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Minute resolution estimates of the diffuse fraction of global irradiance for southeastern Australia

机译:东南澳大利亚的全球辐照度扩散分数的分钟分辨率估计

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摘要

Separating global horizontal irradiance measurements into direct and diffuse components has been vigorously discussed over the past half-century of solar radiation research leading to the creation of many models which attempt to compute these components with varying degrees of success. However, over the course of this discussion, nearly all studies have focused on hourly values, with no studies that have proposed a model for minute-level values of irradiance. As data-logging technologies have become much more prolific and their storage capabilities much larger, solar radiation monitoring sites are more commonly logging data at intervals much less than one hour, but no models exists that are designed to separate these measurements into direct and diffuse components. In Australia, the Australian Bureau of Meteorology and the Australian Solar Institute have compiled a dataset of tens of millions of one-minute global, direct and diffuse solar irradiance observations, comprising data from regions all around Australia. This dataset provides a unique opportunity to investigate the relationships between global irradiance and its direct and diffuse components at higher resolution than has previously been possible. Herein, the largest and most complete diffuse fraction model analysis yet undertaken for Australian solar radiation data, and. the first ever to focus on minute resolution data is reported. Nine of the most prominent diffuse fraction, or "separation", models are tested against minute resolution radiation data from three datasets. The first removed cloud enhancement events in accordance with practices undertaken by the majority of studies in the literature. The second retains these events in order to assess which model would be best suited for operational purposes. The third consisted of only clear sky observations, in order to assess the performance of diffuse fraction models under clear skies. Through the course of this study only the Perez model was found to perform satisfactorily for minute resolution data at sites in southeastern Australia. Three new diffuse models proposed in this study, one trained for each of the three datasets, were found to greatly exceed the performance of existing modeling techniques, with slight improvements over the Perez model. (c) 2015 Elsevier Ltd. All rights reserved.
机译:在过去的半个世纪的太阳辐射研究中,已经进行了激烈的讨论,将整体水平辐照度测量分为直接分量和散射分量,从而导致创建了许多模型,这些模型试图以不同程度的成功来计算这些分量。但是,在整个讨论过程中,几乎所有研究都集中在小时值上,没有研究提出了辐照度的分钟级值模型。随着数据记录技术变得越来越多产并且它们的存储能力变得越来越大,太阳辐射监测站点更经常地以不到一小时的时间间隔记录数据,但是不存在用于将这些测量结果分为直接分量和扩散分量的模型。 。在澳大利亚,澳大利亚气象局和澳大利亚太阳能研究所已经汇编了一个数千万个一分钟的全球,直接和散布的太阳辐照度观测数据集,包括来自澳大利亚各地的数据。该数据集提供了一个独特的机会,可以以比以前更高的分辨率研究全局辐照度及其直接分量和扩散分量之间的关系。在此,对澳大利亚太阳辐射数据进行了最大,最完整的扩散分数模型分析。据报道,这是第一个专注于分钟分辨率数据的报告。针对来自三个数据集的微小分辨率辐射数据,测试了九个最突出的扩散部分或“分离”模型。根据文献中大多数研究采取的做法,第一次消除了云增强事件。第二个保留这些事件,以便评估哪种模型最适合运营目的。第三部分仅包括晴朗的天空观测,以评估在晴朗的天空下扩散分数模型的性能。在本研究过程中,仅发现Perez模型在澳大利亚东南部站点的分钟分辨率数据上表现令人满意。在这项研究中提出的三个新的扩散模型,其中一个针对三个数据集进行了训练,被发现大大超过了现有建模技术的性能,对Perez模型进行了一些改进。 (c)2015 Elsevier Ltd.保留所有权利。

著录项

  • 来源
    《Solar Energy》 |2015年第6期|215-237|共23页
  • 作者

    Engerer N. A.;

  • 作者单位

    Australian Natl Univ, Fenner Sch Environm & Soc, Canberra, ACT, Australia|Natl ICT Australia, Canberra Res Lab, Canberra, ACT, Australia;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Solar radiation; Diffuse fraction; Radiation model; Cloud enhancement; Validation; DNI;

    机译:太阳辐射;扩散分数;辐射模型;云增强;验证;DNI;

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