Abstract
A multi-layer, deep-learning (DL) architecture consisting of stacked Convolutional Long Short Term Memory (sConvLSTM1D) layers is proposed to forecast the sunspot number (SSN) more effectively. The proposed model with optimized hyper-parameters performs efficiently on four kinds of sunspot data with different frequencies of time that are yearly, monthly, daily, and 13-month smoothed provided by the World Data Center-Sunspot Index and Long Term Solar Observation (WDC-SILSO), the Royal Observatory of Belgium (SILSO World Data Center). The model was contrasted with other traditional DL models on different performance metrics, namely root-mean-square error (RMSE), mean-absolute error (MAE), mean-absolute-percentage error (MAPE), and mean-absolute-scaled error (MASE). A non-parametric statistical test has also been carried out to confirm the model’s effectiveness. The prediction of the highest yearly mean of total sunspot number (SSN) in Solar Cycle 25 (SC25) has also been performed. The proposed sConvLSTM1D model suggests that the solar cycle exhibits the characteristics of a weak cycle. However, it is anticipated to be stronger than the preceding Solar Cycle 24 (SC24). The year of peak sunspot number will be 2024, as per the prediction, with the peak value of yearly mean sunspot number as 140.84, which is 24.3% higher than the peak value of the yearly mean of total sunspot number, which was 113.3 in the Solar Cycle 24 in the year 2014.
Similar content being viewed by others
References
Arfianti, U.I., Novitasari, D.C.R., Widodo, N., Hafiyusholeh, M., Utami, W.D.: 2021, Sunspot number prediction using Gated Recurrent Unit (GRU) algorithm. Indones. J. Comp. Cybern. Sys. 15, 141. DOI.
Bai, Y., Zeng, B., Li, C., Zhang, J.: 2019, An ensemble long short-term memory neural network for hourly PM2. 5 concentration forecasting. Chemosphere 222, 286. DOI.
Benson, B., Pan, W., Prasad, A., Gary, G., Hu, Q.: 2020, Forecasting solar cycle 25 using deep neural networks. Solar Phys. 295, 65. DOI.
Büyükşahin, Ü.Ç., Ertekin, Ş.: 2019, Improving forecasting accuracy of time series data using a new ARIMA-ANN hybrid method and empirical mode decomposition. Neurocomputing 361, 151. DOI.
Cantillo-Luna, S., Moreno-Chuquen, R., Celeita, D., Anders, G.: 2023, Deep and machine learning models to forecast photovoltaic power generation. Energies 16, 4097. DOI.
Chattopadhyay, S., Jhajharia, D., Chattopadhyay, G.: 2011, Trend estimation and univariate forecast of the sunspot numbers: development and comparison of ARMA, ARIMA and autoregressive neural network models. C. R. Géosci. 343, 433. DOI.
Covas, E., Peixinho, N., Fernandes, J.: 2019, Neural network forecast of the sunspot butterfly diagram. Solar Phys. 294, 24. DOI.
Dang, Y., Chen, Z., Li, H., Shu, H.: 2022, A comparative study of non-deep learning, deep learning, and ensemble learning methods for sunspot number prediction. Appl. Artif. Intell. 36, 2074129. DOI.
Demšar, J.: 2006, Statistical comparisons of classifiers over multiple data sets. J. Mach. Learn. Res. 7, 1.
Du, Z.: 2020, The solar cycle: predicting the peak of solar cycle 25. Astrophys. Space Sci. 365, 104. DOI.
Du, Z.: 2022, Predicting the maximum amplitude of solar cycle 25 using the early value of the rising phase. Solar Phys. 297, 61. DOI.
Elgamal, M.: 2020, Sunspot time series forecasting using deep learning. Int. J. Comp. Inform. Tech. 2279(0764), 9. DOI.
Gonçalves, Í.G., Echer, E., Frigo, E.: 2020, Sunspot cycle prediction using warped Gaussian process regression. Adv. Space Res. 65, 677. DOI.
Goodfellow, I., Bengio, Y., Courville, A.: 2016, Deep Learning, MIT, Cambridge USA.
Han, Y., Yin, Z.: 2019, A decline phase modeling for the prediction of solar cycle 25. Solar Phys. 294, 107. DOI.
Hasoon, S.O., Al-Hashimi, M.M.: 2022, Hybrid deep neural network and long short term memory network for predicting of sunspot time series. Int. J. Math. Comput. Sci. 17, 955.
Hochreiter, S., Schmidhuber, J.: 1997, Long short-term memory. Neural Comp. 9(8), 1735. DOI.
Kakad, B., Kakad, A., Ramesh, D.S.: 2017, Shannon entropy-based prediction of solar cycle 25. Solar Phys. 292, 1. DOI.
Kumar, B., Sunil, Yadav, Y.: 2023, A novel hybrid model combining \(\beta \)SARMA and LSTM for time series forecasting. Appl. Soft Comput. 134, 110019. DOI.
Labonville, F., Charbonneau, P., Lemerle, A.: 2019, A dynamo-based forecast of solar cycle 25. Solar Phys. 294, 82. DOI.
Lee, T.: 2020, EMD and LSTM hybrid deep learning model for predicting sunspot number time series with a cyclic pattern. Solar Phys. 295, 82. DOI.
Li, F., Kong, D., Xie, J., Xiang, N., Xu, J.: 2018, Solar cycle characteristics and their application in the prediction of cycle 25. J. Atmos. Solar-Terr. Phys. 181, 110. DOI.
Marques, C., Leal-Júnior, A., Kumar, S.: 2023, Multifunctional integration of optical fibers and nanomaterials for aircraft systems. Materials 16, 1433. DOI.
McIntosh, S.W., Chapman, S., Leamon, R.J., Egeland, R., Watkins, N.W.: 2020, Overlapping magnetic activity cycles and the sunspot number: forecasting sunspot cycle 25 amplitude. Solar Phys. 295, 1. DOI.
Nghiem, T.-L., Le, V.-D., Le, T.-L., Maréchal, P., Delahaye, D., Vidosavljevic, A.: 2022, Applying Bayesian inference in a hybrid CNN-LSTM model for time-series prediction. In: 2022 Internat. Conf. Multimedia Analy. Pattern Recog. (MAPR), 1, IEEE, Los Alamitos. DOI.
Okoh, D., Seemala, G., Rabiu, A., Uwamahoro, J., Habarulema, J., Aggarwal, M.: 2018, A hybrid regression-neural network (HR-NN) method for forecasting the solar activity. Space Weather 16, 1424. DOI.
Pala, Z., Atici, R.: 2019, Forecasting sunspot time series using deep learning methods. Solar Phys. 294, 50. DOI.
Panigrahi, S., Pattanayak, R.M., Sethy, P.K., Behera, S.K.: 2021, Forecasting of sunspot time series using a hybridization of ARIMA, ETS and SVM methods. Solar Phys. 296, 1. DOI.
Peguero, J., Carrasco, V.: 2023, A critical comment on “can solar cycle 25 be a new Dalton Minimum?”. Solar Phys. 298, 48. DOI.
Pesnell, W.D.: 2008, Predictions of solar cycle 24. Solar Phys. 252, 209. DOI.
Pesnell, W.D., Schatten, K.H.: 2018, An early prediction of the amplitude of solar cycle 25. Solar Phys. 293, 112. DOI.
Prasad, A., Roy, S., Sarkar, A., Panja, S.C., Patra, S.N.: 2022, Prediction of solar cycle 25 using deep learning based long short-term memory forecasting technique. Adv. Space Res. 69, 798. DOI.
Ramachandran, P., Zoph, B., Le, Q.V.: 2017, Searching for activation functions. DOI. arXiv.
Ramadevi, B., Bingi, K.: 2022, Time series forecasting model for sunspot number. In: 2022 Internat. Conf. on Intelligent Control. Comp. Smart Power (ICICCSP), 1, IEEE, Los Alamitos. DOI.
Shi, X., Chen, Z., Wang, H., Yeung, D.-Y., Wong, W.-K., Woo, W.-C.: 2015, Convolutional LSTM network: a machine learning approach for precipitation nowcasting. In: Cortes, C., Lawrence, N., Lee, D., Sugiyama, M., Garnett, R. (eds.) Adv. Neural Inform. Proc. Sys. 28, Curran Associates, Red Hook. URL.
Shi, C., Zhang, Z., Zhang, W., Zhang, C., Xu, Q.: 2022, Learning multiscale temporal–spatial–spectral features via a multipath convolutional LSTM neural network for change detection with hyperspectral images. IEEE Trans. Geosci. Remote Sens. 60, 1. DOI.
SILSO World Data Center: The International Sunspot Number. International Sunspot Number Monthly Bulletin and online catalogue. URL.
Singh, A., Bhargawa, A.: 2017, An early prediction of 25th solar cycle using Hurst exponent. Astrophys. Space Sci. 362, 199. DOI.
Szandała, T.: 2021, Review and comparison of commonly used activation functions for deep neural networks. Bio-Inspir. Comput. 903, 203. DOI.
Upton, L.A., Hathaway, D.H.: 2018, An updated solar cycle 25 prediction with AFT: the modern minimum. Geophys. Res. Lett. 45, 8091. DOI.
Vokhmyanin, M., Arlt, R., Zolotova, N.: 2020, Sunspot positions and areas from observations by Thomas Harriot. Solar Phys. 295, 39. DOI. ADS.
Wang, Q.-J., Li, J.-C., Guo, L.-Q.: 2021, Solar cycle prediction using a long short-term memory deep learning model. Res. Astron. Astrophys. 21, 012. DOI.
Wibawa, A.P., Utama, A.B.P., Elmunsyah, H., Pujianto, U., Dwiyanto, F.A., Hernandez, L.: 2022, Time-series analysis with smoothed convolutional neural network. J. Big Data 9, 44. DOI.
Zhang, L., Lu, L., Wang, X., Zhu, R.M., Bagheri, M., Summers, R.M., Yao, J.: 2019, Spatio-temporal convolutional LSTMs for tumor growth prediction by learning 4D longitudinal patient data. IEEE Trans. Med. Imaging 39, 1114. DOI.
Zhu, H., Zhu, W., He, M.: 2022, Solar cycle 25 prediction using an optimized long short-term memory mode with F10. 7. Solar Phys. 297, 157. DOI.
Zhu, H., Chen, H., Zhu, W., He, M.: 2023, Predicting solar cycle 25 using an optimized long short-term memory model based on sunspot area data. Adv. Space Res. 71, 3521. DOI.
Acknowledgments
The authors thank the WDC-SILSO, Royal Observatory of Belgium, Brussels, for the sunspot-number data.
Author information
Authors and Affiliations
Contributions
Abhijeet Kumar developed the methodology, performed the experimental analysis for the article and prepared the original draft. Vipin Kumar did the conceptualisation of the article, and methodology, supervised, reviewed and validated the work, formal analysis.
Corresponding author
Ethics declarations
Competing interests
The authors declare no competing interests.
Additional information
Publisher’s Note
Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
Appendix: Loss Plots of Different Models for Different Datasets
Appendix: Loss Plots of Different Models for Different Datasets
Rights and permissions
Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
About this article
Cite this article
Kumar, A., Kumar, V. Stacked 1D Convolutional LSTM (sConvLSTM1D) Model for Effective Prediction of Sunspot Time Series. Sol Phys 298, 121 (2023). https://doi.org/10.1007/s11207-023-02209-3
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s11207-023-02209-3