THE MIDDLE ULTRAVIOLET REACHING THE GROUND*

Abstract— We present a semi-empirical analytic formula for calculating the direct, diffuse and global solar middle-ultraviolet radiation (280–340 nm) reaching the ground. The formula accommodates variations in wavelength, solar angle, ozone thickness, aerosol thickness, ground albedo, ground elevation, and cloudiness. Analytic representations of biological action spectra are also presented for use in calculations of effective dose at any time of day. Our purpose is to provide a basis for estimating approximate changes in middle-ultraviolet radiation levels reaching the ground caused by anthropogenic changes in the intervening atmosphere.     

MIDDLE ULTRAVIOLET RADIATION REACHING THE OCEAN SURFACE*

Abstract— Direct measurements of the downwelling spectral irradiance in the middle UV (280–340 nm) have been made for a range of solar zenith angles (20°-70°). These measurements were made for a marine atmosphere at equatorial latitudes. We fit these data to two semi-empirical analytic representations, from which quantitative calculations of spectral irradiance in the middle UV incident at the ocean surface can be made. The formulae accommodate variation in wavelength, solar zenith angle, ozone thickness, aerosol thickness and surface albedo. Our purpose is to provide marine photobiologists and photochemists with a basis for estimating middle UV radiation levels reaching the ocean surface and the approximate changes caused by manmade alterations of the ozone layer.     

LONG-TERM VARIATIONS IN ULTRAVIOLET SUNLIGHT REACHING THE BIOSPHERE: . CALCULATIONS FOR THE PAST THREE DECADES

The long-term data base on atmospheric ozone combined with a set of radiative transfer calculations provides estimates of the variability in ultraviolet (UV) sunlight that should have occurred over the period1957–1988 under clear, pollution-free skies. Results refer to the earth's surface at specific locations in the Northern Hemisphere and to averages over collections of sites located in three latitude bands from 30 to 64°N. For any one year the annually integrated solar irradiance, weighted by the action spectrum for erythema, typically lies within3–4% of the 32-year mean. No statistically significant trends span the entire 32-year time frame. However, over the shorter time period1970–1988 the annually integrated erythemal irradiance shows an upward trend of +2.1 ± 1.2% per decade based on all ozone data at latitudes from 40 to 52°N. No trends exist in lower (30-39°N) and higher (53-64°N) latitude bands. We caution that a trend line provides a very simple index of the variability in UV sunlight, and these results should not necessarily be extrapolated into the future.     

ULTRAVIOLET RADIATION INDUCED CHANGES IN MACROPHAGE ACTIVITY

Abstract— The effect of ultraviolet (UV) radiation on macrophage activity was examined. Thioglycollate-stimulated peritoneal exudate cells were collected from adult C57BL/6 mice. Ninety-five per cent of the cells adhering to plastic petri dishes were macrophages as determined by the presence of a non-specific esterase. Adherent cells were exposed to UV radiation of 0.5-13.2 J/m². Viability and phagocytosis were measured at 0, 24, 48, 72 and 96 h after exposure. A statistically significant UV exposure-dependent decrease in macrophage viability and phagocytic capacity was observed. Macrophage viability and phagocytosis also decreased as a function of time after exposure to UV radiation.     

ULTRAVIOLET RADIATION INDUCES A CHANGE IN CELL MEMBRANE POTENTIAL in vitro: A POSSIBLE SIGNAL FOR ULTRAVIOLET RADIATION INDUCED ALTERATION IN CELL ACTIVITY

The regulation of a transmembrane ionic gradient, reflected by the cellular membrane potential, has been shown in several cell systems to be involved in the regulation of cell function. This investigation presents evidence that biologically relevant doses of ultraviolet radiation (UVR) will alter the membrane potential of keratinocytes in vitro. Estimation of the relative change in the steady-state membrane potential of the murine keratinocyte cell line PAM 212, the murine myelomonocytic cell line P388D1, and normal human keratinocytes in culture, were made through the use of the lipophilic cationic membrane potential sensitive probe; triphenylmethylphosphonium. Our observations indicate that UVR composed primarily of UVB (280-320 nm) radiation at doses as low as 100 J/m2 can induce a depolarization in the murine cell lines and a hyperpolarization in human keratinocytes. Evidence suggests that this difference in the direction of the membrane potential response reflects a difference in Na+/K+ ATPase activity following UVR. These results suggest a possible mechanism for modulation of keratinocyte activity induced by UVR.     

BIOLOGICALLY EFFECTIVE DOSE OF SOLAR ULTRAVIOLET RADIATION ESTIMATED BY SPORE DOSIMETRY IN TOKYO SINCE 1980

Abstract— The biologically effective dose of solar UV radiation has been measured in Tokyo since 1980 using Bacillus subtills spores. To determine the cumulative dose in a half day, several samples of UV-sensitive spores were exposed in successive intervals from the solar-noon time. Because fluence-survival curves were exponential, the number of lethal hits received by the spores was calculated for each interval and termed inactivation dose (ID). The total number of hits obtained in a half day (half-day ID) was correlated with the amount of global insolation by a power-function regression. The regression analyses were performed for the data collected on 35 days from 1980 to 1986 and for the data collected on 53 days from 1989 to 1991. The latter data set yielded significantly larger estimates of half-day ID relative to the insolation than the former. These analyses suggested that the biologically effective dose relative to the insolation increased about 30% at some time in the later part of 1980s at this location. Changes of solar activity, air pollution and stratospheric ozone layer were considered as potentially responsible for this increase, but identification of the causative factors requires further efforts.     

THE EFFECT OF CHANGES IN CELL GEOMETRY ON THE SENSITIVITY TO ULTRAVIOLET RADIATION OF MAMMALIAN CELLULAR CAPACITY

Abstract— We have measured a calcium and magnesium dependent change in cell shape when mammalian cell monolayers are being prepared for irradiation by replacing their growth medium with certain buffers. In some cases, flattened cells (umbonate) assumed a spherical configuration. In order to assume a centrally located target molecule, we used a DNA-dependent cellular function–pacity for herpes viral growth–as the parameter to measure ultraviolet (UV) sensitivity of cells irradiated while in either of the two shapes. Umbonate cells were more sensitive to UV than were spherical cells. Exposures to the cell that lowered the cellular capacity of umbonate cells to the 10% survival level only lowered spherical cells to the 50% level. Twenty-seven per cent additional UV exposure to spherical cells was required to get the same effect as with umbonate cells. Included in the text are photographs of both cell types, survival curves for cellular capacity, a measure of the absorbance of cell homogenates, and a calculation of the relative number of photons absorbed by each cell nucleus.     

TEMPORAL CHANGES IN SURFACE ULTRAVIOLET RADIATION: A STUDY OF THE ROBERTSON-BERGER METER AND DOBSON DATA RECORDS

Abstract— Ultraviolet radiation data sets obtained by Robertson-Berger meters located at Bismarck, ND and Tallahassee, FL show variations over the time period 1974–1985 which we interpret in terms of clouds and ozone. Cloudiness is a major source of variance in the irradiance measurements. When this variance is minimized, the monthly mean Robertson-Berger meter record contains trends which are in good agreement with irradiance calculations based on the Dobson ozone measurements in spring, summer and early autumn. Despite the agreement among trends, predictions based on the ozone data explain 40% or less of the variance in the monthly mean radiation values over the 11-year period. The radiation measurements contain negative trends in winter which are contrary to expectations based on the behavior of ozone alone. These trends remain when we minimize the effects of cloudiness. Based on the information available in this study, it is not possible to determine whether the wintertime trends have an instrumental or environmental origin.     

A PORTABLE INSTRUMENT FOR MEASURING GROUND REFLECTANCE IN THE ULTRAVIOLET

Abstract— A lightweight, battery-powered instrument specifically designed for measuring ground reflectance in the UV is described. The instrument has been used to measure the UV reflectance over different terrains in Saudi Arabia, Canada and England, and data are presented for a number of surfaces including tarmac, grass, wood, concrete and sand. These values agree closely with those obtained by diffuse spectral reflectance measurements.     

WAVELENGTH DEPENDENCE OF THE FORMATION OF SINGLE-STRAND BREAKS AND BASE CHANGES IN DNA BY THE ULTRAVIOLET RADIATION ABOVE 150 nm

The wavelength dependence of the formation of two types of DNA damage, single-strand breaks and base changes, was investigated in the UV region from 150 nm to 254 nm using superhelical closed circular (form I) colicin El DNA with synchrotron radiation. Single-strand breaks were measured by agarose gel electrophoresis as a direct conversion of form I DNA to form II DNA (open circular). Base damages were defined as sensitive sites to a crude extract of endonuclease from Micrococcus luteus. They also were estimated using the same conversion, from form I to form II after the DNA was treated with endonuclease. The fluence-effect relationship could be fitted by a simple exponential function for both types of damage. Action spectra were constructed based on the reciprocal of the 37% fluence. The action spectrum for strand breaks increased rather monotonically over three decades from 254 nm to 150 nm in a logarithmic scale, while that for base damages showed a breaking point at 190 nm, being relatively flat above 190 nm. The characteristics of the action spectra are compared with the absorption spectra of the DNA and its main chain moiety calculated on the basis of data on calf thymus DNA and synthetic polynucleotides. Our main conclusions are (1) that the majority of single-strand breaks were induced by the absorption of photon in the sugar-phosphate group in the vacuum-UV region and (2) that the base changes were induced equally well by absorption in the vacuum-UV and in the far-UV region.     

EFFECTS OF ULTRAVIOLET RADIATION ON THE IMMUNE SYSTEM IN HUMANS

In experimental animals, exposure to UV-B radiation produces selective alterations of immune function which are mainly in the form of suppression of normal immune responses. This immune suppression is important in the development of nonmelanoma skin cancer, may influence the development and course of infectious disease and possibly protects against autoimmune reactions. The evidence that this form of immune suppression occurs in humans is less compelling and very incomplete. The wavelengths of radiation most affected by a depletion of the stratospheric ozone layer are those known to be most immunosuppressive in animals and it is likely that such depletion will increase any suppressive effect of sunlight on immunity in humans. In addition to establishing whether or not UV-B radiation can cause suppression of immune function in humans, studies are required to determine if melanin can provide protection against such suppression, the role of this suppression in the pathogenesis of skin cancer, the development of infectious disease and vaccine effectiveness, and the capacity for humans to develop adaptive, protective mechanisms which may limit damage from continued exposure to UV-B radiation.     

AVERAGE LATITUDINAL VARIATION IN ULTRAVIOLET RADIATION AT THE EARTH''S SURFACE

Abstract— Tabulated values are presented for ultraviolet radiation at the earth's surface as a function of wavelength, latitude, and season, for clear sky and seasonally and latitudinally averaged ozone amounts. These tabulations can be combined with any biological sensitivity function in order to obtain the seasonal and latitudinal variation of the corresponding effective doses. The integrated dosages, based on the erythemal sensitivity curve and on the Robertson-Berger sunburn-meter sensitivity curve, have also been calculated, and these are found to vary with latitude and season in very nearly the same way as 307 and 314 nm radiation, respectively.     

THE ROLE OF SOLAR ULTRAVIOLET RADIATION IN 'NATURAL' WATER PURIFICATION

Abstract— The concentration of Escherichia coli in the input and output of a tertiary wastewater system (4 lagoons) has been monitored over an 11 month period. The integrated flux of biologically active solar ultraviolet (UV) radiation was measured during this period. By also determining (1) the effective temperature in the system, (2) the growth rate of E. coli at the effective temperature, (3) the penetration of the solar UV into the lagoons, (4) the dose-response relation for killing of E. coli by UV and (5) the retention time of water in the system, it is possible to compare the 'die off' expected from solar UV exposure to the actual 'die off' observed for different batches of water.
The observed killing of E. coli was quite close to the values calculated, considering the numerous factors involved. Solar UV light would thus seem to be a very important factor in the natural purification of water. Because each successful species must possess characteristics (physiological or behavioral) which provide adequate resistance to solar UV, the ecological role of solar UV radiation has not been widely appreciated.     

ULTRAVIOLET SOLAR RADIATION IN THE HIGH LATITUDES OF SOUTH AMERICA

Abstract Measurements of the UV solar irradiance are available from Ushuaia, Tierra del Fuego during the spring and summer seasons of 4 consecutive years beginning in 1989. In addition, column ozone amounts derived from satellite-based measurements exist for this location over the entire period from 1980 through 1991. Monthly mean column ozone over Ushuaia shows a general decline over the observing period, and a large day-to-day variability exists within a given month. Ozone amounts for the years 1980 through 1986 combined with a model of radiative transfer provide a climatological baseline against which to interpret the more recent ground-based irradiance data. We focus on monthly mean noontime irradiances integrated over 5 nm wide spectral bands near 305 nm and 340 nm, respectively. Measurements in the 340 nm band show that cloudiness has a large influence on both the absolute monthly mean irradiances and their interannual variability. For example, during December the 340 nm band irradiance varied from approximately 50% of the clear-sky value in 1992 to 65% in 1991. When the influence of cloudiness is removed, most of the months show irradiances in the 305 nm band that are larger than predicted from the climatological ozone amounts. The largest percentage enhancement occurred in October 1991 when the irradiance exceeded the baseline by 56%. The largest absolute irradiances occur in December, where the measurements range from 5.8% below the baseline in 1991 to 31% above in 1990.     

TIME-RESOLVED ULTRAVIOLET ABSORPTION CHANGES IN THE PHOTOCYCLE OF BACTERIORHODOPSIN*

Abstract– The kinetics of the absorption changes associated with the perturbation of aromatic acids during the photocycle of bacteriorhodopsin (bR) were studied at room temperature with microsecond time-resolution. Flash experiments with nanosecond excitation at 532 nm were performed on the purple membrane suspension at a number of measuring wavelengths in the spectral range250–630 nm (to monitor both non-chromophore changes and the photocycle kinetics). The kinetic data collected at different wavelengths were simultaneously fitted with a sum of exponentials to obtain time-resolved UV-VIS difference spectra of photocycle intermediates. This approach allowed us to separate kinetically distinct contributions coupled with tryptophan(s) and tyrosine(s) perturbations. Contributions associated with a reversible perturbation of tryptophans appeared with complex (multistep) kinetics during the bRM transitions and relaxed in a single step during the M0 transition. A contribution associated with perturbation of the local environment of tyrosine appeared before the L and relaxed during the Ob̊ transition.     

SOLAR ULTRAVIOLET RADIATION AT THE EARTH'S SURFACE

The biologically effective ultraviolet irradiance at the earth's surface varies with the elevation of the sun, the atmospheric ozone amount, and with the abundance of scatterers and absorbers of natural and anthropogenic origin. Taken alone, the reported decrease in column ozone over the Northern Hemisphere between 1969 and 1986 implies an increase in erythemal irradiance at the ground of four percent or less during summer. However, an increase in tropospheric absorption, arising from polluting gases or particulates over localized areas, could more than offset the predicted enhancement in radiation. Any such extra absorption is likely to be highly regional in nature and does not imply that a decrease in erythemal radiation has occurred on a global basis. The Antarctic 'ozone hole' represents a special case in which a portion of the earth has experienced ultraviolet radiation levels during spring that are far in excess of those which prevailed prior to the present decade.     

SOLAR ULTRAVIOLET RADIATION IN SOUTHEAST ENGLAND: THE CASE FOR SPECTRAL MEASUREMENTS

Spectral measurements of the solar ultraviolet spectrum have been made at Reading, England, since July 1989. The data presented show the daily and annual changes in the ultraviolet-B (UV-B) part of the spectrum, and illustrate the dominance of the longer wavelengths in grouping the data into a single broadband measurement. The temporal changes (diurnal and annual) cover 2 orders of magnitude at 300 nm, and a factor of 5 at 320 nm. In a single statement of UV-B levels the trend at longer wavelengths predominates, hiding the larger differences at the more biologically important wavelengths. However, the data also show that at mid-high latitudes the UV irradiance at noon in winter is less than that received at any time during the middle 12 h of daylight in summer, and this should be acknowledged when assessing the consequences of ozone depletion. Atmospheric scattering of short wavelength radiation is compared to that of the entire solar spectrum from measurements of diffuse radiation: on a clear day70–100% of UV-B was diffuse in Reading, with a slight wavelength dependency increasing diffuse radiation at short wavelengths. Under the same conditions scattering of total solar radiation was 21%. The effect of cloud cover is briefly discussed for two specific cases of complete, uniform cloud cover, when attenuation by clouds was approx. 40 and 68%, with little wavelength dependence in either case.     

INDUCTION OF SKIN TUMORS IN THE RAT BY SINGLE EXPOSURE TO ULTRAVIOLET RADIATION

Abstract— The dose response for tumor induction in albino rat skin by single exposures of UV radiation has been characterized. The shaved dorsal skin of 202 animals was exposed to either of two sources: one emitting a broad spectrum of wavelengths from 275 to 375 nm, and the other emitting at 254 nm. Skin tumors began to appear within 10 weeks of exposure and continued to appear for 70 weeks. The highest tumor yield was 5.5 tumors per rat and occurred when the rats were exposed to 13.0 times 10⁴ J/m² of the 275–375 nm UV. The 275–375 nm UV was about eight times as effective as the 254 nm UV for the induction of tumors throughout the exposure range from 0.8 times 10⁴ to 26.0 times 10⁴J/m². Tissue destruction and hair follicle damage was found at the highest exposure to 275–375 nm UV but at none of the exposures to 254 nm UV. Repeated weekly exposures to 275–375 nm UV proved less effective than an equivalent single exposure for inducing tumors, even though the multiple exposures caused more severe skin damage. The transmission of the UV through excised samples of rat epidermis indicated that the exposure to the basal cell layer was about 3% of the surface exposure at 254 nm and about 15% of the surface exposure between 275 and 320 nm. The dependence of tumor yield on UV exposure was linear for 254 nm UV but was more complex for the 275–375 nm UV. For the latter more tumors were produced per unit exposure at lower exposures than at higher exposures.     

THE EFFECT OF ULTRAVIOLET RADIATION ON WHEAT ROOT VESICLES ENRICHED IN PLASMA MEMBRANE

Abstract— The irradiation of plant cells with UV radiation (254nm) causes various solutes to leak from the cells. Vesicles enriched in plasma membranes were prepared from wheat roots. These were used to determine whether UV radiation alters membrane function by direct action on the membranes and to distinguish between the chemical effects produced by high and low fluences of UV. The plasma membrane-associated K⁺-stimulated ATPase was very sensitive to UV radiation (100% inhibition with 1.35kJ/m²). ATPase activity measured in the absence of K⁺ and K⁺-stimulated ATPase activity measured in the presence of diethylstilbestrol were much less sensitive. Lipid breakdown, as measured by malondialdehyde production, occurred only at UV fluences greater than 1.8 kJ/m².