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/ Knowledge Base / Thermography Properties

Thermography and Radiometric Properties

Explore the principles of thermography and the radiometric properties essential for accurate temperature measurements with infrared cameras. Learn about the factors that influence field of view, emissivity, and how environmental conditions affect the precision of your infrared readings.

Field of View and Temperature Measurement

The Figure below, shows the horizontal (HFOV) and vertical (VFOV) field of view. Depending on the distance of the camera to the observed scene, the maximum scene width increases. As the distance increases, the resolution on the object to be measured changes.
Since real optics produce an unavoidable blur, the object to be measured should be at least 3 pixels in size to obtain an accurate measurement result.

Thermographic principles for radiometric temperature determination

This chapter is intended to provide a brief overview of the radiometric temperature measurement with infrared cameras. Prerequisite for a temperature measurement with the IRSX is that the camera has a calibration. This can be recognized by the GenICam Nodes Radiometric Control in the camera properties.

The camera series IRSX is exclusively equipped with thermal sensors. An essential feature of these sensors is the direct proportional relationship to the radiant energy incident from an object on the detector. The radiant energy depends nonlinearly on the object temperature and is influenced by environmental conditions as well as by object parameters.

In order to be able to measure the temperature of an object via its infrared radiation, it is essential to know some parameters of the measurement situation. The most important parameters are illustrated in the sketch below.

Emissivity

The emissivity depends on several object properties such as material, surface condition, viewing angle and also on the object temperature itself. Thus, this parameter is one of the most fundamental in thermographic temperature measurement. In practice values between 0.1 (e.g., polished metal surfaces) to 0.98 (e.g., human skin) are common.
The functional relationship between the object temperature and the signal SDet of the camera, taking into account the viewing scene, is described by the following formula:
In order to calculate the object temperature TObj, the camera signal SDet has to be corrected with respect to the environmental influences.

Determination of the Object Emissivity

The emissivity of an object can be provisionally determined, for example, by the methods described below. The object must have a temperature that differs significantly from the ambient temperature. For your orientation, a table with typical values for the emissivity of different materials can be found in the appendix (see section Emissivity Table).

Measurement of the Object Temperature with a Thermocouple

A simple method for the provisional determination of the emissivity is obtained by measuring the object temperature at a point using a thermocouple. Now align the infrared camera to the same point on the object and adjust the emissivity until the temperature displayed by the camera matches the value measured with the thermocouple. The set value is then the emissivity of the object. With this procedure, however, it should be ensured that the temperature of the measurement object differs significantly from the temperature of the environment.

Using a Reference Material

In this method, a reference material with known emissivity is applied to the measurement object. For example this can be paint or a piece of tape. By adjusting the emissivity of the reference material on the camera and measuring the temperature of the ink / adhesive tape, the object temperature is first determined. The emissivity of the measurement object is obtained by looking at the object itself with the camera and adjusting the emissivity until you get the same temperature reading as on the reference material. Again with this method, the object temperature should be significantly different from the ambient temperature.

Temperature Calculation from camera signal (Flux Linear)

The non-linear relationship between camera signal and object temperature is described by the following formula:
The coefficients R, B, F are based on the physical Planck function. The coefficient O describes the signal offset (property of the detector). The determination of these coefficients is part of the factory calibration. The coefficients are found in the GenICam Nodes under the Radiometric Control group in the camera properties.
Tip
The exchange of the lens has an influence on these coefficients. If the lens must be replaced, a recalibration is recommended.

Most IRSX models can store two calibration sets. This allows a replacement of the lens without recalibration. The calibration sets belonging to the lenses can be selected in the GenICam Nodes under the camera property Lens Selector in the group Lens Control. When delivered without a replacement lens, the relevant calibration set is stored under Lens1 as standard. For each calibration set, you can switch between the high and low temperature measurement range using the Temperature Range Selector property.

In the temperature calculation, the external environmental influences such as ambient temperature, must be taken into account. The object temperature can be calculated according to the following formula:

In order to calculate a temperature value from the camera signal, the R, B, F, O parameters are be required. These can be read out of the camera. In addition, the environmental parameters must be known.

Table : Parameters

For the transmission of the atmosphere, 𝜏Atm = 1 can be assumed for short distances. If no protective window is installed, 𝜏Lens = 1 can be used. To calculate the temperature from the signal value, the following parameters must first be calculated.

Calculation of the emissivities:


Calculation of the radiation of the environment (Iamb), of the atmosphere (IAtm) and of the protective window (SAtm):

Calculation of the radiation components (K1, K2):

Calculation of the object signal (SObj):
With the signal SObj and the parameters R, B and F, the object temperature can be calculated in Kelvin.

Temperature Calculation with Camera Temperature Linearization (TLinear)

The IRSX series allows to calculate the output signal directly proportional to the object temperature. There are two levels of accuracy, which differ in their dynamics. The function can be selected in the GenICam Nodes under Radiometric Pixel Format in the group Radiometric Control.

The Figure below shows the selection of temperature linearization with the factor 0.04:

Assuming the signal value in a pixel is 7600, the temperature is calculated as follows:

Temperature in Kelvin

Temperature in Celsius

For measuring temperatures with this method, ambient properties such as emissivity, transmission and temperatures must be set in the camera. You will find these settings in the GenICam Nodes under Radiometric Control.

Emissivity Table


Material

Surface

Temperature [°C]

Emissivity

Aluminum

polished

20

0.04

oxidized, strongly

20

0.83-0.94

Copper

polished

100

0.05

oxidized, strongly

20

0.78

Iron

cast, oxidized

100

0.64

sheet, heavy rusted

20

0.69-0.96

Nickel

polished

20

0.05

Stainless steel (18-8)

polished

20

0.16

oxidized

60

0.85

Steel

polished

100

0.07

oxidized

200

0.79

Brick

red

20

0.93

Carbon


20

0.93

Concrete

dry

35

0.95

Glass

35

0.97

Oil, lubricating


17

0.87

0,03mm film

20

0.27

0,13mm film

20

0.72

Thick coating

20

0.82

Oil paint

Mix from 16 colors

20

0.94

Paper

white

20

0.07-0.90

Plaster


20

0.86-0.90

Rubber

black

20

0.95

Human skin


32

0.98

Soil

dry

20

0.92

saturated with water

20

0.95

Water

distilled

20

0.96

frost crystals

-10

0.98

snow

-10

0.85
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