Book contents
- Frontmatter
- Dedication
- Contents
- Preface
- 1 General Principles
- 2 Waves in a Uniform Medium
- 3 Magnetically Structured Atmospheres
- 4 Surface Waves
- 5 Magnetic Slabs
- 6 Magnetic Flux Tubes
- 7 The Twisted Magnetic Flux Tube
- 8 Connection Formulas
- 9 Gravitational Effects
- 10 Thin Flux Tubes: The Sausage Mode
- 11 Thin Flux Tubes: The Kink Mode
- 12 Damping
- 13 Nonlinear Aspects
- 14 Solar Applications of MHD Wave Theory
- References
- Index
11 - Thin Flux Tubes: The Kink Mode
Published online by Cambridge University Press: 15 July 2019
- Frontmatter
- Dedication
- Contents
- Preface
- 1 General Principles
- 2 Waves in a Uniform Medium
- 3 Magnetically Structured Atmospheres
- 4 Surface Waves
- 5 Magnetic Slabs
- 6 Magnetic Flux Tubes
- 7 The Twisted Magnetic Flux Tube
- 8 Connection Formulas
- 9 Gravitational Effects
- 10 Thin Flux Tubes: The Sausage Mode
- 11 Thin Flux Tubes: The Kink Mode
- 12 Damping
- 13 Nonlinear Aspects
- 14 Solar Applications of MHD Wave Theory
- References
- Index
Summary
The thin tube theory for a kink wave in a stratified flux tube is determined and explored in the case when the tube is unstratified. Perturbations are also considered for this case. Using a multiple scales approach, the wave equation is derived for the kink mode of a thin magnetic flux tube in an unstratified atmosphere, demonstrating the importance of the kink speed. The theory is illustrated for standing waves in a uniform loop and also extended to structured loops with non-uniform density along the structure. Two density profiles are considered in detail. Period ratios for standing waves under coronal conditions are explored. The role of a non-uniform magnetic field is explored, and leads to a wave equation with non-uniform kink speed. Dispersive corrections in a uniform tube are examined and compared with earlier results. Gravity effects are also examined.
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- MHD Waves in the Solar Atmosphere , pp. 311 - 359Publisher: Cambridge University PressPrint publication year: 2019
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