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奥地利紫外线监测网络所采用的质量保证和质量控制方法。

Quality assurance and quality control methodologies used within the Austrian UV monitoring network.

作者信息

Mario Blumthaler

机构信息

Institute for Medical Physics, Muellerstreet 44, A-6020 Innsbruck, Austria.

出版信息

Radiat Prot Dosimetry. 2004;111(4):359-62. doi: 10.1093/rpd/nch054.

Abstract

The Austrian UVB monitoring network is operational since 1997. Nine detectors for measuring erythemally weighted solar UV irradiance are distributed over Austria in order to cover the main populated areas as well as different levels of altitude. The detectors are calibrated to indicate the UV-Index, the internationally agreed unit for erythemally weighted solar UV irradiance. Calibration is carried out in the laboratory for determination of spectral sensitivity of each detector, and under the sun for absolute comparison with a well-calibrated, double-monochromator spectroradiometer. For the conversion from detector-weighted units to erythemally weighted units a lookup table is used, which is calculated using a radiative transfer model and which reflects the dependence of the conversion on the solar zenith angle and total ozone content of the atmosphere. The uncertainty of the calibration is about +/-7%, dominated by the uncertainty of the calibration lamp for the spectroradiometer (+/-4%). The long-term stability of this type of detectors has been found to be not satisfactory. Therefore, routinely every year all detectors are completely recalibrated. Variations of the calibration factors up to +/-10% are found. Thus, during routine operation, several measures take place for quality control. The measured data are compared to results of model calculations with a radiative transfer model, where clear sky and an aerosol-free atmosphere are assumed. At each site, the UV data are also compared with data from a co-located pyranometer measuring total solar irradiance. These two radiation quantities are well correlated, especially on clear days and when the ozone content is taken into account. If suspicious measurements are found for one detector in the network, a well-calibrated travelling reference detector of the same type is set up side-by-side, allowing the identification of relative differences of approximately 3%. If necessary, a recalibration is carried out. As the main aim for the Austrian UV monitoring network is the information of the public about the actual levels of UVB irradiance, the measurement results are published on-line in the Internet (http://www.uibk.ac.at/projects/uv-index). For the previous day and backwards approximately 2 years, the distribution of maximal UVB levels over Austria is shown on a regional map. Additionally, near real-time data of most of the measurement stations are presented with a delay of usually less than half-an-hour. Together with these actually measured data there is also shown the diurnal variation of the maximal expected value of the UV-Index under ideal clear conditions.

摘要

奥地利UVB监测网络自1997年开始运行。九个用于测量红斑加权太阳紫外线辐照度的探测器分布在奥地利各地,以覆盖主要人口聚居区以及不同海拔高度。这些探测器经过校准以指示UV指数,这是国际上认可的红斑加权太阳紫外线辐照度单位。校准在实验室中进行以确定每个探测器的光谱灵敏度,并在阳光下进行与校准良好的双单色仪光谱辐射计的绝对比较。对于从探测器加权单位到红斑加权单位的转换,使用查找表,该表使用辐射传输模型计算得出,反映了转换对太阳天顶角和大气总臭氧含量的依赖性。校准的不确定度约为±7%,主要由光谱辐射计校准灯的不确定度(±4%)主导。已发现此类探测器的长期稳定性不尽人意。因此,每年都会定期对所有探测器进行全面重新校准。发现校准因子的变化高达±10%。因此,在日常运行中,会采取多项质量控制措施。将测量数据与假设晴空且无气溶胶大气的辐射传输模型的模型计算结果进行比较。在每个站点,UV数据还会与并置的测量总太阳辐照度的总日射表的数据进行比较。这两个辐射量具有良好的相关性,特别是在晴天且考虑臭氧含量时。如果在网络中发现某个探测器的测量结果可疑,则会并排放置一个校准良好的同类型移动参考探测器,以便识别约3%的相对差异。如有必要,进行重新校准。由于奥地利UV监测网络的主要目标是向公众提供有关UVB辐照度实际水平的信息,测量结果会在互联网上在线发布(http://www.uibk.ac.at/projects/uv-index)。对于前一天及之前大约两年的时间,奥地利UVB最大水平的分布会在区域地图上显示。此外,大多数测量站的近实时数据通常会延迟不到半小时呈现。除了这些实际测量数据外,还会显示理想晴空条件下UV指数最大预期值的日变化。

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