Mhd Mode conversion around a 2d magnetic null point

A. M.D. Mcdougall, A. W. Hood

Research output: Contribution to conferencePaperpeer-review

Abstract

Mode conversion occurs when a wave passes through a region where the sound and Alfvén 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 twodimensional, coronal null point. As a wave approaches the null it passes from low- to high-β 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.

Original languageEnglish
Pages752-755
Number of pages4
DOIs
Publication statusPublished - 23 Apr 2009
Event15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - St Andrews, St Andrews, United Kingdom
Duration: 21 Jul 200825 Jul 2008

Conference

Conference15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
Country/TerritoryUnited Kingdom
CitySt Andrews
Period21/07/0825/07/08

Keywords

  • Magnetohydrodynamics
  • Sun: corona
  • Sun: oscillations

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