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The solar cycle: predicting the maximum amplitude of the smoothed highest 3-hourly aa index in 3 d for cycle 25 based on a similar-cycle method

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Abstract

A similar-cycle method is introduced to predict the maximum amplitude of the geomagnetic index aa for the 11-yr solar cycle. This method is based on the idea that similar cycles tend to have similar cycle parameters. We use the highest 3-hourly aa index in each 3 days’ interval (\(aa_{ \mathrm{H}}\)), which is further smoothed by 121 points (363 days). The minimum \(aa_{\mathrm{H}}\) (\(aa_{\mathrm{Hmin}}\)) around the beginning of the current cycle 25 [\(aa_{\mathrm{Hmin}}(25)\)] is used as a reference to select the similar cycles to cycle 25: \(n_{\mathrm{s}}=16, 15, 24\), and 12 (in descending order of weights). The maximum \(aa_{\mathrm{H}}\) (\(aa_{\mathrm{Hmax}}\)) is predicted as the weighted average of the corresponding values in the similar cycles with the weight given by the reciprocal of the deviation between \(aa_{\mathrm{Hmin}}(n_{\mathrm{s}})\) and \(aa_{\mathrm{Hmin}}(25)\). Based on this method, the maximum amplitude of \(aa_{\mathrm{H}}\) for cycle 25 is predicted to be \(aa_{\mathrm{Hmax}}(25)=73.8\pm 4.4\) nT, about 14% higher than that in cycle 24 (64.81 nT).

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Data Availability

The data in this study can be downloaded from the International Service of Geomagnetic Indices (ISGI) website (http://isgi.unistra.fr/).

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Acknowledgements

We are grateful to the anonymous reviewer for valuable suggestions that have improved this manuscript.

Funding

This work was supported by National Key R&D Program of China under grant 2021YFA1600504 and the National Science Foundation of China (NSFC) under grants 11873060 and 11973058.

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The data analysis and the manuscript were completed by DZL.

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Correspondence to Z. L. Du.

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Du, Z.L. The solar cycle: predicting the maximum amplitude of the smoothed highest 3-hourly aa index in 3 d for cycle 25 based on a similar-cycle method. Astrophys Space Sci 368, 11 (2023). https://doi.org/10.1007/s10509-023-04167-5

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  • DOI: https://doi.org/10.1007/s10509-023-04167-5

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