Kink Wave Propagation in Thin Isothermal Magnetic Flux Tubes

Solar Physics ◽  
2014 ◽  
Vol 289 (8) ◽  
pp. 3033-3041 ◽  
Author(s):  
I. P. Lopin ◽  
I. G. Nagorny ◽  
E. Nippolainen
2014 ◽  
pp. 411-419
Author(s):  
I. P. Lopin ◽  
I. G. Nagorny ◽  
E. Nippolainen

2018 ◽  
Vol 58 (7) ◽  
pp. 942-946
Author(s):  
Yu. T. Tsap ◽  
A. V. Stepanov ◽  
Yu. G. Kopylova

2013 ◽  
Vol 551 ◽  
pp. A86 ◽  
Author(s):  
R. Soler ◽  
A. J. Díaz ◽  
J. L. Ballester ◽  
M. Goossens

1990 ◽  
Vol 142 ◽  
pp. 159-174
Author(s):  
B Roberts

The basic aspects of wave propagation in a magnetic flux tube are reviewed, with particular emphasis on the types of flux tube that occur in the solar atmosphere. Two fundamental speeds arise naturally in a description of wave propagation in a flux tube: the slow magnetoacoustic (cusp) speed cT, which is both subsonic and sub-Alfvénic, and a mean Alfvén speed ck. Both surface and body modes are supported by a tube. It is stressed that a flux tube may act as a wave guide, similar to the guidance of light by a fibre optic, or sound in an ocean layer, or seismic waves in the Earth's crust.


1998 ◽  
Vol 500 (2) ◽  
pp. 966-977 ◽  
Author(s):  
Sergey Bazdenkov ◽  
Tetsuya Sato

2017 ◽  
Vol 851 (1) ◽  
pp. 42 ◽  
Author(s):  
Jianping Xiong ◽  
Yunfei Yang ◽  
Chunlan Jin ◽  
Kaifan Ji ◽  
Song Feng ◽  
...  

1990 ◽  
Vol 65 (8) ◽  
pp. 1060-1063 ◽  
Author(s):  
S. J. Bending ◽  
K. von Klitzing ◽  
K. Ploog

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