Asymmetric Solar Polar Field Reversals
Leif Svalgaard, Yohsuke Kamide

TL;DR
The paper explains how asymmetric solar activity in the hemispheres influences the timing of polar magnetic field reversals, leading to observable differences in reversal times during solar cycles.
Contribution
It proposes a model linking hemispheric activity asymmetry to the timing of polar field reversals, supported by historical observations of solar cycles.
Findings
Hemispheric activity asymmetry correlates with reversal timing differences.
Historical data shows hemispheric activity peaks align with reversal order.
The model explains variations in reversal times across solar cycles.
Abstract
The solar polar fields reverse because magnetic flux from decaying sunspots moves towards the poles, with a preponderance of flux from the trailing spots. Let us assume that there is a strong asymmetry in the sense that all activity is in the Northern Hemisphere, then that excess flux will move to the North Pole and reverse that pole, while nothing happens in the South. If later on, there is a lot of activity in the South, then that flux will help reverse the South Pole. In this way, we get two humps in solar activity and a corresponding difference in time of reversals. Such difference was first noted by Babcock (1959) from the very first observation of polar field reversal just after the maximum of the strongly asymmetric solar cycle 19. At that time, the Southern Hemisphere was most active before sunspot maximum and the South Pole duly reversed first, followed by the Northern…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · Astro and Planetary Science
