English

BO 2.0: Plasma Wave and Instability Analysis with Enhanced Polarization Calculations

Plasma Physics 2021-03-31 v1 Solar and Stellar Astrophysics Space Physics

Abstract

Besides the relation between the wave vector k\bm k and the complex frequency ω\omega, wave polarization is useful for characterizing the properties of a plasma wave. The polarization of the electromagnetic fields, δE\delta \bm E and δB\delta \bm B, have been widely used in plasma physics research. Here, we derive equations for the density and velocity perturbations, δns\delta n_s and δvs\delta{\bm v}_s, respectively, of each species in the electromagnetic kinetic plasma dispersion relation by using their relation to the species current density perturbation δJs\delta {\bm J}_s. Then we compare results with those of another commonly used plasma dispersion code (WHAMP) and with those of a multi-fluid plasma dispersion relation. We also summarize a number of useful polarization quantities, such as magnetic ellipticity, orientation of the major axis of the magnetic ellipse, various ratios of field energies and kinetic energies, species compressibility, parallel phase ratio, Alfv\'en-ratio, etc., which are useful for plasma physics research, especially for space plasma studies. This work represents an extension of the BO electromagnetic dispersion code [H.S. Xie, Comput. Phys. Comm. 244 (2019) 343-371] to enhance its calculation of polarization and to include the capability of solving the electromagnetic magnetized multi-fluid plasma dispersion relation.

Keywords

Cite

@article{arxiv.2103.16014,
  title  = {BO 2.0: Plasma Wave and Instability Analysis with Enhanced Polarization Calculations},
  author = {Hua-sheng Xie and Richard Denton and Jin-song Zhao and Wen Liu},
  journal= {arXiv preprint arXiv:2103.16014},
  year   = {2021}
}

Comments

15 pages, 4 figures

R2 v1 2026-06-24T00:40:25.054Z