Sunburn: Effects and Management
The salutary benefits of basking in the sun have been sought by human beings since ancient times. Regarded in the past as a deity, the sun still confers its radiant benedictions on its modern devotees who have been persuaded by contemporary fashions that a dark brown tan is a sure sign of well-being, both physical and psychological. At some time, virtually all ardent sun-worshippers discover the unpleasant acute cutaneous reaction commonly called sunburn. PHYSICAL PROPERTIES OF SOLAR RADIATION Constituting a continuous spectrum, the electromagnetic radiation from the sun ranges from the highly energetic short wavelengths to the less energetic longer wavelengths. The wavelengths that impinge on the earth's surface are between 290 and 3,000 nm. On the basis of our visual physiology, they can be arbitrarily divided into visible, ultraviolet, and infrared waves. The portion of solar radiation that elicits the sunburn reaction lies between 290 and 320 nm in the ultraviolet band and is traditionally designated ultraviolet B (UVB). The earth's stratosphere effectively absorbs the potentially more harmful shorter wavelengths. This filtering is accomplished by the thin ozone layer that continually absorbs ultraviolet radiation (UVR) from 200 to 320 nm, completely cutting out all radiation less than 290 nm. The longer ultraviolet wavelengths from 320 to 400 nm, designated ultraviolet A (UVA), are approximately one thousandth as effective as UVB in evoking erythema.