared Focal Plane Array Thermal Viewers<br />

Staring <strong>infrared</strong> focal plane array (lRFPA) thermal viewers are direct<br />

adaplations <strong>of</strong> devices developed for military and aerospace night vision and<br />

missile tracking applications. For these applications, performance emphasis<br />

is on picture quality rather than measurement capability. Instruments using<br />

cooled platinum silicide (PtSi) staring arrays with as many as 512 x 512<br />

elements are available. Instrument using cooled indium antimonide (LnSb)<br />

focal plane arrays are available in models designed to compete with top-<strong>of</strong>the-line<br />

commercial thermal imagers. Some instruments in this category have<br />

the size and weight <strong>of</strong> a commercial video camera that fits in the palm <strong>of</strong> the<br />

hand, as illustrated in Figure 3.12.<br />

Charlie Chong/ Fion Zhang


Figure 3.12: Infrared focal plane array imager for qualitative <strong>thermography</strong><br />

Charlie Chong/ Fion Zhang


Infrared focal plane array imager<br />

Charlie Chong/ Fion Zhang


Infrared focal plane array imager<br />

Charlie Chong/ Fion Zhang


Qualitative IrFPA<br />

Charlie Chong/ Fion Zhang


Infrared focal plane array imager<br />

Charlie Chong/ Fion Zhang


■ Quantitative Thermal Imagers<br />

Quantitative thermal imagers include (1) mechanicatly scanned thermal<br />

imagers (imaging radiometers) and (2) focal plane array radiometers.<br />

● Mechanically Scanned Thermal Imagers<br />

Mechanically scanned thermal imagers (imaging radiometers) provide a<br />

means for measuring apparent target surface temperature with high<br />

resolution image quality and sometimes with extensive on-board diagnostic<br />

s<strong>of</strong>tware. Mosl commercially available imaging radiometers use a single<br />

detector. but some manufacturers <strong>of</strong>fer dual detector or multidctcctor (linear<br />

array) instruments. Most require detector cooling. Imaging radiometers use<br />

refractive reflective or hybrid scanning systems and operate in either the 3 to<br />

5 μm or the 8 to 14 μm atmospheric window. They generally <strong>of</strong>fer<br />

instantaneous fields <strong>of</strong> view on the order <strong>of</strong> 1 to 2 mrad with standard optics<br />

and minimum resolvable temperature differences <strong>of</strong> 0.05 to 0.10 °C (0.09 to<br />

0.18 °F).<br />

Charlie Chong/ Fion Zhang


On-board capabilities include isotherm graphics features, spectral filtering.<br />

interchangeable optics for different total field <strong>of</strong> views. color or monochrome<br />

(black and white) displays, flexible video recording capabilities and computer<br />

compatibility. Most feature compact, field portable, battery operable sensing<br />

heads and control/display units. A complete system including battery and<br />

video recorder can be handled by one person by mounting the components<br />

on a cart or by assembling them on a harness.<br />

Charlie Chong/ Fion Zhang


● Focal Plane Array Radiometers<br />

Focal plane array radiometers are adaptations <strong>of</strong> military and aerospace<br />

forward looking <strong>infrared</strong> scanners. but are designed to measure the apparent<br />

temperature at the target surface and to produce quantitative thermograms.<br />

The capabilities <strong>of</strong> early <strong>infrared</strong> focal plane array imagers were slow in<br />

developing. The quality <strong>of</strong> measurement capabilities has improved since 1990.<br />

Infrared focal plane array cameras <strong>of</strong>fer minimum resolvable temperature<br />

differences comparable to imaging radiometers (0.1 to 0.2 °C; 0.18 to 0.36 °F)<br />

and instantaneous field <strong>of</strong> views considerably better than imaging<br />

radiometers (1 mRad or better with standard optics).<br />

Commercially available quantitative <strong>infrared</strong> focal plane array cameras use<br />

detector arrays made <strong>of</strong> platinum silicide or indium antimonide, either <strong>of</strong><br />

which requires cooling. Quantitative thermal imagers based on uncooled focal<br />

plane arrays (using bolometrie and ferroelectric detectors) have also been<br />

developed. With inherently faster response, no moving <strong>part</strong>s and superior<br />

spatial resolution <strong>infrared</strong> focal plane array cameras have been replacing<br />

<strong>infrared</strong> imaging radiometers for most applications.<br />

Charlie Chong/ Fion Zhang


ccc<br />

Charlie Chong/ Fion Zhang<br />

http://sevutune.tumblr.com/microbolometer


Infrared focal plane array imager<br />

Charlie Chong/ Fion Zhang


Platinum Silicide IrFPA<br />

Charlie Chong/ Fion Zhang<br />

http://www.bealecorner.com/trv900/thermal/therm.html


Quantitative IR Image<br />

Charlie Chong/ Fion Zhang


Quantitative IR Image<br />

Charlie Chong/ Fion Zhang


3.9 Thermal Imaging Display and Diagnostic<br />

S<strong>of</strong>tware<br />

When the personal computer was introduced as <strong>part</strong> <strong>of</strong> thermal imaging<br />

systems, the typical imager produced raw radiometric data. whereas all <strong>of</strong> the<br />

diagnostic s<strong>of</strong>tware was contained in an ancillary. separately packaged<br />

computer that performed all <strong>of</strong> the diagnostics back on the bench. With<br />

improved packaging technology in both computers and thermal imaging<br />

equipment, there has been a gradual trend toward providing more and more<br />

on board s<strong>of</strong>tware so that more diagnostics can be performed on site.<br />

Depending on manufacturer and model, some s<strong>of</strong>tware is incorporated into<br />

instruments and some is available only on computer driven s<strong>of</strong>tware<br />

packages. Although thermographic diagnostic s<strong>of</strong>tware packages are usually<br />

proprietary to a <strong>part</strong>icular manufacturer, there is a trend toward universality in<br />

image storage. Common formats for storing electronic images include tagged<br />

image file format (TIFF) and other bitmapped formats. Retrieving images from<br />

these format is fast and easy.<br />

Charlie Chong/ Fion Zhang


Quantitative Thermal Measurements<br />

Some qualitative thermograms can be converted to quantitative thermograms.<br />

The raw image produced by a quantitative imager may be converted to a<br />

quantitative thermogram; the raw image produced by a viewer may not.<br />

Quantitative thermal measurements provide the user with the true radiance or<br />

apparent temperature value <strong>of</strong> any or all points on the target surface. To<br />

present the thermogram in true radiance measurements, the system<br />

throughput attenuation must be considered as well as losses through the<br />

measurement medium (atmosphere, in most cases). To present the<br />

thermogram in true temperature values. the target effective emissivity must<br />

also be considered. When this capability is provided, a menu instructs the<br />

user to enter system calibration constants on initial setup and a system <strong>of</strong><br />

prompts assures the operator that changes in aperture settings, target<br />

distance, inter-changeable lenses. etc., will be fed into the keyboard each<br />

time a change in operating conditions occurs.<br />

Charlie Chong/ Fion Zhang


Changes in the corrections setting for target effective emissivity are also<br />

monitored. In addition. digital cameras are available to save visible images in<br />

computer compatible format for archiving with corresponding thermograms.<br />

For most systems. the displayed temperature <strong>reading</strong>s are based on the<br />

assumption that the entire target surface has the same effective emissivity.<br />

Some systems. however. allow the assignment <strong>of</strong> several different<br />

emissivities to different areas <strong>of</strong> the target selected by the operator with the<br />

resulting temperature correction. A color scale or gray scale is provided along<br />

one edge <strong>of</strong> the display with temperature shown corresponding to each color<br />

or gray level in the selected range. The operator can place one or more spots<br />

or crosshairs on the image and the apparent temperature value <strong>of</strong> that pixel<br />

will appear in an appropriate location on the display. The isotherm feature<br />

allows the operator to select a temperature band or interval and all areas on<br />

the target within that band then appear enhanced in a predetennined gray<br />

shade or color hue. Detailed processing and image diagnostics relies on<br />

s<strong>of</strong>tware that allows manipulation and analysis <strong>of</strong> each pixel in the<br />

thermogram prescnting information in a wide variety <strong>of</strong> qualitative and<br />

quantitative forms for the convenience <strong>of</strong> the user. Some <strong>of</strong> these capabilities<br />

are described in this chapler.<br />

Charlie Chong/ Fion Zhang


In addition to the spot measurement capability discussed previously. line<br />

pr<strong>of</strong>iles may be selected. The analog trace. in X, Y. or both. <strong>of</strong> the lines on the<br />

image intersecting at the selected spot will then appear at the edge <strong>of</strong> the<br />

display. Some systems allow the operator to display as many as seven sets<br />

<strong>of</strong> pr<strong>of</strong>iles simultaneously. Pr<strong>of</strong>iles <strong>of</strong> skew lines can also be displayed on<br />

some systems. Selected areas on the thermogram in the form <strong>of</strong> circles,<br />

rectangles or point-to-point free forms, can be shifted, expanded. shrunk or<br />

rotated or used to blank out or analyze portions <strong>of</strong> the image.<br />

Detailed analysis <strong>of</strong> the entire image or the pixels within the area can include<br />

maximum, minimum and verage values. number <strong>of</strong> pixels or even a<br />

frequency histogram <strong>of</strong> the values within the area. Color scales can be<br />

created from 256 colors stored in the computer. Electronic zoom features<br />

allow the operator to expand a small area on the display for closer<br />

examination. or to expand the colors for a small measurement range.<br />

Autoscale features provide the optimum display settings for any image if<br />

selected. Three-dimensional features provide an isometric thermal contour<br />

map or thermal pr<strong>of</strong>ile map <strong>of</strong> the target for enhanced recognition <strong>of</strong> thermal<br />

anomalies.<br />

Charlie Chong/ Fion Zhang


Image Recording, Storage and Recovery<br />

Images and data can be stored in and retrieved from memory, hard disk,<br />

floppy diskette, video tape, optical disks (writable compact disks and<br />

digitalvideo disks) and Personal Computer Memory/Computer Industry<br />

Association (PCMCIA) cards.<br />

Commercial thermal imaging systems incorporate some means, such as a<br />

floppy disk drive or a PCMCIA card to store images in the field. Usually. about<br />

forty images. with all accompanying data, can be stored on a 3.5 in diskette.<br />

Some analysis usually can be done with on-board s<strong>of</strong>tware; more extensive<br />

diagnostics usually require a separate computer. Options include IEEE or<br />

RS232 ports for access to additional storage and a video recorder option so<br />

that an entire measurement program can be recorded on video tape. Video<br />

tapes can be played back into the system and images can be saved to disk.<br />

Images can be stored from a frozen frame thermogram <strong>of</strong> a live target on<br />

operator command. or the operator can set up an automatie sequence and a<br />

preset number <strong>of</strong> images will be stored at preset time intervals.<br />

Charlie Chong/ Fion Zhang


Stored images can be retrieved, displayed and further analyzed. Image<br />

comparison (differential <strong>thermography</strong>) allows the automatic comparison <strong>of</strong><br />

thermograms taken at different times. This includes time based comparison <strong>of</strong><br />

images taken <strong>of</strong> the same target as well as the comparison <strong>of</strong> images taken<br />

<strong>of</strong> different but similar targets.<br />

A special s<strong>of</strong>tware program allows the operator to display two images sideby-<br />

ide or in sequence; and to subtract one image from another or one area<br />

from another; and to display a pixel-by-pixel difference thermogram.<br />

Comparison (subtraction) <strong>of</strong> images can be accomplished between two<br />

images retrieved from disk, between a live image and an image retrieved from<br />

disk and between a live image and an image stored in a computers random<br />

access memory, in this way, standard thermal images <strong>of</strong> acceptable<br />

components, assemblies and mechanisms can be archived and used as<br />

models for comparison to subsequently inspected items. It is also possible to<br />

subtract a live image from a previous baseline image for subsequent time<br />

based thermal transient measurements.<br />

Charlie Chong/ Fion Zhang


Database and Documentation<br />

Records, files, data and documents can be saved in an orderly fashion. This<br />

capability provides thc thermographers with a filing system so that records <strong>of</strong><br />

all measurement missions can be maintained on magnetic media, including<br />

actual thermograms, time, date, location, equipment, equipment settings,<br />

measurement conditions and other related observations.<br />

Most manufacturers <strong>of</strong> thermal imaging equipment have developed<br />

comprehensive report preparation s<strong>of</strong>tware to facilitate timely and<br />

comprehensive reporting <strong>of</strong> the findings <strong>of</strong> <strong>infrared</strong> surveys and other<br />

measurement missions. These packages provide templates that allow thc<br />

thermographer to prepare reports in standard word processor formats into<br />

which tagged image file format (TIFF) images. imported from various imaging<br />

radiometers. can be directly incorporated. Additional diagnostic s<strong>of</strong>tware is<br />

customarily provided in these packages so that analysis and trending can be<br />

added to reports.<br />

Charlie Chong/ Fion Zhang


Calibration Accessories<br />

Infrared radiation reference sources are used by manufacturers to calibrate<br />

<strong>infrared</strong> sensing and imaging instruments in the laboratory before they are<br />

shipped. These same reference sources are used later at periodic intervals<br />

thereafter to ensure calibration stability. A radiation reference source is<br />

designed to simulate a blackbody radiator: that is. a target surface with a<br />

stable, adjustable known temperature and a uniform emissivity approaching<br />

1.0 at all appropriate wavelengths. In addition to laboratory reference sources.<br />

there are field portable models suitable for periodic calibration checks <strong>of</strong><br />

fielded thermographic equipment and for other tasks. The setup and<br />

deployment <strong>of</strong> radiation reference sources is discussed in Chapter 4.<br />

Charlie Chong/ Fion Zhang


3.10 Photorecording Accessories for Hard Copies<br />

Since the advent <strong>of</strong> the personal computer and its integration with thermal<br />

imagers, magnetic storage and archiving <strong>of</strong> data (labels. dates. conditions <strong>of</strong><br />

measurement. instrument settings. etc.) as well as thermograms have<br />

become routine. S<strong>of</strong>t copies can be made <strong>of</strong> real time images, processed<br />

images enhanced images and combined images on floppy disks, analog and<br />

digital magnetic tape, recordable optical disks and Personal Computer<br />

Memory/Computer Industry Association (PCMCIA) cards.<br />

Report preparation s<strong>of</strong>tware allows images to be inserted into word<br />

processing documents and printed by conventional laser or inkjet printers.<br />

Making a hard copy directly from a stored or displayed image is done in a<br />

variety <strong>of</strong> ways. A number <strong>of</strong> devices were introduced before magnetic media<br />

were available for directly photographing the display between with<br />

conventional or instant film. Using them generally required considerable skill<br />

because the ambient lighting and the screen curvature had to be considered.<br />

For this reason. it was difficult to achieve repeatable results. online printers<br />

and plotters provide reliable, good quality copies when speed is not a<br />

consideration.<br />

Charlie Chong/ Fion Zhang


Online printers and plotters are relatively slow and may tie up the computer<br />

and related s<strong>of</strong>tware during operation. For real time or high speed photorecording,<br />

portable video printers are usually selected. The video printer<br />

connects to the system's video output. It presents the current image on a<br />

remote display where it is frame grabbed and reproduced in real time under<br />

optimized conditions. Most video printers produce output on integral recorder<br />

paper. Available accessories allow a choice <strong>of</strong> direct instant hardcopies,<br />

negatives or slide transparencies. Although video printers are costly. they<br />

provide consistent quality in a reasonable time and do not require the use <strong>of</strong><br />

the thermal imager or the computer during production time.<br />

Charlie Chong/ Fion Zhang


Chapter 3<br />

Review Questions<br />

Q&A<br />

1. b<br />

2. d<br />

3. a<br />

4. b<br />

5. d<br />

6. a<br />

7. c<br />

8. c<br />

9. d<br />

10. d<br />

11. b<br />

12. a<br />

13. b<br />

14. b<br />

15. a<br />

16. b<br />

17. d<br />

18. b<br />

19. e<br />

20. a<br />

21. d<br />

22. a<br />

23. a<br />

24. d<br />

25. b<br />

Charlie Chong/ Fion Zhang


Q1. The thermal resolution <strong>of</strong> an instrument is the same as:<br />

a. the temperature accuracy.<br />

b. minimum resolvable temperature difference.<br />

c. temperature repeatability.<br />

d. the minimum spot size.<br />

Q2. The speed <strong>of</strong> response <strong>of</strong> an instrument is:<br />

a. the time constant <strong>of</strong> the detector.<br />

b. one half the time constant <strong>of</strong> the detector.<br />

c. the same as the field repetition rate.<br />

d. the time it takes to respond to a step change at the target surface.<br />

Q3. The instantaneous spot size <strong>of</strong> an instrument is related to the:<br />

a. instantaneous field <strong>of</strong> view and the working distance.<br />

b. thermal resolution.<br />

c. spectral bandwidth and the working distance.<br />

d. speed <strong>of</strong> response and the working distance.<br />

Charlie Chong/ Fion Zhang


Q4. The performance parameters that are important for qualitative<br />

<strong>thermography</strong> are:<br />

a. absolute accuracy, repeatability and resolution.<br />

b. spatial resolution and thermal resolution.<br />

c. spatial resolution and absolute accuracy.<br />

d. measurement spatial resolution and thermal resolution.<br />

Q5. Thermal viewers do not provide:<br />

a. high resolution thermograms.<br />

b. recording capabilities.<br />

c. real time scan rates.<br />

d. quantitative thermograms.<br />

Q6. The thermal resolution <strong>of</strong> an instrument tends to:<br />

a. improve as target temperature increases.<br />

b. degrade as target temperature increases.<br />

c. remain constant regardless <strong>of</strong> target temperature.<br />

d. improve with increasing working distance.<br />

Charlie Chong/ Fion Zhang


Q7. The 3 to 5 μm spectral region is ideally suited for operation <strong>of</strong> instruments:<br />

a. measuring subzero temperature targets.<br />

b. measuring targets at extremely long working distances.<br />

c. measuring targets warmer than 200 °C (392 ° F).<br />

d. operating at elevated ambient temperature.<br />

Q8. The total field <strong>of</strong> view <strong>of</strong> an imaging instrument determines the:<br />

a. imaging spatial resolution (lFOV) <strong>of</strong> the instrument.<br />

b. measurement spatial resolution (IFOVmeas) <strong>of</strong> the instrument.<br />

c. image size at the target plane for any given working distance.<br />

d. operating spectral range <strong>of</strong> the instrument.<br />

Q9. The frame repetition rate <strong>of</strong> an imager is defined as the:<br />

a. number <strong>of</strong> imaging pixels in a thermogram.<br />

b. number <strong>of</strong> frames selected for image averaging.<br />

c. electronic image rate <strong>of</strong> the display screen.<br />

d. number <strong>of</strong> times every point on the target is scanned in one second.<br />

Charlie Chong/ Fion Zhang


Q10. The purpose <strong>of</strong> adding an <strong>infrared</strong> spectral filter to an instrument may be<br />

to limit the spectral band:<br />

a. to only wavelengths longer than a specified wavelength.<br />

b. to only wavelengths shorter than a specified wavelength.<br />

c. to only wavelengths between two specified wavelengths.<br />

d. any <strong>of</strong> the above.<br />

Q11. To quickly calculate target spot size, a useful approximation is:<br />

a. π =3.1416.<br />

b. an instantaneous field <strong>of</strong> view <strong>of</strong> 1 degree represents a 60: 1 ratio<br />

between working distance and spot size.<br />

c. there are 2π radians in 360 degrees.<br />

d. a 1°F temperature change is equivalent to a 1.8 °C temperature change.<br />

Q12. For online process control instruments, important features are:<br />

a. environmental housings and long term stability.<br />

b. ready access to emissivity compensation setting.<br />

c. portability and battery life.<br />

d. precision sighting.<br />

Charlie Chong/ Fion Zhang


Q13. A line scanner can be used to produce a thermogram <strong>of</strong> a sheet process<br />

only when:<br />

a. emissivity is known.<br />

b. the sheet process is moving at a uniform rate.<br />

c. the process material is a non graybody.<br />

d. the sheet process is hotter than 200 °C (392 °F).<br />

Q14. Most quantitative <strong>infrared</strong> thermal imagers:<br />

a. are heavier than quantitative imagers and usually require line power.<br />

b. can store thermograms on floppy disks in the field.<br />

c. require frequent infusions <strong>of</strong> detector coolant in the field.<br />

d. use detectors that operate at room temperature.<br />

Q15. Infrared focal plane array imagers:<br />

a. have no scanning optics.<br />

b. cannot be used for quantitative <strong>thermography</strong>.<br />

c. cannot be used for very cool targets.<br />

d. cannot operate on rechargeable batteries.<br />

Charlie Chong/ Fion Zhang


Q16. Most <strong>infrared</strong> focal plane array imagers:<br />

a. use more costly optics than scanning radiometers.<br />

b. <strong>of</strong>fer better spatial resolution than scanning radiometers.<br />

c. <strong>of</strong>fer better thermal resolution than scanning radiometers.<br />

d. <strong>of</strong>fer more diagnostics features than scanning radiometers.<br />

Q17. The number <strong>of</strong> detector elements in an <strong>infrared</strong> focal plane array imager:<br />

a. affects the measurement accuracy <strong>of</strong> the imager.<br />

b. affects the thermal resolution <strong>of</strong> the imager.<br />

c. affects the spectral band <strong>of</strong> the imager.<br />

d. affects the spatial resolution <strong>of</strong> the imager.<br />

Q18. The fact that all elements in a focal plane array imager are always<br />

looking at the target make this kind <strong>of</strong> imager better suited than scanning<br />

imagers<br />

for observing:<br />

a. distant low temperature targets.<br />

b. targets with rapidly changing temperatures.<br />

c. targets with low emissivities.<br />

d. targets with high emissivities.<br />

Charlie Chong/ Fion Zhang


Q19. For which <strong>of</strong> the following applications are quantitative thermograms<br />

most critical?<br />

a. Search and rescue.<br />

b. Nondestructive material testing.<br />

c. Process monitoring and control.<br />

d. Security and surveillance.<br />

Q20. Infrared thermal detectors:<br />

a. have a broad. flat spectral response.<br />

b. usually require cooling to operate properly.<br />

c. have much faster response times than photon detectors.<br />

d. have much greater sensitivity than photon detectors.<br />

Q21. The characteristics <strong>of</strong> <strong>infrared</strong> photodetectors<br />

(photon detectors) include:<br />

a. faster response times than thermal detectors.<br />

b. a requirement for cooling to operate properly.<br />

c. selective spectral response based on operating temperature.<br />

d. all <strong>of</strong> the above.<br />

Charlie Chong/ Fion Zhang


Q22. Filters, lenses and transmitting windows:<br />

a. are all examples <strong>of</strong> refractive optical elements.<br />

b. have negligible transmission loss in the <strong>infrared</strong>.<br />

c. are all examples <strong>of</strong> reflective optical elements.<br />

d. are not spectrally selective.<br />

Q23. Resistance temperature detectors and thermistors operate on the same<br />

principle. that is:<br />

a. a predictable change in resistance as a function <strong>of</strong> temperature.<br />

b. the inverse square law.<br />

c. the known expansion <strong>of</strong> dissimilar materials.<br />

d. the comparison <strong>of</strong> target brightness with a calibrated reference.<br />

Q24. Infrared radiation thermometers are used to measure temperature:<br />

a. without contacting the target.<br />

b. very rapidly.<br />

c. without causing a temperature change at the target.<br />

d. all <strong>of</strong> the above.<br />

Charlie Chong/ Fion Zhang


Q25. Two-color (ratio) pyrometers measure the temperature <strong>of</strong> a target by:<br />

a. taking into account the size and distance to the target.<br />

b. comparing the radiant energy from the target in two narrow spectral<br />

bands.<br />

c. incorporating tables <strong>of</strong> known emissivity.<br />

d. calibrating and correcting for the <strong>infrared</strong> absorption in the measurement<br />

path.<br />

Charlie Chong/ Fion Zhang


End Of Reading<br />

Charlie Chong/ Fion Zhang


Good Luck<br />

Charlie Chong/ Fion Zhang


Good Luck<br />

Charlie Chong/ Fion Zhang


Charlie https://www.yumpu.com/en/browse/user/charliechong<br />

Chong/ Fion Zhang

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