A new simple dynamo model for stellar activity cycle
Nobumitsu Yokoi, Dieter Schmitt, Valery Pipin, and Fujihiro Hamba

TL;DR
This paper introduces a simplified dynamo model for stellar activity cycles that incorporates turbulent cross helicity, offering new insights into magnetic field reversals and stellar magnetic activity through coupled evolution equations.
Contribution
The model uniquely includes the cross-helicity effect as a key dynamo ingredient and solves its evolution alongside magnetic fields, differing from traditional alpha-Omega models.
Findings
Eigenvalue analysis produces a butterfly diagram consistent with observations.
The model shows cross helicity oscillation as a driver of magnetic field reversals.
Results suggest cross helicity reversal causes magnetic activity cycles.
Abstract
A new simple dynamo model for stellar activity cycle is proposed. By considering an inhomogeneous mean flow effect on turbulence, it is shown that turbulent cross helicity (velocity--magnetic-field correlation) should enter the expression of turbulent electromotive force as the coupling coefficient for the mean absolute vorticity. The inclusion of the cross-helicity effect makes the present model different from the current ---type models mainly in two points. First, in addition to the usual (helicity effect) and (turbulent magnetic diffusivity), we consider the coefficient (cross-helicity effect) as a key ingredient of the dynamo process. Second, unlike the and coefficients, which are often treated as an adjustable parameter in the current studies, the spatiotemporal evolution of coefficient is solved simultaneously…
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.
