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.
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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.