Space Science Reviews

, Volume 158, Issue 2–4, pp 289–338 | Cite as

Resonant MHD Waves in the Solar Atmosphere

  • Marcel Goossens
  • Robert Erdélyi
  • Michael S. Ruderman
Article

Abstract

The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The review starts from discussing the properties of driven resonant MHD waves. The dissipative solutions in Alfvén and slow dissipative layers are presented. The important concept of connection formulae is introduced. Next, we proceed on to non-stationary resonant MHD waves. The relation between quasi-modes of ideal MHD and eigenmodes of dissipative MHD are discussed. The solution describing the wave motion in non-stationary dissipative layers is given. It is shown that the connection formulae remain valid for non-stationary resonant MHD waves. The initial-value problem for resonant MHD waves is considered. The application of theory of resonant MHD waves to solar physics is discussed.

Keywords

Plasma Waves MHD Sun 

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© Springer Science+Business Media B.V. 2010

Authors and Affiliations

  • Marcel Goossens
    • 1
  • Robert Erdélyi
    • 2
  • Michael S. Ruderman
    • 2
  1. 1.Centre Plasma AstrophysicaKatholieke Universiteit LeuvenLeuvenBelgium
  2. 2.Solar Physics and Space Plasma Research Centre (SP2RC), Department of Applied MathematicsUniversity of SheffieldSheffieldUK

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