A Gridded Solar Irradiance Ensemble Prediction System Based on WRF-Solar EPS and the Analog Ensemble

被引:3
|
作者
Alessandrini, Stefano [1 ]
Kim, Ju-Hye [1 ]
Jimenez, Pedro A. [1 ]
Dudhia, Jimy [2 ]
Yang, Jaemo [3 ]
Sengupta, Manajit [3 ]
机构
[1] Natl Ctr Atmospher Res, Res Appl Lab, Boulder, CO 80307 USA
[2] Natl Ctr Atmospher Res, Mesoscale & Microscale Meteorol Lab, Boulder, CO 80307 USA
[3] Natl Renewable Energy Lab, Golden, CO 80401 USA
基金
美国国家科学基金会;
关键词
solar irradiance ensemble forecasting; analog ensemble; rare events; ensemble calibration; WIND POWER; PART I; MODEL; FORECASTS; ENERGY; IMPLEMENTATION; UNCERTAINTIES; GENERATION;
D O I
10.3390/atmos14030567
中图分类号
X [环境科学、安全科学];
学科分类号
08 ; 0830 ;
摘要
The WRF-Solar Ensemble Prediction System (WRF-Solar EPS) and a calibration method, the analog ensemble (AnEn), are used to generate calibrated gridded ensemble forecasts of solar irradiance over the contiguous United States (CONUS). Global horizontal irradiance (GHI) and direct normal irradiance (DNI) retrievals, based on geostationary satellites from the National Solar Radiation Database (NSRDB) are used for both calibrating and verifying the day-ahead GHI and DNI predictions (GDIP). A 10-member ensemble of WRF-Solar EPS is run in a re-forecast mode to generate day-ahead GDIP for three years. The AnEn is used to calibrate GDIP at each grid point independently using the NSRDB as the "ground truth". Performance evaluations of deterministic and probabilistic attributes are carried out over the whole CONUS. The results demonstrate that using the AnEn calibrated ensemble forecast from WRF-Solar EPS contributes to improving the overall quality of the GHI predictions with respect to an AnEn calibrated system based only on the deterministic run of WRF-Solar. In fact, the calibrated WRF-Solar EPS's mean exhibits a lower bias and RMSE than the calibrated deterministic WRF-Solar. Moreover, using the ensemble mean and spread as predictors for the AnEn allows a more effective calibration than using variables only from the deterministic runs. Finally, it has been shown that the recently introduced algorithm of correction for rare events is of paramount importance to obtain the lowest values of GHI from the calibrated ensemble (WRF-Solar EPS AnEn), qualitatively consistent with those observed from the NSRDB.
引用
收藏
页数:19
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