Infrared Testing - FAQ

What are the wavelength boundaries of infrared radiation?

FAQ

The infrared radiation is the electromagnetic radiation where wavelengths are between 700 nanometres and 1 millimetre. Thus, it is located between the red limit of visible spectrum and the shortest microwaves.

However, taking into account the major applications of thermal sensors, the main considered spectral range is between 1 µm and 50 µm including 3 major sub spectral ranges corresponding to the atmosphere transmission windows:

  • 1 µm to 3 µm or Short Wave Infrared (SWIR) or band I
  • 3 µm to 5 µm or Middle Wave Infrared (MWIR) or band II
  • 8 µm to 14 µm or Long Wave Infrared (LWIR) or band III.

An IR camera is sometimes sensitive to the temperature difference between an object and its background. Consequently, some tests require to simulate an object and its background and to have a simultaneous and accurate measurement of both.

The simulation of an object and its background is made by placing a target in front of the emissive surface of a blackbody.

An infrared target is a thin sheet coated with high emissivity coating with stuck patterns. The object is made by the blackbody seen through the holes and the background is the solid part of the sheet.

Consequently the temperature of the object is the temperature of the blackbody while the temperature of the background is measured by inserting a temperature sensor into the mount of the target.

As some IR cameras specifications depends on the temperature difference between an object and its background, it is necessary to have the object temperature adjusted with respect to the background temperature. A differential blackbody allows this function by adjusting the temperature of the object in real time to a fixed temperature difference (positive or negative) with respect to the floating temperature of the background.

The tests which can be performed on an IR camera using a blackbody can be divided into 4 categories:

  • Correction and calibration tests: thermal calibration of the signal, non-uniformity correction, dynamic range, linearity measurement, etc.
  • Noise measurement: thermal resolution, temporal noise, NETD, fixed pattern noise, spatial noise, NEI, etc.
  • Spatial resolution and geometrical specifications: LSF, MTF, Field of View, IFOV, alignment, magnification, etc.
  • Range evaluation: MRTD, MDTD, TOD, Detection, Recognition, Identification ranges, etc.

 

HGH offers an efficient solution to the test of IR Cameras through the INFRATEST software

The following table is a suggestion of the recommended targets for the usual tests:

Noise tests usually do not require any target.

The NETD (Noise Equivalent Temperature Difference) is the temperature difference between an object and its environment required to generate a variation of the IR camera signal equal to its temporal noise, i.e. its 1-sigma temporal instability. It can be considered as the thermal resolution of an IR camera.

The MTF (Modulation Transfer Function) curve shows the contrast value (between 0 and 1) of a sinusoidal image focused on a camera as a function of the frequency of the image. It gives information about the spatial response of the camera. This curve is usually obtained by the Fourier transform of the Line Spread Function, i.e. the signal response of the cameras to an extremely thin slot.

The MRTD (Minimum Resolvable Temperature Difference) is a standard performance measurement for Thermal Imagers. This measurement leads to the determination of the DRI ranges (Detection, Recognition, Identification ranges) of the infrared camera under test.

The MRTD measurement is performed using:

  • a differential blackbody, as the infrared reference source
  • a four-bar target, as the reference object, positioned in front of the emissive surface of the reference source
  • a collimator projecting the object in front of the camera under test

 

The differential blackbody enables to set a positive or negative temperature difference between the target bars and their background (the emissive surface of the blackbody). The MRTD curve is plotted by determining the minimum temperature difference between the target and the background, required to distinguish the 4 bars on the thermal image of the camera, as a function of the spatial frequency of the 4-bar target.

To perform a fast and accurate MRTD test, patterns of 4-bar targets, with optimized spatial frequencies, can be computed depending on the Field of View and the resolution of the camera, and on the focal length of the collimator. Download our calculation sheet to determine the target pattern suiting your needs.

For more information, do not hesitate to contact our specialists.

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