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Aviation and the Global Atmosphere

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<strong>Aviation</strong> <strong>and</strong> <strong>the</strong> <strong>Global</strong> <strong>Atmosphere</strong><br />

effects that are weakly wavelength-dependent. In any case, comparison of measured irradiances with modeled irradiances suffers from <strong>the</strong> limited availability <strong>and</strong><br />

quality of data necessary to describe <strong>the</strong> atmosphere (Schw<strong>and</strong>er et al., 1997).<br />

Several studies have compared measured irradiances with model simulations. Measurements made under clear sky conditions <strong>and</strong> no snow cover demonstrate quite<br />

convincingly that lower ozone values result in higher UV irradiance levels at <strong>the</strong> surface of <strong>the</strong> Earth; <strong>the</strong>se data sets have been used to quantify <strong>the</strong> dependence<br />

statistically (McKenzie et al., 1991; Booth <strong>and</strong> Madronich, 1994; Kerr et al., 1994). When <strong>the</strong>se measured dependencies are compared with those computed for clearsky<br />

conditions, no aerosols, <strong>and</strong> low ground reflectivity (no snow cover), reasonable agreement has generally been found (McKenzie et al., 1991; Wang <strong>and</strong> Lenoble,<br />

1994; Forster et al., 1995).<br />

The availability of aerosol optical depth measurements in <strong>the</strong> UV has allowed studies of <strong>the</strong> effects of particulates on ground-level irradiance. Mayer et al. (1997)<br />

compare clear-sky UV spectral data obtained at Garmish-Partenkirchen, Germany, between 1994-96 with model simulations. The model simulations use ozone <strong>and</strong><br />

aerosol optical depth measurements as inputs. Systematic differences between measured irradiance spectra <strong>and</strong> model results were between -11% <strong>and</strong> +2%. It was<br />

necessary to introduce ground-level aerosols into <strong>the</strong> model to achieve agreement to within 5%. From total ozone, aerosol optical depth, <strong>and</strong> spectral UV irradiance<br />

measurements made under clear-sky conditions at Toronto between 1989-91, Kerr (1997) demonstrates that most of <strong>the</strong> observed variability of UV irradiance between<br />

300 <strong>and</strong> 325 nm can be explained by ozone <strong>and</strong> aerosols. The remaining unexplained variability is 4% at 300 nm <strong>and</strong> 2% at 325 nm. Comparison of <strong>the</strong> observed<br />

dependence of UV irradiance on aerosol optical depth with model results suggests that typical aerosols over Toronto are slightly absorbing (Krotkov et al., 1998). The<br />

model also shows that a single scattering albedo of about 0.95 for aerosols gives <strong>the</strong> best agreement with <strong>the</strong> Toronto data.<br />

Surface UV irradiance is also reduced by atmospheric sulfur dioxide (SO2 ), which has strong absorption features at UV wavelengths <strong>and</strong> occurs both naturally from<br />

volcanic emissions <strong>and</strong> anthropogenically from industrial sources (Zerefos, 1997; Kerr et al., 1998). The presence of SO2 can interfere with <strong>the</strong> measurement of ozone<br />

<strong>and</strong> estimates of ozone <strong>and</strong> UV trends at sites affected by local air pollution (Bais et al., 1993; De Meur <strong>and</strong> De Backer, 1993). However, measurements made at<br />

several sites in less-polluted situations suggest that <strong>the</strong> effects of SO2 on UV over wider areas are small (Fioletov et al., 1997).<br />

A method developed recently to calculate surface spectral UV irradiance uses Total Ozone Mapping Spectrometer (TOMS) satellite measurements of ozone <strong>and</strong> UV<br />

reflectivity with a radiative transfer model (Eck et al., 1995; Herman et al., 1996; Krotkov et al., 1998). Comparison of model results with ground-based measurements<br />

made at Toronto under clear skies indicates agreement of absolute irradiance to about 2% after correction for <strong>the</strong> angular response of <strong>the</strong> ground-based instrument.<br />

The effects of surface albedo have been considered in <strong>the</strong> UV-A (324 nm), where <strong>the</strong>re is negligible ozone absorption, by observing <strong>the</strong> difference between<br />

measurements made with <strong>and</strong> without snow cover at several sites (Wardle et al., 1997). The presence of snow was found to enhance irradiance differently from one<br />

site to ano<strong>the</strong>r. The minimum enhancement was 8% at Halifax, Canada; <strong>the</strong> maximum was 39% at Churchill, Canada. The difference between <strong>the</strong>se two sites is likely<br />

to be a result of differences in <strong>the</strong> surrounding terrain <strong>and</strong> snow texture. For example, <strong>the</strong> clean snow on <strong>the</strong> flat terrain around Churchill would result in a higher<br />

average surface albedo than at Halifax, where snow would be dirtier in <strong>the</strong> suburban areas <strong>and</strong> not present on nearby open water. Model results show an<br />

enhancement of about 50% for an albedo of about 1 (Deguen<strong>the</strong>r et al., 1998; Krotkov et al., 1998). Although <strong>the</strong>re are no direct measurements of albedo available<br />

when snow is present, <strong>the</strong> model gives quite reasonable effective albedo values of about 20% at Halifax <strong>and</strong> 90% at Churchill. Model results of Deguen<strong>the</strong>r et al.<br />

(1998) show that irradiance values are affected by surface albedo (snow cover) at distances up to 40 km; most of <strong>the</strong> dependence is influenced by albedo within a<br />

radius of 10 km.<br />

Variability in cloud cover is <strong>the</strong> largest contributor to short-term changes in surface UV irradiance. It is possible to include <strong>the</strong> effects of clouds in radiative transfer<br />

calculations to various levels of approximation. However, routinely available observational data do not allow a rigorous characterization of cloud optical properties.<br />

Measurements show that UV spectral transmittance depends on cloud type, cloud thickness, <strong>and</strong> whe<strong>the</strong>r <strong>the</strong>re are absorbers within <strong>the</strong> cloud. Although detailed<br />

quantification of <strong>the</strong>se dependencies requires fur<strong>the</strong>r research, some general conclusions can be made. The effects of thin clouds are weakly (

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