Abstract
To mitigate the Rayleigh-Taylor (RT) instability, a somewhat non-conventional use of the externally applied axial magnetic field Bz combined with a double-shell gas-puff load is proposed. For stabilization, the whole implosion should be organized in such a way that the frozen-in axial field Bz≅Bθ is concentrated in a thin layer of imploding plasma. This paper presents a theoretical analysis of the thin plasma shell formation in the presence of a Bz magnetic field and results of a numerical simulation.
| Original language | English |
|---|---|
| Article number | 123 |
| Pages (from-to) | 156 |
| Number of pages | 1 |
| Journal | IEEE International Conference on Plasma Science |
| DOIs | |
| Publication status | Published - 1 Jan 2002 |
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