pith. sign in

arxiv: 1009.1051 · v1 · pith:R6ITAXFNnew · submitted 2010-09-06 · 🌌 astro-ph.EP · physics.flu-dyn· physics.geo-ph· physics.plasm-ph

Energy oscillations and a possible route to chaos in a modified Riga dynamo

classification 🌌 astro-ph.EP physics.flu-dynphysics.geo-phphysics.plasm-ph
keywords magneticdynamooscillationsazimuthalbehaviourenergyfieldfrequency
0
0 comments X
read the original abstract

Starting from the present version of the Riga dynamo experiment with its rotating magnetic eigenfield dominated by a single frequency we ask for those modifications of this set-up that would allow for a non-trivial magnetic field behaviour in the saturation regime. Assuming an increased ratio of azimuthal to axial flow velocity, we obtain energy oscillations with a frequency below the eigenfrequency of the magnetic field. These new oscillations are identified as magneto-inertial waves that result from a slight imbalance of Lorentz and inertial forces. Increasing the azimuthal velocity further, or increasing the total magnetic Reynolds number, we find transitions to a chaotic behaviour of the dynamo.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.