Abstract
Solar forecasting is shifting to the probabilistic paradigm due to the inherent uncertainty within the solar resource. Input uncertainty quantification is one of the widely used and best-performing ways to model solar uncertainty. However, compared to other sources of inputs, such as numerical weather prediction models, pure sky image-based probabilistic solar forecasting lags behind. In this research, an occlusion-perturbed convolutional neural network, named the PSolarNet, is developed. The PSolarNet provides very short-term deterministic forecasts, forecast scenarios, and probabilistic forecasts of the global horizontal irradiance from sky image sequences. Case studies based on 6 years of open-source data show that the developed PSolarNet is able to generate accurate 10-minute ahead deterministic forecasts with a 5.62% normalized root mean square error, realistic and diverse forecast scenarios with a 0.966 average correlation with the actual time series, and reliable and sharp probabilistic forecasts with a 2.77% normalized continuous ranked probability score.
| Original language | American English |
|---|---|
| Number of pages | 8 |
| State | Published - 2022 |
| Event | 2022 IEEE Power & Energy Society General Meeting - Denver, Colorado Duration: 17 Jul 2022 → 21 Jul 2022 |
Conference
| Conference | 2022 IEEE Power & Energy Society General Meeting |
|---|---|
| City | Denver, Colorado |
| Period | 17/07/22 → 21/07/22 |
Bibliographical note
See NREL/CP-5D00-84957 for paper as published in proceedingsNLR Publication Number
- NREL/CP-5D00-83163
Keywords
- Bayesian model averaging
- deep learning
- sky image processing
- solar forecasting
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