Introduction

Professor Carl Dorno (founder of PMOD in 1907), who’s main interest was solar radiation and its relation to bioclimatological effects, investigated the very short wavelength part of direct solar radiation already in his early years at Davos. Spectrally resolved measurements were first performed using photochemical and photometrical methods. In honour of his work, the shortest solar radiation penetrating to the Earth surface, became known as “Dornostrahlung”, the spectral part which is nowadays called solar UV-B radiation. Dorno was a strong advocate of the “Cadmiumzell” which from 1916 to the 1930s was routinely used at Davos for spectrally integrated UV-measurements. The large solar height (seasonal dependency) and altitude dependency of solar UV-radiation was deduced from these measurements among other interesting findings.

Dr. Paul Bener conducted intensive investigations of the UV-radiation field between 1954 and 1976. His spectrophotometric measurements of direct, diffuse and global UV-radiation at Davos, Weissfluhgipfel and Basel, allowed him to investigate the UV part of the solar radiation with regard to solar height, altitude, ozone amount and cloud influence. Bener also performed extensive UV calculations to extrapolate into regions in which measurements could not be performed due to technical or logistical reasons. Assumptions had to be made to cover the full picture for a global UV-climatology. Beners investigations were published in many reports and publications.

From 1975 to 1985, Davos was one of 14 stations of the worldwide UV-network which was maintained by the Temple University School of Medicine (Philadelphia, PA, USA). Robertson-Berger Type-500 broadband UV-Biometers, which integrate over the human skin erythema action spectrum, were used at these stations. The network was unfortunately discontinued due to the lack of funding.

Measurements and Research Activities from 1993 to 2005

Broadband

UV broadband measurements resumed in 1993 using UV-Biometers from Solar Light, which weight the UV radiation to the human skin erythema action spectrum and therefore predominantly measure UV-B radiation. Long-term measurements of the direct solar and diffuse sky components, showed positive results with regard to the accuracy of broadband UV measurements and to the understanding of the radiation field. Direct radiation was measured with a full-view angle of 8° whereas the instrument measuring diffuse radiation had a shading disc covering the sun, also with a full-view angle of 8°. An additional UV-Biometer measuring global radiation was used for redundancy and quality control of the measurements. The UV-A radiation was separately measured with a global Solar Light UV-A bandpass instrument.

Calibration was maintained by periodically comparing UV-Biometers to the SWISS reference instrument using the sun as a source. The SWISS reference instrument took part in the WMO/STUK 1995 intercomparison at Helsinki and was periodically compared to spectroradiometers.

Although this instrumentation was not accurate enough to measure long term-trends, it was well-suited to establish a UV climatology and to provide the necessary information for UV forecasts and warnings.

Narrowband

Following the long tradition of sunphotometry at PMOD/WRC, filter radiometric techniques were extended to the UV-range. UV Precision Filter Radiometers (UV-PFR) with narrowband interference filters were used to measure UV radiation at fixed wavelengths. The final layout of the UV-PFR basically follows the design of PFRs built at PMOD/WRC for accurate aerosol optical depth measurements. The instrument has four channels, three in the UV-B range with center wavelengths at 303, 310 and 319 nm and one channel in the UV-A range at 340 nm with respective bandwidths of 1, 2, 2 and 4 nm. UV-PFRs were periodically calibrated against trap-detectors in the laboratory which allows a very high accuracy of about 0.5%, and are therefore well suited for UV trend measurements.

UV-Network

In collaboration with the Swiss Meteorological Institute (SMI; nowadays called MeteoSwiss), the three component broadband UV-B (direct, diffuse and global) and UV-A instrumentation were installed on a limited number of RASTA-UV stations in order to build a Swiss National UV network. All stations are additionally equipped with direct, diffuse and global solar shortwave (SW) instruments and a pyrgeometer measuring downwelling longwave (LW) radiation as well as a sunphotometer to measure aerosol optical depth. The Swiss national UV-network is part of the Swiss Atmospheric Radiation Monitoring programme (SACRAM). Besides the station at Davos (1610 m asl), three other stations are in operation at Payerne (490 m asl), the Jungfraujoch (3580 m asl) and Locarno-Monti (370m asl). PMOD/WRC also equipped a UV research station in the observation and investigation field of the Swiss Federal Institute for Snow and Avalanche Research (SLF) which is located in the vicinity of the Weissfluhjoch (2540 m asl), Davos. At this station additional instruments measure reflected UV-B, UV-A, SW and upwelling LW radiation for albedo investigations. These four operational stations of the Swiss National UV network provide an interesting vertical profile of the UV radiation field over Switzerland going from 490 to 3580m asl.

Routine ozone measurements are now being conducted at Davos with Dobson and Brewer instruments from the former MeteoSwiss station at Arosa. Ozone profiles from the ground to the stratosphere are routinely measured at Payerne using radiosondes.

For further information please contact: Dr. Julian Gröbner, Dr. Gregor Hülsen, Dr. Luca Egli