# Infrared

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Infrared (IR), sometimes called infrared light, is electromagnetic radiation (EMR) with wavelengths longer than those of visible light. It is therefore generally invisible to the human eye, although IR at wavelengths up to 1050  nanometers (nm)s from specially pulsed lasers can be seen by humans under certain conditions. [1] [2] [3] [4] IR wavelengths extend from the nominal red edge of the visible spectrum at 700  nanometers (frequency 430  THz), to 1  millimeter (300  GHz). [5] Most of the thermal radiation emitted by objects near room temperature is infrared. As with all EMR, IR carries radiant energy and behaves both like a wave and like its quantum particle, the photon.

## Contents

Infrared radiation was discovered in 1800 by astronomer Sir William Herschel, who discovered a type of invisible radiation in the spectrum lower in energy than red light, by means of its effect on a thermometer. [6] Slightly more than half of the total energy from the Sun was eventually found[ when? ] to arrive on Earth in the form of infrared. The balance between absorbed and emitted infrared radiation has a critical effect on Earth's climate.

Infrared radiation is emitted or absorbed by molecules when they change their rotational-vibrational movements. It excites vibrational modes in a molecule through a change in the dipole moment, making it a useful frequency range for study of these energy states for molecules of the proper symmetry. Infrared spectroscopy examines absorption and transmission of photons in the infrared range. [7]

Infrared radiation is used in industrial, scientific, military, law enforcement, and medical applications. Night-vision devices using active near-infrared illumination allow people or animals to be observed without the observer being detected. Infrared astronomy uses sensor-equipped telescopes to penetrate dusty regions of space such as molecular clouds, detect objects such as planets, and to view highly red-shifted objects from the early days of the universe. [8] Infrared thermal-imaging cameras are used to detect heat loss in insulated systems, to observe changing blood flow in the skin, and to detect overheating of electrical apparatus. [9]

Extensive uses for military and civilian applications include target acquisition, surveillance, night vision, homing, and tracking. Humans at normal body temperature radiate chiefly at wavelengths around 10 μm (micrometers). Non-military uses include thermal efficiency analysis, environmental monitoring, industrial facility inspections, detection of grow-ops, remote temperature sensing, short-range wireless communication, spectroscopy, and weather forecasting.

## Definition and relationship to the electromagnetic spectrum

Infrared radiation extends from the nominal red edge of the visible spectrum at 700 nanometers (nm) to 1 millimeter (mm). This range of wavelengths corresponds to a frequency range of approximately 430  THz down to 300  GHz. Below infrared is the microwave portion of the electromagnetic spectrum.

Name Wavelength Frequency (Hz) Photon energy (eV) Light comparison [10] Gamma ray less than 0.01 nm more than 30 EHz more than 124 keV X-ray 0.01 nm – 10 nm 30 EHz – 30 PHz 124 keV – 124 eV Ultraviolet 10 nm – 400 nm 30 PHz – 790 THz 124 eV – 3.3 eV Visible 400 nm–700 nm 790 THz – 430 THz 3.3 eV – 1.7 eV Infrared 700 nm – 1 mm 430 THz – 300 GHz 1.7 eV – 1.24 meV Microwave 1 mm – 1 meter 300 GHz – 300 MHz 1.24 meV – 1.24 μeV Radio 1 meter – 100,000 km 300 MHz – 3 Hz 1.24 μeV – 12.4 feV

## Natural infrared

Sunlight, at an effective temperature of 5780  kelvins (5510 °C, 9940 °F), is composed of near-thermal-spectrum radiation that is slightly more than half infrared. At zenith, sunlight provides an irradiance of just over 1  kilowatt per square meter at sea level. Of this energy, 527 watts is infrared radiation, 445 watts is visible light, and 32 watts is ultraviolet radiation. [11] Nearly all the infrared radiation in sunlight is near infrared, shorter than 4 micrometers.

On the surface of Earth, at far lower temperatures than the surface of the Sun, some thermal radiation consists of infrared in the mid-infrared region, much longer than in sunlight. However, black-body, or thermal, radiation is continuous: it gives off radiation at all wavelengths. Of these natural thermal radiation processes, only lightning and natural fires are hot enough to produce much visible energy, and fires produce far more infrared than visible-light energy. [12]

## Regions within the infrared

In general, objects emit infrared radiation across a spectrum of wavelengths, but sometimes only a limited region of the spectrum is of interest because sensors usually collect radiation only within a specific bandwidth. Thermal infrared radiation also has a maximum emission wavelength, which is inversely proportional to the absolute temperature of object, in accordance with Wien's displacement law.

Therefore, the infrared band is often subdivided into smaller sections.

### Commonly used sub-division scheme

A commonly used sub-division scheme is: [13]

Division nameAbbreviationWavelengthFrequencyPhoton energyTemperature [lower-roman 1] Characteristics
Near-infraredNIR, IR-A DIN 0.75–1.4  μm 214–400  THz 886–1653  meV 3,864–2,070  K
(3,591–1,797  °C )
Defined by water absorption,[ clarification needed ] and commonly used in fiber optic telecommunication because of low attenuation losses in the SiO2 glass (silica) medium. Image intensifiers are sensitive to this area of the spectrum; examples include night vision devices such as night vision goggles. Near-infrared spectroscopy is another common application.
Short-wavelength infraredSWIR, IR-B DIN1.4–3 μm100–214 THz413–886 meV2,070–966  K
(1,797–693  °C )
Water absorption increases significantly at 1450 nm. The 1530 to 1560 nm range is the dominant spectral region for long-distance telecommunications.
Mid-wavelength infraredMWIR, IR-C DIN; MidIR. [15] Also called intermediate infrared (IIR)3–8 μm37–100 THz155–413 meV966–362  K
(693–89  °C )
In guided missile technology the 3–5 μm portion of this band is the atmospheric window in which the homing heads of passive IR 'heat seeking' missiles are designed to work, homing on to the Infrared signature of the target aircraft, typically the jet engine exhaust plume. This region is also known as thermal infrared.
Long-wavelength infraredLWIR, IR-C DIN8–15 μm20–37 THz83–155 meV362–193  K
(89 – −80  °C )
The "thermal imaging" region, in which sensors can obtain a completely passive image of objects only slightly higher in temperature than room temperature - for example, the human body - based on thermal emissions only and requiring no illumination such as the sun, moon, or infrared illuminator. This region is also called the "thermal infrared".
Far infrared FIR15–1000 μm0.3–20 THz1.2–83 meV193–3  K
(−80.15 – −270.15  °C )
A comparison of a thermal image (top) and an ordinary photograph (bottom). The plastic bag is mostly transparent to long-wavelength infrared, but the man's glasses are opaque.

NIR and SWIR is sometimes called "reflected infrared", whereas MWIR and LWIR is sometimes referred to as "thermal infrared". Due to the nature of the blackbody radiation curves, typical "hot" objects, such as exhaust pipes, often appear brighter in the MW compared to the same object viewed in the LW.

### CIE division scheme

The International Commission on Illumination (CIE) recommended the division of infrared radiation into the following three bands: [16]

AbbreviationWavelengthFrequency
IR-A700 nm – 1400 nm
(0.7 μm – 1.4 μm)
215 THz – 430 THz
IR-B1400 nm – 3000 nm
(1.4 μm – 3 μm)
100 THz – 215 THz
IR-C3000 nm – 1 mm
(3 μm – 1000 μm)
300 GHz – 100 THz

### ISO 20473 scheme

ISO 20473 specifies the following scheme: [17]

DesignationAbbreviationWavelength
Near-InfraredNIR0.78–3 μm
Mid-InfraredMIR3–50 μm
Far-InfraredFIR50–1000 μm

### Astronomy division scheme

Astronomers typically divide the infrared spectrum as follows: [18]

DesignationAbbreviationWavelength
Near-InfraredNIR(0.7–1) to 5 μm
Mid-InfraredMIR5 to (25–40) μm
Far-InfraredFIR(25–40) to (200–350) μm.

These divisions are not precise and can vary depending on the publication. The three regions are used for observation of different temperature ranges, and hence different environments in space.

The most common photometric system used in astronomy allocates capital letters to different spectral regions according to filters used; I, J, H, and K cover the near-infrared wavelengths; L, M, N, and Q refer to the mid-infrared region. These letters are commonly understood in reference to atmospheric windows and appear, for instance, in the titles of many papers.

### Sensor response division scheme

A third scheme divides up the band based on the response of various detectors: [19]

• Near-infrared: from 0.7 to 1.0 μm (from the approximate end of the response of the human eye to that of silicon).
• Short-wave infrared: 1.0 to 3 μm (from the cut-off of silicon to that of the MWIR atmospheric window). InGaAs covers to about 1.8 μm; the less sensitive lead salts cover this region.
• Mid-wave infrared: 3 to 5 μm (defined by the atmospheric window and covered by indium antimonide [InSb] and mercury cadmium telluride [HgCdTe] and partially by lead selenide [PbSe]).
• Long-wave infrared: 8 to 12, or 7 to 14 μm (this is the atmospheric window covered by HgCdTe and microbolometers).
• Very-long wave infrared (VLWIR) (12 to about 30 μm, covered by doped silicon).

Near-infrared is the region closest in wavelength to the radiation detectable by the human eye. mid- and far-infrared are progressively further from the visible spectrum. Other definitions follow different physical mechanisms (emission peaks, vs. bands, water absorption) and the newest follow technical reasons (the common silicon detectors are sensitive to about 1,050 nm, while InGaAs's sensitivity starts around 950 nm and ends between 1,700 and 2,600 nm, depending on the specific configuration). No international standards for these specifications are currently available.

The onset of infrared is defined (according to different standards) at various values typically between 700 nm and 800 nm, but the boundary between visible and infrared light is not precisely defined. The human eye is markedly less sensitive to light above 700 nm wavelength, so longer wavelengths make insignificant contributions to scenes illuminated by common light sources. However, particularly intense near-IR light (e.g., from IR lasers, IR LED sources, or from bright daylight with the visible light removed by colored gels) can be detected up to approximately 780 nm, and will be perceived as red light. Intense light sources providing wavelengths as long as 1050 nm can be seen as a dull red glow, causing some difficulty in near-IR illumination of scenes in the dark (usually this practical problem is solved by indirect illumination). Leaves are particularly bright in the near IR, and if all visible light leaks from around an IR-filter are blocked, and the eye is given a moment to adjust to the extremely dim image coming through a visually opaque IR-passing photographic filter, it is possible to see the Wood effect that consists of IR-glowing foliage. [20]

### Telecommunication bands in the infrared

In optical communications, the part of the infrared spectrum that is used is divided into seven bands based on availability of light sources transmitting/absorbing materials (fibers) and detectors: [21]

BandDescriptorWavelength range
O bandOriginal1260–1360 nm
E bandExtended1360–1460 nm
S bandShort wavelength1460–1530 nm
C band Conventional1530–1565 nm
L bandLong wavelength1565–1625 nm
U bandUltralong wavelength1625–1675 nm

The C-band is the dominant band for long-distance telecommunication networks. The S and L bands are based on less well established technology, and are not as widely deployed.

## Heat

Infrared radiation is popularly known as "heat radiation", [22] but light and electromagnetic waves of any frequency will heat surfaces that absorb them. Infrared light from the Sun accounts for 49% [23] of the heating of Earth, with the rest being caused by visible light that is absorbed then re-radiated at longer wavelengths. Visible light or ultraviolet-emitting lasers can char paper and incandescently hot objects emit visible radiation. Objects at room temperature will emit radiation concentrated mostly in the 8 to 25 μm band, but this is not distinct from the emission of visible light by incandescent objects and ultraviolet by even hotter objects (see black body and Wien's displacement law). [24]

Heat is energy in transit that flows due to a temperature difference. Unlike heat transmitted by thermal conduction or thermal convection, thermal radiation can propagate through a vacuum. Thermal radiation is characterized by a particular spectrum of many wavelengths that are associated with emission from an object, due to the vibration of its molecules at a given temperature. Thermal radiation can be emitted from objects at any wavelength, and at very high temperatures such radiation is associated with spectra far above the infrared, extending into visible, ultraviolet, and even X-ray regions (e.g. the solar corona). Thus, the popular association of infrared radiation with thermal radiation is only a coincidence based on typical (comparatively low) temperatures often found near the surface of planet Earth.

The concept of emissivity is important in understanding the infrared emissions of objects. This is a property of a surface that describes how its thermal emissions deviate from the idea of a black body. To further explain, two objects at the same physical temperature may not show the same infrared image if they have differing emissivity. For example, for any pre-set emissivity value, objects with higher emissivity will appear hotter, and those with a lower emissivity will appear cooler (assuming, as is often the case, that the surrounding environment is cooler than the objects being viewed). When an object has less than perfect emissivity, it obtains properties of reflectivity and/or transparency, and so the temperature of the surrounding environment is partially reflected by and/or transmitted through the object. If the object were in a hotter environment, then a lower emissivity object at the same temperature would likely appear to be hotter than a more emissive one. For that reason, incorrect selection of emissivity and not accounting for environmental temperatures will give inaccurate results when using infrared cameras and pyrometers.

## Applications

### Night vision

Infrared is used in night vision equipment when there is insufficient visible light to see. [25] Night vision devices operate through a process involving the conversion of ambient light photons into electrons that are then amplified by a chemical and electrical process and then converted back into visible light. [25] Infrared light sources can be used to augment the available ambient light for conversion by night vision devices, increasing in-the-dark visibility without actually using a visible light source. [25]

The use of infrared light and night vision devices should not be confused with thermal imaging, which creates images based on differences in surface temperature by detecting infrared radiation (heat) that emanates from objects and their surrounding environment. [26]

### Thermography

Infrared radiation can be used to remotely determine the temperature of objects (if the emissivity is known). This is termed thermography, or in the case of very hot objects in the NIR or visible it is termed pyrometry. Thermography (thermal imaging) is mainly used in military and industrial applications but the technology is reaching the public market in the form of infrared cameras on cars due to greatly reduced production costs.

Thermographic cameras detect radiation in the infrared range of the electromagnetic spectrum (roughly 900–14,000 nanometers or 0.9–14 μm) and produce images of that radiation. Since infrared radiation is emitted by all objects based on their temperatures, according to the black-body radiation law, thermography makes it possible to "see" one's environment with or without visible illumination. The amount of radiation emitted by an object increases with temperature, therefore thermography allows one to see variations in temperature (hence the name).

### Hyperspectral imaging

A hyperspectral image is a "picture" containing continuous spectrum through a wide spectral range at each pixel. Hyperspectral imaging is gaining importance in the field of applied spectroscopy particularly with NIR, SWIR, MWIR, and LWIR spectral regions. Typical applications include biological, mineralogical, defence, and industrial measurements.

Thermal infrared hyperspectral imaging can be similarly performed using a thermographic camera, with the fundamental difference that each pixel contains a full LWIR spectrum. Consequently, chemical identification of the object can be performed without a need for an external light source such as the Sun or the Moon. Such cameras are typically applied for geological measurements, outdoor surveillance and UAV applications. [28]

### Other imaging

In infrared photography, infrared filters are used to capture the near-infrared spectrum. Digital cameras often use infrared blockers. Cheaper digital cameras and camera phones have less effective filters and can "see" intense near-infrared, appearing as a bright purple-white color. This is especially pronounced when taking pictures of subjects near IR-bright areas (such as near a lamp), where the resulting infrared interference can wash out the image. There is also a technique called 'T-ray' imaging, which is imaging using far-infrared or terahertz radiation. Lack of bright sources can make terahertz photography more challenging than most other infrared imaging techniques. Recently T-ray imaging has been of considerable interest due to a number of new developments such as terahertz time-domain spectroscopy.

### Tracking

Infrared tracking, also known as infrared homing, refers to a passive missile guidance system, which uses the emission from a target of electromagnetic radiation in the infrared part of the spectrum to track it. Missiles that use infrared seeking are often referred to as "heat-seekers" since infrared (IR) is just below the visible spectrum of light in frequency and is radiated strongly by hot bodies. Many objects such as people, vehicle engines, and aircraft generate and retain heat, and as such, are especially visible in the infrared wavelengths of light compared to objects in the background. [29]

### Heating

Infrared radiation can be used as a deliberate heating source. For example, it is used in infrared saunas to heat the occupants. It may also be used in other heating applications, such as to remove ice from the wings of aircraft (de-icing). [30] Infrared can be used in cooking and heating food as it predominantly heats the opaque, absorbent objects, rather than the air around them.

Infrared heating is also becoming more popular in industrial manufacturing processes, e.g. curing of coatings, forming of plastics, annealing, plastic welding, and print drying. In these applications, infrared heaters replace convection ovens and contact heating.

Efficiency is achieved by matching the wavelength of the infrared heater to the absorption characteristics of the material.

### Cooling

A variety of technologies or proposed technologies take advantage of infrared emissions to cool buildings or other systems. The LWIR (8–15 μm) region is especially useful since some radiation at these wavelengths can escape into space through the atmosphere.

### Communications

IR data transmission is also employed in short-range communication among computer peripherals and personal digital assistants. These devices usually conform to standards published by IrDA, the Infrared Data Association. Remote controls and IrDA devices use infrared light-emitting diodes (LEDs) to emit infrared radiation that is focused by a plastic lens into a narrow beam. The beam is modulated, i.e. switched on and off, to prevent interference from other sources of infrared (like sunlight or artificial lighting). The receiver uses a silicon photodiode to convert the infrared radiation to an electric current. It responds only to the rapidly pulsing signal created by the transmitter, and filters out slowly changing infrared radiation from ambient light. Infrared communications are useful for indoor use in areas of high population density. IR does not penetrate walls and so does not interfere with other devices in adjoining rooms. Infrared is the most common way for remote controls to command appliances. Infrared remote control protocols like RC-5, SIRC, are used to communicate with infrared.

Free space optical communication using infrared lasers can be a relatively inexpensive way to install a communications link in an urban area operating at up to 4 gigabit/s, compared to the cost of burying fiber optic cable, except for the radiation damage. "Since the eye cannot detect IR, blinking or closing the eyes to help prevent or reduce damage may not happen." [31]

Infrared lasers are used to provide the light for optical fiber communications systems. Infrared light with a wavelength around 1,330 nm (least dispersion) or 1,550 nm (best transmission) are the best choices for standard silica fibers.

IR data transmission of encoded audio versions of printed signs is being researched as an aid for visually impaired people through the RIAS (Remote Infrared Audible Signage) project. Transmitting IR data from one device to another is sometimes referred to as beaming.

### Spectroscopy

Infrared vibrational spectroscopy (see also near-infrared spectroscopy) is a technique that can be used to identify molecules by analysis of their constituent bonds. Each chemical bond in a molecule vibrates at a frequency characteristic of that bond. A group of atoms in a molecule (e.g., CH2) may have multiple modes of oscillation caused by the stretching and bending motions of the group as a whole. If an oscillation leads to a change in dipole in the molecule then it will absorb a photon that has the same frequency. The vibrational frequencies of most molecules correspond to the frequencies of infrared light. Typically, the technique is used to study organic compounds using light radiation from 4000–400 cm−1, the mid-infrared. A spectrum of all the frequencies of absorption in a sample is recorded. This can be used to gain information about the sample composition in terms of chemical groups present and also its purity (for example, a wet sample will show a broad O-H absorption around 3200 cm−1). The unit for expressing radiation in this application, cm−1, is the spectroscopic wavenumber. It is the frequency divided by the speed of light in vacuum.

### Thin film metrology

In the semiconductor industry, infrared light can be used to characterize materials such as thin films and periodic trench structures. By measuring the reflectance of light from the surface of a semiconductor wafer, the index of refraction (n) and the extinction Coefficient (k) can be determined via the Forouhi-Bloomer dispersion equations. The reflectance from the infrared light can also be used to determine the critical dimension, depth, and sidewall angle of high aspect ratio trench structures.

### Meteorology

Weather satellites equipped with scanning radiometers produce thermal or infrared images, which can then enable a trained analyst to determine cloud heights and types, to calculate land and surface water temperatures, and to locate ocean surface features. The scanning is typically in the range 10.3–12.5 μm (IR4 and IR5 channels).

High, cold ice clouds such as cirrus or cumulonimbus show up bright white, lower warmer clouds such as stratus or stratocumulus show up as grey, with intermediate clouds shaded accordingly. Hot land surfaces will show up as dark-grey or black. One disadvantage of infrared imagery is that low cloud such as stratus or fog can have a temperature similar to the surrounding land or sea surface and does not show up. However, using the difference in brightness of the IR4 channel (10.3–11.5 μm) and the near-infrared channel (1.58–1.64 μm), low cloud can be distinguished, producing a fog satellite picture. The main advantage of infrared is that images can be produced at night, allowing a continuous sequence of weather to be studied.

These infrared pictures can depict ocean eddies or vortices and map currents such as the Gulf Stream, which are valuable to the shipping industry. Fishermen and farmers are interested in knowing land and water temperatures to protect their crops against frost or increase their catch from the sea. Even El Niño phenomena can be spotted. Using color-digitized techniques, the gray-shaded thermal images can be converted to color for easier identification of desired information.

The main water vapour channel at 6.40 to 7.08 μm can be imaged by some weather satellites and shows the amount of moisture in the atmosphere.

### Climatology

In the field of climatology, atmospheric infrared radiation is monitored to detect trends in the energy exchange between the earth and the atmosphere. These trends provide information on long-term changes in Earth's climate. It is one of the primary parameters studied in research into global warming, together with solar radiation.

A pyrgeometer is utilized in this field of research to perform continuous outdoor measurements. This is a broadband infrared radiometer with sensitivity for infrared radiation between approximately 4.5 μm and 50 μm.

### Astronomy

Astronomers observe objects in the infrared portion of the electromagnetic spectrum using optical components, including mirrors, lenses and solid state digital detectors. For this reason it is classified as part of optical astronomy. To form an image, the components of an infrared telescope need to be carefully shielded from heat sources, and the detectors are chilled using liquid helium.

The sensitivity of Earth-based infrared telescopes is significantly limited by water vapor in the atmosphere, which absorbs a portion of the infrared radiation arriving from space outside of selected atmospheric windows. This limitation can be partially alleviated by placing the telescope observatory at a high altitude, or by carrying the telescope aloft with a balloon or an aircraft. Space telescopes do not suffer from this handicap, and so outer space is considered the ideal location for infrared astronomy.

The infrared portion of the spectrum has several useful benefits for astronomers. Cold, dark molecular clouds of gas and dust in our galaxy will glow with radiated heat as they are irradiated by imbedded stars. Infrared can also be used to detect protostars before they begin to emit visible light. Stars emit a smaller portion of their energy in the infrared spectrum, so nearby cool objects such as planets can be more readily detected. (In the visible light spectrum, the glare from the star will drown out the reflected light from a planet.)

Infrared light is also useful for observing the cores of active galaxies, which are often cloaked in gas and dust. Distant galaxies with a high redshift will have the peak portion of their spectrum shifted toward longer wavelengths, so they are more readily observed in the infrared. [8]

### Infrared cleaning

Infrared cleaning is a technique used by some motion picture film scanners, film scanners and flatbed scanners to reduce or remove the effect of dust and scratches upon the finished scan. It works by collecting an additional infrared channel from the scan at the same position and resolution as the three visible color channels (red, green, and blue). The infrared channel, in combination with the other channels, is used to detect the location of scratches and dust. Once located, those defects can be corrected by scaling or replaced by inpainting. [32]

### Art conservation and analysis

Infrared reflectography [33] can be applied to paintings to reveal underlying layers in a non-destructive manner, in particular the artist's underdrawing or outline drawn as a guide. Art conservators use the technique to examine how the visible layers of paint differ from the underdrawing or layers in between (such alterations are called pentimenti when made by the original artist). This is very useful information in deciding whether a painting is the prime version by the original artist or a copy, and whether it has been altered by over-enthusiastic restoration work. In general, the more pentimenti, the more likely a painting is to be the prime version. It also gives useful insights into working practices. [34] Reflectography often reveals the artist's use of carbon black, which shows up well in reflectograms, as long as it has not also been used in the ground underlying the whole painting.

Recent progress in the design of infrared-sensitive cameras makes it possible to discover and depict not only underpaintings and pentimenti, but entire paintings that were later overpainted by the artist. [35] Notable examples are Picasso's Woman Ironing and Blue Room , where in both cases a portrait of a man has been made visible under the painting as it is known today.

Similar uses of infrared are made by conservators and scientists on various types of objects, especially very old written documents such as the Dead Sea Scrolls, the Roman works in the Villa of the Papyri, and the Silk Road texts found in the Dunhuang Caves. [36] Carbon black used in ink can show up extremely well.

### Biological systems

The pit viper has a pair of infrared sensory pits on its head. There is uncertainty regarding the exact thermal sensitivity of this biological infrared detection system. [37] [38]

Other organisms that have thermoreceptive organs are pythons (family Pythonidae), some boas (family Boidae), the Common Vampire Bat (Desmodus rotundus), a variety of jewel beetles ( Melanophila acuminata ), [39] darkly pigmented butterflies ( Pachliopta aristolochiae and Troides rhadamantus plateni ), and possibly blood-sucking bugs ( Triatoma infestans ). [40]

Some fungi like Venturia inaequalis require near-infrared light for ejection [41]

Although near-infrared vision (780–1000 nm) has long been deemed impossible due to noise in visual pigments, [42] sensation of near-infrared light was reported in the common carp and in three cichlid species. [42] [43] [44] [45] [46] Fish use NIR to capture prey [42] and for phototactic swimming orientation. [46] NIR sensation in fish may be relevant under poor lighting conditions during twilight [42] and in turbid surface waters. [46]

### Photobiomodulation

Near-infrared light, or photobiomodulation, is used for treatment of chemotherapy-induced oral ulceration as well as wound healing. There is some work relating to anti-herpes virus treatment. [47] Research projects include work on central nervous system healing effects via cytochrome c oxidase upregulation and other possible mechanisms. [48]

### Health hazards

Strong infrared radiation in certain industry high-heat settings may be hazardous to the eyes, resulting in damage or blindness to the user. Since the radiation is invisible, special IR-proof goggles must be worn in such places. [49]

## History of infrared science

The discovery of infrared radiation is ascribed to William Herschel, the astronomer, in the early 19th century. Herschel published his results in 1800 before the Royal Society of London. Herschel used a prism to refract light from the sun and detected the infrared, beyond the red part of the spectrum, through an increase in the temperature recorded on a thermometer. He was surprised at the result and called them "Calorific Rays". [50] [51] The term "infrared" did not appear until late 19th century. [52]

Other important dates include: [19]

## Notes

1. Temperatures of black bodies for which spectral peaks fall at the given wavelengths, according to Wien's displacement law [14]

## Related Research Articles

The electromagnetic spectrum is the range of frequencies of electromagnetic radiation and their respective wavelengths and photon energies.

In physics, radiation is the emission or transmission of energy in the form of waves or particles through space or through a material medium. This includes:

Wien's displacement law states that the black-body radiation curve for different temperatures will peak at different wavelengths that are inversely proportional to the temperature. The shift of that peak is a direct consequence of the Planck radiation law, which describes the spectral brightness of black-body radiation as a function of wavelength at any given temperature. However, it had been discovered by Wilhelm Wien several years before Max Planck developed that more general equation, and describes the entire shift of the spectrum of black-body radiation toward shorter wavelengths as temperature increases.

Forward-looking infrared (FLIR) cameras, typically used on military and civilian aircraft, use a thermographic camera that senses infrared radiation.

Thermal radiation is electromagnetic radiation generated by the thermal motion of particles in matter. All matter with a temperature greater than absolute zero emits thermal radiation. Particle motion results in charge-acceleration or dipole oscillation which produces electromagnetic radiation.

A thermographic camera is a device that creates an image using infrared radiation, similar to a common camera that forms an image using visible light. Instead of the 400–700 nanometre range of the visible light camera, infrared cameras are sensitive to wavelengths from about 1,000 nm (1 μm) to about 14,000 nm (14 μm). The practice of capturing and analyzing the data they provide is called thermography.

Infrared thermography (IRT), thermal imaging, and thermal video are examples of infrared imaging science. Thermographic cameras usually detect radiation in the long-infrared range of the electromagnetic spectrum and produce images of that radiation, called thermograms. Since infrared radiation is emitted by all objects with a temperature above absolute zero according to the black body radiation law, thermography makes it possible to see one's environment with or without visible illumination. The amount of radiation emitted by an object increases with temperature; therefore, thermography allows one to see variations in temperature. When viewed through a thermal imaging camera, warm objects stand out well against cooler backgrounds; humans and other warm-blooded animals become easily visible against the environment, day or night. As a result, thermography is particularly useful to the military and other users of surveillance cameras.

Black-body radiation is the thermal electromagnetic radiation within or surrounding a body in thermodynamic equilibrium with its environment, emitted by a black body. It has a specific spectrum of wavelengths, inversely related to intensity that depend only on the body's temperature, which is assumed for the sake of calculations and theory to be uniform and constant.

The emissivity of the surface of a material is its effectiveness in emitting energy as thermal radiation. Thermal radiation is electromagnetic radiation that may include both visible radiation (light) and infrared radiation, which is not visible to human eyes. The thermal radiation from very hot objects is easily visible to the eye. Quantitatively, emissivity is the ratio of the thermal radiation from a surface to the radiation from an ideal black surface at the same temperature as given by the Stefan–Boltzmann law. The ratio varies from 0 to 1. The surface of a perfect black body emits thermal radiation at the rate of approximately 448 watts per square metre at room temperature ; all real objects have emissivities less than 1.0, and emit radiation at correspondingly lower rates.

Many ceramic materials, both glassy and crystalline, have found use as optically transparent materials in various forms from bulk solid-state components to high surface area forms such as thin films, coatings, and fibers. Such devices have found widespread use for various applications in the electro-optical field including: optical fibers for guided lightwave transmission, optical switches, laser amplifiers and lenses, hosts for solid-state lasers and optical window materials for gas lasers, and infrared (IR) heat seeking devices for missile guidance systems and IR night vision.

Far infrared (FIR) is a region in the infrared spectrum of electromagnetic radiation. Far infrared is often defined as any radiation with a wavelength of 15 micrometers (μm) to 1 mm, which places far infrared radiation within the CIE IR-B and IR-C bands. The long-wave side of the FIR spectrum overlaps with so named terahertz radiation. Different sources use different boundaries for the far infrared; for example, astronomers sometimes define far infrared as wavelengths between 25 μm and 350 μm.

A multispectral image is one that captures image data within specific wavelength ranges across the electromagnetic spectrum. The wavelengths may be separated by filters or detected via the use of instruments that are sensitive to particular wavelengths, including light from frequencies beyond the visible light range, i.e. infrared and ultra-violet. Spectral imaging can allow extraction of additional information the human eye fails to capture with its visible receptors for red, green and blue. It was originally developed for military target identification and reconnaissance. Early space-based imaging platforms incorporated multispectral imaging technology to map details of the Earth related to coastal boundaries, vegetation, and landforms. Multispectral imaging has also found use in document and painting analysis.4

A passive infrared sensor is an electronic sensor that measures infrared (IR) light radiating from objects in its field of view. They are most often used in PIR-based motion detectors. PIR sensors are commonly used in security alarms and automatic lighting applications.

Ultraviolet photography is a photographic process of recording images by using light from the ultraviolet (UV) spectrum only. Images taken with ultraviolet light serve a number of scientific, medical or artistic purposes. Images may reveal deterioration of art works or structures not apparent under visible light. Diagnostic medical images may be used to detect certain skin disorders or as evidence of injury. Some animals, particularly insects, use ultraviolet wavelengths for vision; ultraviolet photography can help investigate the markings of plants that attract insects, while invisible to the unaided human eye. Ultraviolet photography of archaeological sites may reveal artifacts or traffic patterns not otherwise visible.

An infrared heater or heat lamp is a body with a higher temperature which transfers energy to a body with a lower temperature through electromagnetic radiation. Depending on the temperature of the emitting body, the wavelength of the peak of the infrared radiation ranges from 780 nm to 1 mm. No contact or medium between the two bodies is needed for the energy transfer. Infrared heaters can be operated in vacuum or atmosphere.

The absorption of electromagnetic radiation by water depends on the state of the water.

Cosmic infrared background is infrared radiation caused by stellar dust.

A flame detector is a sensor designed to detect and respond to the presence of a flame or fire, allowing flame detection. Responses to a detected flame depend on the installation, but can include sounding an alarm, deactivating a fuel line, and activating a fire suppression system. When used in applications such as industrial furnaces, their role is to provide confirmation that the furnace is working properly; it can be used to turn off the ignition system though in many cases they take no direct action beyond notifying the operator or control system. A flame detector can often respond faster and more accurately than a smoke or heat detector due to the mechanisms it uses to detect the flame.

Infrared vision is the capability of biological or artificial systems to detect infrared radiation. The terms thermal vision and thermal imaging, are also commonly used in this context since infrared emissions from a body are directly related to their temperature: hotter objects emit more energy in the infrared spectrum than colder ones.

Non-ionizingradiation refers to any type of electromagnetic radiation that does not carry enough energy per quantum to ionize atoms or molecules—that is, to completely remove an electron from an atom or molecule. Instead of producing charged ions when passing through matter, non-ionizing electromagnetic radiation has sufficient energy only for excitation, the movement of an electron to a higher energy state. In contrast, ionizing radiation has a higher frequency and shorter wavelength than non-ionizing radiation, and can be a serious health hazard; exposure to it can cause burns, radiation sickness, cancer, and genetic damage. Using ionizing radiation requires elaborate radiological protection measures, which in general are not required with non-ionizing radiation.

## References

1. Sliney, David H.; Wangemann, Robert T.; Franks, James K.; Wolbarsht, Myron L. (1976). "Visual sensitivity of the eye to infrared laser radiation". Journal of the Optical Society of America . 66 (4): 339–341. Bibcode:1976JOSA...66..339S. doi:10.1364/JOSA.66.000339. PMID   1262982. The foveal sensitivity to several near-infrared laser wavelengths was measured. It was found that the eye could respond to radiation at wavelengths at least as far as 1064 nm. A continuous 1064 nm laser source appeared red, but a 1060 nm pulsed laser source appeared green, which suggests the presence of second harmonic generation in the retina.
2. Lynch, David K.; Livingston, William Charles (2001). Color and Light in Nature (2nd ed.). Cambridge, UK: Cambridge University Press. p. 231. ISBN   978-0-521-77504-5 . Retrieved 12 October 2013. Limits of the eye's overall range of sensitivity extends from about 310 to 1050 nanometers
3. Dash, Madhab Chandra; Dash, Satya Prakash (2009). Fundamentals Of Ecology 3E. Tata McGraw-Hill Education. p. 213. ISBN   978-1-259-08109-5 . Retrieved 18 October 2013. Normally the human eye responds to light rays from 390 to 760 nm. This can be extended to a range of 310 to 1,050 nm under artificial conditions.
4. Saidman, Jean (15 May 1933). "Sur la visibilité de l'ultraviolet jusqu'à la longueur d'onde 3130" [The visibility of the ultraviolet to the wave length of 3130]. Comptes rendus de l'Académie des sciences (in French). 196: 1537–9.
5. Liew, S. C. "Electromagnetic Waves". Centre for Remote Imaging, Sensing and Processing. Retrieved 2006-10-27.
6. Michael Rowan-Robinson (2013). Night Vision: Exploring the Infrared Universe. Cambridge University Press. p. 23. ISBN   1107024765.
7. Reusch, William (1999). "Infrared Spectroscopy". Michigan State University. Archived from the original on 2007-10-27. Retrieved 2006-10-27.
8. "IR Astronomy: Overview". NASA Infrared Astronomy and Processing Center. Archived from the original on 2006-12-08. Retrieved 2006-10-30.
9. Chilton, Alexander (2013-10-07). "The Working Principle and Key Applications of Infrared Sensors". AZoSensors. Retrieved 2020-07-11.
10. Haynes, William M., ed. (2011). CRC Handbook of Chemistry and Physics (92nd ed.). CRC Press. p. 10.233. ISBN   978-1-4398-5511-9.
11. "Reference Solar Spectral Irradiance: Air Mass 1.5" . Retrieved 2009-11-12.
12. Byrnes, James (2009). Unexploded Ordnance Detection and Mitigation. Springer. pp. 21–22. Bibcode:2009uodm.book.....B. ISBN   978-1-4020-9252-7.
13. "Peaks of Blackbody Radiation Intensity" . Retrieved 27 July 2016.
14. "Photoacoustic technique 'hears' the sound of dangerous chemical agents". R&D Magazine . August 14, 2012. rdmag.com. Retrieved September 8, 2012.
15. Henderson, Roy. "Wavelength considerations". Instituts für Umform- und Hochleistungs. Archived from the original on 2007-10-28. Retrieved 2007-10-18.
16. ISO 20473:2007
17. "Near, Mid and Far-Infrared". NASA IPAC. Archived from the original on 2012-05-29. Retrieved 2007-04-04.
18. Miller, Principles of Infrared Technology (Van Nostrand Reinhold, 1992), and Miller and Friedman, Photonic Rules of Thumb, 2004. ISBN   978-0-442-01210-6 [ page needed ]
19. Griffin, Donald R.; Hubbard, Ruth; Wald, George (1947). "The Sensitivity of the Human Eye to Infra-Red Radiation". Journal of the Optical Society of America. 37 (7): 546–553. Bibcode:1947JOSA...37..546G. doi:10.1364/JOSA.37.000546. PMID   20256359.
20. Ramaswami, Rajiv (May 2002). "Optical Fiber Communication: From Transmission to Networking". IEEE Communications Magazine. 40 (5): 138–147. doi:10.1109/MCOM.2002.1006983.
21. "Infrared Radiation". Infrared Radiation. Van Nostrand's Scientific Encyclopedia. John Wiley & Sons, Inc. 2007. doi:10.1002/0471743984.vse4181.pub2. ISBN   978-0471743989.
22. "Introduction to Solar Energy". Passive Solar Heating & Cooling Manual. Rodale Press, Inc. 1980. Archived from the original (DOC) on 2009-03-18. Retrieved 2007-08-12.
23. McCreary, Jeremy (October 30, 2004). "Infrared (IR) basics for digital photographers-capturing the unseen (Sidebar: Black Body Radiation)". Digital Photography For What It's Worth. Retrieved 2006-11-07.
24. "How Night Vision Works". American Technologies Network Corporation. Retrieved 2007-08-12.
25. Bryant, Lynn (2007-06-11). "How does thermal imaging work? A closer look at what is behind this remarkable technology". Archived from the original on 2007-07-28. Retrieved 2007-08-12.
26. Holma, H., (May 2011), Thermische Hyperspektralbildgebung im langwelligen Infrarot Archived 2011-07-26 at the Wayback Machine , Photonik
27. Frost&Sullivan, Technical Insights, Aerospace&Defence (Feb 2011): World First Thermal Hyperspectral Camera for Unmanned Aerial Vehicles.
28. Mahulikar, S.P.; Sonawane, H.R.; Rao, G.A. (2007). "Infrared signature studies of aerospace vehicles" (PDF). Progress in Aerospace Sciences. 43 (7–8): 218–245. Bibcode:2007PrAeS..43..218M. CiteSeerX  . doi:10.1016/j.paerosci.2007.06.002.
29. White, Richard P. (2000) "Infrared deicing system for aircraft"
30. Dangers of Overexposure to ultraviolet, infrared and high-energy visible light | 2013-01-03. ISHN. Retrieved on 2017-04-26.
31. Digital ICE. kodak.com
32. "IR Reflectography for Non-destructive Analysis of Underdrawings in Art Objects". Sensors Unlimited, Inc. Retrieved 2009-02-20.
33. "The Mass of Saint Gregory: Examining a Painting Using Infrared Reflectography". The Cleveland Museum of Art. Archived from the original on 2009-01-13. Retrieved 2009-02-20.
34. Infrared reflectography in analysis of paintings at ColourLex.
35. "International Dunhuang Project An Introduction to digital infrared photography and its application within IDP". Idp.bl.uk. Retrieved 2011-11-08.
36. Jones, B.S.; Lynn, W.F.; Stone, M.O. (2001). "Thermal Modeling of Snake Infrared Reception: Evidence for Limited Detection Range". Journal of Theoretical Biology. 209 (2): 201–211. doi:10.1006/jtbi.2000.2256. PMID   11401462.
37. Gorbunov, V.; Fuchigami, N.; Stone, M.; Grace, M.; Tsukruk, V. V. (2002). "Biological Thermal Detection: Micromechanical and Microthermal Properties of Biological Infrared Receptors". Biomacromolecules. 3 (1): 106–115. doi:10.1021/bm015591f. PMID   11866562.
38. Evans, W.G. (1966). "Infrared receptors in Melanophila acuminata De Geer". Nature. 202 (4928): 211. Bibcode:1964Natur.202..211E. doi:10.1038/202211a0. PMID   14156319.
39. Campbell, Angela L.; Naik, Rajesh R.; Sowards, Laura; Stone, Morley O. (2002). "Biological infrared imaging and sensing". Micrometre. 33 (2): 211–225. doi:10.1016/S0968-4328(01)00010-5. PMID   11567889.
40. Brook, P. J. (26 April 1969). "Stimulation of Ascospore Release in Venturia inaequalis by Far Red Light". Nature. 222 (5191): 390–392. Bibcode:1969Natur.222..390B. doi:10.1038/222390a0. ISSN   0028-0836.
41. Meuthen, Denis; Rick, Ingolf P.; Thünken, Timo; Baldauf, Sebastian A. (2012). "Visual prey detection by near-infrared cues in a fish". Naturwissenschaften. 99 (12): 1063–6. Bibcode:2012NW.....99.1063M. doi:10.1007/s00114-012-0980-7. PMID   23086394.
42. Endo, M.; Kobayashi R.; Ariga, K.; Yoshizaki, G.; Takeuchi, T. (2002). "Postural control in tilapia under microgravity and the near infrared irradiated conditions". Nippon Suisan Gakkaish. 68 (6): 887–892. doi:.
43. Kobayashi R.; Endo, M.; Yoshizaki, G.; Takeuchi, T. (2002). "Sensitivity of tilapia to infrared light measured using a rotating striped drum differs between two strains". Nippon Suisan Gakkaish. 68 (5): 646–651. doi:.
44. Matsumoto, Taro; Kawamura, Gunzo (2005). "The eyes of the common carp and Nile tilapia are sensitive to near-infrared". Fisheries Science. 71 (2): 350–355. doi:10.1111/j.1444-2906.2005.00971.x.
45. Shcherbakov, Denis; Knörzer, Alexandra; Hilbig, Reinhard; Haas, Ulrich; Blum, Martin (2012). "Near-infrared orientation of Mozambique tilapia Oreochromis mossambicus". Zoology. 115 (4): 233–238. doi:10.1016/j.zool.2012.01.005. PMID   22770589.
46. Hargate, G (2006). "A randomised double-blind study comparing the effect of 1072-nm light against placebo for the treatment of herpes labialis". Clinical and Experimental Dermatology. 31 (5): 638–41. doi:10.1111/j.1365-2230.2006.02191.x. PMID   16780494.
47. Desmet KD, Paz DA, Corry JJ, Eells JT, Wong-Riley MT, Henry MM, Buchmann EV, Connelly MP, Dovi JV, Liang HL, Henshel DS, Yeager RL, Millsap DS, Lim J, Gould LJ, Das R, Jett M, Hodgson BD, Margolis D, Whelan HT (May 2006). "Clinical and experimental applications of NIR-LED photobiomodulation". Photomedicine and Laser Surgery. 24 (2): 121–8. doi:10.1089/pho.2006.24.121. PMID   16706690.
48. Rosso, Monona l (2001). The Artist's Complete Health and Safety Guide. Allworth Press. pp. 33–. ISBN   978-1-58115-204-3.
49. Herschel, William (1800). "Experiments on the refrangibility of the invisible rays of the Sun". Philosophical Transactions of the Royal Society of London. 90: 284–292. doi:. JSTOR   107057.
50. "Herschel Discovers Infrared Light". Coolcosmos.ipac.caltech.edu. Archived from the original on 2012-02-25. Retrieved 2011-11-08.
51. In 1867, French physcist Edmond Becquerel coined the term infra-rouge (infra-red):
The word infra-rouge was translated into English as "infrared" in 1874, in a translation of an article by Vignaud Dupuy de Saint-Florent (1830–1907), an engineer in the French army, who attained the rank of lieutenant colonel and who pursued photography as a pastime.
• de Saint-Florent (10 April 1874). "Photography in natural colours". The Photographic News. 18: 175–176. From p. 176: "As to the infra-red rays, they may be absorbed by means of a weak solution of sulphate of copper, ..."
52. In 1737, Du Châtelet anonymously submitted her essay – Dissertation sur la nature et la propagation du feu (Dissertation on the nature and propagation of fire) – to the Académie Royale des Sciences, which had made the nature of fire the subject of a prize competition. Her essay was published as a book in 1739 and a second edition was published in 1744. See: Du Chatelet, Émilie (1744). Dissertation sur la nature et la propagation du feu [Dissertation on the nature and propagation of fire] (in French) (2nd ed.). Paris, France: Prault, Fils. From (Châtelet, 1744), p. 70: "Une expérience bien curieuse ... une plus grande chaleur que les violets, &c. ... " ... " ... les rouges échauffent davantage que les violets, les jaunes que les bleus, &c. car ils sont des impressions plus fortes sur les yeux ; ... " ("A quite curious experiment (if it's possible) would be to gather separately enough homogeneous rays [of each color of the solar spectrum] in order to test whether the original rays that excite in us the sensation of different colors, would not have different burning powers; if the reds, for example, would give a greater heat than the violets, etc. ... " ... " ... the reds heat more than the violets, the yellows [more] than the blues, etc., for they make stronger impressions on the eyes ; ... ").
53. See:
54. Herschel, John F. W. (1840). "On chemical action of rays of solar spectrum on preparation of silver and other substances both metallic and nonmetallic and on some photographic processes". Philosophical Transactions of the Royal Society of London. 130: 1–59. Bibcode:1840RSPT..130....1H. doi:10.1098/rstl.1840.0002. The term "thermograph" is coined on p. 51: " ... I have discovered a process by which the calorific rays in the solar spectrum are made to leave their impress on a surface properly prepared for the purpose, so as to form what may be called a thermograph of the spectrum, ... ".
55. See:
56. See:
57. See:
58. Stefan, J. (1879). "Über die Beziehung zwischen der Wärmestrahlung und der Temperatur" [On the relation between heat radiation and temperature]. Sitzungsberichte der Kaiserlichen Akademie der Wissenschaften [Wien]: Mathematisch-naturwissenschaftlichen Classe (Proceedings of the Imperial Academy of Philosophy [in Vienna]: Mathematical-scientific Class) (in German). 79: 391–428.
59. See:
60. Julius, Willem Henri (1892). Bolometrisch onderzoek van absorptiespectra (in Dutch). J. Müller.
61. See:
62. See:
63. Coblentz, William Weber (1905). Investigations of Infra-red Spectra: Part I, II. Carnegie institution of Washington.
64. Coblentz, William Weber (1905). Investigations of Infra-red Spectra: Part III, IV. University of Michigan. Washington, D.C., Carnegie institution of Washington.
65. Coblentz, William Weber (August 1905). Investigations of Infra-red Spectra: Part V, VI, VII. University of California Libraries. Washington, D.C. : Carnegie Institution of Washington.
66. Waste Energy Harvesting: Mechanical and Thermal Energies. Springer Science & Business Media. 2014. p. 406. ISBN   9783642546341 . Retrieved 2020-01-07.
67. Marion B. Reine (2015). "Interview with Paul W. Kruse on the Early History of HgCdTe (1980)" (PDF). doi:10.1007/s11664-015-3737-1 . Retrieved 2020-01-07.Cite journal requires `|journal=` (help)
68. J Cooper (1962). "A fast-response pyroelectric thermal detector". Journal of Scientific Instruments. 39 (9): 467–472. Bibcode:1962JScI...39..467C. doi:10.1088/0950-7671/39/9/308.
69. "History of Army Night Vision". C5ISR Center. Retrieved 2020-01-07.
70. "Implant gives rats sixth sense for infrared light". Wired UK. 14 February 2013. Retrieved 14 February 2013.