There are many considerations when choosing the operating waveband of a thermal infrared camera.

An important parameter to consider is the estimated temperature range of the object to be measured. The Planck emission curve dictates that solid objects over approximately 150 °C will have their maximum emission in the midwave region of the IR spectrum, with fainter signal in the LW. Conversaly, solid objects closer to room temperature will almost exclusively emit in the longwave region of the IR spectrum, with only faint emissions in the MW region. Nevertheless, a MW camera can still be used for measuring an object close to room temperature with an appropriate exposure time. And in the same way, a LW camera can still be used to measure hot solid targets.

Care must also be given to the spectral requirements of the envisioned application. Objects under measurement can feature varying spectral emission and absorption behaviours (referred to as signature) that can be better matched with a camera’s spectral range. Combustion, for example, shows varying signal across the MW spectral range, and minerals can have varying signature in the LW that can help in distinguishing them. Prior knowledge of the spectral signatures of the target material of interest is essential when choosing the spectral range of an infrared imager.

In general, LW cameras feature a larger dynamic range and are better suited for experiments that involve a large temperature range. They are also well suited for low-smear measurement of fast-moving objects that require shorter exposure time.

Contact a Telops expert if you need help when choosing your infrared camera to make sure it is well-suited for your application.

Typically, infrared cameras are factory-calibrated using high-precision blackbody reference sources to implement a non-uniformity correction (NUC) for improved image quality and a radiometric calibration to relate observed detector response (digital counts) to blackbody temperature for a single exposure time. If the experiment requires temperature measurements at other exposure time values additional calibration data sets must be acquired, a time-consuming and tedious process.

The Telops proprietary permanent radiometric calibration operates its magic by measuring the electron flux generated by the detector (obtained from dividing digital counts by the exposure time) as a function of a blackbody temperature filling the camera’s Field Of View. The flux generated by the detector is independent of the exposure time and as such, this calibration strategy supports a wide range of operating parameters without the need for sporadic or periodic recalibration. All Telops high-speed broadband and multispectral imagers are delivered with this permanent calibration fully implemented and are ready to use from power-on.

With this technique, a Telops camera is permanently calibrated:
- For the whole range of the camera operating temperature;
- For the whole range of target temperature, from – 40 °C to + 2 500 °C;
- For the whole range of exposure time, continuously and without gaps.

This unique calibration allows the user to operate the IR camera with Automatic Exposure Control (AEC). The camera self-adjusts the exposure time of all pixels simultaneously, in real time, to always maximize the signal to noise ratio, without reaching saturation.

A thermal infrared camera measures a quantity called radiometric temperature by interpreting the infrared radiation emitted from the surface of objects within the scene. Each object is modeled as a blackbody with a unitary, spectrally flat emissivity profile that emits radiation only according to its temperature. Real objects do not have a unitary emissivity value and in fact, most materials have spectrally varying emissivity profiles. Additionally, the thermal radiation from objects within the scene entering the camera is modified by the transmission properties of the intervening atmosphere. In order to convert the radiometric temperature measured by an infrared camera to the true thermodynamic temperature of an object, it is necessary to compensate for both the true material emissivity and atmospheric transmission properties.

For this purpose, Telops provides a user-friendly compensation toolbox as part of its standard software suite.