Yunxiao Chen , Chaojing Lin , Jinfu Liu , Daren Yu
{"title":"One-hour-ahead solar irradiance forecast based on real-time K-means++ clustering on the input side and CNN-LSTM","authors":"Yunxiao Chen , Chaojing Lin , Jinfu Liu , Daren Yu","doi":"10.1016/j.jastp.2024.106405","DOIUrl":null,"url":null,"abstract":"<div><div>With the increasing proportion of photovoltaic power generation in the power system, accurate solar irradiance forecasting is crucial for power grid scheduling. The paper proposes a approach of clustering modeling and joint forecasting for solar irradiance: firstly, by using the real-time K-means++ to cluster the GHI sequence on the input side of the model, the model input is divided into 4 clusters. The number of clusters and clustering methods are quickly determined through sensitivity experiments. Then 4 CNN-LSTM models, corresponding to the 4 clusters, are separately established and trained to fully extract multivariate and multi-temporal information from the input side. These 4 models are combined to achieve 1-h-ahead solar irradiance forecast with higher accuracy. To verify the effectiveness of the proposed method, Auto regressive (AR), Convolutional neural network (CNN), Long short-term memory (LSTM) and Gradient boosting decision tree (GBDT) are used as comparative models. The results indicate that the proposed K-means++_CNN-LSTM is a feasible method, with MAE decreasing by about 9.13%, RMSE decreasing by about 6.58%, and <span><math><mrow><mi>ρ</mi></mrow></math></span> increasing by about 1.46%, compared to K-means++_AR. Finally, T-test is used to verify the positive impact of the proposed framework on model accuracy.</div></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":"266 ","pages":"Article 106405"},"PeriodicalIF":1.8000,"publicationDate":"2025-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Atmospheric and Solar-Terrestrial Physics","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1364682624002335","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
With the increasing proportion of photovoltaic power generation in the power system, accurate solar irradiance forecasting is crucial for power grid scheduling. The paper proposes a approach of clustering modeling and joint forecasting for solar irradiance: firstly, by using the real-time K-means++ to cluster the GHI sequence on the input side of the model, the model input is divided into 4 clusters. The number of clusters and clustering methods are quickly determined through sensitivity experiments. Then 4 CNN-LSTM models, corresponding to the 4 clusters, are separately established and trained to fully extract multivariate and multi-temporal information from the input side. These 4 models are combined to achieve 1-h-ahead solar irradiance forecast with higher accuracy. To verify the effectiveness of the proposed method, Auto regressive (AR), Convolutional neural network (CNN), Long short-term memory (LSTM) and Gradient boosting decision tree (GBDT) are used as comparative models. The results indicate that the proposed K-means++_CNN-LSTM is a feasible method, with MAE decreasing by about 9.13%, RMSE decreasing by about 6.58%, and increasing by about 1.46%, compared to K-means++_AR. Finally, T-test is used to verify the positive impact of the proposed framework on model accuracy.
期刊介绍:
The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them.
The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions.
Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.