4.7 Article

Spectral UV measurements in Austria from 1994 to 2006: investigations of short- and long-term changes

Journal

ATMOSPHERIC CHEMISTRY AND PHYSICS
Volume 8, Issue 23, Pages 7033-7043

Publisher

COPERNICUS GESELLSCHAFT MBH
DOI: 10.5194/acp-8-7033-2008

Keywords

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Funding

  1. Austrian Ministry for Environment
  2. Commission of the European Communities

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The influence of variability of atmospheric parameters on short- and long-term changes of spectral UV irradiance measured at the Sonnblick observatory (47.03 degrees N, 12.57 degrees E, 3106m) during the period from 1994 to 2006 is studied. Measurements were performed with the Brewer # 093 single-monochromator spectrophotometer and with a Bentham DM 150 spectroradiometer (double-monochromator). The influence of ozone, albedo, snowline and clouds on UV variability is evaluated for each parameter separately using 10-year climatology. It is found that the effect of total ozone on short- term variability of UV irradiance at 305 nm can be more than 200% and on average more than 50%. Clouds can cause variability of 150% or more and on average 35%. Variability caused by albedo reaches a maximum of 32% in April (6% on average). In summer and autumn, total ozone and clouds strongly influence the variability of UV radiation, whereas in winter and spring ozone has the more pronounced effect. A decrease in snowline height from 3000m to 800ma.s.l. enhances the UV irradiance by a factor of 1.24 for clear sky conditions and by a factor of 1.7 for 8/8 cloud cover. Long-term trends are investigated for the time period from 1994 to 2006 based on clear-sky measurements, using the non-parametric Mann-Kendall trend test. Significant downward trends (99% confidence level) are found for solar zenith angle 55 degrees at wavelengths from 305 nm to 324 nm and erythemally weighted irradiance according to CIE, which are caused by an increase in sunshine duration during periods of high total column ozone. Significant trends (90% confidence level) were also found for other combinations of wavelength and SZA.

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