English

MHD Mode Conversion around a 2D Magnetic Null Point

Solar and Stellar Astrophysics 2009-07-10 v1

Abstract

Mode conversion occurs when a wave passes through a region where the sound and Alfven speeds are equal. At this point there is a resonance, which allows some of the incident wave to be converted into a different mode. We study this phenomenon in the vicinity of a two-dimensional, coronal null point. As a wave approaches the null it passes from low- to high-beta plasma, allowing conversion to take place. We simulate this numerically by sending in a slow magnetoacoustic wave from the upper boundary; as this passes through the conversion layer a fast wave can clearly be seen propagating ahead. Numerical simulations combined with an analytical WKB investigation allow us to determine and track both the incident and converted waves throughout the domain.

Keywords

Cite

@article{arxiv.0907.1541,
  title  = {MHD Mode Conversion around a 2D Magnetic Null Point},
  author = {A. M. D. McDougall and A. W. Hood},
  journal= {arXiv preprint arXiv:0907.1541},
  year   = {2009}
}

Comments

4 pages, 2 figures

R2 v1 2026-06-21T13:23:05.741Z