Long Wavelength Helical Plasma Equilibrium with a Free Boundary

1973 ◽  
Vol 34 (6) ◽  
pp. 1645-1648
Author(s):  
Masatoshi Tanaka ◽  
Masafumi Azumi ◽  
Takasi Tuda
1988 ◽  
Vol 39 (3) ◽  
pp. 521-538 ◽  
Author(s):  
S. Kanellopoulos ◽  
M. Coppins ◽  
M. G. Haines

A study of the ideal magnetohydrodynamic linear eigenvalue spectrum for free-boundary modes in the Z-pinch is presented. The application of a variational method to estimate eigenvalues is described and limitations imposed by the nature of the spectrum are discussed. An analytic expression for the long-wavelengthm= 0 growth rate is derived


Author(s):  
Hsuan-Yi Chen ◽  
Li-Shing Lin

Abstract The dynamics of of the free boundary of a two-dimensional aggregate of active rod-shaped particles in the nematic phase is considered theoretically. The aggregate is in contact with a hard boundary at $y=0$, a free boundary at $y=H(x,t)$, and in the $x$-direction the aggregate is of infinite size. The analysis shows that the behavior for an aggregate with steady-state particle density $\rho _s$, strength of active stress $\chi$, bulk modulus $\rho_s \beta$, and particles aligned perpendicular to the boundaries can be mapped to one with active stress strength $- \chi$, bulk modulus $\rho_s(\beta - \chi)$, and particles aligned parallel to the boundaries. For a contractile aggregate, when the particles are aligned parallel to the boundaries, the system is unstable in long wavelengths at any strength of contractility for any $H$, and the critical wavelength increases as $H$ increases; when the particles are aligned perpendicular to the boundaries, the system acquires a finite-wavelength instability at a critical active stress whose strength decreases as $H$ increases. The stability of an extensile aggregate can be obtained from the analysis for contractile aggregates and the aforementioned mapping, even though the corresponding physical mechanisms for the instabilities are different. Finally, in the limit $H \rightarrow \infty$, the free boundary is unstable for any contractile or extensile systems in the long wavelength limit.


1979 ◽  
Vol 44 ◽  
pp. 307-313
Author(s):  
D.S. Spicer

A possible relationship between the hot prominence transition sheath, increased internal turbulent and/or helical motion prior to prominence eruption and the prominence eruption (“disparition brusque”) is discussed. The associated darkening of the filament or brightening of the prominence is interpreted as a change in the prominence’s internal pressure gradient which, if of the correct sign, can lead to short wavelength turbulent convection within the prominence. Associated with such a pressure gradient change may be the alteration of the current density gradient within the prominence. Such a change in the current density gradient may also be due to the relative motion of the neighbouring plages thereby increasing the magnetic shear within the prominence, i.e., steepening the current density gradient. Depending on the magnitude of the current density gradient, i.e., magnetic shear, disruption of the prominence can occur by either a long wavelength ideal MHD helical (“kink”) convective instability and/or a long wavelength resistive helical (“kink”) convective instability (tearing mode). The long wavelength ideal MHD helical instability will lead to helical rotation and thus unwinding due to diamagnetic effects and plasma ejections due to convection. The long wavelength resistive helical instability will lead to both unwinding and plasma ejections, but also to accelerated plasma flow, long wavelength magnetic field filamentation, accelerated particles and long wavelength heating internal to the prominence.


1991 ◽  
Vol 161 (11) ◽  
pp. 95 ◽  
Author(s):  
A.I. Frank
Keyword(s):  

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