混合集成深度学习模型增强太阳黑子预测和太阳周期26的预报

IF 2.4 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Aman Kumar, Vipin Kumar
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引用次数: 0

摘要

本研究综合评估了三种类型的太阳黑子数据的深度学习模型:13个月平滑的太阳黑子数(SSN)、年度SSN和月平均SSN数据。将LSTM、GRU、CNN、RNN和BiLSTM等传统模型与混合模型进行比较:Hybrid1 (CNN- dilatedlstm -BiLSTM-GRU)、Hybrid2 (CNN-GRU-RNN带Dropout正则化)、Hybrid3 (CNN-GRU)、Hybrid4 (CNN-GRU-RNN不带Dropout) (Hybrid2和Hybrid4都集成了CNN-GRU-RNN架构,但Hybrid2引入Dropout层以减少过拟合,使其成为Hybrid4的正则化版本)和混合集成模型(Hybrid2 + Hybrid4)。像RMSE、MAE、MSE和R2这样的关键指标被用来评估模型的性能。结果表明,混合模型在所有数据集上的表现都优于传统模型。具体而言,Hybrid Ensemble实现了更高的预测精度,13个月平滑SSN数据的RMSE为4.062,R2为0.9964,年SSN数据的RMSE为22.11,R2为0.8920,月平均SSN数据的RMSE为24.61,R2为0.8826。这些发现证明了混合模型,特别是混合集合,能够有效地捕获太阳黑子时间序列数据中的复杂模式。除了模型评估之外,本研究还提供了太阳活动周期26的SSN预测值,预测太阳活动从2025年(SSN: 112.39)逐渐增加到2036年(SSN: 165.35)达到峰值,随后在2037年(SSN: 155.25)略有下降,最低SSN发生在2032年(SSN: 10.41)。这些预测与已知的太阳周期变化非常吻合,并为即将到来的太阳活动及其对空间天气、气候和技术的影响提供了有价值的见解。对模型性能进行了Friedman非参数检验,确认Hybrid Ensemble为最佳表现。经霍尔姆校正的多重比较显示出可以忽略不计的差异,这加强了混合方法和集合方法的稳健性。这项研究强调了结合不同架构来提高预测精度的价值,特别是对于复杂的科学时间序列数据,如太阳活动。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Hybrid-Ensemble Deep-Learning Models to Enhance the Sunspot Prediction and Forecasting of Solar Cycle 26

Hybrid-Ensemble Deep-Learning Models to Enhance the Sunspot Prediction and Forecasting of Solar Cycle 26

This study comprehensively evaluates deep-learning models across three types of sunspot data: 13-month smoothed Sunspot Number (SSN), yearly SSN, and mean monthly SSN data. Traditional models such as LSTM, GRU, CNN, RNN, and BiLSTM are compared against proposed hybrid models: Hybrid1 (CNN-DilatedLSTM-BiLSTM-GRU), Hybrid2 (CNN-GRU-RNN with Dropout Regularization), Hybrid3 (CNN-GRU), Hybrid4 (CNN-GRU-RNN without Dropout) (Hybrid2 and Hybrid4 both integrate CNN-GRU-RNN architectures, but Hybrid2 introduces Dropout layers to reduce overfitting, making it a regularized version of Hybrid4), and a Hybrid Ensemble model (Hybrid2 + Hybrid4). Key metrics like RMSE, MAE, MSE, and R2 are used to assess model performance. The results indicate that hybrid models consistently outperform traditional models across all datasets. Specifically, the Hybrid Ensemble achieves enhanced predictive accuracy, recording an RMSE of 4.062 and R2 of 0.9964 for 13-month smoothed SSN data, an RMSE of 22.11 and R2 of 0.8920 for yearly SSN data, and an RMSE of 24.61 and R2 of 0.8826 for mean monthly SSN data. These findings demonstrate the ability of hybrid models, especially the Hybrid Ensemble, to effectively capture complex patterns in sunspot time-series data.

In addition to model evaluation, this study provides forecasted SSN values for Solar Cycle 26, projecting a gradual increase in solar activity from 2025 (SSN: 112.39) to a peak in 2036 (SSN: 165.35), followed by a slight decline in 2037 (SSN: 155.25), with the lowest SSN occurring in 2032 (SSN: 10.41). These forecasts align well with known solar cycle variations and offer valuable insights into upcoming solar activity and its implications for space weather, climate, and technology. A Friedman non-parametric test was conducted to rank model performance, confirming the Hybrid Ensemble as the top performer. Holm-adjusted multiple comparisons showed negligible differences, reinforcing the robustness of the hybrid and ensemble approaches. This research highlights the value of combining different architectures to improve forecasting accuracy, especially for complex scientific time-series data such as solar activity.

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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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