Another Mini Solar Maximum in the Offing: A Prediction for the Amplitude of Solar Cycle 25
Susanta Kumar Bisoi, P. Janardhan, S. Ananthakrishnan

TL;DR
This study predicts that Solar Cycle 25 will have a mini maximum, likely stronger than Cycle 24 but weaker than Cycle 23, based on magnetic field data and revised sunspot numbers, indicating a reduced heliospheric magnetic field floor.
Contribution
It introduces a revised correlation between magnetic fields and sunspot numbers, leading to a new prediction for Solar Cycle 25's amplitude and characteristics.
Findings
Cycle 24 showed anti-solar magnetic variation.
HMF floor level breached before Cycle 24 minimum.
Predicted Cycle 25 will have a mini maximum, stronger than Cycle 24.
Abstract
We examine the temporal changes in both solar polar magnetic field (PMF) at latitudes and heliospheric magnetic field (HMF) at 1 AU during solar cycles 21--24 with emphasis on the recent activity changes after July 2015, the so called "mini solar maximum" of cycle 24. While unsigned PMF shows a solar-cycle-like variation in cycles 21 and 22, it shows an anti-solar-cycle-like variation in cycle 24. In addition, the floor level of the HMF (of 4.6 nT), i.e. the value that the HMF returns to at each solar minimum, is breached about two years prior to cycle 24 minimum, indicating a reduced HMF floor level in the upcoming cycle 24 minimum. In light of the change of unsigned PMF and the availability of a revised smoothed sunspot number (SSN) after July 2015, we have revisited the correlation of unsigned PMF and HMF at solar minimum. The correlation is used to estimate a new…
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