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Stochastic generation of synthetic minutely irradiance time series derived from mean hourly weather observation data

机译:从每小时平均天气观测数据得出的合成微小辐照时间序列的随机生成

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摘要

Synthetic minutely irradiance time series are utilised in non-spatial solar energy system research simulations. It is necessary that they accurately capture irradiance fluctuations and variability inherent in the solar resource. This article describes a methodology to generate a synthetic minutely irradiance time series from widely available hourly weather observation data. The weather observation data are used to produce a set of Markov chains taking into account seasonal, diurnal, and pressure influences on transition probabilities of cloud cover. Cloud dynamics are based on a power-law probability distribution, from which cloud length and duration are derived. Atmospheric transmission losses are simulated with minutely variability, using atmospheric profiles from meteorological reanalysis data and cloud attenuation derived real-world observations. Both direct and diffuse irradiance are calculated, from which total irradiance is determined on an arbitrary plane. The method is applied to the city of Leeds, UK, and validated using independent hourly radiation measurements from the same site. Variability and ramp rate are validated using 1-min resolution irradiance data from the town of Cambourne, Cornwall, UK. The hourly irradiance frequency distribution correlates with R-2 = 0.996 whilst the mean hourly irradiance correlates with R-2 = 0.971, the daily variability indices cumulative probability distribution function (CDF), 1-min irradiance ramp rate CDF and 1-min irradiance frequency CDF are also shown to correlate with R-2 = 0.9903, 1.000, and 0.9994 respectively. Kolmogorov Smirnov tests on 1-min data for each day show that the ramp rate frequency of occurrence is captured with a high significance level of 99.99%, whilst the irradiance frequency distribution and minutely variability indices are captured at significances of 99% and 97.5% respectively. The use of multiple Markov chains and detailed consideration of the atmospheric losses are shown to be essential elements for the generation of realistic minutely irradiance time series over a typical meteorological year. A freely downloadable example of the model is made available and may be configured to the particular requirements of users or incorporated into other models. (C) 2015 The Authors. Published by Elsevier Ltd.
机译:合成的微小辐照时间序列被用于非空间太阳能系统的研究模拟中。它们必须准确捕获太阳能资源固有的辐照度波动和可变性。本文介绍了一种方法,可从广泛使用的每小时天气观测数据中生成合成的分钟辐照时间序列。气象观测数据用于生成一组马尔可夫链,其中考虑了季节,昼夜和压力对云层过渡概率的影响。云动力学基于幂律概率分布,从中得出云的长度和持续时间。利用来自气象再分析数据的大气廓线和通过云衰减得出的真实世界观测值,可以对大气传输损失进行微小的变化模拟。计算直接辐照度和漫射辐照度,由此确定任意平面上的总辐照度。该方法应用于英国利兹市,并使用来自同一地点的独立每小时辐射测量结果进行了验证。使用来自英国康沃尔郡Cambourne镇的1分钟分辨率辐照数据验证了变异性和斜率。每小时辐照度频率分布与R-2 = 0.996相关,而平均每小时辐照度与R-2 = 0.971相关,日变化指数累积概率分布函数(CDF),1分钟辐照度斜率CDF和1分钟辐照频率还显示了CDF分别与R-2 = 0.9903、1.000和0.9994相关。每天用1分钟数据进行的Kolmogorov Smirnov测试表明,捕获的斜坡速率发生频率具有99.99%的高显着性水平,而辐照频率分布和微小变异性指数分别具有99%和97.5%的显着性。 。在典型的气象年中,使用多个马尔可夫链和详细考虑大气损失是生成现实的细微辐照时间序列的基本要素。该模型的一个可免费下载的示例可用,可以根据用户的特定要求进行配置,也可以合并到其他模型中。 (C)2015作者。由Elsevier Ltd.发布

著录项

  • 来源
    《Solar Energy》 |2015年第5期|229-242|共14页
  • 作者单位

    Univ Leeds, Energy Res Inst, Sch Chem & Proc Engn, Leeds LS2 9JT, W Yorkshire, England;

    Univ Leeds, Energy Res Inst, Sch Chem & Proc Engn, Leeds LS2 9JT, W Yorkshire, England;

    Univ Leeds, Energy Res Inst, Sch Chem & Proc Engn, Leeds LS2 9JT, W Yorkshire, England|Univ Leeds, Sustainabil Res Inst, Sch Earth & Environm, Leeds LS2 9JT, W Yorkshire, England|Univ Leeds, Ctr Integrated Energy Res, Leeds LS2 9JT, W Yorkshire, England;

    Univ Leeds, Energy Res Inst, Sch Chem & Proc Engn, Leeds LS2 9JT, W Yorkshire, England;

  • 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

    Irradiance generation; Resource modelling; Minute resolution; Stochastic modelling; Cloud cover;

    机译:辐照度产生;资源建模;分钟分辨率;随机建模;云量;

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