Observation-Based Iterative Map for Solar Cycles. II. The Gnevyshev-Ohl Rule and its Generation Mechanism
Zi-Fan Wang, Jie Jiang, Jing-Xiu Wang

TL;DR
This paper investigates the Gnevyshev-Ohl rule in solar cycles using an observation-based iterative map, revealing it as a manifestation of nonlinear stochastic dynamics rather than a strict physical law.
Contribution
It introduces a generalized rule for solar cycle strength succession and explains the G-O rule as a natural outcome of nonlinear stochastic processes.
Findings
The G-O rule can arise randomly over long timescales.
Short-term behavior depends on initial conditions and parameters.
G-O-like behavior is a generic property of nonlinear stochastic systems.
Abstract
The Gnevyshev-Ohl (G-O) rule, or even-odd effect, is an important observational phenomenon in solar cycles, originally suggesting that even-numbered cycles are typically followed by stronger odd-numbered ones. However, subsequent studies have reported varied forms and often conflicting manifestations of this rule, along with diverse interpretations of its physical origin. Using an observation-based iterative map, we investigate these different forms of the G-O rule and propose a more general underlying rule: statistically, a given solar cycle is more likely to be followed by a stronger one, regardless of even-odd numbering. This transition asymmetry arises from the map's inherent asymmetry relative to the diagonal. Over timescales comparable to historical observations, both the G-O rule and its reversal can arise randomly, without a consistent preference. The short-term behavior of the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsSolar and Space Plasma Dynamics · Solar Radiation and Photovoltaics
