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Reconstruction of daily solar UV irradiation from 1893 to 2002 in Potsdam, Germany

机译:从1893年到2002年在德国波茨坦重建每日太阳紫外线辐射

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摘要

Long-term records of solar UV radiation reaching the Earth's surface are scarce. Radiative transfer calculations and statistical models are two options used to reconstruct decadal changes in solar UV radiation from long-term records of measured atmospheric parameters that contain information on the effect of clouds, atmospheric aerosols and ground albedo on UV radiation. Based on earlier studies, where the long-term variation of daily solar UV irradiation was derived from measured global and diffuse irradiation as well as atmospheric ozone by a non-linear regression method [Feister et al. (2002) Photochem Photobiol 76:281-293], we present another approach for the reconstruction of time series of solar UV radiation. An artificial neural network (ANN) was trained with measurements of solar UV irradiation taken at the Meteorological Observatory in Potsdam, Germany, as well as measured parameters with long-term records such as global and diffuse radiation, sunshine duration, horizontal visibility and column ozone. This study is focussed on the reconstruction of daily broad-band UV-B (280-315 nm), UV-A (315-400 nm) and erythemal UV irradiation (ER). Due to the rapid changes in cloudiness at mid-latitude sites, solar UV irradiance exhibits appreciable short-term variability. One of the main advantages of the statistical method is that it uses doses of highly variable input parameters calculated from individual spot measurements taken at short time intervals, which thus do represent the short-term variability of solar irradiance.
机译:很少有太阳紫外线辐射到达地球表面的长期记录。辐射传递计算和统计模型是从长期测量的大气参数记录中重建太阳UV辐射年代际变化的两个选项,这些记录包含有关云,大气气溶胶和地面反照率对UV辐射影响的信息。根据较早的研究,每天的紫外线辐射的长期变化是通过非线性回归方法从实测的总辐射和漫辐射以及大气臭氧中得出的[Feister等。 (2002)Photochem Photobiol 76:281-293],我们提出了重建太阳紫外线辐射时间序列的另一种方法。训练了一个人工神经网络(ANN),其测量方法是在德国波茨坦的气象台进行太阳紫外线辐射的测量,并具有长期记录的测量参数,例如全球和漫辐射,日照时间,水平能见度和柱臭氧。这项研究的重点是重建每日宽带UV-B(280-315 nm),UV-A(315-400 nm)和红斑紫外线(ER)。由于中纬度地区的乌云迅速变化,太阳紫外线辐射表现出明显的短期变化。统计方法的主要优点之一是,它使用根据在短时间间隔进行的单个点测量值计算出的高度可变输入参数的剂量,因此确实代表了太阳辐照度的短期变化。

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