Issue |
A&A
Volume 377, Number 1, October I 2001
|
|
---|---|---|
Page(s) | 330 - 342 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361:20011094 | |
Published online | 15 October 2001 |
Hidden problems of thin-flux-tube approximation
1
Center for Plasma Astrophysics, K.U. Leuven, 3001 Heverlee, Belgium
2
IZMIRAN, Troitsk, Moscow Region, 142092, Russia
Corresponding author: Y. Zhugzhda, yvzef@coot.kis.uni-freiburg.de
Received:
9
November
2000
Accepted:
31
July
2001
This paper scrutinizes the validity of the thin-flux-tube
approximation for magnetic flux tubes embedded in a surrounding
magnetic plasma. It is shown that the thin-flux-tube
approximation gives an accurate description of surface waves for
, body waves for
and surface leaky waves for
. The Leibovich-Roberts equation for nonlinear
surface waves in a flux tube embedded in a field free plasma is
generalized to a flux tube immersed in a magnetic plasma. The
generalized Leibovich-Roberts (GLR) equation describes the
propagation of nonlinear slow surface, body and surface leaky
waves in tubes. The shortcomings of the GLR equation are
discussed. The Korteweg-de Vries equation (KdV) is generalized
for surface waves. The advantage of the second order
thin-flux-tube approximation is shown. Two scenarios for the
heating of coronal loops are discussed. It is emphasized, that
the application of the thin-flux-tube approximation to thin tubes
of non-zero diameter has to take into account possible wave
emission by the tube and shock front formation for amplitudes in
excess of some critical value.
Key words: Magnetohydrodynamics (MHD) / waves / Sun: atmosphere / Sun: general
© ESO, 2001
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