利用太阳黑子数量观测数据的维平-深度-分解-再分解滚动窗口(vD2R2w)模型加强太阳周期 25 和 26 的预报工作

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Vipin Kumar
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引用次数: 0

摘要

有效预测太阳黑子数(SSN)是研究空间天气、太阳活动、卫星通信和地球气候的复杂任务。开发可靠的 SSN 预测模型非常困难,因为 SSN 时间序列表现出复杂的模式、非线性和非平稳性特征。最新研究表明,深度学习模型往往需要帮助才能捕捉 SSN 数据的复杂动态和长期依赖性。SSN 时间序列的分解趋势、季节和残差特征可为有效学习提供更好的长期依赖性和相关动态信息。在这项研究中,结合时间序列分解、深度学习模型和滚动窗口方法,提出了 vipin-deep-decomposed-recomposed rolling-window (vD2R2w) 模型,以准确预测 SSN。对所提出的 vD2R2w 模型在四个数据集上进行了评估,结果一致优于传统的深度学习模型。在 SSN_Daily 数据集上,该模型在 RMSE、MAPE 和 \(R^{2}\)方面提高了性能:84.18%(RMSE)、10.38%(MAPE)和 3.504%(\(R^{2}\));SSN_Monthly:39.5%(RMSE)、26.06%(MAPE)和 7.258%(\(R^{2}\));SSN_MonthlyMeanly:178.32%(RMSE)、54.83%(MAPE)和 1.56%(\(R^{2}\));SSN_Yearly:6.06%(RMSE)、10.36%(MAPE)和 1.366%(\(R^{2}\))。此外,vD2R2w 模型的优越性还通过 AIC & BIC、Diebold Mariano 检验和 Friedman 排名统计检验得到了验证。此外,vD2R2w 模型还预测了太阳周期(SC)的峰值和时间,即 2025 年的 SC25:127.16(± 6.83)和 2035 年的 SC26:191.71(± 43.37)。通过对所提出模型的性能进行分析,并利用四个 SSN 对各种指标进行统计验证,得出结论:vD2R2w 模型优于传统模型,是 SSN 时间序列预测的可靠框架。实施所提出的模型可使空间气象监测、卫星通信规划和太阳能预报等依赖精确 SSN 预测的领域受益。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Enhancing Solar Cycle 25 and 26 Forecasting with Vipin-Deep-Decomposed-Recomposed Rolling-window (vD2R2w) Model on Sunspot Number Observations

Enhancing Solar Cycle 25 and 26 Forecasting with Vipin-Deep-Decomposed-Recomposed Rolling-window (vD2R2w) Model on Sunspot Number Observations

Effective predicting sunspot numbers (SSN) is the complex task of studying space weather, solar activity, satellite communication, and Earth’s climate. Developing a reliable SSN forecasting model is difficult because SSN time series exhibit complex patterns, nonlinearity, and nonstationarity characteristics. The state-of-the-art shows that deep-learning models often need help capturing SSN data’s intricate dynamics and long-term dependencies. The SSN time series’ decomposed trend and seasonal and residual characteristics may provide better information on long-term dependencies and associated dynamics for effective learning. In this research, the vipin-deep-decomposed-recomposed rolling-window (vD2R2w) models have been proposed with a combination of time-series decomposition, deep-learning models, and a rolling-window method to predict the SSN accurately. The proposed vD2R2w models have been evaluated over four datasets and consistently outperform traditional deep-learning models. The model improves the performance in terms of RMSE, MAPE, and \(R^{2}\) over the datasets as SSN_Daily: 84.18% (RMSE), 10.38% (MAPE), and 3.504% (\(R^{2}\)); SSN_Monthly: 39.5% (RMSE), 26.06% (MAPE), and 7.258% (\(R^{2}\)); SSN_MonthlyMean: 178.32% (RMSE), 54.83% (MAPE), and 1.56% (\(R^{2}\)); and SSN_Yearly: 6.06% (RMSE), 10.36% (MAPE), and 1.366% (\(R^{2}\)). Further, the superiority of the vD2R2w models is validated through AIC & BIC, Diebold Mariano test, and Friedman ranking statistical tests. Additionally, the vD2R2w model has forecasted the peak value of Solar Cycles (SC) and time, i.e., SC25: 127.16 (± 6.83) in 2025 and SC26: 191.71 (± 43.37) in 2035. The analysis of proposed model performances and statistical validation over various measures with four SSNs have concluded that the vD2R2w model outperforms the traditional models and is a reliable framework for SSN time series forecasting. Implementing the proposed model may benefit domains such as space-weather monitoring, satellite communication planning, and solar energy forecasting that rely on accurate SSN predictions.

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来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
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