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Ultraviolet
Ultraviolet
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Portable ultraviolet lamp (UVA and UVB)
UV radiation is also produced by electric arcs. Arc welders must wear eye protection and cover their skin to prevent photokeratitis and serious sunburn.

Ultraviolet radiation, also known as simply UV, is electromagnetic radiation of wavelengths of 10–400 nanometers, shorter than that of visible light, but longer than X-rays. UV radiation is present in sunlight and constitutes about 10% of the total electromagnetic radiation output from the Sun. It is also produced by electric arcs, Cherenkov radiation, and specialized lights, such as mercury-vapor lamps, tanning lamps, and black lights.

The photons of ultraviolet have greater energy than those of visible light, from about 3.1 to 12 electron volts, around the minimum energy required to ionize atoms.[1]: 25–26  Although long-wavelength ultraviolet is not considered an ionizing radiation[2] because its photons lack sufficient energy, it can induce chemical reactions and cause many substances to glow or fluoresce. Many practical applications, including chemical and biological effects, are derived from the way that UV radiation can interact with organic molecules. These interactions can involve exciting orbital electrons to higher energy states in molecules potentially breaking chemical bonds. In contrast, the main effect of longer wavelength radiation is to excite vibrational or rotational states of these molecules, increasing their temperature.[1]: 28  Short-wave ultraviolet light is ionizing radiation.[2] Consequently, short-wave UV damages DNA and sterilizes surfaces with which it comes into contact.

For humans, suntan and sunburn are familiar effects of exposure of the skin to UV, along with an increased risk of skin cancer. The amount of UV radiation produced by the Sun means that the Earth would not be able to sustain life on dry land if most of that light were not filtered out by the atmosphere.[3] More energetic, shorter-wavelength "extreme" UV below 121 nm ionizes air so strongly that it is absorbed before it reaches the ground.[4] However, UV (specifically, UVB) is also responsible for the formation of vitamin D in most land vertebrates, including humans.[5] The UV spectrum, thus, has effects both beneficial and detrimental to life.

The lower wavelength limit of the visible spectrum is conventionally taken as 400 nm. Although ultraviolet rays are not generally visible to humans, 400 nm is not a sharp cutoff, with shorter and shorter wavelengths becoming less and less visible in this range.[6] Insects, birds, and some mammals can see near-UV (NUV), i.e., somewhat shorter wavelengths than what humans can see.[7]

Visibility

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Humans generally cannot use ultraviolet rays for vision. The lens of the human eye and surgically implanted lens produced since 1986 blocks most radiation in the near UV wavelength range of 300–400 nm; shorter wavelengths are blocked by the cornea.[8] Humans also lack color receptor adaptations for ultraviolet rays. The photoreceptors of the retina are sensitive to near-UV but the lens does not focus this light, causing UV light bulbs to look fuzzy.[9][10] People lacking a lens (a condition known as aphakia) perceive near-UV as whitish-blue or whitish-violet.[6] Near-UV radiation is visible to insects, some mammals, and some birds. Birds have a fourth color receptor for ultraviolet rays; this, coupled with eye structures that transmit more UV gives smaller birds "true" UV vision.[11][12]

History and discovery

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"Ultraviolet" means "beyond violet" (from Latin ultra, "beyond"), violet being the color of the highest frequencies of visible light. Ultraviolet has a higher frequency (thus a shorter wavelength) than violet light.

UV radiation was discovered in February 1801 when the German physicist Johann Wilhelm Ritter observed that invisible rays just beyond the violet end of the visible spectrum darkened silver chloride-soaked paper more quickly than violet light itself. He announced the discovery in a very brief letter to the Annalen der Physik[13][14] and later called them "(de-)oxidizing rays" (German: de-oxidierende Strahlen) to emphasize chemical reactivity and to distinguish them from "heat rays", discovered the previous year at the other end of the visible spectrum. The simpler term "chemical rays" was adopted soon afterwards, and remained popular throughout the 19th century, although some said that this radiation was entirely different from light (notably John William Draper, who named them "tithonic rays"[15][16]). The terms "chemical rays" and "heat rays" were eventually dropped in favor of ultraviolet and infrared radiation, respectively.[17][18] In 1878, the sterilizing effect of short-wavelength light by killing bacteria was discovered. By 1903, the most effective wavelengths were known to be around 250 nm. In 1960, the effect of ultraviolet radiation on DNA was established.[19]

The discovery of the ultraviolet radiation with wavelengths below 200 nm, named "vacuum ultraviolet" because it is strongly absorbed by the oxygen in air, was made in 1893 by German physicist Victor Schumann.[20] The division of UV into UVA, UVB, and UVC was decided "unanimously" by a committee of the Second International Congress on Light on August 17th, 1932, at the Castle of Christiansborg in Copenhagen.[21]

Subtypes

[edit]

The electromagnetic spectrum of ultraviolet radiation (UVR), defined most broadly as 10–400 nanometers, can be subdivided into a number of ranges recommended by the ISO standard ISO 21348:[22]

Name Photon energy (eVaJ) Notes/alternative names
Abbreviation Wavelength (nm)
Ultraviolet A 3.10–3.94
0.497–0.631
Long-wave UV, blacklight, not absorbed by the ozone layer: soft UV.
UVA 315–400
Ultraviolet B 3.94–4.43
0.631–0.710
Medium-wave UV, mostly absorbed by the ozone layer: intermediate UV; Dorno radiation.
UVB 280–315
Ultraviolet C 4.43–12.4
0.710–1.987
Short-wave UV, germicidal UV, ionizing radiation at shorter wavelengths, completely absorbed by the ozone layer and atmosphere: hard UV.
UVC 100–280
Near ultraviolet 3.10–4.13
0.497–0.662
Visible to birds, insects, and fish.
NUV 300–400
Middle ultraviolet 4.13–6.20
0.662–0.993
MUV 200–300
Far ultraviolet 6.20–10.16
0.993–1.628
Ionizing radiation at shorter wavelengths.
FUV 122–200
Hydrogen
Lyman-alpha
10.16–10.25
1.628–1.642
Spectral line at 121.6 nm, 10.20 eV.
H Lyman‑α 121–122
Extreme ultraviolet 10.25–124
1.642–19.867
Entirely ionizing radiation by some definitions; completely absorbed by the atmosphere.
EUV 10–121
Far-UVC 5.28–6.20
0.846–0.993
Germicidal but strongly absorbed by outer skin layers, so does not reach living tissue.
200–235
Vacuum ultraviolet 6.20–124
0.993–19.867
Strongly absorbed by atmospheric oxygen, though 150–200 nm wavelengths can propagate through nitrogen.
VUV 10–200

Several solid-state and vacuum devices have been explored for use in different parts of the UV spectrum. Many approaches seek to adapt visible light-sensing devices, but these can suffer from unwanted response to visible light and various instabilities. Ultraviolet can be detected by suitable photodiodes and photocathodes, which can be tailored to be sensitive to different parts of the UV spectrum. Sensitive UV photomultipliers are available. Spectrometers and radiometers are made for measurement of UV radiation. Silicon detectors are used across the spectrum.[23]

Vacuum ultraviolet

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Vacuum UV, or VUV, wavelengths (shorter than 200 nm) are strongly absorbed by molecular oxygen in the air, though the longer wavelengths around 150–200 nm can propagate through nitrogen. Scientific instruments can, therefore, use this spectral range by operating in an oxygen-free atmosphere (pure nitrogen, or argon for shorter wavelengths), without the need for costly vacuum chambers. Significant examples include 193-nm photolithography equipment (for semiconductor manufacturing) and circular dichroism spectrometers.[24]

Technology for VUV instrumentation was largely driven by solar astronomy for many decades. While optics can be used to remove unwanted visible light that contaminates the VUV, in general, detectors can be limited by their response to non-VUV radiation, and the development of solar-blind devices has been an important area of research. Wide-gap solid-state devices or vacuum devices with high-cutoff photocathodes can be attractive compared to silicon diodes.

Extreme ultraviolet

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Extreme UV (EUV or sometimes XUV) is characterized by a transition in the physics of interaction with matter. Wavelengths longer than about 30 nm interact mainly with the outer valence electrons of atoms, while wavelengths shorter than that interact mainly with inner-shell electrons and nuclei. The long end of the EUV spectrum is set by a prominent He+ spectral line at 30.4 nm. EUV is strongly absorbed by most known materials, but synthesizing multilayer optics that reflect up to about 50% of EUV radiation at normal incidence is possible. This technology was pioneered by the NIXT and MSSTA sounding rockets in the 1990s, and it has been used to make telescopes for solar imaging. See also the Extreme Ultraviolet Explorer satellite.[citation needed]

Hard and soft ultraviolet

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Some sources use the distinction of "hard UV" and "soft UV". For instance, in the case of astrophysics, the boundary may be at the Lyman limit (wavelength 91.2 nm, the energy needed to ionise a hydrogen atom from its ground state), with "hard UV" being more energetic;[25] the same terms may also be used in other fields, such as cosmetology, optoelectronic, etc. The numerical values of the boundary between hard/soft, even within similar scientific fields, do not necessarily coincide; for example, one applied-physics publication used a boundary of 190 nm between hard and soft UV regions.[26]

Solar ultraviolet

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Levels of ozone at various altitudes (DU/km) and blocking of different bands of ultraviolet radiation: In essence, all UVC is blocked by diatomic oxygen (100–200 nm) or by ozone (triatomic oxygen) (200–280 nm) in the atmosphere. The ozone layer then blocks most UVB. Meanwhile, UVA is hardly affected by ozone, and most of it reaches the ground. UVA makes up almost all UV light that penetrates the Earth's atmosphere.

Very hot objects emit UV radiation (see black-body radiation). The Sun emits ultraviolet radiation at all wavelengths, including the extreme ultraviolet where it crosses into X-rays at 10 nm. Extremely hot stars (such as O- and B-type) emit proportionally more UV radiation than the Sun. Sunlight in space at the top of Earth's atmosphere (see solar constant) is composed of about 50% infrared light, 40% visible light, and 10% ultraviolet light, for a total intensity of about 1400 W/m2 in vacuum.[27]

The atmosphere blocks about 77% of the Sun's UV, when the Sun is highest in the sky (at zenith), with absorption increasing at shorter UV wavelengths. At ground level with the sun at zenith, sunlight is 44% visible light, 3% ultraviolet, and the remainder infrared.[28][29] Of the ultraviolet radiation that reaches the Earth's surface, more than 95% is the longer wavelengths of UVA, with the small remainder UVB. Almost no UVC reaches the Earth's surface.[30] The fraction of UVA and UVB which remains in UV radiation after passing through the atmosphere is heavily dependent on cloud cover and atmospheric conditions. On "partly cloudy" days, patches of blue sky showing between clouds are also sources of (scattered) UVA and UVB, which are produced by Rayleigh scattering in the same way as the visible blue light from those parts of the sky. UVB also plays a major role in plant development, as it affects most of the plant hormones.[31] During total overcast, the amount of absorption due to clouds is heavily dependent on the thickness of the clouds and latitude, with no clear measurements correlating specific thickness and absorption of UVA and UVB.[32]

The shorter bands of UVC, as well as even more-energetic UV radiation produced by the Sun, are absorbed by oxygen and generate the ozone in the ozone layer when single oxygen atoms produced by UV photolysis of dioxygen react with more dioxygen. The ozone layer is especially important in blocking most UVB and the remaining part of UVC not already blocked by ordinary oxygen in air.[citation needed]

Blockers, absorbers, and windows

[edit]

Ultraviolet absorbers are molecules used in organic materials (polymers, paints, etc.) to absorb UV radiation to reduce the UV degradation (photo-oxidation) of a material. The absorbers can themselves degrade over time, so monitoring of absorber levels in weathered materials is necessary.[citation needed]

In sunscreen, ingredients that absorb UVA/UVB rays, such as avobenzone, oxybenzone[33] and octyl methoxycinnamate, are organic chemical absorbers or "blockers". They are contrasted with inorganic absorbers/"blockers" of UV radiation such as titanium dioxide and zinc oxide.[34]

For clothing, the ultraviolet protection factor (UPF) represents the ratio of sunburn-causing UV without and with the protection of the fabric, similar to sun protection factor (SPF) ratings for sunscreen.[citation needed] Standard summer fabrics have UPFs around 6, which means that about 20% of UV will pass through.[citation needed]

Suspended nanoparticles in stained-glass prevent UV rays from causing chemical reactions that change image colors.[citation needed] A set of stained-glass color-reference chips is planned to be used to calibrate the color cameras for the 2019 ESA Mars rover mission, since they will remain unfaded by the high level of UV present at the surface of Mars.[citation needed]

Common soda–lime glass, such as window glass, is partially transparent to UVA, but is opaque to shorter wavelengths, passing about 90% of the light above 350 nm, but blocking over 90% of the light below 300 nm.[35][36][37] A study found that car windows allow 3–4% of ambient UV to pass through, especially if the UV was greater than 380 nm.[38] Other types of car windows can reduce transmission of UV that is greater than 335 nm.[38] Fused quartz, depending on quality, can be transparent even to vacuum UV wavelengths. Crystalline quartz and some crystals such as CaF2 and MgF2 transmit well down to 150 nm or 160 nm wavelengths.[39]

Wood's glass is a deep violet-blue barium-sodium silicate glass with about 9% nickel(II) oxide developed during World War I to block visible light for covert communications. It allows both infrared daylight and ultraviolet night-time communications by being transparent between 320 nm and 400 nm and also the longer infrared and just-barely-visible red wavelengths. Its maximum UV transmission is at 365 nm, one of the wavelengths of mercury lamps.[40]

Artificial sources

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"Black lights"

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Two black light fluorescent tubes, showing use. The longer tube is a F15T8/BLB 18 inch, 15 watt tube, shown in the bottom image in a standard plug-in fluorescent fixture. The shorter is an F8T5/BLB 12 inch, 8 watt tube, used in a portable battery-powered black light sold as a pet urine detector.

A black light lamp emits long-wave UVA radiation and little visible light. Fluorescent black light lamps work similarly to other fluorescent lamps, but use a phosphor on the inner tube surface which emits UVA radiation instead of visible light. Some lamps use a deep-bluish-purple Wood's glass optical filter that blocks almost all visible light with wavelengths longer than 400 nanometers.[41] The purple glow given off by these tubes is not the ultraviolet itself, but visible purple light from mercury's 404 nm spectral line which escapes being filtered out by the coating. Other black lights use plain glass instead of the more expensive Wood's glass, so they appear light-blue to the eye when operating.[citation needed]

Incandescent black lights are also produced, using a filter coating on the envelope of an incandescent bulb that absorbs visible light (see section below). These are cheaper but very inefficient, emitting only a small fraction of a percent of their power as UV. Mercury-vapor black lights in ratings up to 1 kW with UV-emitting phosphor and an envelope of Wood's glass are used for theatrical and concert displays.[citation needed]

Black lights are used in applications in which extraneous visible light must be minimized; mainly to observe fluorescence, the colored glow that many substances give off when exposed to UV light. UVA / UVB emitting bulbs are also sold for other special purposes, such as tanning lamps and reptile-husbandry.[citation needed]

Short-wave ultraviolet lamps

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9 watt germicidal UV bulb, in compact fluorescent (CF) form factor
Commercial germicidal lamp in butcher shop

Shortwave UV lamps are made using a fluorescent lamp tube with no phosphor coating, composed of fused quartz or vycor, since ordinary glass absorbs UVC. These lamps emit ultraviolet light with two peaks in the UVC band at 253.7 nm and 185 nm due to the mercury within the lamp, as well as some visible light. From 85% to 90% of the UV produced by these lamps is at 253.7 nm, whereas only 5–10% is at 185 nm.[42] The fused quartz tube passes the 253.7 nm radiation but blocks the 185 nm wavelength. Such tubes have two or three times the UVC power of a regular fluorescent lamp tube. These low-pressure lamps have a typical efficiency of approximately 30–40%, meaning that for every 100 watts of electricity consumed by the lamp, they will produce approximately 30–40 watts of total UV output. They also emit bluish-white visible light, due to mercury's other spectral lines. These "germicidal" lamps are used extensively for disinfection of surfaces in laboratories and food-processing industries.[43]

Incandescent lamps

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'Black light' incandescent lamps are also made from an incandescent light bulb with a filter coating which absorbs most visible light. Halogen lamps with fused quartz envelopes are used as inexpensive UV light sources in the near UV range, from 400 to 300 nm, in some scientific instruments. Due to its black-body spectrum a filament light bulb is a very inefficient ultraviolet source, emitting only a fraction of a percent of its energy as UV, as explained by the black body spectrum.

Gas-discharge lamps

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Specialized UV gas-discharge lamps containing different gases produce UV radiation at particular spectral lines for scientific purposes. Argon and deuterium arc lamps are often used as stable sources, either windowless or with various windows such as magnesium fluoride.[44] These are often the emitting sources in UV spectroscopy equipment for chemical analysis.[citation needed]

Other UV sources with more continuous emission spectra include xenon arc lamps (commonly used as sunlight simulators), deuterium arc lamps, mercury-xenon arc lamps, and metal-halide arc lamps.[citation needed]

The excimer lamp, a UV source developed in the early 2000s, is seeing increasing use in scientific fields. It has the advantages of high-intensity, high efficiency, and operation at a variety of wavelength bands into the vacuum ultraviolet.[citation needed]

Ultraviolet LEDs

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A 380 nanometer UV LED makes some common household items fluoresce.

Light-emitting diodes (LEDs) can be manufactured to emit radiation in the ultraviolet range. In 2019, following significant advances over the preceding five years, UVA LEDs of 365 nm and longer wavelength were available, with efficiencies of 50% at 1.0 W output. Currently, the most common types of UV LEDs are in 395 nm and 365 nm wavelengths, both of which are in the UVA spectrum. The rated wavelength is the peak wavelength that the LEDs put out, but light at both higher and lower wavelengths are present.[45]

The cheaper and more common 395 nm UV LEDs are much closer to the visible spectrum, and give off a purple color. Other UV LEDs deeper into the spectrum do not emit as much visible light.[46] LEDs are used for applications such as UV curing applications, charging glow-in-the-dark objects such as paintings or toys, and lights for detecting counterfeit money and bodily fluids. UV LEDs are also used in digital print applications and inert UV curing environments. As technological advances beginning in the early 2000s have improved their output and efficiency, they have become increasingly viable alternatives to more traditional UV lamps for use in UV curing applications, and the development of new UV LED curing systems for higher-intensity applications is a major subject of research in the field of UV curing technology.[47]

UVC LEDs are developing rapidly, but may require testing to verify effective disinfection. Citations for large-area disinfection are for non-LED UV sources[48] known as germicidal lamps.[49] Also, they are used as line sources to replace deuterium lamps in liquid chromatography instruments.[50]

Ultraviolet lasers

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Gas lasers, laser diodes, and solid-state lasers can be manufactured to emit ultraviolet rays, and lasers are available that cover the entire UV range. The nitrogen gas laser uses electronic excitation of nitrogen molecules to emit a beam that is mostly UV. The strongest ultraviolet lines are at 337.1 nm and 357.6 nm in wavelength. Another type of high-power gas lasers are excimer lasers. They are widely used lasers emitting in ultraviolet and vacuum ultraviolet wavelength ranges. Presently, UV argon-fluoride excimer lasers operating at 193 nm are routinely used in integrated circuit production by photolithography. The current[timeframe?] wavelength limit of production of coherent UV is about 126 nm, characteristic of the Ar2* excimer laser.[citation needed]

Direct UV-emitting laser diodes are available at 375 nm.[51] UV diode-pumped solid state lasers have been demonstrated using cerium-doped lithium strontium aluminum fluoride crystals (Ce:LiSAF), a process developed in the 1990s at Lawrence Livermore National Laboratory.[52] Wavelengths shorter than 325 nm are commercially generated in diode-pumped solid-state lasers. Ultraviolet lasers can also be made by applying frequency conversion to lower-frequency lasers.[53]

Ultraviolet lasers have applications in industry (laser engraving), medicine (dermatology, and keratectomy), chemistry (MALDI), free-air secure communications, computing (optical storage), and manufacture of integrated circuits.[54][55]

Tunable vacuum ultraviolet (VUV)

[edit]

The vacuum ultraviolet (V‑UV) band (100–200 nm) can be generated by non-linear 4 wave mixing in gases by sum or difference frequency mixing of 2 or more longer wavelength lasers. The generation is generally done in gasses (e.g. krypton, hydrogen which are two-photon resonant near 193 nm)[56] or metal vapors (e.g. magnesium). By making one of the lasers tunable, the V‑UV can be tuned. If one of the lasers is resonant with a transition in the gas or vapor then the V‑UV production is intensified. However, resonances also generate wavelength dispersion, and thus the phase matching can limit the tunable range of the 4 wave mixing. Difference frequency mixing (i.e., f1 + f2f3) has an advantage over sum frequency mixing because the phase matching can provide greater tuning.[56]

In particular, difference frequency mixing two photons of an ArF (193 nm) excimer laser with a tunable visible or near IR laser in hydrogen or krypton provides resonantly enhanced tunable V‑UV covering from 100 nm to 200 nm.[56] Practically, the lack of suitable gas / vapor cell window materials above the lithium fluoride cut-off wavelength limit the tuning range to longer than about 110 nm. Tunable V‑UV wavelengths down to 75 nm was achieved using window-free configurations.[57]

Plasma and synchrotron sources of extreme UV

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Lasers have been used to indirectly generate non-coherent extreme UV (E‑UV) radiation at 13.5 nm for extreme ultraviolet lithography. The E‑UV is not emitted by the laser, but rather by electron transitions in an extremely hot tin or xenon plasma, which is excited by an excimer laser.[58] This technique does not require a synchrotron, yet can produce UV at the edge of the X‑ray spectrum. Synchrotron light sources can also produce all wavelengths of UV, including those at the boundary of the UV and X‑ray spectra at 10 nm.[citation needed]

[edit]

The impact of ultraviolet radiation on human health has implications for the risks and benefits of sun exposure and is also implicated in issues such as fluorescent lamps and health. Getting too much sun exposure can be harmful, but in moderation, sun exposure is beneficial.[59]

Beneficial effects

[edit]

UV (specifically, UVB) causes the body to produce vitamin D,[60] which is essential for life. Humans need some UV radiation to maintain adequate vitamin D levels. According to the World Health Organization:[61]

There is no doubt that a little sunlight is good for you! But 5–15 minutes of casual sun exposure of hands, face and arms two to three times a week during the summer months is sufficient to keep your vitamin D levels high.

Vitamin D can also be obtained from food and supplementation.[62] Excess sun exposure produces harmful effects, however.[61]

Skin conditions

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UV rays also treat certain skin conditions. Modern phototherapy has been used to successfully treat psoriasis, eczema, jaundice, vitiligo, atopic dermatitis, and localized scleroderma.[63][64] In addition, UV radiation, in particular UVB radiation, has been shown to induce cell cycle arrest in keratinocytes, the most common type of skin cell.[65] As such, sunlight therapy can be a candidate for treatment of conditions such as psoriasis and exfoliative cheilitis, conditions in which skin cells divide more rapidly than usual or necessary.[66]

Harmful effects

[edit]
Sunburn effect (as measured by the UV index) is the product of the sunlight spectrum (radiation intensity) and the erythemal action spectrum (skin sensitivity) across the range of UV wavelengths. Sunburn production per milliwatt of radiation intensity is increased by nearly a factor of 100 between the near UVB wavelengths of 315–295 nm.

In humans, excessive exposure to UV radiation can result in acute and chronic harmful effects on the eye's dioptric system and retina. The risk is elevated at high altitudes and people living in high latitude areas where snow covers the ground right into early summer and sun positions even at zenith are low, are particularly at risk.[67] Skin, the circadian system, and the immune system can also be affected.[68]

The differential effects of various wavelengths of light on the human cornea and skin are sometimes called the "erythemal action spectrum".[69] The action spectrum shows that UVA does not cause immediate reaction, but rather UV begins to cause photokeratitis and skin redness (with lighter skinned individuals being more sensitive) at wavelengths starting near the beginning of the UVB band at 315 nm, and rapidly increasing to 300 nm. The skin and eyes are most sensitive to damage by UV at 265–275 nm, which is in the lower UVC band. At still shorter wavelengths of UV, damage continues to happen, but the overt effects are not as great with so little penetrating the atmosphere. The WHO-standard ultraviolet index is a widely publicized measurement of total strength of UV wavelengths that cause sunburn on human skin, by weighting UV exposure for action spectrum effects at a given time and location. This standard shows that most sunburn happens due to UV at wavelengths near the boundary of the UVA and UVB bands.[citation needed]

Skin damage

[edit]
Ultraviolet photons harm the DNA molecules of living organisms in different ways. In one common damage event, adjacent thymine bases bond with each other, instead of across the "ladder". This "thymine dimer" makes a bulge, and the distorted DNA molecule does not function properly.

Overexposure to UVB radiation not only can cause sunburn but also some forms of skin cancer. However, the degree of redness and eye irritation (which are largely not caused by UVA) do not predict the long-term effects of UV, although they do mirror the direct damage of DNA by ultraviolet.[70]

All bands of UV radiation damage collagen fibers and accelerate aging of the skin. Both UVA and UVB destroy vitamin A in skin, which may cause further damage.[71]

UVB radiation can cause direct DNA damage.[72] This cancer connection is one reason for concern about ozone depletion and the ozone hole.

The most deadly form of skin cancer, melanoma, is mostly caused by DNA damage independent from UVA radiation. This can be seen from the absence of a direct UV signature mutation in 92% of all melanoma.[73] Occasional overexposure and sunburn are probably greater risk factors for melanoma than long-term moderate exposure.[74] UVC is the highest-energy, most-dangerous type of ultraviolet radiation, and causes adverse effects that can variously be mutagenic or carcinogenic.[75]

In the past, UVA was considered not harmful or less harmful than UVB, but today it is known to contribute to skin cancer via indirect DNA damage (free radicals such as reactive oxygen species).[76] UVA can generate highly reactive chemical intermediates, such as hydroxyl and oxygen radicals, which in turn can damage DNA. The DNA damage caused indirectly to skin by UVA consists mostly of single-strand breaks in DNA, while the damage caused by UVB includes direct formation of thymine dimers or cytosine dimers and double-strand DNA breakage.[77] UVA is immunosuppressive for the entire body (accounting for a large part of the immunosuppressive effects of sunlight exposure), and is mutagenic for basal cell keratinocytes in skin.[78]

UVB photons can cause direct DNA damage. UVB radiation excites DNA molecules in skin cells, causing aberrant covalent bonds to form between adjacent pyrimidine bases, producing a dimer. Most UV-induced pyrimidine dimers in DNA are removed by the process known as nucleotide excision repair that employs about 30 different proteins.[72] Those pyrimidine dimers that escape this repair process can induce a form of programmed cell death (apoptosis) or can cause DNA replication errors leading to mutation.[citation needed]

UVB damages mRNA[79] This triggers a fast pathway that leads to inflammation of the skin and sunburn. mRNA damage initially triggers a response in ribosomes though a protein known as ZAK-alpha in a ribotoxic stress response. This response acts as a cell surveillance system. Following this detection of RNA damage leads to inflammatory signaling and recruitment of immune cells. This, not DNA damage (which is slower to detect) results in UVB skin inflammation and acute sunburn.[80]

As a defense against UV radiation, the amount of the brown pigment melanin in the skin increases when exposed to moderate (depending on skin type) levels of radiation; this is commonly known as a sun tan. The purpose of melanin is to absorb UV radiation and dissipate the energy as harmless heat, protecting the skin against both direct and indirect DNA damage from the UV. UVA gives a quick tan that lasts for days by oxidizing melanin that was already present and triggers the release of the melanin from melanocytes. UVB yields a tan that takes roughly 2 days to develop because it stimulates the body to produce more melanin.[citation needed]

Sunscreen safety debate

[edit]
Demonstration of the effect of sunscreen. The left image is a regular photograph of his face; the right image is of reflected UV light. The man's face has sunscreen on his right side only. It appears darker because the sunscreen absorbs the UV light.

Medical organizations recommend that patients protect themselves from UV radiation by using sunscreen. Five sunscreen ingredients have been shown to protect mice against skin tumors. However, some sunscreen chemicals produce potentially harmful substances if they are illuminated while in contact with living cells.[81][82] The amount of sunscreen that penetrates into the lower layers of the skin may be large enough to cause damage.[83]

Sunscreen reduces the direct DNA damage that causes sunburn, by blocking UVB, and the usual SPF rating indicates how effectively this radiation is blocked. SPF is, therefore, also called UVB-PF, for "UVB protection factor".[84] This rating, however, offers no data about important protection against UVA,[85] which does not primarily cause sunburn but is still harmful, since it causes indirect DNA damage and is also considered carcinogenic. Several studies suggest that the absence of UVA filters may be the cause of the higher incidence of melanoma found in sunscreen users compared to non-users.[86][87][88][89][90] Some sunscreen lotions contain titanium dioxide, zinc oxide, and avobenzone, which help protect against UVA rays.

The photochemical properties of melanin make it an excellent photoprotectant. However, sunscreen chemicals cannot dissipate the energy of the excited state as efficiently as melanin and therefore, if sunscreen ingredients penetrate into the lower layers of the skin, the amount of reactive oxygen species may be increased.[91][81][82][92] The amount of sunscreen that penetrates through the stratum corneum may or may not be large enough to cause damage.

In an experiment by Hanson et al. that was published in 2006, the amount of harmful reactive oxygen species (ROS) was measured in untreated and in sunscreen treated skin. In the first 20 minutes, the film of sunscreen had a protective effect and the number of ROS species was smaller. After 60 minutes, however, the amount of absorbed sunscreen was so high that the amount of ROS was higher in the sunscreen-treated skin than in the untreated skin.[91] The study indicates that sunscreen must be reapplied within 2 hours in order to prevent UV light from penetrating to sunscreen-infused live skin cells.[91]

Aggravation of certain skin conditions

[edit]

Ultraviolet radiation can aggravate several skin conditions and diseases, including[93] systemic lupus erythematosus, Sjögren's syndrome, Sinear Usher syndrome, rosacea, dermatomyositis, Darier's disease, Kindler–Weary syndrome and Porokeratosis.[94]

Eye damage

[edit]
Signs are often used to warn of the hazard of strong UV sources.

The eye is most sensitive to damage by UV in the lower UVC band at 265–275 nm. Radiation of this wavelength is almost absent from sunlight at the surface of the Earth but is emitted by artificial sources such as the electrical arcs employed in arc welding. Unprotected exposure to these sources can cause "welder's flash" or "arc eye" (photokeratitis) and can lead to cataracts, pterygium and pinguecula formation. To a lesser extent, UVB in sunlight from 310 to 280 nm also causes photokeratitis ("snow blindness"), and the cornea, the lens, and the retina can be damaged.[95]

Protective eyewear is beneficial to those exposed to ultraviolet radiation. Since light can reach the eyes from the sides, full-coverage eye protection is usually warranted if there is an increased risk of exposure, as in high-altitude mountaineering. Mountaineers are exposed to higher-than-ordinary levels of UV radiation, both because there is less atmospheric filtering and because of reflection from snow and ice.[96][97] Ordinary, untreated eyeglasses give some protection. Most plastic lenses give more protection than glass lenses, because, as noted above, glass is transparent to UVA and the common acrylic plastic used for lenses is less so. Some plastic lens materials, such as polycarbonate, inherently block most UV.[98]

Degradation of polymers, pigments and dyes

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UV damaged polypropylene rope (left) and new rope (right)

UV degradation is one form of polymer degradation that affects plastics exposed to sunlight. The problem appears as discoloration or fading, cracking, loss of strength or disintegration. The effects of attack increase with exposure time and sunlight intensity. The addition of UV absorbers inhibits the effect.

IR spectrum showing carbonyl absorption due to UV degradation of polyethylene

Sensitive polymers include thermoplastics and speciality fibers like aramids. UV absorption leads to chain degradation and loss of strength at sensitive points in the chain structure. Aramid rope must be shielded with a sheath of thermoplastic if it is to retain its strength.[citation needed]

Many pigments and dyes absorb UV and change colour, so paintings and textiles may need extra protection both from sunlight and fluorescent lamps, two common sources of UV radiation. Window glass absorbs some harmful UV, but valuable artifacts need extra shielding. Many museums place black curtains over watercolour paintings and ancient textiles, for example. Since watercolours can have very low pigment levels, they need extra protection from UV. Various forms of picture framing glass, including acrylics (plexiglass), laminates, and coatings, offer different degrees of UV (and visible light) protection.[99]

Applications

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Because of its ability to cause chemical reactions and excite fluorescence in materials, ultraviolet radiation has a number of applications. The following table[100] gives some uses of specific wavelength bands in the UV spectrum.

Photography

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A portrait taken using only UV light between the wavelengths of 335 and 365 nanometers

Photographic film responds to ultraviolet radiation but the glass lenses of cameras usually block radiation shorter than 350 nm. Slightly yellow UV-blocking filters are often used for outdoor photography to prevent unwanted bluing and overexposure by UV rays. For photography in the near UV, special filters may be used. Photography with wavelengths shorter than 350 nm requires special quartz lenses which do not absorb the radiation. Digital cameras sensors may have internal filters that block UV to improve color rendition accuracy. Sometimes these internal filters can be removed, or they may be absent, and an external visible-light filter prepares the camera for near-UV photography. A few cameras are designed for use in the UV.[102]

Photography by reflected ultraviolet radiation is useful for medical, scientific, and forensic investigations, in applications as widespread as detecting bruising of skin, alterations of documents, or restoration work on paintings. Photography of the fluorescence produced by ultraviolet illumination uses visible wavelengths of light.[citation needed]

Aurora at Jupiter's north pole as seen in ultraviolet light by the Hubble Space Telescope

In ultraviolet astronomy, measurements are used to discern the chemical composition of the interstellar medium, and the temperature and composition of stars. Because the ozone layer blocks many UV frequencies from reaching telescopes on the surface of the Earth, most UV observations are made from space.[103]

Electrical and electronics industry

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Corona discharge on electrical apparatus can be detected by its ultraviolet emissions. Corona causes degradation of electrical insulation and emission of ozone and nitrogen oxide.[104]

EPROMs (Erasable Programmable Read-Only Memory) are erased by exposure to UV radiation. These modules have a transparent (quartz) window on the top of the chip that allows the UV radiation in.

Fluorescent dye uses

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Colorless fluorescent dyes that emit blue light under UV are added as optical brighteners to paper and fabrics. The blue light emitted by these agents counteracts yellow tints that may be present and causes the colors and whites to appear whiter or more brightly colored.

UV fluorescent dyes that glow in the primary colors are used in paints, papers, and textiles either to enhance color under daylight illumination or to provide special effects when lit with UV lamps. Blacklight paints that contain dyes that glow under UV are used in a number of art and aesthetic applications.[citation needed]

A bird appears on many Visa credit cards when they are held under a UV light source.

To help prevent counterfeiting of currency, or forgery of important documents such as driver's licenses and passports, the paper may include a UV watermark or fluorescent multicolor fibers that are visible under ultraviolet light. Postage stamps are tagged with a phosphor that glows under UV rays to permit automatic detection of the stamp and facing of the letter.

UV fluorescent dyes are used in many applications (for example, biochemistry and forensics). Some brands of pepper spray will leave an invisible chemical (UV dye) that is not easily washed off on a pepper-sprayed attacker, which would help police identify the attacker later.

In some types of nondestructive testing UV stimulates fluorescent dyes to highlight defects in a broad range of materials. These dyes may be carried into surface-breaking defects by capillary action (liquid penetrant inspection) or they may be bound to ferrite particles caught in magnetic leakage fields in ferrous materials (magnetic particle inspection).

Analytic uses

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Forensics

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UV is an investigative tool at the crime scene helpful in locating and identifying bodily fluids such as semen, blood, and saliva.[105] For example, ejaculated fluids or saliva can be detected by high-power UV sources, irrespective of the structure or colour of the surface the fluid is deposited upon.[106] UV–vis microspectroscopy is also used to analyze trace evidence, such as textile fibers and paint chips, as well as questioned documents.

Other applications include the authentication of various collectibles and art, and detecting counterfeit currency. Even materials not specially marked with UV sensitive dyes may have distinctive fluorescence under UV exposure or may fluoresce differently under short-wave versus long-wave ultraviolet.

Enhancing contrast of ink

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Using multi-spectral imaging it is possible to read illegible papyrus, such as the burned papyri of the Villa of the Papyri or of Oxyrhynchus, or the Archimedes palimpsest. The technique involves taking pictures of the illegible document using different filters in the infrared or ultraviolet range, finely tuned to capture certain wavelengths of light. Thus, the optimum spectral portion can be found for distinguishing ink from paper on the papyrus surface.

Simple NUV sources can be used to highlight faded iron-based ink on vellum.[107]

Sanitary compliance

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A person wearing full protective gear, glowing in ultraviolet light
After a training exercise involving fake body fluids, a healthcare worker's personal protective equipment is checked with ultraviolet to find invisible drops of fluids. These fluids could contain deadly viruses or other contamination.

Ultraviolet helps detect organic material deposits that remain on surfaces where periodic cleaning and sanitizing may have failed. It is used in the hotel industry, manufacturing, and other industries where levels of cleanliness or contamination are inspected.[108][109][110][111]

Perennial news features for many television news organizations involve an investigative reporter using a similar device to reveal unsanitary conditions in hotels, public toilets, hand rails, and such.[112][113]

Chemistry

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UV/Vis spectroscopy is widely used as a technique in chemistry to analyze chemical structure, the most notable one being conjugated systems. UV radiation is often used to excite a given sample where the fluorescent emission is measured with a spectrofluorometer. In biological research, UV radiation is used for quantification of nucleic acids or proteins. In environmental chemistry, UV radiation could also be used to detect Contaminants of emerging concern in water samples.[114]

In pollution control applications, ultraviolet analyzers are used to detect emissions of nitrogen oxides, sulfur compounds, mercury, and ammonia, for example in the flue gas of fossil-fired power plants.[115] Ultraviolet radiation can detect thin sheens of spilled oil on water, either by the high reflectivity of oil films at UV wavelengths, fluorescence of compounds in oil, or by absorbing of UV created by Raman scattering in water.[116] UV absorbance can also be used to quantify contaminants in wastewater. Most commonly used 254 nm UV absorbance is generally used as a surrogate parameters to quantify NOM.[114] Another form of light-based detection uses an excitation-emission matrix (EEM) to detect and identify contaminants based on their fluorescence properties.[114][117] EEM could be used to discriminate different groups of NOM based on the difference in light emission and excitation of fluorophores. NOMs with certain molecular structures are reported to have fluorescent properties in a wide range of excitation/emission wavelengths.[118][114]

A collection of mineral samples fluorescing brilliantly at various wavelengths as seen while being irradiated by UV

Ultraviolet lamps are also used as part of the analysis of some minerals and gems.

Material science uses

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Fire detection

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In general, ultraviolet detectors use either a solid-state device, such as one based on silicon carbide or aluminium nitride, or a gas-filled tube as the sensing element. UV detectors that are sensitive to UV in any part of the spectrum respond to irradiation by sunlight and artificial light. A burning hydrogen flame, for instance, radiates strongly in the 185- to 260-nanometer range and only very weakly in the IR region, whereas a coal fire emits very weakly in the UV band yet very strongly at IR wavelengths; thus, a fire detector that operates using both UV and IR detectors is more reliable than one with a UV detector alone. Virtually all fires emit some radiation in the UVC band, whereas the Sun's radiation at this band is absorbed by the Earth's atmosphere. The result is that the UV detector is "solar blind", meaning it will not cause an alarm in response to radiation from the Sun, so it can easily be used both indoors and outdoors.

UV detectors are sensitive to most fires, including hydrocarbons, metals, sulfur, hydrogen, hydrazine, and ammonia. Arc welding, electrical arcs, lightning, X-rays used in nondestructive metal testing equipment (though this is highly unlikely), and radioactive materials can produce levels that will activate a UV detection system. The presence of UV-absorbing gases and vapors will attenuate the UV radiation from a fire, adversely affecting the ability of the detector to detect flames. Likewise, the presence of an oil mist in the air or an oil film on the detector window will have the same effect.

Photolithography

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Ultraviolet radiation is used for very fine resolution photolithography, a procedure wherein a chemical called a photoresist is exposed to UV radiation that has passed through a mask. The exposure causes chemical reactions to occur in the photoresist. After removal of unwanted photoresist, a pattern determined by the mask remains on the sample. Steps may then be taken to "etch" away, deposit on or otherwise modify areas of the sample where no photoresist remains.

Photolithography is used in the manufacture of semiconductors, integrated circuit components,[119] and printed circuit boards. Photolithography processes used to fabricate electronic integrated circuits presently use 193 nm UV and are experimentally using 13.5 nm UV for extreme ultraviolet lithography.

Polymers

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Electronic components that require clear transparency for light to exit or enter (photovoltaic panels and sensors) can be potted using acrylic resins that are cured using UV energy. The advantages are low VOC emissions and rapid curing.

Effects of UV on finished surfaces in 0, 20 and 43 hours

Certain inks, coatings, and adhesives are formulated with photoinitiators and resins. When exposed to UV light, polymerization occurs, and so the adhesives harden or cure, usually within a few seconds. Applications include glass and plastic bonding, optical fiber coatings, the coating of flooring, UV coating and paper finishes in offset printing, dental fillings, and decorative fingernail "gels".

UV sources for UV curing applications include UV lamps, UV LEDs, and excimer flash lamps. Fast processes such as flexo or offset printing require high-intensity light focused via reflectors onto a moving substrate and medium so high-pressure Hg (mercury) or Fe (iron, doped)-based bulbs are used, energized with electric arcs or microwaves. Lower-power fluorescent lamps and LEDs can be used for static applications. Small high-pressure lamps can have light focused and transmitted to the work area via liquid-filled or fiber-optic light guides.

The impact of UV on polymers is used for modification of the (roughness and hydrophobicity) of polymer surfaces. For example, a poly(methyl methacrylate) surface can be smoothed by vacuum ultraviolet.[120]

UV radiation is useful in preparing low-surface-energy polymers for adhesives. Polymers exposed to UV will oxidize, thus raising the surface energy of the polymer. Once the surface energy of the polymer has been raised, the bond between the adhesive and the polymer is stronger.

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Air purification

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UV-C light is used in air conditioning systems as a method of improving indoor air quality by disinfecting the air and preventing microbial growth. UV-C light is effective at killing or inactivating harmful microorganisms, such as bacteria, viruses, mold, and mildew. When integrated into an air conditioning system, the ultraviolet light is typically placed in areas like the air handler or near the evaporator coil. In air conditioning systems, UV-C light works by irradiating the airflow within the system, killing or neutralizing harmful microorganisms before they are recirculated into the indoor environment. The effectiveness of it in air conditioning systems depends on factors such as the intensity of the light, the duration of exposure, airflow speed, and the cleanliness of system components.[121][122]

Using a catalytic chemical reaction from titanium dioxide and UVC exposure, oxidation of organic matter converts pathogens, pollens, and mold spores into harmless inert byproducts. However, the reaction of titanium dioxide and UVC is not a straight path. Several hundreds of reactions occur prior to the inert byproducts stage and can hinder the resulting reaction creating formaldehyde, aldehyde, and other VOC's en route to a final stage. Thus, the use of titanium dioxide and UVC requires very specific parameters for a successful outcome. The cleansing mechanism of UV is a photochemical process. Contaminants in the indoor environment are almost entirely organic carbon-based compounds, which break down when exposed to high-intensity UV at 240 to 280 nm. Short-wave ultraviolet radiation can destroy DNA in living microorganisms.[123] UVC's effectiveness is directly related to intensity and exposure time.

UV has also been shown to reduce gaseous contaminants such as carbon monoxide and VOCs.[124][125][126] UV lamps radiating at 184 and 254 nm can remove low concentrations of hydrocarbons and carbon monoxide if the air is recycled between the room and the lamp chamber. This arrangement prevents the introduction of ozone into the treated air. Likewise, air may be treated by passing by a single UV source operating at 184 nm and passed over iron pentaoxide to remove the ozone produced by the UV lamp.

Sterilization and disinfection

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A low-pressure mercury vapor discharge tube floods the inside of a hood with shortwave UV light when not in use, sterilizing microbiological contaminants from irradiated surfaces.

Ultraviolet lamps are used to sterilize workspaces and tools used in biology laboratories and medical facilities. Commercially available low-pressure mercury-vapor lamps emit about 86% of their radiation at 254 nanometers (nm), with 265 nm being the peak germicidal effectiveness curve. UV at these germicidal wavelengths damage a microorganism's DNA/RNA so that it cannot reproduce, making it harmless, (even though the organism may not be killed).[127] Since microorganisms can be shielded from ultraviolet rays in small cracks and other shaded areas, these lamps are used only as a supplement to other sterilization techniques.

UVC LEDs are relatively new to the commercial market and are gaining in popularity.[failed verification][128] Due to their monochromatic nature (±5 nm)[failed verification] these LEDs can target a specific wavelength needed for disinfection. This is especially important knowing that pathogens vary in their sensitivity to specific UV wavelengths. LEDs are mercury free, instant on/off, and have unlimited cycling throughout the day.[129]

Disinfection using UV radiation is commonly used in wastewater treatment applications and is finding an increased usage in municipal drinking water treatment. Many bottlers of spring water use UV disinfection equipment to sterilize their water. Solar water disinfection[130] has been researched for cheaply treating contaminated water using natural sunlight. The UVA irradiation and increased water temperature kill organisms in the water.

Ultraviolet radiation is used in several food processes to kill unwanted microorganisms. UV can be used to pasteurize fruit juices by flowing the juice over a high-intensity ultraviolet source. The effectiveness of such a process depends on the UV absorbance of the juice.

Pulsed light (PL) is a technique of killing microorganisms on surfaces using pulses of an intense broad spectrum, rich in UVC between 200 and 280 nm. Pulsed light works with xenon flash lamps that can produce flashes several times per second. Disinfection robots use pulsed UV.[131]

The antimicrobial effectiveness of filtered far-UVC (222 nm) light on a range of pathogens, including bacteria and fungi showed inhibition of pathogen growth, and since it has lesser harmful effects, it provides essential insights for reliable disinfection in healthcare settings, such as hospitals and long-term care homes.[132] UVC has also been shown to be effective at degrading SARS-CoV-2 virus.[133]

Biological

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Birds, reptiles, insects such as bees, and mammals such as mice, reindeer, dogs, and cats can see near-ultraviolet wavelengths.[134] Many fruits, flowers, and seeds stand out more strongly from the background in ultraviolet wavelengths as compared to human color vision. Scorpions glow or take on a yellow to green color under UV illumination, thus assisting in the control of these arachnids. Many birds have patterns in their plumage that are invisible at usual wavelengths but observable in ultraviolet, and the urine and other secretions of some animals, including dogs, cats, and human beings, are much easier to spot with ultraviolet. Urine trails of rodents can be detected by pest control technicians for proper treatment of infested dwellings.

Butterflies use ultraviolet as a communication system for sex recognition and mating behavior. For example, in the Colias eurytheme butterfly, males rely on visual cues to locate and identify females. Instead of using chemical stimuli to find mates, males are attracted to the ultraviolet-reflecting color of female hind wings.[135] In Pieris napi butterflies it was shown that females in northern Finland with less UV-radiation present in the environment possessed stronger UV signals to attract their males than those occurring further south. This suggested that it was evolutionarily more difficult to increase the UV-sensitivity of the eyes of the males than to increase the UV-signals emitted by the females.[136]

Many insects use the ultraviolet wavelength emissions from celestial objects as references for flight navigation. A local ultraviolet emitter will normally disrupt the navigation process and will eventually attract the flying insect.

Entomologist using a UV lamp for collecting beetles in Chaco, Paraguay

The green fluorescent protein (GFP) is often used in genetics as a marker. Many substances, such as proteins, have significant light absorption bands in the ultraviolet that are of interest in biochemistry and related fields. UV-capable spectrophotometers are common in such laboratories.

Ultraviolet traps called bug zappers are used to eliminate various small flying insects. They are attracted to the UV and are killed using an electric shock, or trapped once they come into contact with the device. Different designs of ultraviolet radiation traps are also used by entomologists for collecting nocturnal insects during faunistic survey studies.

Therapy

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Ultraviolet radiation is helpful in the treatment of skin conditions such as psoriasis and vitiligo. Exposure to UVA, while the skin is hyper-photosensitive, by taking psoralens is an effective treatment for psoriasis. Due to the potential of psoralens to cause damage to the liver, PUVA therapy may be used only a limited number of times over a patient's lifetime.

UVB phototherapy does not require additional medications or topical preparations for the therapeutic benefit; only the exposure is needed. However, phototherapy can be effective when used in conjunction with certain topical treatments such as anthralin, coal tar, and vitamin A and D derivatives, or systemic treatments such as methotrexate and Soriatane.[137]

Herpetology

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Reptiles need UVB for biosynthesis of vitamin D, and other metabolic processes.[138] Specifically cholecalciferol (vitamin D3), which is needed for basic cellular / neural functioning as well as the utilization of calcium for bone and egg production.[citation needed] The UVA wavelength is also visible to many reptiles and might play a significant role in their ability survive in the wild as well as in visual communication between individuals.[citation needed] Therefore, in a typical reptile enclosure, a fluorescent UV a/b source (at the proper strength / spectrum for the species), must be available for many[which?] captive species to survive. Simple supplementation with cholecalciferol (Vitamin D3) will not be enough as there is a complete biosynthetic pathway[which?] that is "leapfrogged" (risks of possible overdoses), the intermediate molecules and metabolites[which?] also play important functions in the animals health.[citation needed] Natural sunlight in the right levels is always going to be superior to artificial sources, but this might not be possible for keepers in different parts of the world.[citation needed]

It is a known problem that high levels of output of the UVa part of the spectrum can both cause cellular and DNA damage to sensitive parts of their bodies – especially the eyes where blindness is the result of an improper UVa/b source use and placement photokeratitis.[citation needed] For many keepers there must also be a provision for an adequate heat source this has resulted in the marketing of heat and light "combination" products.[citation needed] Keepers should be careful of these "combination" light/ heat and UVa/b generators, they typically emit high levels of UVa with lower levels of UVb that are set and difficult to control so that animals can have their needs met.[citation needed] A better strategy is to use individual sources of these elements and so they can be placed and controlled by the keepers for the max benefit of the animals.[139]

Evolutionary significance

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The evolution of early reproductive proteins and enzymes is attributed in modern models of evolutionary theory to ultraviolet radiation. UVB causes thymine base pairs next to each other in genetic sequences to bond together into thymine dimers, a disruption in the strand that reproductive enzymes cannot copy. This leads to frameshifting during genetic replication and protein synthesis, usually killing the cell. Before formation of the UV-blocking ozone layer, when early prokaryotes approached the surface of the ocean, they almost invariably died out. The few that survived had developed enzymes that monitored the genetic material and removed thymine dimers by nucleotide excision repair enzymes. Many enzymes and proteins involved in modern mitosis and meiosis are similar to repair enzymes, and are believed to be evolved modifications of the enzymes originally used to overcome DNA damages caused by UV.[140]

Elevated levels of ultraviolet radiation, in particular UV-B, have also been speculated as a cause of mass extinctions in the fossil record.[141]

Photobiology

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Photobiology is the scientific study of the beneficial and harmful interactions of non-ionizing radiation in living organisms, conventionally demarcated around 10 eV, the first ionization energy of oxygen. UV ranges roughly from 3 to 30 eV in energy. Hence photobiology entertains some, but not all, of the UV spectrum.

See also

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References

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Further reading

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Ultraviolet (UV) radiation constitutes a segment of the electromagnetic spectrum with wavelengths spanning approximately 10 to 400 nanometers, positioned between visible light and X-rays, and thus imperceptible to the human eye. It is conventionally divided into three bands based on wavelength: UVA (315–400 nm), which penetrates deeply into materials; UVB (280–315 nm), which is partially absorbed by the Earth's ozone layer; and UVC (100–280 nm), which is almost entirely blocked by atmospheric ozone and poses the highest energy per photon. The primary natural source of UV radiation is the Sun, where it constitutes about 10% of total solar output, though artificial sources such as mercury-vapor lamps and LEDs replicate these wavelengths for various uses. UV radiation interacts with matter through photochemical reactions, exciting electrons in atoms and molecules to induce fluorescence, dissociation, or ionization, which underpins both its biological effects and technological applications. Biologically, moderate UVB exposure triggers cutaneous synthesis of vitamin D, essential for calcium homeostasis and immune function, yet prolonged or intense exposure—particularly UVA and UVB—damages DNA via pyrimidine dimer formation, leading to erythema (sunburn), premature skin aging, and elevated risk of non-melanoma skin cancers and melanoma. UVC, while germicidal due to its capacity to inactivate microorganisms by disrupting their nucleic acids, does not naturally reach the surface but is harnessed artificially for disinfection. Notable applications exploit UV's high-energy properties, including sterilization of air, water, and surfaces via UVC lamps, which achieve log reductions in pathogens without chemical residues; UV curing of inks, adhesives, and coatings in manufacturing for rapid polymerization; and fluorescence induction in forensics, mineralogy, and counterfeit detection. Astronomically, UV observations reveal hot stellar phenomena and planetary atmospheres, as evidenced by Hubble Space Telescope imagery of Jupiter's auroras. Despite benefits, overreliance on UV tanning devices has drawn scrutiny for accelerating carcinogenesis, prompting regulatory limits in many jurisdictions.

Physical Characteristics

Wavelength Classification and Subtypes

Ultraviolet radiation occupies the portion of the electromagnetic spectrum with wavelengths from 10 to 400 nanometers (nm), shorter than visible light (approximately 400–700 nm) but longer than X-rays (below 10 nm). This range is subdivided primarily into UVA, UVB, and UVC bands, a classification established to distinguish differences in atmospheric absorption, biological impact, and applications. The boundaries align with empirical observations of ozone layer attenuation, where shorter wavelengths are more strongly absorbed. The standard divisions are as follows:
BandWavelength Range (nm)Characteristics
UVA315–400Longest UV wavelengths; penetrates deeply into materials and skin; constitutes about 95% of UV reaching Earth's surface from solar radiation.
UVB280–315Intermediate wavelengths; partially absorbed by ozone; responsible for most sunburn and skin cancer risk from solar exposure.
UVC100–280Shortest wavelengths in the primary classification; almost entirely absorbed by atmospheric oxygen and ozone; highly germicidal but hazardous without shielding.
These ranges, adopted by organizations including the World Health Organization and the U.S. Food and Drug Administration, facilitate consistent measurement and risk assessment in fields like photobiology and radiation safety. Variations in exact boundaries exist across standards, such as slight shifts in UVB-UVC cutoffs (e.g., 290 nm for terrestrial solar contexts), reflecting practical measurement thresholds rather than sharp physical discontinuities. Beyond these, finer subtypes address propagation and specialized uses. Vacuum ultraviolet (VUV), spanning roughly 10–200 nm, is absorbed by ambient air and thus requires vacuum conditions for transmission, limiting its terrestrial applications to controlled environments like spectroscopy. Extreme ultraviolet (EUV), from 10–121 nm (overlapping with VUV), ionizes gases readily and is employed in semiconductor lithography and astrophysical observations, as it does not penetrate Earth's atmosphere. Far UV (around 190–220 nm) represents a narrow band within UVC noted for protein damage without deep penetration, emerging in disinfection research. These extended subtypes emphasize causal differences in photon energy and interaction with matter, where higher energy (shorter wavelength) correlates with increased ionization potential and absorption by molecular bonds.

Visibility and Perception Across Species

The human eye does not perceive ultraviolet (UV) radiation due to absorption by the crystalline lens, which blocks wavelengths below approximately 400 nm, primarily through crystallins that absorb over 90% of UV-B (280–315 nm) and much of UV-A (315–400 nm). This filtration protects the retina from UV damage but renders UV invisible to humans, with sensitivity limited to the visible spectrum starting at violet light around 380–400 nm. UV sensitivity is widespread among non-mammalian vertebrates and invertebrates, enabled by ocular media that transmit short wavelengths and specialized photoreceptors with peak sensitivities around 360–373 nm in UV-sensitive (UVS) species or 402–426 nm in violet-sensitive (VS) types. Insects such as honeybees possess trichromatic vision incorporating UV, with spectral sensitivity from 300 to 650 nm, allowing detection of UV-reflective patterns on flowers that serve as nectar guides invisible to humans; these patterns enhance foraging efficiency by signaling rewarding areas. Birds universally exhibit UV vision, with transparent lenses and UVS or VS pigments facilitating roles in orientation, prey detection, and intraspecific signaling; for instance, UV reflectance in plumage reinforces structural color patterns used in mate choice, as demonstrated in species like starlings where UV components predict female preferences. Among mammals, UV perception is rare but documented in reindeer (Rangifer tarandus), whose retinas include UV-sensitive cones adapted for Arctic conditions; snow reflects up to 90% of UV, creating high contrast for detecting UV-absorbing lichens (a winter food source), urine trails indicating predators or conspecifics, and wolf fur against reflective backgrounds. This adaptation likely evolved post-migration to high latitudes, enhancing survival in low-visibility environments dominated by UV-reflective snow.

Historical Development

Early Observations and Discovery

In the late 18th century, investigations into the composition of sunlight using prisms had delineated the visible spectrum, with researchers such as Isaac Newton identifying its colored bands from red to violet. Following William Herschel's 1800 discovery of infrared radiation beyond the red end—demonstrated by thermometric heating of materials—attention turned to potential invisible rays at the opposite violet boundary. German physicist Johann Wilhelm Ritter, working in Jena, hypothesized that analogous effects might occur there, driven by observations of chemical reactivity in spectral regions. On February 22, 1801, Ritter conducted experiments exposing silver chloride-impregnated paper to sunlight dispersed through a prism. The paper, known to darken under visible light via photoreduction, exhibited maximal blackening not in the violet band but in an adjacent invisible region beyond it, indicating the presence of energetic rays with greater chemical potency than visible violet light. These rays, which Ritter termed "chemical rays" or "deoxidizing rays" due to their accelerating effect on silver chloride decomposition, were later recognized as ultraviolet radiation. Ritter's findings, published in Gilbert's Annalen der Physik, established ultraviolet as a distinct spectral extension, though he lacked precise wavelength measurements or understanding of its electromagnetic nature. Prior to Ritter, indirect hints of ultraviolet effects appeared in scattered observations, such as accelerated photographic darkening or fluorescence under certain lights, but these lacked systematic attribution to a specific spectral domain. Ritter's work thus marked the first deliberate identification of ultraviolet radiation as an invisible continuum analogous to infrared, laying groundwork for subsequent photochemical and spectroscopic studies despite initial skepticism regarding its uniformity and propagation.

Key Scientific Advancements and Instrumentation

Johann Wilhelm Ritter discovered ultraviolet radiation in 1801 through experiments demonstrating that silver chloride darkened more rapidly when exposed to light beyond the violet end of the visible spectrum than to visible light itself, establishing the existence of a shorter-wavelength region. This finding built on William Herschel's 1800 discovery of infrared, prompting systematic exploration of the electromagnetic spectrum's boundaries. In the late 19th century, advancements in detection included the bolometer invented by Samuel Langley in 1878, which measured radiant heat including ultraviolet by detecting temperature changes in absorbing materials, enabling quantitative assessment of UV intensity. Quartz prisms and lenses, transparent to UV unlike glass, facilitated early spectrographic instruments around 1900, allowing separation and study of UV wavelengths in emission and absorption spectra. These tools revealed UV lines in stellar spectra and atomic emissions, such as hydrogen's Lyman series in the far UV, measured using vacuum spectrographs by Robert Millikan in 1920 with high-intensity nickel spark sources. The commercialization of precise UV instrumentation accelerated in the 20th century with the development of the DU spectrophotometer by Arnold Beckman in 1941, the first viable commercial device for measuring ultraviolet light absorption with high resolution and low stray light, revolutionizing quantitative UV-Vis spectroscopy for chemical analysis. This instrument employed a quartz prism monochromator and photomultiplier tube detector, achieving wavelength accuracy to 1 nm and enabling applications in biochemistry and material science. Subsequent innovations, such as double-beam designs in the 1950s like the Cary 14, improved stability by compensating for source fluctuations, reducing analysis time from minutes to seconds. These advancements underpinned discoveries in molecular structure, including protein and nucleic acid characterization via UV absorbance at 280 nm and 260 nm, respectively.

Natural Sources

Solar Emission and Spectrum

The Sun's ultraviolet emission originates primarily from its photosphere for wavelengths above approximately 200 nm, with contributions from the chromosphere and corona at shorter wavelengths due to higher temperatures in those layers. The photosphere's effective temperature of 5770 K yields a spectral radiance that approximates blackbody radiation, peaking in the visible range near 500 nm but extending continuously into the ultraviolet with decreasing intensity toward shorter wavelengths. This results in substantial flux in the UVA (315–400 nm) and UVB (280–315 nm) bands from thermal continuum emission, while UVC (100–280 nm) features both weak continuum and strong discrete atomic and ionic lines from plasma at temperatures exceeding 10,000 K. At 1 astronomical unit, the total solar irradiance integrates to about 1366 W/m², with the ultraviolet component (100–400 nm) comprising roughly 8%, or approximately 110 W/m², based on high-resolution spectral measurements. Within this, UVA dominates with 70–85 W/m², UVB contributes 10–15 W/m², and UVC adds only a few W/m², primarily through emission lines rather than broadband continuum, as the Planck function falls exponentially below 300 nm for photospheric temperatures. Spectral data indicate peak irradiance near 300 nm at several mW/m²/nm, dropping to microwatts per m² per nm by 200 nm, reflecting the tail of the thermal spectrum. Ultraviolet emission, particularly below 200 nm, exhibits variability tied to the 11-year solar cycle, with increases of up to 100% in EUV flux during solar maximum due to enhanced chromospheric and coronal activity, while longer-wavelength UV varies by only a few percent. Observations from satellites like SORCE and TIMED have refined these profiles, confirming deviations from ideal blackbody behavior, such as excess emission in far-UV from non-thermal processes.

Atmospheric Absorption and Transmission

Earth's atmosphere significantly attenuates incoming solar ultraviolet (UV) radiation through absorption by molecular species, preventing most short-wavelength UV from reaching the surface. Molecular oxygen (O2) in the upper atmosphere absorbs UVC wavelengths (100–280 nm) via the Schumann-Runge bands (175–205 nm) and Herzberg continuum (200–240 nm), while stratospheric ozone (O3) provides the primary absorption for UVB (280–315 nm) through its Hartley band, peaking near 255 nm and extending to about 320 nm. UVC is effectively completely absorbed above 100 km altitude, and nearly all UVB is filtered out, with water vapor, carbon dioxide, and nitrogen contributing minor additional absorption. Transmission to the surface varies by UV subtype: virtually no UVC penetrates, approximately 5% of UVB reaches sea level under overhead sun conditions with typical total ozone column of 300 Dobson units (DU), and over 95% of arriving UV is UVA (315–400 nm), which experiences low absorption except for weak O3 tail effects above 340 nm. The ozone layer, concentrated between 15–35 km altitude, accounts for the bulk of UVB shielding, with absorption efficiency increasing with path length through the atmosphere; at higher solar zenith angles, transmission decreases due to longer optical paths. Atmospheric transmission exhibits "windows" where absorption is minimal, notably in the UVA range (320–400 nm), allowing penetration for photochemical and biological processes, though aerosols and clouds can further attenuate by 10–40% depending on optical depth and type. Variations in total ozone column—ranging from 220 DU at poles to 300+ DU in tropics—affect UVB transmission inversely, with depletions of 1% increasing surface UVB by about 1.3–2% at mid-latitudes. Oxygen and ozone dissociation products in the mesosphere also contribute to far-UV absorption, maintaining the planet's radiative balance by converting UV energy to heat.

Artificial Generation

Conventional Lamps and Discharges

Low-pressure mercury-vapor discharge lamps represent a primary conventional source of ultraviolet radiation, operating by ionizing mercury vapor at pressures around 1 Pa (0.01 mbar) to produce prominent emission lines at 253.7 nm and 185.0 nm within the UVC range. These lamps, encased in quartz or fused silica envelopes to transmit short wavelengths, generate UV through electron collisions exciting mercury atoms, followed by de-excitation. Commercial germicidal variants emerged in the 1930s via Westinghouse, targeting microbial inactivation without chemical additives. High-pressure mercury arc lamps, by contrast, sustain discharges at 10–100 atm, yielding a continuum spectrum overlaid with atomic lines across UVA (315–400 nm), UVB (280–315 nm), and UVC, alongside visible output. Emission efficiency peaks in UV bands like 365 nm and 405 nm, with total radiant flux scaling to hundreds of watts; these require robust cooling due to thermal loads exceeding 1000 K. Applications include photolithography and curing, where the broader band enables material excitation beyond narrow-line sources. Deuterium (D₂) arc lamps provide a continuous UV spectrum from approximately 160 nm to 400 nm, with negligible visible and infrared output, achieved via a continuous electrical discharge through deuterium gas in a quartz bulb. Operating at currents of 5–30 A, they deliver stable flux for spectroscopy, outperforming hydrogen variants in deep-UV intensity due to isotopic effects on molecular emission. Lifetimes typically reach 1000–2000 hours before significant degradation. Xenon short-arc lamps generate broadband UV from 200 nm upward through high-current (20–500 A) arcs in xenon gas at 10–50 atm, mimicking solar spectra with strong lines below 400 nm. These ozone-free designs (emitting insufficient <242 nm to form O₃ in air paths) suit microscopy and solar simulation, though UV output constitutes 10–20% of total power. Electrode erosion limits operational life to 1000 hours at full intensity. Fluorescent discharge tubes, often mercury-based with phosphors, convert 254 nm excitation to UVA (e.g., 365 nm peak) for blacklight applications, extending effective emission while filtering harmful shorter wavelengths.

Modern Technologies Including LEDs and Lasers

Ultraviolet light-emitting diodes (UV LEDs) emerged as compact, mercury-free alternatives to conventional UV lamps, leveraging semiconductor materials like aluminum gallium nitride (AlGaN) for emission across UVA (315–400 nm), UVB (280–315 nm), and UVC (100–280 nm) bands. Efforts to develop UV LEDs intensified in Japan during the 1980s, culminating in the first UV-emitting LED in 1992. Commercial UVC LEDs followed in 2002, initially limited by low efficiency and output power but enabling initial applications in curing and sensing. Deep-UV LEDs, targeting wavelengths below 280 nm for germicidal purposes, achieved early prototypes around 2001, with sufficient stability for biochemical detection by 2005. Advancements in epitaxial growth and defect reduction have improved performance, though challenges persist at shorter wavelengths due to high aluminum content increasing dislocation densities and reducing quantum efficiency. By 2020, UVA LEDs at 395 nm reached wall-plug efficiencies of 60% in optimized designs incorporating advanced quantum wells. Shorter-wavelength UVC LEDs exhibit lower efficiencies, often below 10% for 265 nm emission, with power outputs scaling inversely with wavelength—typically milliwatts for deep UVC versus watts for UVA. These devices offer instantaneous response, directional emission, and lifetimes exceeding 10,000 hours, surpassing gas-discharge lamps in reliability for portable disinfection and water purification systems. Ultraviolet lasers generate coherent UV radiation through stimulated emission, providing superior beam quality and intensity for micromachining, spectroscopy, and photolithography compared to incoherent sources. Solid-state UV lasers, such as frequency-tripled neodymium-doped yttrium aluminum garnet (Nd:YAG) systems, produce 355 nm output by converting 1064 nm infrared via nonlinear crystals like beta barium borate, with pulse energies reaching joules in Q-switched configurations. Excimer lasers, employing electrically excited rare-gas halide mixtures (e.g., KrF at 248 nm or ArF at 193 nm), deliver high peak powers in the kilowatt range per pulse, essential for semiconductor patterning since their commercialization in the late 1970s. Recent progress favors all-solid-state architectures over gas-based excimers, minimizing maintenance and enabling continuous-wave operation at powers up to hundreds of milliwatts in the 200–400 nm range. Direct diode-pumped UV lasers and fiber-based systems further enhance efficiency, achieving conversion efficiencies above 20% for deep-UV harmonics, though vacuum-ultraviolet (below 200 nm) remains dominated by excimer types due to material absorption limits. These technologies prioritize precision over broad-area illumination, with applications constrained by cost and complexity relative to LEDs.

Interactions with Materials

Absorption Mechanisms and Protective Materials

Ultraviolet radiation is absorbed by materials primarily through electronic transitions in molecules, where photons excite valence electrons from ground states to higher-energy orbitals, such as π→π* transitions in conjugated systems or n→π* transitions involving non-bonding electrons. This process follows the Beer-Lambert law, where absorbance A=ϵclA = \epsilon c l (with ϵ\epsilon as molar absorptivity, cc as concentration, and ll as path length), determining the extent of attenuation at specific wavelengths typically between 200–400 nm. Chromophores like aromatic rings or carbonyl groups dictate absorption spectra; for instance, in wood absorbs UVB (280–315 nm) via its phenolic structures, initiating photodegradation through radical formation. In polymers and organic materials, UV absorption often leads to bond cleavage or energy transfer, causing chain scission or cross-linking; polyethylene, for example, absorbs below 300 nm due to carbonyl impurities, accelerating oxidation. Inorganic materials like metal oxides (e.g., TiO₂) absorb via band-gap excitations, with TiO₂'s gap at ~3.2 eV corresponding to ~387 nm, enabling photocatalysis but also protection when engineered. Protective materials mitigate UV damage via absorption, reflection, or scattering. Organic UV absorbers, such as 2-hydroxybenzophenones or benzotriazoles, are incorporated into polymers at 0.1–2% concentrations; they harvest UV photons (290–400 nm), undergo keto-enol tautomerism or intramolecular proton transfer, and dissipate energy as heat without emitting harmful radiation. Inorganic blockers like zinc oxide or titanium dioxide nanoparticles (20–100 nm) reflect and scatter UVA/UVB via Mie scattering, with ZnO effective up to 380 nm due to its 3.37 eV band gap, often used in sunscreens at 5–25% loadings for broad-spectrum coverage. ![UV and Visible Sunscreen demonstration][float-right] Hybrid systems combine these; for coatings and plastics, blends of absorbers with hindered amine light stabilizers (HALS) extend durability by scavenging radicals post-absorption, as seen in automotive clearcoats where UV stabilizers maintain gloss retention beyond 2000 hours of accelerated weathering. Fabrics treated with UV-absorbing dyes or metal nanoparticles achieve UPF ratings >50, blocking >98% transmission, though laundering reduces efficacy by 20–30% over 20 cycles due to leaching. These mechanisms prioritize causal prevention of photodegradation, with efficacy verified by spectrophotometry and accelerated aging tests per ISO 4892-2 standards.

Degradation Effects on Polymers, Pigments, and Organics

Ultraviolet radiation induces photodegradation in polymers through photo-oxidative processes, where UV photons are absorbed by chromophoric groups, generating excited states that react with oxygen to form free radicals, leading to chain scission, cross-linking, and reduced molecular weight. This results in mechanical property losses, including decreased tensile strength, elongation, and impact resistance, as well as surface chalking and cracking in materials like polyethylene and polypropylene. For instance, exposure to UV-B (280-315 nm) accelerates embrittlement in high-density polyethylene (HDPE), with studies showing significant yellowing and structural weakening after prolonged irradiation. Polypropylene exhibits particularly rapid degradation under sunlight, forming carbonyl groups indicative of oxidation. In pigments and dyes, UV light triggers photochemical reactions that break molecular bonds, causing fading by altering chromophores and reducing the pigment's ability to absorb or reflect specific wavelengths. Darker pigments, which absorb more UV due to broader spectral coverage, fade faster than lighter ones, as seen in exterior paints where UV exposure leads to loss of vibrancy over months to years. Organic pigments like anthraquinone derivatives show enhanced polymer degradation when incorporated into plastics, promoting brittle fragmentation under UV, while high-lightfastness dyes require UV energy above visible light thresholds for breakdown. Organic materials, including natural polymers like cellulose in wood and synthetic organics, undergo similar photolytic cleavage, producing lower molecular weight fragments such as organic acids and releasing volatile compounds. In finished wood surfaces, UV exposure causes lignin breakdown, resulting in graying, surface erosion, and loss of gloss within weeks of outdoor exposure, as the 290-400 nm range penetrates and oxidizes phenolic structures. For dyes in textiles or coatings, UV-induced radical formation leads to decolorization, with unstable variants fading under combined UV and visible light, emphasizing the role of oxygen in accelerating these reactions. These effects underscore UV's causal role in material aging, driven by energy transfer exceeding bond dissociation thresholds in C-H, C-C, and C=O linkages.

Biological Interactions

Photobiology Fundamentals

Ultraviolet radiation interacts with biological systems through absorption by key biomolecules, initiating photochemical reactions that can alter molecular structure and function. In photobiology, UV wavelengths, particularly UVB (280–315 nm), are absorbed primarily by nucleic acids and proteins due to their chromophoric groups. DNA bases, especially pyrimidines like thymine and cytosine, exhibit strong absorption maxima around 260 nm, enabling direct excitation upon UV exposure. This absorption promotes electrons to higher energy states, often resulting in ultrafast non-radiative decay or, critically, the formation of covalent lesions such as cyclobutane pyrimidine dimers (CPDs). The predominant direct photoproduct from UVB irradiation is the cis-syn cyclobutane thymine dimer (T<>T), formed between adjacent thymine bases in DNA via a [2+2] cycloaddition reaction occurring on femtosecond timescales. Similar dimers involving cytosine or mixed pyrimidine pairs, as well as 6-4 photoproducts, distort the DNA helix, impeding replication and transcription, which can lead to mutations if unrepaired. UVA radiation (315–400 nm), while weakly absorbed by native DNA, induces indirect damage through photosensitization of endogenous chromophores, generating reactive oxygen species (ROS) like singlet oxygen and superoxide that oxidize DNA bases, forming strand breaks or oxidized lesions such as 8-oxoguanine. Proteins absorb UV via aromatic amino acids—tryptophan (peak ~280 nm), tyrosine (~275 nm), and phenylalanine (~260 nm)—leading to excited state reactions that can cause protein cross-linking, fragmentation, or unfolding, thereby disrupting enzymatic function and cellular signaling. These absorption events underpin UV's dual role in photobiology: potential for mutagenesis and cell death from acute doses, contrasted with regulated low-dose responses like DNA repair activation via nucleotide excision repair pathways. Overall, UV photobiology hinges on wavelength-specific absorption efficiencies and the balance between damage induction and biological repair capacities.

Evolutionary Adaptations and Ecological Roles

Organisms across taxa have evolved physiological, behavioral, and biochemical adaptations to counteract ultraviolet (UV) radiation's damaging effects, such as DNA lesions and oxidative stress, while harnessing UV for sensory and signaling functions. In plants, the UV RESISTANCE LOCUS 8 (UVR8) protein initiates a signaling pathway that triggers accumulation of UV-absorbing compounds like flavonoids in epidermal cells, shielding underlying tissues from UV-B penetration; this mechanism traces back to early land plants, enabling colonization of terrestrial environments under high UV flux before full ozone layer development. Animals exhibit convergent adaptations, including melanin-based pigmentation gradients correlated with ambient UV intensity—darker constitutive pigmentation in equatorial human populations reduces folate depletion and skin cancer risk from chronic exposure, whereas lighter skin in higher latitudes facilitates vitamin D synthesis under low UV conditions. In aquatic ecosystems, zooplankton demonstrate local genetic adaptations for UV tolerance, including enhanced behavioral diel vertical migration to deeper, UV-attenuated waters and upregulation of photoprotective pigments like mycosporine-like amino acids (MAAs). Vertebrates, particularly birds, reptiles, and fish, retain UV-sensitive opsins derived from ancestral violet/UV vision systems, with substitutions in opsin amino acids shifting sensitivity from UV to longer wavelengths in lineages like primates; this retention supports functions beyond protection. Insects and amphibians often possess tetrachromatic vision incorporating UV receptors, facilitating detection of UV-reflective patterns invisible to humans. Ecologically, UV radiation modulates trophic dynamics and biodiversity patterns by influencing foraging, predation, and reproduction. Flowers of many angiosperms reflect UV patterns that guide pollinators like bees, which perceive UV as contrasting "bullseye" nectar guides, enhancing pollination efficiency and plant fitness in UV-abundant environments. In avian species, UV-reflective plumage signals mate quality—males with higher UV reflectance achieve greater reproductive success, as females assess these cues for genetic vigor. Predatory interactions benefit from UV vision; for instance, snakes display UV-iridescent scales that disrupt prey detection or deter predators via aposematic signaling, with phylogenetic analyses indicating stronger selective pressure for defense over sexual display. UV also drives nutrient cycling by photolyzing dissolved organic matter (DOM) in surface waters, increasing bioavailability for microbial uptake and releasing carbon as CO2, thereby altering primary production and food web efficiency in both freshwater and marine systems.

Human Health Effects

Beneficial Physiological Impacts

Ultraviolet B (UVB) radiation, specifically wavelengths between 290 and 320 nm, induces the cutaneous synthesis of vitamin D3 by converting 7-dehydrocholesterol in the epidermis to previtamin D3, which thermally isomerizes to vitamin D3 (cholecalciferol). This process is the primary natural source of vitamin D for most humans, supporting calcium and phosphorus absorption, bone mineralization, and skeletal health; deficiency from insufficient UVB exposure contributes to conditions like rickets and osteomalacia. The World Health Organization recommends 5 to 15 minutes of midday sun exposure several times per week for fair-skinned individuals to achieve adequate vitamin D levels without risking overexposure. Recent trials confirm that controlled UVB exposure enhances vitamin D production in healthy adults without eliciting significant inflammation. Beyond vitamin D, ultraviolet radiation yields nitric oxide (NO) through photolysis of nitrates and nitrosothiols in skin, promoting vasodilation and reducing blood pressure, which correlates with lower cardiovascular disease mortality in observational data. Higher lifetime UV exposure has been associated with up to 50% reduced risk of cardiovascular death and 65% reduced non-cancer, non-cardiovascular mortality, independent of vitamin D status in some analyses. UVB also modulates immune responses, suppressing symptoms of multiple sclerosis via mechanisms separate from vitamin D, including T-cell regulation and cytokine shifts. Narrowband UVB phototherapy (around 311 nm) exploits these physiological pathways therapeutically, inducing apoptosis in hyperproliferative keratinocytes and reducing inflammation in conditions like psoriasis, where it achieves clear or nearly clear skin in 25-33% of patients after consistent sessions. Similar benefits occur in vitiligo through melanocyte stimulation and repigmentation, and in atopic dermatitis via suppression of Th2-dominated responses, with meta-analyses showing sustained remission rates superior to topical agents alone. These effects demonstrate UV's capacity to recalibrate epidermal and dermal homeostasis at sub-erythemal doses, though long-term benefits require balancing against cumulative risks.

Adverse Effects and Dose-Response Relationships

Ultraviolet radiation (UVR) induces acute skin erythema, commonly known as sunburn, primarily through UVB wavelengths (280–315 nm), with a threshold dose termed the minimal erythema dose (MED), typically ranging from 20–80 mJ/cm² in fair-skinned individuals depending on phototype. Erythema exhibits a sigmoidal dose-response curve, where doses below the MED elicit no visible response, but exceeding it leads to inflammation via cytokine release and vasodilation, peaking 12–24 hours post-exposure. UVA (315–400 nm) contributes synergistically at higher doses, lowering the effective UVB threshold by up to 50% in combined exposures, though its erythema action spectrum peaks at longer wavelengths with lower efficiency. Solar UVR exposure is the primary preventable cause of skin cancer,[] with even sub-erythemal (non-burning) doses accumulating DNA damage, photoaging such as wrinkles, and elevated melanoma risk over time.[] Chronic UVR exposure drives dose-dependent skin carcinogenesis, with non-melanoma skin cancers (basal cell and squamous cell carcinomas) showing a near-linear increase in incidence proportional to cumulative lifetime dose; for instance, doubling cumulative UV flux in adulthood elevates squamous cell carcinoma risk by over twofold. Melanoma risk follows a similar dose-response but with evidence of intermittency effects, where high-intensity episodic exposures amplify hazard beyond total dose alone, particularly in lighter skin types. UVB induces direct DNA cyclobutane pyrimidine dimers, while UVA generates oxidative lesions; both accumulate mutations without a clear repair threshold, yielding excess relative risks of 52 per Sv for radiation-induced skin cancers in epidemiological data. Photoaging, manifesting as wrinkles and elastosis, correlates sublinearly with total dose, mediated by matrix metalloproteinase upregulation. Ocular adverse effects include acute photokeratitis from UVB overexposure, with symptoms like pain and photophobia emerging at corneal doses above 0.1–1 mJ/cm² at 300 nm, resolving within 24–48 hours via epithelial sloughing. Cataract formation, primarily cortical and nuclear subtypes, exhibits a cumulative dose-response, with risks rising linearly above chronic thresholds equivalent to 60 mJ/cm² at 350 nm or lower at shorter wavelengths, involving protein denaturation and oxidative stress. UVA exacerbates lens damage through deeper penetration, though UVB predominates in epidemiological links to higher ambient exposure latitudes. UVR suppresses cutaneous and systemic immunity in a dose-dependent manner, with sub-erythemal UVB doses (e.g., 50–200 J/m²) reducing contact hypersensitivity by 40–70% via Langerhans cell depletion and regulatory T-cell induction, facilitating carcinogenesis. Higher doses may reverse local suppression through inflammation, but chronic low-level exposure promotes tolerance, increasing infection susceptibility and malignancy escape, as evidenced in human volunteer studies. Overall, adverse outcomes underscore UVR's dual-threshold (acute) and no-threshold (chronic mutagenic) profiles, with individual variability in repair capacity modulating responses.

Controversies in Exposure Guidelines and Interventions

Public health organizations such as the World Health Organization (WHO) recommend minimizing unprotected exposure to ultraviolet (UV) radiation to reduce risks of skin cancer, photoaging, and immunosuppression, emphasizing interventions like sunscreen use, protective clothing, and shade during peak hours. These guidelines attribute a significant portion of non-melanoma skin cancers and melanomas to cumulative or intermittent UV exposure, with UK estimates suggesting up to 86% of melanomas could be prevented through sun avoidance. However, critics contend that such recommendations conflate chronic low-level exposure, which may confer benefits, with acute high-intensity burns that elevate cancer risk, potentially leading to over-cautious policies that promote vitamin D deficiency. Epidemiological evidence indicates that moderate solar UV exposure correlates with higher serum 25-hydroxyvitamin D levels and lower incidence of certain cancers, including colorectal and breast, as well as reduced cardiovascular mortality, challenging the net harm narrative of UV radiation. Studies from regions like Sweden and the UK link greater lifetime sun exposure to decreased all-cause mortality, with no direct evidence tying overall sun exposure to increased mortality despite established UV carcinogenicity for skin cancers. Organizations like the American Cancer Society advocate obtaining vitamin D primarily through diet or supplements rather than sun exposure, citing insufficient safe solar doses to meet requirements without cancer risk elevation. In contrast, Australian Cancer Council guidelines posit that incidental midday sun exposure for short durations (e.g., 6-8 minutes for light skin types when UV index ≥3) suffices for vitamin D needs without substantial burn risk. Sunscreen interventions, central to many exposure guidelines, face scrutiny over chemical absorbers like oxybenzone (benzophenone-3), which laboratory and animal studies suggest may act as endocrine disruptors by mimicking estrogen or altering thyroid function, prompting bans in Hawaii and Key West since 2021 due to environmental and potential human health concerns. While human epidemiological data show limited evidence of systemic absorption causing harm at typical doses, recent warnings highlight risks from high-concentration products, with calls for mineral-based alternatives like zinc oxide that reflect UV without penetration. Paradoxically, sunscreen use may inadvertently increase UV exposure duration by reducing perceived burn risk, potentially offsetting photoprotection benefits. Occupational exposure guidelines, such as those from the International Commission on Non-Ionizing Radiation Protection (ICNIRP), set limits (e.g., 30 J/m² effective dose for UVB at 270 nm over 8 hours) to prevent acute effects like erythema, but debates persist on balancing these against vitamin D benefits for outdoor workers, whose chronic exposure elevates non-melanoma skin cancer rates yet may lower other disease incidences. Interventions like UV-blocking films or timed shifts remain contentious, as enforced avoidance could exacerbate widespread vitamin D insufficiency observed in indoor populations. Emerging research underscores the need for personalized guidelines accounting for skin type, latitude, and genetic factors influencing UV sensitivity and vitamin D synthesis efficiency.

Applications

Analytical and Forensic Techniques

Ultraviolet-visible (UV-Vis) spectroscopy serves as a fundamental analytical technique for determining the concentration and identity of substances by measuring their absorption of ultraviolet (typically 200-400 nm) and visible (400-800 nm) light. The method relies on the excitation of electrons from ground to higher energy states, producing characteristic spectra that reflect molecular electronic transitions, such as π→π* in conjugated systems. Quantitative analysis follows the Beer-Lambert law, expressed as A=ϵlcA = \epsilon l c, where AA is absorbance, ϵ\epsilon is the molar extinction coefficient, ll is the path length, and cc is concentration, enabling precise measurements in solutions or solids. Applications span pharmaceuticals for purity assays, environmental monitoring for pollutants like nitrates, and biochemistry for protein quantification via aromatic amino acid absorption at 280 nm. Despite its versatility, UV-Vis spectroscopy faces limitations, including sensitivity to impurities causing baseline shifts and inability to resolve fine structural details without complementary methods like NMR, as spectra often overlap for similar compounds. Sample preparation requires solvents transparent in the UV range, such as water or ethanol, to avoid confounding absorption. Instrumental setups typically involve a deuterium or xenon lamp for UV emission, a monochromator for wavelength selection, and a detector like a photomultiplier tube, with modern diode-array detectors enabling rapid full-spectrum acquisition. In forensic investigations, ultraviolet illumination exploits fluorescence and absorption properties to reveal latent evidence invisible under white light. Bodily fluids such as semen, saliva, and urine fluoresce under 365 nm UV light due to organic compounds like tryptophan or flavins, emitting visible wavelengths that contrast against backgrounds, with detection rates enhanced by 30-45% per National Institute of Justice guidelines. Latent fingerprints on porous surfaces may luminesce from residual oils or treated with fluorescent dyes, while bloodstains often absorb UV strongly, appearing as dark voids or exhibiting quenching of background fluorescence. Forensic light sources, portable devices emitting narrow UV bands (e.g., 350-450 nm), facilitate on-site examinations of fibers, gunshot residue, and questioned documents, where UV-induced fluorescence distinguishes security features in currencies or inks. Reflected ultraviolet photography captures patterns from UV-reflective materials, such as altered bruises or fabric weaves, by using UV-pass filters on cameras to exclude visible light. Prolonged UV exposure risks photodegradation of evidence, necessitating controlled application and protective gear to mitigate investigator exposure to potential biohazards revealed.

Industrial and Manufacturing Processes

Ultraviolet radiation plays a central role in UV curing processes, where high-intensity UV light triggers photochemical reactions in photoinitiator-containing formulations, rapidly polymerizing liquid monomers and oligomers into solid, crosslinked networks. This method achieves cure times of seconds, compared to hours for thermal curing, enabling high-throughput manufacturing while minimizing energy use and volatile organic compound emissions by eliminating solvents. In industries such as printing, UV-curable inks solidify instantly on substrates like paper or plastic, supporting speeds exceeding 1,000 meters per minute in flexographic presses and reducing defects from ink migration. In electronics and automotive assembly, UV curing bonds adhesives and conformal coatings onto circuit boards and components, enhancing durability against vibration and thermal cycling; for instance, it secures optical fibers in telecommunications manufacturing with bond strengths up to 20 MPa. Polymer processing benefits from UV-induced crosslinking, which strengthens materials like acrylics and epoxies for applications in medical devices and packaging, where cure depths reach several millimeters under optimized wavelengths around 365 nm. Systems typically employ mercury arc lamps or UV LEDs emitting in the UVA (315–400 nm) and UVB (280–315 nm) ranges, with LEDs offering longer lifespans (over 10,000 hours) and lower heat output for heat-sensitive substrates. Photolithography in semiconductor fabrication relies on ultraviolet light to expose photoresist-coated wafers through patterned masks, selectively etching circuits with feature sizes down to 10 nm using deep UV (e.g., 193 nm argon fluoride lasers) or extreme UV (13.5 nm) sources. This step, repeated dozens of times per wafer, defines transistors and interconnects in integrated circuits, with EUV enabling denser chips compliant with Moore's Law projections through 2030. Exposure doses are precisely controlled at 20–50 mJ/cm² to avoid overexposure, which could degrade resolution, and the process integrates vacuum environments to prevent contamination. UV also facilitates non-destructive testing in manufacturing, such as fluorescent penetrant inspection for welds and castings, where UV illumination at 365 nm reveals surface cracks via dye fluorescence, improving defect detection rates to over 95% in aerospace components. In polymer degradation simulation, accelerated UV weathering chambers expose materials to intensities 5–10 times solar levels, quantifying lifespan via standards like ASTM G154, aiding quality control in plastics and coatings production.

Medical and Disinfection Technologies

Ultraviolet radiation in the UVB (280–315 nm) and UVA (315–400 nm) ranges is employed in phototherapy to treat dermatological conditions such as psoriasis, eczema, and vitiligo by modulating immune responses and inducing apoptosis in hyperproliferative skin cells. Narrowband UVB (NB-UVB) at 311–313 nm has demonstrated high efficacy for plaque psoriasis, achieving complete response rates of 80% in clinical studies involving multiple sessions. Randomized trials confirm that home-based NB-UVB phototherapy is equivalent in effectiveness to office-based treatments for guttate and plaque psoriasis, with clearance rates comparable after standardized dosing protocols. PUVA therapy, combining psoralen sensitization with UVA exposure, yields repigmentation in 50–75% of vitiligo cases on the face, trunk, and limbs, though it carries risks of phototoxicity and potential carcinogenesis with prolonged use. For disinfection, UV-C radiation (200–280 nm), primarily at 254 nm from low-pressure mercury lamps, inactivates microorganisms by damaging DNA through pyrimidine dimer formation, requiring doses as low as 5 mJ/cm² for viruses like SARS-CoV-2. UV germicidal irradiation (UVGI) achieves up to 99.9% inactivation of SARS-CoV-2 on surfaces and in air when direct exposure is ensured, though efficacy diminishes with shadowing, organic soiling, or indirect paths. In water treatment, EPA guidelines recommend UV systems delivering at least 40 mJ/cm² for microbial reduction in surface water, validated through biodosimetry to account for flow dynamics and lamp degradation. Airborne UVGI in HVAC systems provides 76% disinfection efficacy against bacteria at high airflow velocities, while far-UVC at 222 nm enables continuous occupied-space decontamination with reduced human tissue penetration. Emerging UV-LED technologies offer mercury-free alternatives for portable surface disinfection, though commercial devices often fail to deliver required doses for robust pathogen kill without extended exposure times. Standards from organizations like NWRI emphasize validation of UV dose delivery to prevent under-dosing in real-world applications.

References

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