English

The Role of Helical and Non-Helical Drives on the evolution of Self-Consistent Dynamos

Plasma Physics 2024-07-23 v1 Astrophysics of Galaxies Computational Physics Fluid Dynamics

Abstract

In the self-consistent dynamo limit, the magnetic feedback on the velocity field is sufficiently strong to induce a change in the topology of the magnetic field. Consequently, the magnetic energy reaches a state of non-linear saturation. Here, we investigate the role played by helical and non-helical drives in the triggering and the eventual saturation of a self-consistent dynamo. Evidence of small-scale dynamo (SSD) activity is found for both helical and non-helical forcing, driven at the largest possible scale. Based on the spectrum analysis, we find that the evolution of kinetic energy follows Kolmogorov's k53k^-{\frac{5}{3}} law while that of magnetic energy follows Kazantsev's k32k^{\frac{3}{2}} scaling. Also, we have verified that the aforementioned scalings remain valid for various magnetic Prandtl numbers (Pm). Statistical analysis is found to support our numerical finds.

Keywords

Cite

@article{arxiv.2407.14810,
  title  = {The Role of Helical and Non-Helical Drives on the evolution of Self-Consistent Dynamos},
  author = {Shishir Biswas and Rajaraman Ganesh},
  journal= {arXiv preprint arXiv:2407.14810},
  year   = {2024}
}