高分辨率全球辐照度时间序列的分钟分辨率降尺度算法

Diamantis Almpantis , Henrik Davidsson , Martin Andersson
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引用次数: 0

摘要

大量研究表明,太阳辐照数据的分辨率对每小时生产模型的结果有重大影响。光伏(PV)系统的精确集成有时需要高分辨率的全球水平辐照度(GHI)时间序列,以捕捉辐照度快速变化引起的光伏发电量的快速波动。大多数现有数据库提供的数据都是以小时为单位的分辨率,导致光伏模拟缺乏准确性。现有的开放源全球水平辐照度小时平均值无法充分反映这种波动性,尤其是当光伏系统与快速斜率技术相结合时。本研究采用了一种易于使用的算法,从每小时平均值和晴空辐照度数据集中合成高分辨率的全球水平辐照度时间序列。通过采用线性插值(一种有助于实现所需的时间分辨率的技术)和计算关键因素,该算法可识别以短期天气现象为特征的时段,从而创建一个能准确反映这些动态的高分辨率时间序列。避免使用概率成分和机器学习技术可节省计算能力并缩短计算时间,但这是以降低结果再现的保真度为代价的。提高光伏模拟的准确性并不总是与再现真实现象直接相关,但提高数据所含的信息量就足够了。本研究的方法增强了用户友好性,便于无缝集成到现有的能源建模框架中,旨在以亚小时为单位的时间步长进行表示。通过将模型应用于每小时平均数据,将其还原为一分钟时间步长,最后将合成的一分钟 GHI 数据与原始测量数据进行比较,证明了该算法的有效性。合成数据与测量数据的对比分析表明,两者之间的一致性很高,归一化平均偏差(MBE)值在 1.8%至 9.6%之间,归一化均方根误差(NRMSE)值在 2.7%至 16.1%之间,具体取决于天气条件。此外,判定系数(R2)始终保持在 0.64 以上。成功的算法验证使我们的算法适用于具有类似气候特征的气象数据集和地点。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A minute-resolution downscaling algorithm for high-resolution global irradiance time series
Numerous studies have demonstrated the significant impact of the resolution of solar irradiation data on the outcomes of hourly production models. Accurate integration of photovoltaic (PV) systems sometimes demands a high-resolution global horizontal irradiance (GHI) time series to capture the rapid fluctuations in PV power output induced by swift irradiance changes. Most of the available databases provide data at hourly resolution, leading to a lack of accuracy in PV simulations. Those existing hourly averages of global horizontal irradiance in open sources fail to represent this volatility adequately, especially when PV systems are coupled with fast ramp rate technologies. In the present work, an easy-to-use algorithm is implemented to synthesize high-resolution GHI time series from hourly averaged and clear sky irradiance datasets. By employing Linear interpolation, a technique that helps to achieve the desired time resolution and afterward computing critical factors, the algorithm identifies periods characterized by short-term weather phenomena, thus creating a high-resolution time series that accurately represents these dynamics. Avoiding the probabilistic components and machine learning techniques conserves computational power and reduces calculation time, but this comes at the cost of reduced fidelity in reproducing the results. Improving accuracy in PV simulations is not always directly related to reproducing real phenomena, but enhancing the amount of information contained in the data is sufficient. This study’s approach enhances user-friendliness and facilitates seamless integration into existing energy modeling frameworks, aiming for representation with sub-hourly time steps. The algorithm’s effectiveness is demonstrated by applying the model to hourly averaged data to revert them to a one-minute time step, and finally comparing the synthetically produced one-minute GHI data to the original measured data. The comparative analysis between synthesized and measured data demonstrated a strong agreement, with normalized mean bias error (MBE) values ranging between 1.8% and 9.6% and normalized root mean square error (NRMSE) values between 2.7% and 16.1%, depending on weather conditions. Additionally, the coefficient of determination (R2) consistently remained above 0.64. Successful algorithm validation makes our algorithm suitable for use in meteorological datasets and locations, with similar climatic characteristics.
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