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The Sun as a revolving-field magnetic alternator with a wobbling-core rotator from real data

Omerbashich, Mensur

Rather than as a star classically assumed to feature elusive dynamo or a proverbial engine and impulsively alternating polarity, the Sun reveals itself in the 385.8–2.439-nHz (1-month–13-years) band of polar (φSun>|70°|) wind's decadal dynamics, dominated by the fast (>700 km s^‑1) winds, as a globally completely vibrating revolving-field ma…