taken in mid-infrared ("thermal") light (
false-color) A
thermographic camera (also called an
infrared camera or
thermal imaging camera,
thermal camera or
thermal imager) is a device that creates an image using
infrared (IR) radiation, similar to a normal
camera that forms an image using
visible light. Instead of the 400–700
nanometre (nm) range of the visible light camera, infrared cameras are sensitive to
wavelengths from about 1,000 nm (1
micrometre or μm) to about 14,000 nm (14 μm). The practice of capturing and analyzing the data they provide is called
thermography. Thermal cameras convert the
energy in the far infrared wavelength into a visible light display. All objects above absolute zero emit thermal infrared energy, so thermal cameras can passively see all objects, regardless of ambient light. However, most thermal cameras are sensitive to objects warmer than . Some
specification parameters of an infrared camera system are number of
pixels,
frame rate,
responsivity,
noise-equivalent power,
noise-equivalent temperature difference (NETD), spectral band, distance-to-spot ratio (D:S), minimum focus distance, sensor lifetime,
minimum resolvable temperature difference (MRTD),
field of view,
dynamic range, input power, and mass and volume. Their resolution is considerably lower than that of optical cameras, often around 160×120 or 320×240 pixels, although more expensive ones can achieve a resolution of 1280×1024 pixels. Thermographic cameras are much more expensive than their visible-spectrum counterparts, though low-performance add-on thermal cameras for
smartphones became available for hundreds of US dollars in 2014.
Types Thermographic cameras can be broadly divided into two types: those with cooled infrared image detectors and those with uncooled detectors.
Cooled infrared detectors , one of the signs of
infection. Cooled detectors are typically contained in a vacuum-sealed case or
Dewar and
cryogenically cooled. Cooling is necessary for the operation of the semiconductor materials used. Typical
operating temperatures range from to just below room temperature, depending on the detector technology. Most modern cooled detectors operate in the 60 Kelvin (K) to 100 K range (−213 to −173 °C), depending on type and performance level. Without cooling, these sensors (which detect and convert light in much the same way as common digital cameras, but are made of different materials) would be 'blinded' or flooded by their own radiation. The drawbacks of cooled infrared cameras are that they are expensive both to produce and to run. Cooling is both energy-intensive and time-consuming. The camera may need several minutes to cool down before it can begin working. The most commonly used cooling systems are
peltier coolers which, although inefficient and limited in cooling capacity, are relatively simple and compact. To obtain better image quality or for imaging low temperature objects
Stirling cryocoolers are needed. Although the cooling apparatus may be comparatively bulky and expensive, cooled infrared cameras provide greatly superior image quality compared to uncooled ones, particularly of objects near or below room temperature. Additionally, the greater sensitivity of cooled cameras also allow the use of higher
F-number lenses, making high performance long focal length lenses both smaller and cheaper for cooled detectors. An alternative to Stirling coolers is to use gases bottled at high pressure, nitrogen being a common choice. The pressurised gas is expanded via a micro-sized orifice and passed over a miniature heat exchanger resulting in regenerative cooling via the
Joule–Thomson effect. For such systems the supply of pressurized gas is a logistical concern for field use. Materials used for cooled infrared detection include
photodetectors based on a wide range of
narrow gap semiconductors including
indium antimonide (3–5 μm),
indium arsenide,
mercury cadmium telluride (MCT) (1–2 μm, 3–5 μm, 8–12 μm),
lead sulfide, and
lead selenide. Infrared photodetectors can also be created with structures of high bandgap semiconductors such as in
quantum well infrared photodetectors. Cooled bolometer technologies can be superconducting or non-superconducting. Superconducting detectors offer extreme sensitivity, with some able to register individual photons. For example,
ESA's
Superconducting camera (SCAM). However, they are not in regular use outside of scientific research. In principle,
superconducting tunneling junction devices could be used as infrared sensors because of their very narrow gap. Small arrays have been demonstrated, but they have not been broadly adopted for use because their high sensitivity requires careful shielding from background radiation.
Uncooled infrared detectors Uncooled thermal cameras use a sensor operating at ambient temperature, or a sensor stabilized at a temperature close to ambient using small temperature control elements. Modern uncooled detectors all use sensors that work by the change of
resistance,
voltage or
current when heated by infrared radiation. These changes are then measured and compared to the values at the operating temperature of the sensor. In uncooled detectors the temperature differences at the sensor pixels are minute; a 1 °C difference at the scene induces just a 0.03 °C difference at the sensor. The pixel response time is also fairly slow, at the range of tens of milliseconds. Uncooled infrared sensors can be stabilized to an operating temperature to reduce image noise, but they are not cooled to low temperatures and do not require bulky, expensive, energy consuming cryogenic coolers. This makes infrared cameras smaller and less costly. However, their resolution and image quality tend to be lower than cooled detectors. This is due to differences in their fabrication processes, limited by currently available technology. An uncooled thermal camera also needs to deal with its own heat signature. Uncooled detectors are mostly based on
pyroelectric and
ferroelectric materials or
microbolometer technology. The material are used to form pixels with highly temperature-dependent properties, which are thermally insulated from the environment and read electronically. Ferroelectric detectors operate close to
phase transition temperature of the sensor material; the pixel temperature is read as the highly temperature-dependent polarization charge. The achieved
NETD of ferroelectric detectors with
f/1 optics and 320×240 sensors is 70–80 mK. A possible sensor assembly consists of barium strontium titanate bump-bonded by
polyimide thermally insulated connection. Silicon microbolometers can reach NETD down to 20 mK. They consist of a layer of
amorphous silicon, or a thin film
vanadium(V) oxide sensing element suspended on
silicon nitride bridge above the silicon-based scanning electronics. The electric resistance of the sensing element is measured once per frame. Current improvements of uncooled focal plane arrays (UFPA) are focused primarily on higher sensitivity and pixel density. In 2013
DARPA announced a five-micron LWIR camera that uses a 1280 × 720 focal plane array (FPA). Some of the materials used for the
sensor arrays are
amorphous silicon (a-Si),
vanadium(V) oxide (VOx), lanthanum barium manganite (LBMO),
lead zirconate titanate (PZT),
lanthanum doped lead zirconate titanate (PLZT),
lead scandium tantalate (PST), lead lanthanum titanate (PLT),
lead titanate (PT), lead zinc niobate (PZN), lead strontium titanate (PSrT),
barium strontium titanate (BST),
barium titanate (BT), antimony sulfoiodide (SbSI), and
polyvinylidene difluoride (PVDF).
CCD and CMOS thermography Non-specialized
charge-coupled device (CCD) and
CMOS sensors have most of their spectral sensitivity in the visible light wavelength range. However, by utilizing the "trailing" area of their spectral sensitivity, namely the part of the infrared spectrum called
near-infrared (NIR), and by using off-the-shelf CCTV camera it is possible under certain circumstances to obtain true thermal images of objects with temperatures at about and higher. At temperatures of 600 °C and above, inexpensive cameras with CCD and CMOS sensors have also been used for pyrometry in the visible spectrum. They have been used for soot in flames, burning coal particles, heated materials,
SiC filaments, and smoldering embers. This pyrometry has been performed using external filters or only the sensor's
Bayer filters. It has been performed using color ratios, grayscales, and/or a hybrid of both.
Infrared films Infrared (IR) film is sensitive to
black-body radiation in the range, while the range of thermography is approximately . So, for an IR film to work thermographically, the measured object must be over or be reflecting infrared radiation from something that is at least that hot.
Comparison with night-vision devices Starlight-type
night-vision devices generally only magnify
ambient light and are not thermal imagers. Some infrared cameras marketed as night vision are sensitive to near-infrared just beyond the visual spectrum, and can see emitted or reflected near-infrared in complete visual darkness. However, these are not usually used for thermography due to the high equivalent
black-body temperature required, but are instead used with active near-IR illumination sources. ==Passive vs. active thermography==