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The 11-Year Magnetic Solar Cycle: Chaos Control Due to Jupiter
Luleå University of Technology, Department of Engineering Sciences and Mathematics, Material Science.ORCID iD: 0000-0002-7200-4962
2022 (English)In: Solar system research, ISSN 0038-0946, E-ISSN 1608-3423, Vol. 56, no 3, p. 191-194Article in journal (Refereed) Published
Abstract [en]

The observed magnetic field of the Sun is believed to originate from a “dynamo-effect” in its convective surface layer. However, there is no natural 11-year timescale in such models. We show that this timescale in the mean naturally and automatically arise through magnetic “chaos-control” of the inherently chaotic solar dynamo, mainly due to Jupiter, while also conforming to real and observed sunspot characteristics.

Place, publisher, year, edition, pages
Elsevier, 2022. Vol. 56, no 3, p. 191-194
National Category
Fusion, Plasma and Space Physics
Research subject
Applied Physics
Identifiers
URN: urn:nbn:se:ltu:diva-91239DOI: 10.1134/S0038094622030030ISI: 000809162100007Scopus ID: 2-s2.0-85131731194OAI: oai:DiVA.org:ltu-91239DiVA, id: diva2:1667634
Note

Validerad;2022;Nivå 2;2022-06-17 (hanlid)

Available from: 2022-06-10 Created: 2022-06-10 Last updated: 2022-06-30Bibliographically approved

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Hansson, Johan

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