https:\/\/www.epa.gov\/sites\/production\/files\/documents\/sunuvu.pdf<\/a><\/p>\n\n\n\n“While some exposure to sunlight is enjoyable, too much can be dangerous and cause immediate effects like blistering sunburns and long-term problems like skin cancer and cataracts. Overexposure also causes wrinkling and aging of the skin. Scientists are concerned that ultraviolet (UV) radiation might even impair the human immune system.<\/em><\/p>\n\n\n\n<\/span>UV Radiation<\/strong><\/em><\/span><\/h3>\n\n\n\nThe sun gives out energy over a broad spectrum of wavelengths. UV radiation, which has a shorter wavelength than either visible blue or violet light, is responsible for sunburn and other adverse health effects. Fortunately for life on earth, stratospheric ozone screens most harmful UV radiation. What gets through the ozone layer, however, can cause the following health problems, particularly for people who spend <\/em>substantial time outdoors:<\/em><\/p>\n\n\n\n\n- Skin cancer and other skin disorders<\/em><\/li>\n\n\n\n
- Cataracts and other eye damage<\/em><\/li>\n\n\n\n
- Immune suppression<\/em><\/li>\n<\/ul>\n\n\n\n
Because of these adverse health effects, you should limit your exposure to UV radiation and protect yourself when working, playing, or exercising outdoors.<\/em><\/p>\n\n\n\n<\/span>Types of UV Radiation<\/strong><\/em><\/span><\/h3>\n\n\n\nScientists have classified UV radiation into three types:<\/em><\/p>\n\n\n\n\n- UVA<\/em><\/li>\n\n\n\n
- UVB<\/em><\/li>\n\n\n\n
- UVC.<\/em><\/li>\n<\/ul>\n\n\n\n
The stratospheric ozone layer absorbs some but not all of these types of UV radiation:<\/em><\/p>\n\n\n\nUVA – <\/em><\/strong>Not absorbed by the ozone layer<\/em><\/p>\n\n\n\nUVB<\/strong> – <\/em>Partially absorbed by the ozone layer<\/em><\/p>\n\n\n\nUVC – <\/em>Completely absorbed by oxygen and ozone in the atmosphere<\/em><\/p>\n\n\n\nUVA<\/strong> and especially UVB penetrate into the skin and eyes, and can cause the adverse health effects listed above.<\/em><\/p>\n\n\n\n<\/span>UV Levels Depend on a Number of Factors<\/strong><\/em><\/span><\/h3>\n\n\n\n<\/span>Stratospheric Ozone<\/em><\/span><\/h4>\n\n\n\nThe ozone layer absorbs most of the sun’s harmful UV rays, but its thickness varies depending on the time of year and changing weather patterns. The ozone layer has thinned in certain areas due to the emission of ozone-depleting chemicals.<\/em><\/p>\n\n\n\n<\/span>Time of Day<\/em><\/span><\/h4>\n\n\n\nThe sun is at its highest in the sky around noon. At that time, the sun’s rays have the least distance to travel through the atmosphere, and UVB levels are at their highest. In the early morning and late afternoon, the sun’s rays pass obliquely through the atmosphere, and the intensity of UVB is greatly reduced. UVA levels are not sensitive to ozone and vary throughout the day much like visible sunlight does.<\/em><\/p>\n\n\n\n<\/span>Time of Year<\/em><\/span><\/h4>\n\n\n\nThe sun’s angle varies with the seasons, causing the intensity of UV rays to vary. UV intensity tends to be highest during the summer months.<\/em><\/p>\n\n\n\n<\/span>Latitude<\/em><\/span><\/h4>\n\n\n\nThe sun’s rays are strongest at the equator where the sun is most directly overhead and where UV rays must travel the least distance through the atmosphere. Ozone also is naturally thinner in the tropics as compared to the mid- and high-latitudes, so there is less ozone to absorb the UV radiation as it passes through the atmosphere. At higher latitudes the sun is lower in the sky, so UV rays must travel a greater distance through ozone-rich portions of the atmosphere and in turn expose those latitudes to less UV radiation.<\/em><\/p>\n\n\n\n<\/span>Altitude<\/em><\/span><\/h4>\n\n\n\nUV intensity increases with altitude because there is less atmosphere to absorb the damaging rays.<\/em><\/p>\n\n\n\n<\/span>Weather Conditions<\/em><\/span><\/h4>\n\n\n\nCloud cover reduces UV levels, but not completely. Depending on the thickness of the cloud cover, it is possible to burn on a cloudy day even if it does not feel very warm.<\/em><\/p>\n\n\n\n<\/span>Ozone Depletion<\/em><\/span><\/h4>\n\n\n\nThe ozone layer forms a thin shield in the stratosphere, protecting life on earth from the sun’s harmful UV rays. In the 1980s, scientists began accumulating evidence that the ozone layer was being depleted. Depletion of the ozone layer can result in increased UV radiation reaching the earth’s surface, which can lead to a greater chance of overexposure to UV radiation and consequent health effects including skin cancer, cataracts, and immune suppression.<\/em><\/p>\n\n\n\n<\/span>How Stratospheric Ozone Protects Us<\/strong><\/em><\/span><\/h3>\n\n\n\nOzone is a naturally occurring gas that is found in two layers in the atmosphere. In the layer surrounding the earth’s surface-the Stroposphere-ground-level or “bad” ozone is an air pollutant that damages human health and vegetation and is a key ingredient of urban smog. The troposphere extends up to the stratosphere, which is where the “good” ozone protects life on earth by absorbing some of the sun’s ultraviolet rays. Stratospheric ozone is most concentrated between 6 to 30 miles above the earth’s surface.<\/em><\/p>\n\n\n\nOzone is formed when oxygen molecules absorb UV radiation and split apart into two oxygen atoms (0), which combine with other oxygen molecules (02) to form ozone molecules (03). Ozone also is broken apart as it absorbs UV radiation. In this way, UV radiation helps sustain the natural balance of ozone in the stratosphere, while ozone in turn absorbs UV radiation, protecting life on earth from harmful radiation.<\/em><\/p>\n\n\n\n<\/span>How Ozone Is Depleted<\/strong><\/em><\/span><\/h3>\n\n\n\nUntil recently, chlorofluorocarbons (CFCs) were used widely in industry and elsewhere as refrigerants, insulating foams, and solvents. They migrate into the upper atmosphere after use, carried by air currents into the stratosphere. This process can take as long as 5 to 10 years. These chemicals absorb UV radiation, break apart, and react with ozone, taking one oxygen atom away and forming highly reactive chlorine monoxide. Chlorine monoxide in turn breaks down 03 again<\/em>
by pulling away from a single oxygen atom, creating two 02 molecules, and allowing the chlorine to move freely to another ozone molecule. In this way, each chlorine atom acts as a catalyst, repeatedly combining with and breaking apart as many as 100,000 ozone molecules during its stratospheric life.<\/em><\/p>\n\n\n\nOther compounds also damage the ozone layer in much the same way as do CFCs. These ozone-depleting substances include pesticides such as methyl bromide, halons used in fire extinguishers, and methyl chloroform used in industrial processes.<\/em><\/p>\n\n\n\n<\/span>Effect of Ozone Depletion on UV Radiation Levels<\/strong><\/em><\/span><\/h3>\n\n\n\nCurrent studies predict that CFC levels in the atmosphere should peak by around 2000 and should fall to pre-1980 levels by about 2050. As international control measures reduce the release of CFCs and other ozone-depleting substances, natural atmospheric processes will repair the ozone layer. Until that time, we can expect increased levels of UV radiation at the earth’s surface. These increased UV radiation levels can lead to a greater chance of overexposure to UV radiation and consequent health effects.<\/em><\/p>\n\n\n\n<\/span>Health Effects From Overexposure to the Sun<\/strong><\/em><\/span><\/h3>\n\n\n\nAmericans love the sun and spend a great deal of time outside-working, playing, exercising-often in clothing that exposes a lot of skin to the sun. Most people are now aware that too much sun has been linked to skin cancer. However, few know the degree of risk posed by overexposure, and fewer are aware that the risks go beyond skin cancer. Recent medical research has shown that overexposure to the<\/em>
sun’s UV radiation can contribute to serious health problems. Each year, for example, more than 1 million cases of skin cancer are diagnosed in the United States, and one person dies every hour from melanoma or nonmelanoma skin cancer. This section provides a quick overview of the major problems linked to excess UV exposure: skin <\/em>cancer (i.e., melanoma, basal cell carcinoma, and squamous cell carcinoma); other skin problems; cataracts and other eye damage; and immune system suppression. Understanding these risks and taking a few sensible precautions described in this article will help you to enjoy the sun while lowering your chances of sun-related health problems later in life.<\/em><\/p>\n\n\n\n<\/span>A Word About Risk<\/strong><\/em><\/span><\/h3>\n\n\n\nOverexposure to UV radiation poses the risk of serious health effects for everyone, but not everyone is equally at risk. For example, you may be at greater risk of contracting skin cancer if your skin always burns, or burns easily, and if you have blond or red hair, or blue, green, or gray eyes. Other factors indicating an increased risk of skin cancer include a history of blistering sunburns in early childhood, usually from acute sun overexposure; the presence of many moles; or a family history of skin cancer. Also, people who work or otherwise spend a large amount of time outdoors (i.e., chronic exposure to the sun) may be at higher risk of health effects. It’s a good idea to remember that anyone can contract skin cancer and that all people, no matter what skin type, are equally at risk of eye damage<\/strong>.<\/em><\/p>\n\n\n\n<\/span>Melanoma<\/strong><\/em><\/span><\/h3>\n\n\n\nMelanoma, the most serious form of skin cancer, also is one of the fastest-growing types of cancer in the United States. Many scientists believe there might be a link between childhood sunburns and malignant melanoma later in life. Melanoma cases in this country have more than doubled in the past 2 decades; according to the American<\/em>
Cancer Society, about 44,200 new cases of melanoma and 7,300 deaths are currently reported each year.<\/em><\/p>\n\n\n\n<\/span>Nonmelanoma Skin Cancers<\/strong><\/em><\/span><\/h3>\n\n\n\nUnlike melanoma, nonmelanoma skin cancers are rarely fatal. Nevertheless, they should not be taken lightly. Untreated, they can spread and cause more serious health problems. An estimated 1 million Americans will develop nonmelanoma skin cancers this year, while 1,900 will die from the disease.<\/em><\/p>\n\n\n\n<\/span>Actinic Keratoses<\/strong><\/em><\/span><\/h3>\n\n\n\nThese sun-induced skin growths occur on body areas exposed to the sun. The face, hands, forearms, and the “V” of the neck are especially susceptible to this type of blemish. They are premalignant, but if left untreated, actinic keratoses can become malignant. Look for raised, reddish, rough-textured growths. See a dermatologist promptly if you notice these growths.<\/em><\/p>\n\n\n\n<\/span>Premature Aging of the Skin<\/strong><\/em><\/span><\/h3>\n\n\n\nChronic exposure to the sun causes changes in the skin called actinic (or solar) degeneration. Over time, the skin becomes thick, wrinkled, and leathery. Since it occurs gradually, often manifesting itself many years after the majority of a person’s exposure to the sun, this condition is often regarded as unavoidable, a normal part of growing older. With proper protection from W radiation, however, premature aging of the skin can be substantially avoided.<\/em><\/p>\n\n\n\n<\/span>Cataracts and Other Eye Damage<\/strong><\/em><\/span><\/h3>\n\n\n\nCataracts are a form of eye damage, a loss of transparency in the lens that clouds vision. Left untreated, cataracts can rob people of vision. Research has shown that W radiation increases the likelihood of certain cataracts. Although curable with modern eye surgery, cataracts diminish the eyesight of millions of Americans and necessitate billions of dollars of eye surgery each year. Other kinds of eye damage include: pterygium (tissue growth on the white of the eye that can block vision), skin cancer around the eyes, and degeneration of the macula (the part of the retina near the center, where visual perception is most acute). All of these problems could be lessened with proper eye protection from W radiation.<\/em><\/p>\n\n\n\n<\/span>Immune Suppression<\/strong><\/em>