Hostname: page-component-7bb8b95d7b-w7rtg Total loading time: 0 Render date: 2024-09-27T06:20:43.049Z Has data issue: false hasContentIssue false

A new mechanism for the butterfly diagram of the solar cycle

Published online by Cambridge University Press:  28 September 2023

Zebin Zhang
Affiliation:
School of Space and Environment, Beihang University, Beijing, China Key Laboratory of Space Environment monitoring and Information Processing of MIIT, Beijing, China
Jie Jiang
Affiliation:
School of Space and Environment, Beihang University, Beijing, China Key Laboratory of Space Environment monitoring and Information Processing of MIIT, Beijing, China
Haowei Zhang
Affiliation:
School of Space and Environment, Beihang University, Beijing, China Key Laboratory of Space Environment monitoring and Information Processing of MIIT, Beijing, China
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The butterfly diagram of the solar cycle is the equatorward migration of sunspot’s emergence latitudes as the solar cycle evolves, which was attributed to the equatorward flow at the base of the convection zone. However, helioseismological studies indicate controversial forms of the flow, and even present poleward flow at the base, which poses a big challenge to the wide-accepted mechanism. So we aim to propose a new mechanism, that is the latitude-dependent radial flux transport.

Type
Poster Paper
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

References

Guerrero, G. & de Gouveia Dal Pino, E. M. 2008, A&A, 485, 267 Google Scholar
Jiang, J., Cameron, R. H., Schmitt, D., & Işk, E. 2013, A&A, 553, A128 Google Scholar
Pipin, V. V. & Kosovichev, A. G. 2011, ApJ Letters, 727, L45 CrossRefGoogle Scholar
Zhao, J., Bogart, R. S., Kosovichev, A. G., Duvall, T. L., J., & Hartlep, T. 2013, ApJ Letters, 774, L29CrossRefGoogle Scholar
Supplementary material: PDF

Zhang et al. supplementary material

Zhang et al. supplementary material

Download Zhang et al. supplementary material(PDF)
PDF 1 MB