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Open AccessJournal ArticleDOI

Detailed mathematical and numerical analysis of a dynamo model

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 Low-Order Solar Dynamo Model: Inferred Meridional Circulation Variations Since 1750

TL;DR: In this paper, the authors present the possible variations that the meridional circulation of the Sun might have undergone during the last 250 years by using phase space analysis of the superficialtoroidal magnetic field.
Journal ArticleDOI

Low-order stellar dynamo models

TL;DR: In this paper, the authors used normal-form theory to derive a third-order model with robust behaviour, which is able to reproduce many of the basic types of behaviour found in observations of solar-type stars.
Journal ArticleDOI

A Simple Model for the Solar Cycle

TL;DR: A simple nonlinear model which describes the 11-year solar cycle can be derived from the usual α−ω dynamo theory in the form of a Van der Pol equation.
Journal ArticleDOI

Weak hysteresis in a simplified model of the L-H transition

TL;DR: In this paper, a simple one-field L-H transition model is studied in detail, analytically and numerically, and it is shown that by shaping the heating rate temporal profile, one can reduce the average power required for the transition to the QH-mode.
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