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Open Access | Just Accepted

Long-term forecasting of 10.7 cm solar radio flux using neurodynamics

Min Li1,2Xiuxian Li1,2Kecai Jiang1,2( )Jingnan Liu1,2( )Yujie Fu3Qile Zhao1,2Guo Chen1,2Renhai Mu1,2Yubin Wang1,2

1 GNSS Research Center, Wuhan University, Wuhan 430079, China

2 School of Geodesy and Geomatics, Wuhan University, Wuhan 430079, China

3 College of Safety and Environment Engineering, Shandong University of Science and Technology, Qingdao, 266590, China

 

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Abstract

The solar radio index F10.7 is a critical indicator of solar activity intensity. Accurate forecasting of F10.7 is essential for advancing many fields. A promising direction for addressing such complex forecast problems is known as neurodynamics, which incorporates dynamic perspectives into neural networks. In this study, we introduce a forecast model based on neurodynamics to achieve high-precision, long-term forecasting of the F10.7 index. First, we construct an F10.7 dataset making up for the missing period of F10.7 measurements by converting sunspot numbers, and we propose a new fitting method, improving the accuracy of converting sunspot number to F10.7 index. For the forecast modeling, we employ a neurodynamics model to capture the variation characteristics of historical datasets selected by clustering. This approach enhances the objectivity of long-term F10.7 forecasting, enabling accurate forecast spanning even an entire solar cycle. In the cycle used to validate the forecasting method, the model effectively captured the long-term trend of F10.7 index, and the forecasted values closely matched the observed values. To simplify forecasting, we develop a method for calculating F10.7 for an entire solar cycle using only the Modified Julian Day, thereby expanding the usability of the forecasts.

Tsinghua Science and Technology
Cite this article:
Li M, Li X, Jiang K, et al. Long-term forecasting of 10.7 cm solar radio flux using neurodynamics. Tsinghua Science and Technology, 2025, https://doi.org/10.26599/TST.2025.9010037

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Received: 24 January 2025
Revised: 28 February 2025
Accepted: 13 March 2025
Available online: 08 April 2025

© The author(s) 2025

he articles published in this open access journal are distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/).

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