Application of Synoptic Magnetograms to Global Solar Activity Forecast
Irina N. Kitiashvili

TL;DR
This study integrates synoptic magnetograms into a mean-field dynamo model using Ensemble Kalman Filter to forecast solar activity, predicting a weaker Solar Cycle 25 with specific timing and hemispheric differences.
Contribution
It introduces a novel data assimilation approach combining synoptic magnetograms with a mean-field dynamo model for improved solar activity forecasting.
Findings
Predicted Solar Cycle 25 will be weaker than Cycle 24.
A deep solar minimum is expected during 2019-2021.
The next solar maximum will occur in 2024-2025 with specific hemispheric differences.
Abstract
Synoptic magnetograms provide us with knowledge about the evolution of magnetic fields on the solar surface and present important information for forecasting future solar activity. In this work, poloidal and toroidal magnetic field components derived from synoptic magnetograms are assimilated, using the Ensemble Kalman Filter method, into a mean-field dynamo model based on Parker's migratory dynamo theory complemented by magnetic helicity conservation. It was found that the predicted toroidal field is in good agreement with observations for almost the entire following solar cycle. However, poloidal field predictions agree with observations only for the first 2 - 3 years of the predicted cycle. The results indicate that the upcoming Solar Maximum of Cycle 25 (SC25) is expected to be weaker than the current Cycle 24. The model results show that a deep extended solar activity minimum is…
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