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An application of the ECMWF Ensemble Prediction System for short-term solar power forecasting

机译:ECMWF集合预报系统在太阳能短期预报中的应用

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Solar energy production is steadily growing in several countries. Depending on meteorological variables such as solar irradiance, cloud cover and temperature, solar power production predictability is limited by the chaotic nature of these parameters. This work presents an application of the European Centre for Medium-Range Weather Forecasts (ECMWF) Ensemble Prediction System (EPS) to produce short-term probabilistic solar power forecasts (SPF). The EPS is based on running a meteorological model multiple times, starting from slightly perturbed initial conditions. The distribution of these different runs allows estimating the prediction uncertainty. We use about two years of power data from three solar farms located in different parts of Italy, characterized by different climatic conditions. We retrieve ensemble members of meteorological variables to build a power probability density function (PDF) for 0-72 h forecast horizons. A neural network (NN) is applied to reduce model bias and to generate a PDF of power starting from the ensemble of meteorological variables. Then two statistical methods are applied to calibrate further the ensemble of power predictions, which results in the final probabilistic power forecast. The first technique has been already tested for wind power forecasting (WPF), and it is based on estimating the variance deficit (VD) or "lack of spread" of the ensemble distribution. The second is a well-established method to calibrate probabilistic predictions based on Ensemble Model Output Statistics (EMOS). Also, a persistence ensemble (PE) is used as a baseline technique. PE builds the ensemble members from the most recent power measurements available at the same lead time. It is shown that EPS coupled with VD and EMOS is a valid method to produce skillful probabilistic SPF in different climatic conditions. VD and EMOS show a similar level of statistical consistency and forecast skill for each test case. Overall, the performances of VD and EMOS appear significantly better than those of PE. (C) 2016 Elsevier Ltd. All rights reserved.
机译:几个国家的太阳能生产稳定增长。取决于气象变量,例如太阳辐照度,云量和温度,太阳能发电的可预测性受到这些参数的混乱性质的限制。这项工作介绍了欧洲中距离天气预报中心(ECMWF)集合预报系统(EPS)的应用,用于产生短期概率太阳能预报(SPF)。 EPS是从多次扰动的初始条件开始,多次运行气象模型。这些不同运行的分布允许估计预测不确定性。我们使用来自意大利不同地区的三个太阳能发电场的大约两年的电力数据,这些太阳能发电场具有不同的气候条件。我们检索气象变量的集合成员,以建立0-72小时的预测范围的功率概率密度函数(PDF)。应用神经网络(NN)减少模型偏差并从气象变量集合开始生成幂的PDF。然后使用两种统计方法进一步校正功率预测的集合,从而得出最终的概率功率预测。第一种技术已经针对风能预测(WPF)进行了测试,它基于估计总体分布的方差赤字(VD)或“无扩展”。第二种是基于集合模型输出统计(EMOS)的用于校准概率预测的成熟方法。而且,持久性合奏(PE)用作基线技术。 PE根据在相同提前期获得的最新功率测量结果来构建集成成员。结果表明,EPS结合VD和EMOS是在不同气候条件下产生熟练的概率SPF的有效方法。 VD和EMOS对每个测试用例显示出相似的统计一致性和预测技能。总体而言,VD和EMOS的性能明显优于PE。 (C)2016 Elsevier Ltd.保留所有权利。

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