Issue |
A&A
Volume 415, Number 2, February IV 2004
|
|
---|---|---|
Page(s) | 751 - 754 | |
Section | The Sun | |
DOI | https://doi.org/10.1051/0004-6361:20035820 | |
Published online | 11 February 2004 |
Research Note
Tube waves: Exact and approximate
Kiepenheuer-Institut für Sonnenphysik, Schöneckstr. 6, 79104 Freiburg, Germany
Corresponding author: stix@kis.uni-freiburg.de
Received:
8
December
2003
Accepted:
15
December
2003
This note deals with magnetohydrodynamic body waves in a
magnetic cylinder. It is shown that the solution obtained by the
thin-tube expansion is, term by term,
identical to the Taylor expansion of the
exact solution. Each level of approximation adds a pair of modes,
a slow and a fast one, and corrects the frequencies and
eigenfunctions of the previous approximation. All eigenfrequencies,
approximate and exact, can be read off from a single graph. All
slow modes have phase velocities between the tube speed cT and
, all fast modes have phase velocities above
.
Key words: magnetohydrodynamics (MHD) / waves / methods: analytical / Sun: magnetic fields
© ESO, 2004
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