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Neural network for the estimation of UV erythemal irradiance using solar broadband irradiance

机译:神经网络,利用太阳宽带辐照度估算紫外线红斑辐照度

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In recent years there has been a substantial increase in attempts to model radiative flux of ultraviolet radiation, UV. In this paper we present the development of an artificial neural network (ANN) model that can be used to estimate solar UV erythemal irradiance, UVER, based on optical air mass, ozone columnar content and broadband solar irradiance. The study was developed at seven stations in the Iberian Peninsula using data recorded at A Coruna, Malaga, Murcia and Santander, during 2000-2003; at Madrid in the period 2000-2002; at Valencia in 2000, 2001 and 2003: and at Zaragoza, from 2001 to 2003. The UVER observations are recorded as half-hour average values. The measurements were performed in the framework of the Spanish UV-B radiometric network operated and maintained by the Spanish Meteorological Institute. In order to train and validate the Multi-layer Perceptron neural networks, independent subsets of data were extracted from the complete database at each station. The networks developed at each place when applied to an independent data set recorded at the same location provide estimates with mean bias deviation less than 1% and root mean square deviation below 17% for all the sites. The generalization network developed using data registered at A Coruna, Madrid, Murcia and Zaragoza provides estimates at all the locations with RMSD below 19%. According to these results, the use of solar broadband irradiances for the estimation of ultraviolet erythemal irradiance provides a tool that can solve the difficulties associated to the retrieval of appropriate information on the cloud field by human observers. In this sense, the proposed method seems appropriate to use the widespread networks of solar broadband irradiance to obtain ultraviolet erythemal irradiance data sets in places where this radiative flux is not measured or to extend back in time the existing data sets. Copyright (C) 2007 Royal Meteorological Society.
机译:近年来,对紫外线辐射的辐射通量进行建模的尝试已大大增加。在本文中,我们介绍了一个人工神经网络(ANN)模型的开发,该模型可用于根据光学空气质量,臭氧柱状含量和宽带太阳辐照度来估算太阳紫外线红斑辐照度UVER。这项研究是根据2000-2003年在拉科鲁尼亚,马拉加,穆尔西亚和桑坦德的记录在伊比利亚半岛的七个站点进行的; 2000-2002年在马德里;分别在2000年,2001年和2003年在巴伦西亚;以及在2001年至2003年在萨拉戈萨。UVER观测值记录为半小时平均值。这些测量是在由西班牙气象研究所运营和维护的西班牙UV-B辐射网络的框架内进行的。为了训练和验证多层感知器神经网络,从每个站点的完整数据库中提取了独立的数据子集。当将其应用于在同一位置记录的独立数据集时,在每个位置开发的网络提供的估计值对所有站点均小于1%,均方根小于17%。使用在拉科鲁尼亚,马德里,穆尔西亚和萨拉戈萨注册的数据开发的概括网络提供了RMSD低于19%的所有地点的估计值。根据这些结果,使用太阳能宽带辐照度估算紫外线红斑辐照度可提供一种工具,可以解决与人类观察者在云场中检索适当信息有关的困难。从这个意义上讲,所提出的方法似乎适合于使用广泛的太阳能宽带辐照度网络在未测量该辐射通量的地方获得紫外线红斑辐照度数据集,或将时间范围扩展到现有数据集。皇家气象学会(C)2007。

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