1ST SOUTHERN-HEMISPHERE INTERCOMPARISON OF MEASURED SOLAR UV SPECTRA

Citation
Rl. Mckenzie et al., 1ST SOUTHERN-HEMISPHERE INTERCOMPARISON OF MEASURED SOLAR UV SPECTRA, Geophysical research letters, 20(20), 1993, pp. 2223-2226
Citations number
13
Categorie Soggetti
Geosciences, Interdisciplinary
ISSN journal
00948276
Volume
20
Issue
20
Year of publication
1993
Pages
2223 - 2226
Database
ISI
SICI code
0094-8276(1993)20:20<2223:1SIOMS>2.0.ZU;2-7
Abstract
Three UV spectroradiometers from the National Institute of Water and A tmospheric Research (NIWA) New Zealand, the Fraunhofer Institute (IFU) Germany, and the Australian Radiation Laboratory (ARL) Australia were intercompared at Lauder NZ on 23 February 1993. Over the spectral ran ge 290-400 nm, the agreement between the IFU and NIWA instruments was better than 5%. At noon on this day, the irradiances measured by all t hree instruments agreed within +/- 10%, except at wavelengths shorter than 300 nm, where the ARL instrument gave higher readings. At larger solar zenith angles (SZA) the differences at short wavelengths were mo re pronounced, and at wavelengths above 300 nm the ARL measurements we re systematically lower. The reasons for these differences are discuss ed. Having established the differences between the sets of instrumenta tion, spectra of maximum clear sky UV irradiances observed by these gr oups in New Zealand, Australia, and Europe are compared. The erythemal ly weighted irradiance observed in Melbourne Australia was the highest (0.35 W m-2. Respective maxima for Lauder NZ and for Neuherberg Germa ny were 85% and 66% of that in Australia. Differences are larger for D NA-weighted UV.