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Detailed mathematical and numerical analysis of a dynamo model

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TLDR
In this paper, the role of nonlinear feedback by α-quenching, flux losses, and feedback by differential rotations in dynamo was investigated, and it was shown that the effect of flux loss and α quenching is boosted when combined with toroidal flux loss, indicating that the dynamic balance of dynamo is optimized.
Abstract
We investigate the role of nonlinear feedback by α-quenching, flux losses, and feedback by differential rotations in dynamo. Specifically, by studying the nonlinear dynamo model analytically and numerically, we unfold how frequency p of magnetic field, magnetic field strength |B|, and phase φ are influenced by different types of nonlinear feedback in the limit of a very weak mean and/or fluctuating differential rotation. We find that p and φ are controlled by both flux losses with no influence by α-quenching when there is no back reaction because of fluctuating differential rotation. We find a similar effect of poloidal flux loss and toroidal flux loss on p and |B| in the absence of a back reaction of shear. Their effect becomes totally different with the inclusion of this back reaction. Detailed investigations suggest that toroidal flux loss tends to have more influence than poloidal flux loss (with or without α-quenching) in the presence of fluctuating shear. Furthermore, the effect of α-quenching is boosted when combined with toroidal flux loss, indicating that the dynamic balance of dynamo is optimized in the presence of both α-quenching and flux loss. These results highlight the importance of nonlinear transport coefficients and differential rotation in the regulation of a dynamo.

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Journal ArticleDOI

Dynamical model for spindown of solar-type stars

TL;DR: In this article, a spindown model is proposed where loss of angular momentum by magnetic fields is evolved dynamically, instead of being kinematically prescribed, and the authors highlight the importance of self-regulation of magnetic fields and rotation by direct and indirect interactions involving nonlinear feedback in stellar evolution.
Dissertation

Investigation of regulation of stellar magnetism and rotation

Aditi Sood
TL;DR: In this paper, a simple parameterized model was proposed to understand the evolution of rotation rate and magnetic fields in the solar dynamo and the spindown of solar-type stars.
Journal ArticleDOI

Geometric method for forming periodic orbits in the Lorenz system

TL;DR: The non-detailed balance observable representation (NOR) provides a useful methodology for understanding the evolution of non-equilibrium complex systems, by mapping out the correlation between two states to a metric space where a small distance represents a strong correlation.
Journal ArticleDOI

Dynamical model for spindown of solar-type stars

TL;DR: In this paper, a spindown model is proposed where loss of angular momentum by magnetic fields evolves dynamically, instead of being prescibed kinematically, and the authors show that their extended model reproduces key observations and is capable of explaining the presence of two branches of (fast and slow rotating) stars.
References
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Journal ArticleDOI

A Babcock-Leighton Flux Transport Dynamo with Solar-like Differential Rotation

TL;DR: In this article, the authors investigate the properties of a kinematic -ux transport solar dynamo model, which is characterised by a solar-like internal diUerential rotation, a single-cell meridional -ow in the convective envelope that is directed poleward at the surface, and a magnetic diUusivity that is constant within the envelope but decreases sharply at the core-envelope interface.
Journal ArticleDOI

Time evolution of the magnetic activity cycle period. II. Results for an expanded stellar sample

TL;DR: In this article, the magnetic dynamo cycle period Pcyc, the rotational period Prot, the activity level (as observed in Ca II HK), and other stellar properties were explored by expanding the stellar sample studied in the first paper.
Journal ArticleDOI

The relation between stellar rotation rate and activity cycle periods

TL;DR: In this article, the authors investigated the empirical relation between rotation period, spectral type, and activity cycle period for a sample of 13 slowly rotating lower main-sequence stars, including the Sun, all of which show longterm chromospheric variability like that of the solar cycle.
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