A Possible Source of Multiple Polarity Reversals of the Polar Magnetic Field during the Maximum Phase of Solar Cycle

A Possible Source of Multiple Polarity Reversals of the Polar Magnetic Field during the Maximum Phase of Solar Cycle

During the maximum phase of solar activity, it is quite common for the polar magnetic field to undergo multiple polarity reversals. In this study, we aim to provide the likely source of this phenomenon. By analyzing synoptic magnetograms from the Michelson Doppler Imagers on the Solar and Helioseism...

Full description

Saved in:
Bibliographic Details
Main Authors: Chunlan Jin, Shuhong Yang, Guiping Zhou, Jialiang Hu, Jingxiu Wang
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Solar cycle
Solar dynamo
Stellar activity
Solar photosphere
Online Access:https://doi.org/10.3847/1538-4357/ade681
Tags: Add Tag
No Tags, Be the first to tag this record!
Login for hold and recall information

Internet

https://doi.org/10.3847/1538-4357/ade681

Similar Items