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Introduction
A monograph entitled Environmental
Health Criteria 160 "Ultraviolet Radiation" was published in
1994 by the World Health Organization, jointly in collaboration with the
United Nations Environment Programme and the International Commission on
Non-Ionizing Radiation Protection. The monograph was the result of an
in-depth review of the scientific literature and was primarily concerned
with the effects of ultraviolet (UV) radiation exposure on human health
and the environment. The penultimate draft was subjected to a WHO Task
Group for final peer review prior to publication. Such a review was
considered particularly timely in view of the consequences of increasing
levels of UV at the surface of the earth resulting from depletion of
stratospheric ozone.
The purpose of this document is to
provide a summarised form of the monograph, allowing the subject to be
reviewed by a more general readership, and to update activities that
have resulted from the recommendations of the Task Group that reviewed
the monograph.
Exposure to UV occurs from both natural
and artificial sources. The sun is the principal source of exposure for
most people. Solar UV undergoes significant absorption by the
atmosphere. With depletion of the stratospheric ozone people and the
environment will be exposed to higher intensities of UV. The
consequences of this added UV exposure are considered so serious that it
was a major topic for discussion at the World Environment Conference,
held in Rio de Janeiro in 1992. In Agenda 21, adopted by the Conference,
it was specifically recommended to "undertake, as a matter of
urgency, research on the effects on human health of the increasing
ultraviolet radiation reaching the earth's surface as the consequence of
depletion of the stratospheric ozone layer." It is this issue that
underscores the current need to better understand the potential health
and environmental risks of UV exposure. INTERSUN, global UV project, is
WHO's response to the need to disseminate information about the health
and environmental hazards of excessive UV exposure. INTERSUN has
developed a document entitled "UV Protective Measures" in
response to the need to educate the public and workers on measures they
can take to reduce their UV exposure, and has been involved in the
development of a Solar UV Index, an index related to daily UV exposure,
reported with the news and weather, that facilitates a continuing
educational process about possible health effects and measures to reduce
UV exposure. More details on these programmes are given at the end of
this text.
Summary of the major
health concerns
Skin cancer and cataracts are important
public health concerns. The social cost of these diseases, such as
death, disfigurement and blindness, can be overwhelming both in terms of
human suffering and the financial burden. Solar UV exposure is known to
be associated with various skin cancers, accelerated skin aging,
cataract of the lens of the eye and other eye diseases, and possibly has
an adverse effect a person's ability to resist infectious diseases. Most
of these health concerns could be avoided by reducing exposure to solar
UV.
The United Nations Environment
Programme has estimated that over 2 million non-melanoma skin cancers
and 200,000 malignant melanomas occur globally each year. In the event
of a 10% decrease in stratospheric ozone, with current trends and
behaviour, an additional 300,000 non-melanoma and 4,500 melanoma skin
cancers could be expected world-wide.
Some 12 to 15 million people in the
world are blind because they have cataracts. WHO has estimated that up
to 20% of cataracts or 3 million per year could be due to UV exposure to
the eye. It has been estimated that for each 1% sustained decrease in
stratospheric ozone there would be an increase of 0.5% in the number of
cataracts caused by solar UV (van der Leun et al 1989). In the United
States alone, it costs the US Government $US 3.4 billion for 1.2 million
cataract operations per year. Substantial savings in cost to health care
can be made by prevention or delay in the onset of cataracts.
Ultraviolet radiation
UV is one of the non-ionizing
radiations in the electromagnetic spectrum and lies within the range of
wavelengths 100 nm to 400 nm (see figure 1). The short wavelength limit
of the UV region is often taken as the boundary between the ionizing
radiation spectrum (wavelengths < 100 nm) and the non-ionizing
radiation spectrum. UV can be classified into UVA (315 - 400 nm), UVB
(280 - 315 nm) and UVC (100 - 280 nm) regions, although other
conventions for UVA, UVB and UVC wavelength bands are in use.
Most artificial sources of UV, except
for lasers, emit a spectral continuum of UV containing characteristic
peaks, troughs and lines. These sources include various lamps used in
medicine, industry, commerce, research and the home.

Figure 1: Solar optical emissions
before and after absorption by the atmosphere.
Since UV is normally absorbed over a
surface it can be measured as a radiant exposure, the incident UV energy
divided by the receptor surface area in joules per square metre (J m-2).
UV can also be measured as an irradiance, the incident power divided by
the receptor surface area in watts per square metre (W m-2).
Biological
effectiveness of UV
UV-induced biological effects depend on
the wavelengths of the radiation emitted by the source. Thus, for a
proper determination of hazard it is necessary to have information on
the spectral (range of wavelength) emissions. These consist of spectral
irradiance (W m-2 nm-1) measurements from the
source. The total irradiance (W m-2) is obtained by summing
over all wavelengths emitted. The biological or hazard weighted
irradiance (W m-2 effective), commonly called the effective
UV irradiance or dose rate (exposure), is determined by multiplying the
spectral irradiance at each wavelength by the biological or hazard
weighting factor (which quantifies the relative efficacy at each
wavelength for causing the effect) and summing over all wavelengths.
Such factors or weighting functions are obtained from action spectra.
Action Spectrum and
Minimum Erythemal Dose
An action spectrum is a graph that
provides information on the effectiveness of the UV wavelengths in
producing a biological effect, eg erythema. It is the reciprocal of the
radiant exposure required to produce the given effect at each
wavelength. Figure 2 depicts the ICNIRP-CIE action spectrum for erythema.
All the data in such curves are normalized to the most effective
wavelength(s). By summing the biologically effective irradiance over the
exposure period, the biologically effective radiant exposure (J m-2
effective) can be calculated.
For UV induced erythema, the action
spectrum adopted by the International Commission on Non-Ionizing
Radiation Protection (ICNIRP), International Commission on Illumination
(CIE), the International Electrotechnical Commission (IEC) and various
national bodies, is a composite curve obtained by statistical analysis
of many research results on the minimum radiant exposure of UV at
different wavelengths necessary to just cause erythema.

Figure 2: Action spectrum for erythema.
The most commonly used quantity for
describing the erythemal potential of an exposure to UV is the number of
minimum erythemal doses (MEDs) represented by the exposure. An MED is
the radiant exposure of UV that produces a just noticeable erythema on a
previously unexposed skin. It corresponds to a radiant exposure of
monochromatic radiation at the maximum spectral efficacy for erythema
(around 300 nm) of approximately 150 to 2000 J m-2 effective,
depending on skin type. Values of 200 - 300 J m-2 effective
are commonly used as the value of 1 MED for comparative safety purposes
for white skin.
Cellular and Molecular
Studies
To produce any change, UV must be
absorbed by a biological molecule. This involves absorption of a single
photon by the molecule and the production of an excited state in which
one electron of the absorbing molecule is raised to a higher energy
level. The primary products caused by UV exposure are generally reactive
species or free radicals which form extremely quickly but which can
produce effects that can last for hours, days or even years. DNA is the
most critical target for damage by UVB and UVC. Figure 3 indicates the
formation of pyrimidine dimers in DNA. While a considerable amount of
knowledge is available concerning the interaction of UV with nucleic
acids, controversy exists as to which lesion constitutes the most
important type of pre-mutagenic damage.
Cell death, chromosome changes,
mutation and morphological transformations are observed after UV
exposure of procaryotic and eucaryotic cells. Many different genes and
several viruses (including HIV) are activated by UV exposure. The genes
activated by UVB and UVC are different from those activated by UVA.
Studies of DNA repair defective disorders have clearly established a
link between UV induced DNA damage in skin and various types of cancer.
Animal Studies
Skin cancer
Solar UV exposure has been shown to
produce cancers in domestic and food animals. In experimental animals UV
causes predominantly squamous cell carcinomas (SCCs). UVB is most
effective at producing SCCs, although they are produced by UVA but at
much higher intensities, similar to the levels needed for erythema and
tanning. The effectiveness of UVC is unknown except at one wavelength
(254 nm). At this wavelength the effectiveness is less than UVB.
Melanomas are much less common and only
two animal models have been found for induction of melanoma by UV alone.
An initial action spectrum determined for a type of hybrid fish
indicates a peak in the UVB range but also shows a high level of
effectiveness in the UVA. Basal cell carcinomas are rare in animals.
Immune response
Exposure to suberythemal doses of UV
have been shown to exacerbate a variety of infections in rodent models.
UV affects infections both at the site of exposure and at distant sites.
Recent work indicates that systemic infections without skin involvement
may be affected. Enhanced susceptibility appears to result from T-helper
cell activity. The mechanisms associated with this suppression appear to
be the same as those identified with suppression to contact and delayed
type hypersensitivity responses. Suppression of these immune responses
appears to be mediated by release of soluble mediators from UVB exposed
skin which alters the antigen presentation by Langerhans and other cells
so that they fail to activate TH1 cells. The resulting immune
suppression is antigen specific, can occur regardless of whether or not
antigen is applied at the site of exposure, and is relatively long
lasting. UV exposure also prevents the development of protection
immunity to a variety of infections in mice and rats.
Effects on the eye
Many studies in experimental animals
have demonstrated that UV exposure can cause both acute and delayed
effects such as cataract, photokeratitis, damage to the corneal
epithelium and various retinal effects. Studies of photochemical retinal
injury in aphakic monkeys have shown that the retina is six times more
vulnerable to photochemical damage from UV than the visible wavelengths.
Health Effects on
Humans
Skin
The degree of damage that UV produces
in skin will depend on the incident intensity and wavelength content (UVA
or UVB), and on the depth of penetration of these wavelengths into the
skin (see figure 4). Acute effects on the skin consist of solar erythema,
"sunburn", which, if severe enough, may result in blistering
and destruction of the surface of the skin with secondary infection and
systemic effects, similar to those resulting from a first or second
degree heat burn. Although UVC is very efficiently absorbed by nucleic
acids, the overlying dead layers of skin absorb the radiation to such a
degree that there is only mild erythema and, usually, no late sequelae,
even after repeated exposures. Much less is known about the biological
effects of UVA. However, doses of UVA, which alone may not show any
biological effect, can, in the presence of certain environmental,
consumer and medicinal chemical agents,

Figure 3: Depth of penetration of UV
into the skin.
Chronic skin changes due to UV consist
of skin cancer (both melanoma and non-melanocytic), benign abnormalities
of melanocytes (freckles, melanocytic naevi and solar or senile
lentigines), and a range of other chronic injuries resulting from UV
exposure to keratinocytes, blood vessels and fibrous tissue, often
described as "photoaging" (solar elastosis). The much
increased rates of skin cancer in patients with xeroderma pigmentosum,
who have a deficiency in the capacity to repair UV-induced DNA damage,
suggest that direct UV damage of the DNA may be a step in the cause of
these cancers. This suggestion has also been supported by the
observation of UV specific mutations of the p53 tumour suppressor gene
in a proportion of patients with non-melanocytic skin cancer. Oxidative
and immune suppressant effects may also contribute to the capacity of UV
to cause skin cancers.
Cancer of the lip is much more common
in fair than dark skin populations and is associated with outdoor work.
However possible confounding with tobacco and alcohol use has not been
adequately controlled in any study, and so it is not possible at present
to associate directly solar UV exposure in the cause of this cancer.
Strong epidemiological evidence exists
that sun exposure causes cutaneous melanoma and non-melanocytic skin
cancer. Their incidence is less in darker than light skin groups living
in the same geographical area. Risk of skin cancer decreases with
increasing pigmentation. The anatomical site most seen for squamous cell
carcinoma (SCC) is the head and neck, areas most exposed to the sun.
Incidence of both melanoma and non-melanocytic skin cancer are increased
in areas of high ambient solar UV radiation.
The worldwide incidence of malignant
melanoma has continued to increase. Cutaneous melanoma is the result of
neoplastic transformation of melanocytes, the pigment producing cells in
the epidermis. Four basic categories of melanoma have been identified in
humans: superficial spreading melanoma, nodular melanoma, lentigo
malignant melanoma (also known as Hutchinson's melanotic freckle), and
unclassified melanoma.
Melanoma is strongly related to
frequency of recreational exposure to the sun and to history of
sunburns. The evidence that risk of melanoma is related to intermittent
exposure to UV, especially in childhood, is inferred from the locations
of the melanomas over the body (larger numbers on irregularly exposed
sites), higher occurrence in indoor than outdoor workers, and higher
levels of exposure during childhood (prior to 15-20 years of age).
There is suggestive evidence that
exposure to sunlamps may increase the risk of melanoma, but the studies
conducted so far have not consistently controlled confounding factors.
Immune system
A number of studies suggest that UV
exposures at environmental levels suppress immune responses in both
rodents and man. In rodents this immune suppression results in enhanced
susceptibility to certain infectious diseases with skin involvement and
some systemic infections. Mechanisms associated with UV-induced
immunosuppression and host defence mechanisms which provide for
protection against infectious agents, are similar in rodents and man. It
is therefore reasonable to assume that exposure to UV may enhance the
risk of infection and decrease the effectiveness of vaccines in humans.
However additional research is necessary to substantiate this.
Eye
UV exposure of the eye depends on many
factors: ground reflection, degree of brightness in the sky leading to
activation of the squint reflex, the amount of atmospheric reflection
and the use of eyewear. In addition, the target for UV-induced damage
will depend on the wavelength of the incident radiation as shown in
figure 5.
The acute effects of UV on the eyes
consist of the development of photokeratitis and photoconjunctivitis,
which are unpleasant but usually reversible and easily prevented by
appropriate eyewear. Chronic effects on the eye consist of the
development of pterygium and squamous cell cancer of the conjunctiva and
cataracts. A review of the studies suggests that there is sufficient
evidence to link acute ocular exposure to photokeratitis but our
knowledge of the effects of chronic exposure is less certain. While
there is sufficient evidence that cortical and posterior subcapsular
cataracts (PSC) can be caused by UVB in laboratory animals, there is
limited evidence to link cortical and PSC cataracts in humans to chronic
ocular exposure to UVB.

Figure 4: Depth of penetration of UV
into the eye.
Insufficient information is available
to separate out the other factors contributing to cataract formation, or
to state the proportion of cataracts which can be attributed to UVB
exposure. There is also limited evidence to link the development of
climatic droplet keratopathy and pterygium, but insufficient evidence to
link uveal melanoma with UV exposure.
Environment
Increased levels of UV due to ozone
layer depletion may have serious consequences for living organisms. A
10% reduction in ozone could lead to as much as a 15-20% increase in UV
exposure depending on the biological process being considered. While the
impact on human health, crop production, fisheries etc. is largely
unknown, adverse effects of increased exposure to UVB have been reported
on plant growth, photosynthesis and disease resistance. Further, the
impact of increased UV levels on aquatic ecosystems (the major
contributor to the earth's biomass) may be substantial (see figure 6).

Figure 5: Biological food web in a
marine ecosystem.
Phytoplankton, at the base of the
aquatic food chain, serves as food for larvae of fish and shrimp. These
in turn are consumed by fish, which subsequently provide an essential
food source for many human beings and other animals. A significant
reduction in phytoplankton from increased UVB exposure will directly
affect the human and animal marine food source.
Guidelines on Exposure
Limits
Guidance on exposure limits for UV are
described in chapter 13. International guidelines published by the
International Commission on Non-Ionizing Radiation Protection define
exposure limits (ELs) below which it is expected that nearly all people
may be repeatedly exposed without adverse effects. The ELs are intended
to be used to evaluate potentially hazardous exposures from, for
example, solar radiation, arcs, gas and vapour discharges, fluorescent
lamps and incandescent sources. The ELs are generally below levels which
are often used for the UV exposure of patients required as part of
medical treatment and below levels associated with sunbed exposure. ELs
are not intended to apply to exposure of pathologically photosensitive
individuals, to people concomitantly exposed to photosensitising agents
or to neonates.
Protective Measures
Typical protection and control measures
for reducing UV exposure include the containment of UV sources, and
methods for personal protection including the use of sunscreen
preparations, clothing, eye and skin protection, and behavioural
modifications.
While topical application of sunscreen
is a preferred method of absorbing UVB, some preparations do not absorb
the longer wavelength UVA effectively. Moreover, some have been found to
contain ingredients that are mutagenic in sunlight. There is still much
research necessary before the impact on health of increased levels of
UVA will be known. In the meantime people using sunscreens should use
only those with the highest sun protection factor (SPF) and be aware
that they are for their protection from the sun and not for tanning
purposes. Use of wide brimmed hats, protective clothing and UV absorbing
eye glasses is still the best personal protection against the adverse
effects of UV exposure.
With increasing levels of solar UV
resulting from depletion of the ozone layer, and the continuing rise in
the level of melanoma worldwide, people should become more aware of
their UV exposure and take appropriate precautions. These precautions
include staying out of the sun during the period around noon (the period
when the UV levels are highest), or wearing UV protective clothing, hats
and sun glasses. Broad spectrum (UVB and UVA protective) sunscreens
should be used when other means of protection are not feasible. These
sunscreens should be used to reduce exposure rather than lengthen the
period of exposure to the sun. Protection of young children is
particularly important for the prevention of long-term consequences of
UV exposure. In general behavioural patterns must change to protect
against increasing solar UV levels.
Education
UV Protective Measures Publication
This INTERSUN publication provides
information to people on how to protect themselves from the potentially
harmful effects of exposure to ultraviolet radiation (UV). Following a
detailed review of the scientific literature conducted by a WHO Task
Group meeting, a number of adverse health effects resulting from
exposure to UV have been identified that need to be addressed through
further research and more particularly through educational programmes
for people most exposed to UV.

Figure 6: UV Exposure from
various parts of our living environment (Modified from Diffey BL and
Larkö O, Clinical climatology. Photodermatology 1984, 1:30-37. With
permission.)
The purpose of this document is to
provide information to the general public and workers on the various
health hazards known to be associated with excessive exposure to UV and
measures that can be taken to reduce this exposure to acceptable levels.
Solar UV Index
A joint initiative of the World
Meteorological Organization, UNEP and WHO has resulted in the drafting
of a report that outlines the details of a solar UV index whose use will
be encouraged in the radio and TV news and weather programmes, and in
the print media, worldwide. The solar UV index is related to the UV
exposure a person would receive outdoors. It identifies periods of the
day when UV exposure may be intense and provides a tool to educate the
public and outdoor workers about the hazards of excessive UV exposure
and what precautions may be necessary to avoid such exposure. The
initiative for this project is being taken by the WHO Collaborating
Centre in the German Government's Institute for Radiation Hygiene.
Further reading
Environmental Health Criteria 160,
Ultraviolet Radiation, United Nations Environment Programme, World
Health Organization, International Commission on Non-Ionizing Radiation
Protection. WHO Geneva 1994.
Environmental Effects of Ozone
Depletion: Environmental Effects Panel Report, JC van der Luen, M
Trevini, RC Worress (eds), United Nations Environment Programme,
Nairobi, Kenya, 1989.
Environmental Effects of Ozone Layer
Depletion: 1994 Assessment. United Nations Environment Programme,
Nairobi, Kenya, 1994.
Health, solar UV radiation and
environmental change. A Kricker, BK Armstrong and RD Burton (eds), Lyon,
International Agency for Research on Cancer (IARC Technical Report 13),
IARC 1993.
INTERSUN: UV REPORT, Update on
activities of the INTERSUN Project. Office of Global and Integrated
Environmental Health, World Health Organization, Geneva, Switzerland.
Report WHO/EHG/94.18, 1994.
International Radiation Protection
Association/ International Non-Ionizing Radiation Protection Committee.
In: Duchene AS, Lakey JRA and Repacholi MH (eds), IRPA guidelines on
protection against non-ionizing radiation. New York, McGraw Hill. 1991.
Solar and ultraviolet radiation. Lyon,
International Agency for Research on Cancer, Monographs on the
evaluation of Chemical Carcinogenic Risks to Humans, Volume 55. IARC
1992.
World Meteorological Organization
Report of the second meeting of the ozone research managers of the
parties of the Vienna Convention for the protection of the ozone layer.
WMO, Geneva 10-12 March 1993.
For further
information on any of the material above, please contact:
Occupational and Environmental Health (OEH)
World Health Organization
1211 Geneva 27, Switzerland
Fax:+41 22 791 4123
Programme Officer
United Nations Environment Programme (UNEP)
Human Health, Welfare and Settlements Unit
PO Box 30552 Nairobi, Kenya
Tel:+252 2 621234
Fax:+252 2 226890
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