Spin magnetoacoustic wave

2019 ◽  
Vol 26 (11) ◽  
pp. 112101 ◽  
Author(s):  
Z. Iqbal ◽  
Mehak Younas ◽  
Imran A. Khan ◽  
G. Murtaza
Keyword(s):  
2013 ◽  
Vol 550 ◽  
pp. A1 ◽  
Author(s):  
M. Karlický ◽  
H. Mészárosová ◽  
P. Jelínek

2016 ◽  
Vol 591 ◽  
pp. A103 ◽  
Author(s):  
J. A. McLaughlin ◽  
G. J. J. Botha ◽  
S. Régnier ◽  
D. L. Spoors
Keyword(s):  

2001 ◽  
Vol 203 ◽  
pp. 517-519
Author(s):  
Y. Voitenko ◽  
M. Goossens

A nonlinear mechanism for the damping of fast magnetoacoustic wave in the solar corona is studied. It is shown that the nonlinear coupling of finite-amplitude fast waves to small-scale Alfven waves can be much faster than damping mechanisms involving classic transport coefficients.


1985 ◽  
Vol 108 (7) ◽  
pp. 344-346 ◽  
Author(s):  
N.N. Rao ◽  
M.Y. Yu ◽  
P.K. Shukla ◽  
R.K. Varma

1994 ◽  
Vol 12 (10/11) ◽  
pp. 1022-1026 ◽  
Author(s):  
A. E. Kozlovsky ◽  
V. V. Safargaleev ◽  
W. B. Lyatsky

Abstract. A mechanism for the transformation of a magnetoacoustic wave into an Alfvén wave is proposed. During the compression of the magnetosphere by the solar wind the inner edge of the plasma sheet and the contours of B=const move in different ways. In the case of asymmetrical compression, the contours of B=const will cross the inner edge of the plasma sheet. To close the drift currents - that flow in the plasma sheet along the contours of B=const - the appearance of the field-aligned currents is necessary. This appearance corresponds to the generation of the Alfvén wave.


1994 ◽  
Vol 12 (10/11) ◽  
pp. 1018-1021 ◽  
Author(s):  
V. V. Safargaleev ◽  
V. B. Lyatsky

Abstract. A guided propagation of magnetoacoustic wave in the plasma sheet located between two lobes of the magnetotail is investigated. The dispersion equation for the wave and equation connecting a disturbance of plasma pressure inside the plasma sheet and amplitude of the plasma sheet boundary oscillations are obtained. For some value of plasma pressure disturbance, the displacement of the plasma sheet boundaries becomes of order of the half-thickness of the plasma sheet. In the case of symmetrical oscillations of the boundaries ("sausage-like" mode), it creates the favourable conditions for reconnection of the magnetic field lines in the magnetotail and may lead to triggering of a substorm. The magnetoacoustic wave may be generated by sudden impulse of the solar wind plasma pressure.


Scilight ◽  
2019 ◽  
Vol 2019 (34) ◽  
pp. 340003
Author(s):  
Jodi Ackerman Frank

2014 ◽  
Vol 568 ◽  
pp. A20 ◽  
Author(s):  
D. J. Pascoe ◽  
V. M. Nakariakov ◽  
E. G. Kupriyanova

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