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Analysis investigates solar wind mass-loss rate correlated with open solar magnetic flux across solar cycles, indicating a strong predictive relationship.
We investigate the solar wind mass‐loss rate and its relationship with open solar magnetic flux (OSF) over Solar Cycles 23–25 using OMNI, SIDC, and SOHO/LASCO data. The solar wind mass‐loss rate correlates more strongly with OSF than with sunspot number, establishing OSF as a superior predictor of heliospheric mass‐loss.
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Mirtoshev et al. (2026) studied this question.
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