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

Author:

Liu Xiaohuan12,Zeng Shuguang12,Deng Linhua3,Zeng Xiangyun12,Zheng Sheng12

Affiliation:

1. Center for Astronomy and Space Sciences, China Three Gorges University , Yichang 443000, People’s Republic of China

2. College of Science, China Three Gorges University , Yichang 443000, People’s Republic of China

3. Yunnan Observatories, Chinese Academy of Sciences , Kunming 650216, People’s Republic of China

Abstract

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.

Funder

Yunnan Key Laboratory of Solar Physics and Space Science

National Natural Science Foundation of China

CAS

Yunnan Fundamental Research Projects

Yunnan Province XingDian Talent Support Program

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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