The m=1 high-latitude inertial mode frequency implies solar rotation of 365.3 nHz at 75° latitude and 0.8 R_sun, exceeding the p-mode reference by 8.1 nHz.
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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.
Over 63% of solar active region flux in Cycle 24 clusters in three bands whose drift rates match phase speeds of slow magneto-Rossby waves with toroidal field ~4 kG.
citing papers explorer
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Towards inertial-mode helioseismology: Direct sensing of solar rotation at 75 deg latitude and 0.8 Rsun
The m=1 high-latitude inertial mode frequency implies solar rotation of 365.3 nHz at 75° latitude and 0.8 R_sun, exceeding the p-mode reference by 8.1 nHz.
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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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Long-Term Clustering Pattern of Solar Active Regions and Their Potential Connection with Magneto-Rossby Waves
Over 63% of solar active region flux in Cycle 24 clusters in three bands whose drift rates match phase speeds of slow magneto-Rossby waves with toroidal field ~4 kG.