Fluid instabifities of a uniformly imploding ablatively driven shell
- 1 February 1980
- journal article
- research article
- Published by Cambridge University Press (CUP) in Journal of Plasma Physics
- Vol. 23 (3) , 521-533
- https://doi.org/10.1017/s0022377800022522
Abstract
The linear stability of a uniformly imploding shell, modelled as an ideal polytropic fluid, is investigated. Two types of unstable modes are found: incompressible irrotational perturbations localized at the outer surface, ascribable to Rayleigh—Taylor instability, and compressible modes, associated with convective instabiiity. Kidder's result for the Rayleigh—Taylor modes is shown to hold independently of the form of the shell density profile. By means of a variational principle it is shown that the criterion for convective instability is the existence of a region within which d(pp-γ)/dr> 0. Analytic solutions for both spatial and temporal dependence of the perturbations are presented, and the results applied to pellets imploded by the action of a laser or charged-particle beam.Keywords
This publication has 4 references indexed in Scilit:
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- Acoustic Amplification in Imploding Spherical ShellsPhysical Review Letters, 1978
- Rayleigh-Taylor instability of a self-similar spherical expansionThe Astrophysical Journal, 1978
- Laser-driven compression of hollow shells: power requirements and stability limitationsNuclear Fusion, 1976