IIRT Level-1 Infrared Cheat Sheet

(Not available anywhere else)

 

Definitions

  • Infrared thermography is a technique that uses infrared cameras to detect and measure heat emitted by objects, creating visual images that show temperature variations on their surfaces.
  • Infrared radiation travels in all directions from its source, radiating outward in a straight line until it is absorbed, reflected, or transmitted by other objects.

 

Benefits

  • Early Problem Detection
    • Preventive Maintenance: Spot issues early to avoid major breakdowns.
    • Electrical Safety: Detect hot spots and overheating in electrical systems to prevent fires.
  • Cost Savings
    • Lower Repair Costs: Fixing small issues early is cheaper than big repairs.
    • Energy Efficiency: Find and fix energy losses to save on bills.
  • Safety
    • Fire Prevention: Early detection of overheating components can prevent fires.
    • Non-Invasive: Inspections are done without touching equipment, making it safer.
  • Quality Control
    • Manufacturing: Ensure product quality by checking for consistent heating or cooling.
    • Building Inspections: Find structural issues, moisture problems, and insulation gaps.
  • Environmental Benefits
    • Energy Conservation: Fixing inefficiencies helps reduce energy use and environmental impact.
    • Sustainability: Preventing breakdowns reduces waste and resource use.
  • Documentation
    • Detailed Reports: Provide visual evidence and detailed findings.
    • Baseline Data: Track changes over time by comparing with initial inspections.
  • Versatility
    • Multiple Applications: Useful in various fields like electrical, mechanical, building, medical, and manufacturing.
    • Non-Destructive Testing: Inspect without damaging the item.

 

Infrared Waves & the Electromagnetic Spectrum

  • Infrared radiation was discovered by Sir William Herschel in 1800 when he used a prism to split sunlight and detected a temperature increase beyond the red part of the visible spectrum.
  • Electromagnetic Spectrum – Position of Infrared: Between visible light and microwaves. 
  • Infrared waves travel at the speed of light.
  • Infrared region: Wavelengths from 0.7 micrometers (µm) to 1 millimeter (mm).
  • Subdivisions within the infrared spectrum: Near-infrared (NIR), mid-infrared (MIR), and far-infrared (FIR).
  • Infrared radiation is not visible to the human eye.
  • As such, normal light does not affect your infrared thermography but is important in the aspect of safety and your digital photo used for reference.
  • All objects at temperatures above absolute zero emit thermal radiation.
  • Temperature Units
    • Absolute Scales: Rankine & Kelvin
    • Relative Scales: Fahrenheit & Celsius

 

Important Infrared Thermography Laws

    • Kirchoff’s Law: A + R + T = 1
  • Absorptivity + Reflectivity + Transmissivity = 1
    • A: Emissivity (or Absorptivity) is the measure of an object’s ability to emit infrared energy, expressed as a value between 0 and 1. It indicates how efficiently an object radiates heat compared to a perfect black body.
    • A black body is a perfect emitter and absorber of infrared radiation. Ie. A or E = 1
    • A grey body is an emitter and absorber of infrared radiation of less than 1.
    • A white body reflects all incident radiation completely. It does not absorb or emit any radiation.
    • E value of PVC Tape: 0.95
    • E value of Skin: 0.98
    • E value of Water: 0.95 – 0.98 (distilled water)
  • These are idealised objects for scientific understanding purposes, they do not actually exist.
  • Surface Condition: Polished surfaces have lower emissivity than rough or oxidised surfaces.
  • R: Reflectivity is when infrared radiation is reflected by a surface.
  • High reflectivity can cause false readings by reflecting surrounding temperature. While doing inspections, move around to avoid or identify reflections. 
  • T: Transmissivity is when  infrared radiation passes through a material, such as certain plastics, many types of glass do not allow IR to pass through.
  • Planck’s Law: Describes the spectral density of electromagnetic radiation emitted by a blackbody in thermal equilibrium at a given temperature. Key to understanding how infrared radiation varies with wavelength and temperature.
  • Stefan-Boltzmann Law: W = kT4
  • Wien’s Law: λm = b/T

 

Thermal Energy Concepts

  • Conduction:
    • Transfer of heat through a material (solid) without the material itself moving.
    • Example: Heat moving through a metal rod.
  • Convection:
    • Transfer of heat by the physical movement of a fluid (liquid or gas).
    • Example: Warm air rising and cool air sinking to form convection currents.
  • Radiation:
    • Transfer of heat in the form of electromagnetic waves. Possible through a vacuum. 
    • Example: Sun warming the Earth’s surface.
  • Thermal Equilibrium is where all parts of a system have the same temperature and no heat flows.
  • To get more accurate measurements, ensure that there is enough temperature difference, eg. outdoor inspections on a rainy day or later in the evening instead of at noon.
  • Dust and cavities can have higher emissivity. With little gaps or holes impacted by the cavity effect. 
  • Temperature is a measure of the average vibrating kinetic energy of the particles in matter. 
  • Thermal energy is the total vibrational kinetic energy in molecules.
  • Heat is the flow of Thermal energy. It is the transfer of thermal energy from one object or substance to another due to a temperature difference.
  • First Law of Thermodynamics (Law of Energy Conservation)
    • Energy cannot be created or destroyed, only transformed from one form to another. 
  • Second Law of Thermodynamics
    • Thermal Energy will flow from one of higher temperature to one of lower temperature.

 

Thermal Cameras & Inspections

    • Calibration: Ensuring accurate temperature measurements by periodically calibrating the infrared camera. Usually annually or every 6-months for high-usage. 
  • Temperature measurement methods: Contact vs. Non-contact
    • Camera Detector Types: Cooled vs. Uncooled
  • Infrared Camera Types: Long-wave, Mid-wave, Short-wave, Near-wave 
  • Spatial Resolution: Defined by the number of pixels in the detector array. eg.: 320×240 pixels, 640×480 pixels.
  • Thermal Resolution (NETD – Noise Equivalent Temperature Difference): Measures the camera’s ability to distinguish small temperature differences. Lower NETD values indicate higher sensitivity. Eg: 50 mK (millikelvin).
  • Infrared Thermal Cameras ONLY detect surface temperature.
  • Due to how infrared thermal cameras are manufactured, Temperature and Emissivity values are inversely related.
  • FOV: Field-of-view. The total observable area that the thermal camera can capture at a given moment. It is usually expressed in degrees.
  • IFOV: Instantaneous Field of View. The smallest detail a thermal camera can resolve from a given distance. The IFOV is a fixed property of the camera’s optics and detector. It does not change with distance. But the spot size (in mm or inches) changes with distance.
  • Focus is VERY important, as it cannot be adjusted in software. Ensure your thermal images are focused.
  • Image Fusion: Combining infrared images with visible light images to enhance understanding and clarity of the inspection area. Eg. MSX in FLIR Thermal Cameras.
  • Hot Spots: Areas with significantly higher temperatures compared to the surrounding environment. Common causes include electrical faults, mechanical friction, and heat-generating processes.
  • In electrical systems, overheating is usually due to high electrical resistance.
  • The usual maximum functional temperature of PVC components is 70°C. Higher for more heat resistant applications especially in marine offshore and in oil and gas industries.
  • Cold Spots: Areas with significantly lower temperatures. Often indicative of moisture presence, insulation failures, or cooling system malfunctions. In electrical systems, it could indicate inactive or broken circuits.
  • Baseline Comparisons: Comparing current thermal images with baseline images taken under similar conditions helps in identifying deviations and anomalies.
  • In our Specifications-based Technique, we inspect with the reference temperature of the target in mind. Eg. the max operating temperature of PVC being about 70°C
  • Leveling refers to adjusting the mid-point of the temperature range displayed in the thermal image. This mid-point is often called the “level” or “center temperature.” Adjusting the level helps to focus on the specific temperature range of interest within the scene.
    • Purpose: To bring out details in a specific temperature range by adjusting the image’s overall brightness.
    • Eg.: If you’re inspecting an electrical panel and want to highlight components around 50°C, you might set the level to 50°C to enhance the visibility of those components.
  • Spanning refers to adjusting the range of temperatures (span) displayed in the thermal image. This range is the difference between the highest and lowest temperatures shown.
    • Purpose: To increase or decrease the contrast of the thermal image by adjusting the temperature range.
    • Eg.: If the thermal scene has temperatures ranging from 20°C to 70°C, setting a narrow span (e.g., 40°C to 60°C) will provide higher contrast for temperatures within that range, making it easier to see subtle temperature differences.

 

IIRT Level-2 Infrared Cheat Sheet

(Not available anywhere else)

This sheet assumes the Level 1 fundamentals are already known.
It focuses only on the additional concepts tested at Level 2.


 

Specific Heat

Specific heat is the amount of heat energy required to raise the temperature of:

1 gram of a material by 1°C

Different materials require different amounts of energy to produce the same temperature change.

Important Values
MaterialSpecific Heat
Gold0.126 J/g°C
Copper0.386 J/g°C
Aluminium0.897 J/g°C
Water4.18 J/g°C

Key concept

Higher specific heat → more energy required to change temperature.

Water has a relatively high specific heat, so it heats and cools more slowly than many metals.


 

Heat Energy Calculation

Use:

Q = m × c × ΔT

Where:

  • Q = heat energy, Joules

  • m = mass, grams

  • c = specific heat, J/g°C

  • ΔT = temperature change, °C

Example

200 g of water:

30°C → 90°C

ΔT = 60°C

Q = 200 × 4.18 × 60

Q = 50,160 J

 

Useful number

Heating 1 kg of water by 1°C:

1000 × 4.18 × 1 = 4180 J

 


 

Thermal Capacitance

Thermal capacitance refers to the amount of thermal energy an object can store.

It depends mainly on:

  • mass

  • specific heat

Conceptually:

Thermal Capacitance = mass × specific heat

Higher thermal capacitance means the object generally:

  • requires more energy to change temperature

  • changes temperature more slowly

  • can store more thermal energy

Do not confuse:

Specific Heat: Property of the material.

Thermal Capacitance: Thermal storage capability of the whole object.

 


 

Thermal Resistance

Thermal resistance describes how strongly a material resists the flow of heat through it.

Higher resistance → less heat transfer.

Lower resistance → greater heat transfer.

 

It is affected by factors such as:

  • material thermal conductivity

  • material thickness

  • area through which heat travels

Important Distinction
PropertyMeaning
Specific HeatEnergy required to change temperature
Thermal CapacitanceAmount of thermal energy an object can store
Thermal ResistanceResistance to heat flow

 

Celsius to Kelvin

Radiation calculations require absolute temperature.

Use:

K = °C + 273

More precisely:

K = °C + 273.15

 

Example

90°C:

90 + 273 = 363 K

 

Why Kelvin matters

Infrared radiation laws depend on absolute temperature rather than relative Celsius temperature.

 


 

Wien’s Law Calculations

Wien’s Law relates temperature to the wavelength where the object emits its maximum amount of radiation.

λmax = b / T

Where:

  • λmax = peak wavelength

  • T = temperature in Kelvin

  • b ≈ 2898 µm·K

Example:

70°C object

Convert first:

70 + 273 = 343 K

Then:

2898 / 343 ≈ 8.45 µm

 

Remember

Higher temperature → shorter peak wavelength.

Lower temperature → longer peak wavelength.

 

For the test, know how to calculate the wavelength, not only the general principle.

 


 

MRTD

MRTD = Minimum Resolvable Temperature Difference

MRTD describes the ability of the complete imaging system to distinguish a temperature difference between small spatial features.

It combines aspects of:

  • thermal contrast

  • spatial resolution

  • image-system performance

Think of it as:

Can I actually distinguish two small features that have only a small temperature difference?

This is different from simply detecting that some temperature difference exists.

 


 

NETD vs MRTD

Although NETD is introduced at Level 1, Level 2 requires understanding its relationship with MRTD.

ParameterMain Question
NETDHow small a temperature difference can the detector detect?
MRTDHow small a thermal difference can actually be resolved as a spatial feature?

Simple memory aid

NETD = Detect

MRTD = Resolve

A camera can theoretically detect a small temperature difference but may not necessarily resolve it clearly on a small target.

 


 

Target Size, Distance & IFOV Application

At Level 2, IFOV becomes a measurement problem, not merely a definition.

The target must occupy enough detector pixels for reliable temperature measurement.

 

Approximate relationship:

Target size ≈ Distance × IFOV

 

Practical consequence

As distance increases:

  • each pixel covers a larger physical area

  • small targets occupy fewer pixels

  • temperature measurements become less reliable

If the target is too small: move closer.

Focusing the camera better does not compensate for insufficient detector coverage.

 

Important principle

Being able to see an object does not necessarily mean you can accurately measure it.


 

Measurement IFOV vs Detection IFOV

For temperature measurement, the target normally needs to cover more than one detector pixel.

This is why:

  • detection distance

  • recognition distance

  • accurate measurement distance

are not the same thing.

 

A hot object may be visible at a large distance while its reported temperature is still inaccurate because surrounding pixels influence the measurement.

 


 

Cavity Effect

A cavity can have an effective emissivity higher than the original surface emissivity.

Radiation entering the cavity undergoes repeated:

  • reflections

  • absorption

  • re-emission

before leaving the opening.

This causes the cavity to behave more like a blackbody.

 

Practical implication

A hole or recess may appear thermally different from the surrounding flat surface even when both are:

  • the same material

  • at similar actual temperatures

Key idea

Geometry itself can affect apparent emissivity.

 


 

Effect of Viewing Angle on Emissivity

Level 2 goes beyond simply avoiding reflections.

As the viewing angle becomes increasingly oblique:

  • apparent emissivity can decrease

  • apparent reflectivity can increase

  • measured temperature can become less reliable

For accurate quantitative measurements, viewing close to normal/perpendicular is preferred whenever practical.

 

Important

The material’s emissivity should not always be treated as one fixed number independent of:

  • angle

  • wavelength

  • temperature

  • surface condition

  • camera spectral response

 


 

Emissivity vs Target Temperature Practical

Changing the emissivity setting changes the camera’s calculated target temperature.

The effect becomes particularly significant when:

  • target emissivity is low

  • target temperature differs substantially from reflected surroundings

 

General relationship

For a given amount of radiation reaching the camera:

Lower entered emissivity
→ camera attributes less radiation to the target itself
→ calculated target temperature generally increases.

 

Level 2 lesson

Do not treat emissivity merely as a number to enter into the camera.

Understand how sensitive the final result is to the assumption being made.

 


 

Reflected Apparent Temperature — Measurement Importance

For quantitative measurements, the camera receives radiation consisting partly of:

target emission + reflected environmental radiation

 

The lower the emissivity:

→ the greater the reflected component.

 

Therefore Reflected Apparent Temperature becomes increasingly important for low-emissivity targets.

For high-emissivity surfaces in moderate environments, its effect may be comparatively small.

 

Practical lesson

Do not adjust RAT blindly for every inspection.

Assess whether reflected radiation is actually significant to the measurement uncertainty.

 


 

Slit Response Function

Slit Response Function (SRF) demonstrates how target size influences the temperature reported by an infrared camera.

A controlled thermal target is viewed through a slit.

As slit width increases:

  • more detector pixels are filled by the target

  • influence from the surrounding background decreases

  • indicated temperature approaches the true target temperature

What it demonstrates

A camera may:

  1. Detect an object

  2. Display the object

  3. Yet still be unable to accurately measure its temperature

until the target occupies sufficient detector area.

 

Connection to field inspections

Particularly important for:

  • wires

  • small terminals

  • distant components

  • narrow pipes

  • small electrical contacts

 


 

Lens Filters

An infrared filter allows selected infrared wavelengths to reach the detector while reducing or blocking others.

Filters can be used for specialised applications such as:

  • high-temperature measurement

  • furnaces

  • process monitoring

  • viewing through particular materials

  • suppressing unwanted radiation bands

Important principle

The filter must be matched with:

  • the target

  • required wavelength

  • camera detector

  • camera spectral range

Adding a filter changes the amount and wavelength distribution of radiation reaching the detector.

 


 

Infrared Windows — Measurement Considerations

An IR window allows infrared radiation to pass through an enclosure while keeping the enclosure physically closed.

For quantitative temperature measurement, the window introduces another factor: transmittance

Radiation reaching the camera may now be affected by:

  • target emissivity

  • reflected radiation

  • window transmission

  • window temperature

  • spectral response

Important

Seeing the target through an IR window does not automatically mean its temperature is correct.

The transmission characteristics of the window need to be considered.

 


 

Qualitative vs Quantitative Thermography

Qualitative Thermography

Concerned mainly with:

thermal patterns and relative differences

Questions include:

  • Where is the anomaly?

  • What thermal pattern is abnormal?

  • How does it compare with surrounding areas?

Precise absolute temperature may not be necessary.

 


 

Quantitative Thermography

Concerned with:

temperature measurement

Greater attention is therefore required for:

  • emissivity

  • reflected apparent temperature

  • target size

  • distance

  • transmittance

  • atmospheric effects

  • camera accuracy

Easy distinction

Qualitative = Pattern

Quantitative = Measurement

 


 

Camera Image Clarity — System Approach

A clear thermal image is not determined by detector resolution alone.

Image performance depends on the complete imaging system, including:

  • detector

  • optics/lens

  • electronics

  • display

  • thermal sensitivity

  • spatial resolution

  • focus

Level 2 principle

Do not judge camera performance using a single specification.

A camera with excellent NETD but poor spatial resolution may still be unsuitable for a small target.

Likewise, very high detector resolution does not automatically guarantee good thermal sensitivity.

 


 

Measurement Before Interpretation

The thermographer must first establish whether the apparent thermal condition is real and measurable.

Before interpreting a thermal anomaly, consider:

Target

  • size

  • material

  • emissivity

  • geometry

Camera

  • focus

  • detector resolution

  • measurement spot size

  • spectral range

Environment

  • reflected radiation

  • atmospheric effects

  • wind

  • external heat sources

Equipment

  • operating state

  • load

  • expected thermal behaviour

Only after these factors are considered should the thermographer determine the likely significance of the anomaly.

 


 

HIGH-PRIORITY FORMULAS & NUMBERS

TopicRemember
Specific heat of water4.18 J/g°C
Heat energyQ = mcΔT
1 kg water raised 1°C4180 J
Celsius → KelvinK = °C + 273
Wien’s Lawλmax = 2898 / T(K)
70°C peak wavelength≈ 8.45 µm
NETDThermal sensitivity / detection
MRTDThermal + spatial resolving ability
IFOV applicationTarget size ≈ Distance × IFOV

 

LAST-MINUTE LEVEL-2 MEMORY MAP

THERMAL MATERIAL PROPERTIES

Specific Heat → Energy required to change material temperature

Thermal Capacitance → Energy storage capability of the whole object

Thermal Resistance → Resistance to heat flowing through material

 


 

CAMERA PERFORMANCE

NETD → Can the detector sense the ΔT?

MRTD → Can the imaging system resolve the ΔT as a feature?

IFOV → How much target does one pixel see?

SRF → How target size affects the measured temperature

 


 

QUANTITATIVE MEASUREMENT

Accurate temperature depends on:

Target + Camera + Environment

Pay particular attention to:

  • emissivity

  • reflected apparent temperature

  • target size

  • viewing angle

  • transmission

  • distance


 

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