Solar Toroidal Field Evolution Spanning Four Sunspot Cycles
Abstract/Contents
- Abstract
- Forty-four years of Wilcox Solar Observatory, 14 years of Michelson Doppler Imager on the Solar and Heliospheric Observatory, and 11 years of Helioseismic and Magnetic Imager on the Solar Dynamics Observatory magnetic field data have been studied to determine the east–west inclination—the toroidal component—of the magnetic field. Maps of the zonal averaged inclination show that each toroidal field cycle begins at around the same time at high latitudes in the northern and southern hemispheres, and ends at the equator. Observation of these maps also shows that each instance of a dominant toroidal field direction starts at high latitudes near sunspot maximum and is still visible near the equator well past the minimum of its cycle, indicating that the toroidal field cycle spans approximately two sunspot cycles. The length of the extended activity cycle is measured to be approximately 16.8 yr.
Description
Type of resource | mixed material, Dataset, text |
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Date created | [ca. September 1, 2021] |
Date modified | September 28, 2022; February 28, 2022; December 5, 2022 |
Publication date | September 28, 2022; February 28, 2022 |
Creators/Contributors
Author | Liu, Allison | |
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Author | Scherrer, Philip |
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Subjects
Subject | solar cycle |
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Subject | Torroidal field of Sun |
Genre | Mixed materials |
Genre | Data |
Genre | Text |
Genre | Data sets |
Genre | Dataset |
Bibliographic information
Related item |
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DOI | https://doi.org/10.25740/yq160kn5895 |
Location | https://purl.stanford.edu/yq160kn5895 |
Access conditions
- Use and reproduction
- User agrees that, where applicable, content will not be used to identify or to otherwise infringe the privacy or confidentiality rights of individuals. Content distributed via the Stanford Digital Repository may be subject to additional license and use restrictions applied by the depositor.
- License
- This work is licensed under a Creative Commons Attribution Non Commercial 4.0 International license (CC BY-NC).
Preferred citation
- Preferred citation
- Liu, A. and Scherrer, P. (2022). Solar Toroidal Field Evolution Spanning Four Sunspot Cycles. Stanford Digital Repository. Available at https://purl.stanford.edu/yq160kn5895
Collection
Solar Physics Group Software and Data for Publications
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