Chandrasekhar-Kendall functions in astrophysical dynamos
Abstract
Some of the contributions of Chandrasekhar to the field of magnetohydrodynamics are highlighted. Particular emphasis is placed on the Chandrasekhar-Kendall functions that allow a decomposition of a vector field into right- and left-handed contributions. Magnetic energy spectra of both contributions are shown for a new set of helically forced simulations at resolutions higher than what has been available so far. For a forcing function with positive helicity, these simulations show a forward cascade of the right-handed contributions to the magnetic field and nonlocal inverse transfer for the left-handed contributions. The speed of inverse transfer is shown to decrease with increasing value of the magnetic Reynolds number.
Cite
@article{arxiv.1103.4976,
title = {Chandrasekhar-Kendall functions in astrophysical dynamos},
author = {Axel Brandenburg},
journal= {arXiv preprint arXiv:1103.4976},
year = {2015}
}
Comments
10 pages, 5 figures, proceedings of the Chandrasekhar Centenary Conference, to be published in PRAMANA - Journal of Physics