English

Thermo-Galvanometric Instabilities in Magnetized Plasma Disks

Solar and Stellar Astrophysics 2015-06-18 v2

Abstract

In this work, we present a linear stability analysis of fully-ionized rotating plasma disks with a temperature gradient and a sub-thermal background magnetic field (oriented towards the axial direction). We describe how the plasma reacts when galvanometric and thermo-magnetic phenomena, such as Hall and Nernst-Ettingshausen effects, are taken into account, and meridian perturbations of the plasma are considered. It is shown how, in the ideal case, this leads to a significant overlap of the Magneto-rotational Instability and the Thermo-magnetic one. Considering dissipative effects, an overall damping of the unstable modes, although not sufficient to fully suppress the instability, appears especially in the thermo-magnetic related branch of the curve.

Keywords

Cite

@article{arxiv.1312.3443,
  title  = {Thermo-Galvanometric Instabilities in Magnetized Plasma Disks},
  author = {Alessio Franco and Giovanni Montani and Nakia Carlevaro},
  journal= {arXiv preprint arXiv:1312.3443},
  year   = {2015}
}

Comments

6 pages, 3 figures

R2 v1 2026-06-22T02:26:09.041Z