Deciphering Solar Magnetic Activity. II. The Solar Cycle Clock and the Onset of Solar Minimum Conditions


Abstract in English

The Suns variability is controlled by the progression and interaction of the magnetized systems that form the 22-year magnetic activity cycle (the Hale Cycle) as they march from their origin at $sim$55 degrees latitude to the equator, over $sim$19 years. We will discuss the end point of that progression, dubbed terminator events, and our means of diagnosing them. Based on the terminations of Hale Magnetic Cycles, we construct a new solar activity clock which maps all solar magnetic activity onto a single normalized epoch. The Terminators appear at phase $0 * 2pi$ on this clock (by definition), then solar polar field reversals commence at $0.2 * 2pi$, and the geomagnetically quiet intervals centered around solar minimum, start at $0.6 * 2pi$ and end at the terminator, lasting 40% of the normalized cycle length. With this onset of quiescence, dubbed a pre-terminator, the Sun shows a radical reduction in active region complexity and (like the terminator events) is associated with the time when the solar radio flux crosses F10.7=90 sfu -- effectively marking the commencement of solar minimum conditions. In this paper we use the terminator-based clock to illustrate a range of phenomena associated with the pre-terminator event that further emphasize the strong interaction of the global-scale magnetic systems of the Hale Cycle.

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