scholarly journals Tearing and surface preserving electron magnetohydrodynamic modes in a current layer

2016 ◽  
Vol 23 (3) ◽  
pp. 032106
Author(s):  
Gurudatt Gaur ◽  
Predhiman K. Kaw
Keyword(s):  
1955 ◽  
Vol 8 (3) ◽  
pp. 319 ◽  
Author(s):  
RE Loughhead

The hydromagnetic stability of a uniform current flowing along a magnetic field and confined within a pair of parallel planes is discussed by the method of normal modes. The condition for marginal stability is derived and discussed with reference to two special cases.


1972 ◽  
Vol 50 (20) ◽  
pp. 2475-2481 ◽  
Author(s):  
C. S. Maclatchy ◽  
A. J. Barnard

The formative phase of a 40 kV Z pinch has been investigated for pressures from 10 to 80 mTorr in H2. The energy spectrum of the electrons on the axis of the vessel, the spatial distribution of the current at the face of the anode, and the total discharge current were monitored. At the initiation of the discharge, a current of electrons with energies in excess of 20 keV is observed on the axis. This observation is in contrast to the normally accepted mode of ionization in which ionization initiates at the wall. The current is observed to switch from the axial region to the wall where it forms a current layer which collapses in accordance with the snow-plough model. The exact nature of the switching mechanism is not understood. The formative phase of the pinch typically takes a few hundred nanoseconds. The observations indicate that the detailed process of current sheet collapse may be affected by the formative phase.


1980 ◽  
Vol 23 (6) ◽  
pp. 431-436
Author(s):  
V. D. Kuznetsov
Keyword(s):  

1993 ◽  
Vol 49 (1) ◽  
pp. 85-100 ◽  
Author(s):  
R. B. Paris

The analouge of the Reyleigh–Taylor instability (the gravitational interchange mode) for an infinitely conducting, approximately one-dimensional plane plasma slab is examined when the gravitational acceleration g is taken to be perpendicular to the equalibrium density gradient δp0. In contrast with the ‘classical’ situation (where g is aligned with δp0), it is found for a current layer with Magnetic shear that there is no instability threshold equivalent to the ‘classical’ situation (where g is aligned with δp0), it is found for a current layer with magnetic shear that there is no instability threshold equivalent to the Suydam criterion: the mode is unstable for all values of |δp0|. In the weak shear limit the growth rate of the instability is shown to exhibit the familiar (g|δp0|/p0)img; scaling characteristic of the gravitational interchange mode.


2010 ◽  
Vol 17 (1) ◽  
pp. 010702 ◽  
Author(s):  
R. L. Fermo ◽  
J. F. Drake ◽  
M. Swisdak

1996 ◽  
Vol 3 (6) ◽  
pp. 2248-2254 ◽  
Author(s):  
O. Z. Zabaidullin ◽  
V. V. Vikhrev

2006 ◽  
Vol 44 (4) ◽  
pp. 497-506 ◽  
Author(s):  
E. N. Vasil’ev ◽  
D. A. Nesterov

Sign in / Sign up

Export Citation Format

Share Document