Infrared cameras are cameras which are sensitive to infrared light. Cameras for different spectral regions are available, which differ substantially in terms of performance (e.g. image resolution, responsivity and frame rate) and application areas. In the following sections, we distinguish near-infrared cameras and mid- or long-wave infrared cameras.
Most infrared cameras have a two-dimensional image sensor (sometimes called a focal plane array) which delivers digital data through some electronic interface, for example of USB, Camera Link or LAN type. However, some special cameras have a line sensor, i.e., only a one-dimensional image sensor; those are often used for continuous imaging of moving items e.g. in production lines and in laser scanners.
Infrared cameras may or may not be sensitive to visible and ultraviolet light. Often, they include an optical filter which transmits only infrared light, so that sensitivity to unwanted wavelengths is avoided.
Typically, infrared cameras do not provide spectral information, but only intensity values for their pixels. This is in contrast to photo cameras, for example. When colorful images from infrared cameras are presented, these usually contain false colors, which only encode intensity values. However, there are also infrared cameras for multispectral imaging or hyperspectral imaging, which typically require a more sophisticated setup, e.g. with dispersive optics and a line scanner.
The usual type of CCD and CMOS image sensors for visible light are based on silicon, and these have some sensitivity up to optical wavelengths somewhere between 1000 nm and 1100 nm – limited by the band gap energy of silicon. Although this is already in the infrared, a real infrared camera often contains a sensor chip based on a indium gallium arsenide (InGaAs), which provides a good responsivity roughly in the wavelength region from 900 nm to 1700 nm. Compared with silicon-based sensors, these are substantially more expensive and typically provide lower resolution – often only a few hundred pixels in the horizontal and vertical direction, i.e., well below one megapixel overall.
Due to the smaller band gap energy of InGaAs, optimum performance in terms of dark current and noise is achieved only at low temperatures; therefore, such as sensor chips are often equipped with a thermoelectric (Peltier) cooler. Unfortunately, that substantially increases the electricity consumption, and the housing often needs to be optimized in terms of heat dissipation, e.g. with cooling fins.
The required imaging optics do not substantially differ from those for visible cameras, since it is not difficult to find optical glasses with high transmittance in that wavelength region. Essentially, one only requires adapted anti-reflection coatings and achromatic lenses.
Near-infrared cameras are often used for inspection purposes. For example, they are used for the inspection of semiconductor wafers, solar cells and various other industrial products, also for agricultural goods like wheat and fruit. Laser beam profilers are another example.
Near-infrared cameras can also provide night vision in conjunction with some infrared illumination. It can be beneficial for surveillance purposes to work only with invisible illumination light, although that might relatively easily be detected. As long as substantial exposure times are acceptable, such cameras can work with rather low infrared light levels.
For thermal imaging around or below room temperature, the near-infrared spectral range is not suitable; for that, one requires mid-infrared cameras (see below), which can register lower-energy photons.
Mid- and Long-wave Infrared Cameras
Mostly for thermal imaging (thermography) applications, mid-infrared cameras are used, which can respond to substantially longer optical wavelengths – sometimes well beyond 10 μm – as are relevant for thermal radiation. It is then possible, for example, to obtain temperature maps of buildings in order to identify locations with excessive heat losses; that must work even at winter temperatures of below 0 °C, where thermal emission is rather low. There is a range of other applications, for example involving medical diagnosis, nondestructive testing, fire detection, satellite-based weather profile monitoring, air pollution monitoring and deforestation mapping, apart from military applications like passive infrared surveillance and heat-seeking missiles.
Spectral regions of special interest are the atmospheric windows at approximately 3 to 5 μm (the mid-wave infrared window, MWIR) and from 8 to 12 μm (long-wave window, LWIR). Here, atmospheric transmission is relatively high, while there is strong infrared absorption in other wavelength regions.
For such long wavelengths, special infrared optics are required. Unfortunately, that substantially contributes to the cost of long-wavelength infrared cameras. The imaging performance of such optics is also usually not great, but that may not matter since the resolution of the required image sensors is anyway quite moderate.
Cooled Infrared Photodetectors
Semiconductor photodetectors for such long wavelengths, corresponding to very low photon energies, have to have a very small bandgap energy. Suitable materials are for example mercury cadmium telluride (HgCdTe, MCT) (suitable even well beyond 10 μm) and indium antimonide (InSb, up to ≈5.5 μm). Similarly, there are focal plane arrays based on quantum well infrared photodetectors (QWIPs). The small bandgap energy also makes them very sensitive to thermal excitation within the sensor itself. Therefore, such infrared detectors often need to be strongly cooled during operation – often to 100 kelvins or even substantially below.
Cooling to the order of 100 K can be done relatively easily with a Stirling cooler, which is essentially a Stirling engine driven with an electric motor. It may take a couple of minutes after switching the device on until the required operation temperature is achieved. The cooled detector must be well insulated against the environment, also for preventing the deposition of ice, and is often placed in a vacuum-sealed case. Of course, the setup is substantially more bulky and expensive compared with that of a camera having only a Peltier cooler.
Their technology with infrared optics, a special long-wavelength image sensor and a cooling arrangement makes cooled infrared cameras quite expensive, but their performance is far better than that of uncooled detectors as described in the following section. The substantial weight, electricity consumption and preparation time are of course practical disadvantages.
For more details, see the article on photoconductive detectors.
Many long-wavelength infrared cameras do not contain a semiconductor detector based on the internal photo effect, but rather a kind of thermal detector, which responds to a temperature increase caused by absorption of incoming infrared light. Such thermal detectors can be based on different technologies:
- Frequently, one uses arrays of very small bolometers (microbolometers), with which some number of pixels (e.g. 160 × 120, 320 × 240, 640 × 480 or 1024 × 768) can be realized on a sensor chip. As the sensing element, each pixel contains a thin infrared-absorbing plate, made e.g. of amorphous silicon (aSi) or vanadium oxide, which is suspended above the chip (with a small air gap between plate and chip) with two electrodes. One can then measure the temperature-dependent electrical resistance of the plate, which decreases with increasing temperature. Note that without incoming infrared light the temperature of the plate will relax towards the substrate temperature, while external radiation will increase the temperature. The readings will thus have to be corrected according to the substrate temperature, if that is not held constant. A metal mirror below the plate may be used to back-reflect non-absorbed infrared light and at the same time to reduce the thermal radiation from the substrate.
- There are pyroelectric materials such as lithium tantalate, generating a small electric voltage in response to a temperature gradient. That temperature gradient results from the heating by incident radiation; the generated heat is conducted to some substrate, and the temperature gradient is proportional to the incident intensity. Such detectors are AC-coupled, i.e., they can be used only to monitor changes, but not constant temperatures.
Such detectors may still be cooled to some extent in order to improve their noise performance, but fundamentally such cooling is not required. Often, they are temperature-stabilized, i.e., the operation temperature is kept constant, typically with a small Peltier cooler, but not at a particularly low temperature.
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