Sunspot number second differences as a precursor of the following 11-year sunspot cycle
Tatiana Podladchikova, Ronald Van der Linden, Astrid M. Veronig

TL;DR
This study introduces a method using sunspot number second differences to forecast the strength of the next 11-year sunspot cycle early in the declining phase, achieving high accuracy within two years after maximum.
Contribution
It presents a new approach to predict the next cycle's strength without needing to know the current cycle's minimum epoch, based on SNSD dynamics.
Findings
High probability (0.96) of correctly predicting cycle strength within 24-31 months after maximum.
Method can forecast whether the next cycle is stronger or weaker early in the declining phase.
Prediction that cycle 25 will be weaker than cycle 24.
Abstract
Forecasting the strength of the sunspot cycle is highly important for many space weather applications. Our previous studies have shown the importance of sunspot number variability in the declining phase of the current 11-year sunspot cycle to predict the strength of the next cycle when the minimum of the current cycle has been observed. In this study we continue this approach and show that we can remove the limitation of having to know the minimum epoch of the current cycle, and that we can already provide a forecast of the following cycle strength in the early stage of the declining phase of the current cycle. We introduce a method to reliably calculate sunspot number second differences (SNSD) in order to quantify the short-term variations of sunspot activity. We demonstrate a steady relationship between the SNSD dynamics in the early stage of the declining phase of a given cycle and…
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