Predicting the 25th and 26th solar cycles using the long short-term memory method

IF 2.2 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Publications of the Astronomical Society of Japan Pub Date : 2023-05-02 DOI:10.1093/pasj/psad029
Xiaohuan Liu, S. Zeng, L. Deng, X. Zeng, S. Zheng
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Abstract

Solar activities directly or indirectly affect space missions, geophysical environment, space climate, and human activities. We used the long short-term memory (LSTM) deep learning method to predict the amplitude and peak time of solar cycles (SCs) 25 and 26 by using the monthly relative sunspot number data taken from the National Astronomical Observatory of Japan (NAOJ). The dataset is divided into eight schemes of two to nine slices for training, showing that the five-slice LSTM model with root mean square error of 11.38 is the optimal model. According to the prediction, SC 25 will be about 21$\%$ stronger than SC 24, with a peak of 135.2 occurring in 2024 April. SC 26 will be similar to SC 25 and reach its peak of 135.0 in 2035 January. Our analysis results indicate that the sunspot data from NAOJ is highly credible and comparable.
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利用长短期记忆法预测第25和26太阳周期
太阳活动直接或间接地影响空间任务、地球物理环境、空间气候和人类活动。利用日本国家天文台(NAOJ)的月相对黑子数数据,采用长短期记忆(LSTM)深度学习方法预测了太阳周期(SCs) 25和26的振幅和峰值时间。将数据集分成2 ~ 9片的8个方案进行训练,结果表明,均方根误差为11.38的5片LSTM模型是最优模型。根据预测,SC 25将比SC 24强约21%,峰值将在2024年4月达到135.2。SC 26将与SC 25相似,并在2035年1月达到135.0的峰值。我们的分析结果表明,来自NAOJ的太阳黑子数据具有很高的可信度和可比性。
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来源期刊
Publications of the Astronomical Society of Japan
Publications of the Astronomical Society of Japan 地学天文-天文与天体物理
CiteScore
4.10
自引率
13.00%
发文量
98
审稿时长
4-8 weeks
期刊介绍: Publications of the Astronomical Society of Japan (PASJ) publishes the results of original research in all aspects of astronomy, astrophysics, and fields closely related to them.
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