English

Robustness of truncated alpha-Omega dynamos with a dynamic alpha

Astrophysics 2015-06-24 v1

Abstract

In a recent work (Covas et al. 1997), the behaviour and the robustness of truncated αΩ\alpha\Omega dynamos with a dynamic α\alpha were studied with respect to a number of changes in the driving term of the dynamic α\alpha equation, which was considered previously by Schmalz and Stix (1991) to be of the form AϕBϕ\sim A_{\phi}B_{\phi}. Here we review and extend our previous work and consider the effect of adding a quadratic quenching term of the form αB2\alpha|B|^2. We find that, as before, such a change can have significant effects on the dynamics of the related truncated systems. We also find intervals of (negative) dynamo numbers, in the system considered by Schmalz and Stix (1991), for which there is sensitivity with respect to small changes in the dynamo number and the initial conditions, similar to what was found in our previous work. This latter behaviour may be of importance in producing the intermittent type of behaviour observed in the sun.

Cite

@article{arxiv.astro-ph/9708094,
  title  = {Robustness of truncated alpha-Omega dynamos with a dynamic alpha},
  author = {Eurico Covas and Andrew Tworkowski and Reza Tavakol and Axel Brandenburg},
  journal= {arXiv preprint arXiv:astro-ph/9708094},
  year   = {2015}
}

Comments

Figures included. Also in http://www.maths.qmw.ac.uk/~eoc

R2 v1 2026-07-22T09:35:05.379Z