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In-out intermittency in partial differential equation and ordinary differential equation models
Eurico Covas1, Reza Tavakol, Peter Ashwin
1Astronomy Unit, Mathematical Sciences, Queen Mary, University of London, Mile End Road, London, United Kingdom.
Chaos (Woodbury, N.Y.)
|June 5, 2003
Summary
In-out intermittency, a novel dynamical behavior, is observed in mean-field dynamo models. This finding provides insights into magnetic variability in stars like our Sun.
Area of Science:
- Dynamical Systems
- Astrophysics
- Plasma Physics
Background:
- Dynamical systems exhibiting intermittency are crucial for understanding complex phenomena.
- Mean-field dynamo models are widely used to study stellar magnetic variability.
- Invariant submanifolds play a key role in the behavior of dynamical systems.
Purpose of the Study:
- To provide concrete evidence for in-out intermittency in partial differential equation (PDE) and ordinary differential equation (ODE) models of mean-field dynamos.
- To differentiate in-out intermittency from on-off intermittency based on system structure.
- To explore the physical relevance of in-out intermittency in various dynamical settings.
Main Methods:
- Analysis of partial differential equation (PDE) and ordinary differential equation (ODE) models.
- Investigation of systems with invariant submanifolds.
- Examination of the absence of skew product structure in dynamical systems.
Main Results:
- Demonstration of in-out intermittency in axisymmetric mean-field dynamo models.
- Confirmation that in-out intermittency requires an absence of skew product structure.
- Identification of dynamics where transverse dynamics alter tangential dynamics away from the invariant manifold.
Conclusions:
- In-out intermittency is a significant dynamical behavior with potential physical relevance.
- The findings contribute to understanding the large-scale magnetic variability observed in the Sun and solar-type stars.
- This study highlights the importance of system structure in the manifestation of intermittency.