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Deciphering Solar Magnetic Activity: The Solar Cycle Clock

The Sun’s 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 ∼55° latitude to the equator, over ∼19 years. We will discuss the end point of that progression, dubbed...

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Bibliografiset tiedot
Päätekijät: Robert J. Leamon, Scott W. McIntosh, Alan M. Title
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: Frontiers Media S.A. 2022-05-01
Sarja:Frontiers in Astronomy and Space Sciences
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Linkit:https://www.frontiersin.org/articles/10.3389/fspas.2022.886670/full
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