Tidal triggers and the predictability of solar activity
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Magneto-Rossby waves in the solar tachocline are currently considered to be one of the main determinants of solar activity. In particular, they can give rise to the quasi-biennial oscillation (QBO). The latter was recently shown to be dominated by a phase-stable period of around 1.7 years. By analyzing 72 ground-level enhancement (GLE) events and 37 S-flares, we determine that this period is close to 1.723 years. This, in turn, is the dominant beat between the periods of the spring tides of the tidally dominant planets Venus, Earth, and Jupiter, which are suspected to synchronize not only the QBO, but also the 11.07-year Schwabe cycle. We demonstrate that recent events, such as the solar storm of 2024 May 10 and the strong X-flare of 2026 February 1, align well with maxima of the combined tidal forcing.
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An optimized tidal-trigger model of the QBO, and some implications for the Carrington event
An optimized tidal-trigger model for solar QBO, incorporating toroidal field strength from sunspot data, achieves up to 0.8 correlation with 109 extreme events versus 0.4 for the field-independent version.
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