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Protecting Workers from Ultraviolet Radiation - icnirp

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<strong>Protecting</strong> <strong>Workers</strong> <strong>from</strong> <strong>Ultraviolet</strong> <strong>Radiation</strong><br />

Eumelanin (black melanin) is produced by melanocytes upon alpha-MSH adsorption on MC1R<br />

gene product (receptor) at the surface of the melanocytes. Phaeomelanin (red melanin) is<br />

produced in melanocytes bearing MC1R variants. Phaeomelanin absorb UV photons and<br />

produce reactive oxygen species (ROS) which are phototoxic. Eumelanin (stable free radical)<br />

absorb UV photons and scavenge free radicals and are photoprotective. All individuals produce<br />

eumelanin and phaeomelanin in different ratios according to genetic makeup and as a<br />

consequence present large differences in solar sensitivity and skin cancer incidence. In addition,<br />

darker skin types have more efficient DNA repair than the skin phototypes I and II (Sheehan et al<br />

2002).<br />

Skin adaptation <strong>from</strong> frequent UVR exposure is not only characterized by the obvious effect of<br />

skin darkening (“tanning” or “melanogenesis”), but also by skin thickening (Table 2).<br />

Thickening of the outermost layers of the skin (epidermis and stratum corneum) takes place as an<br />

adaptation to UVB-related damage. This can be a 3 to 5-fold thickening of the stratum corneum<br />

within one to seven weeks after several exposures to UVB, and returns to normal about one to<br />

two months after ceasing exposure. This thickening after sun exposure leads to a significant<br />

increase in UV protection by a factor of five or greater, and in lightly pigmented skin types,<br />

thickening is probably more important than tanning in providing protection. The thickening of<br />

the skin after prolonged tanning protects sensitive cells (basal keratinocytes, melanocytes) by<br />

absorbing UVB radiation before they reach the basal layer of the epidermis. After some<br />

shedding (peeling) of the stratum corneum, the basal layer can be directly stimulated by UVB<br />

and thus the thickening or protective processes recur and reach a steady state. However, in<br />

darkly pigmented individuals it is likely that skin pigmentation is the most important means of<br />

protection against UVR.<br />

Tanning becomes noticeable within a day or two after sun exposure, gradually increasing for<br />

several days and persisting for a week. Although a tanned skin does confer a degree of<br />

protection, this seems to be no more than a factor of two to three in the absence of skin<br />

thickening. The wavelengths of the radiation that induce tanning are very similar to those of<br />

radiation producing erythema. Table1 describes the range of skin types and sensitivity to UVR<br />

effects. Subjects with sun-reactive, melano-compromised (skin types I and II) are poor tanners<br />

compared to those with melano-competent (skin types III and IV) who tan well. Melanogenesis<br />

can be stimulated in individuals who tan well with solar UV doses that were considerably below<br />

the erythemal doses in the UVA region.<br />

Table 1. Classification of skin types based on their susceptibility to sunburn in sunlight and their<br />

ability to tan. Modified after Fitzpatrick and Bolognia, 1995<br />

Skin<br />

phototype<br />

Sun sensitivity Sunburn susceptibility* Tanning achieved Classes of individuals<br />

I Very sensitive Always sunburn: < 2 SED No tan Melano-compromised<br />

II Moderately sensitive High: 2 – 3 SED Light tan Melano-compromised<br />

III Moderately insensitive Moderate: 3 - 5 SED Medium tan Melano-competent<br />

IV Insensitive Low: 5-7 SED Dark tan Melano-competent<br />

V Insensitive Very low: 7-10 SED Natural brown skin Melano-protected<br />

VI Insensitive Extremely low: > 10 SED Natural black skin Melano-protected<br />

*The ranges of SEDs are not prescriptive but only indicative<br />

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