Dynamics of an Al wire corona of a megaampere Z-pinch

被引:10
|
作者
Kubes, P
Kravárik, J
Renner, O
Krousky, E
Bakshaev, YL
Blinov, PI
Chernenko, AS
Gordeev, EM
Dan'ko, SA
Korolev, VD
Shashkov, AY
机构
[1] Czech Tech Univ, Prague 16627 6, Czech Republic
[2] Inst Phys, Prague 18221 8, Czech Republic
[3] Russian Res Ctr, IV Kurchatov Atom Energy Inst, Moscow 123182, Russia
关键词
Photon Energy; Bright Spot; High Plasma Density; Axial Magnetic Field; Photon Energy Range;
D O I
10.1134/1.1469170
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
It is shown that the development of instabilities in a Z-pinch plasma formed by loading a relatively thick At wire (an initial diameter of 120 mum and a maximum discharge current of 2-3 MA) is slowed down due to the high plasma density in the wire corona. A cylindrically symmetric, regular, and stable corona surrounding the wire contains a helical formation with a dense, cold, and magnetized plasma. X-ray pulses with a photon energy of several keV and an FWHM duration of 10-20 ns are generated by a few imploded neck structures in the pinch phase of the corona evolution (70-100 ns after the current onset). The main part of X radiation emitted by individual bright spots in the photon energy range 1.5-2.4 keV (up to 40 J at a peak power of 4 GW) consists of the continuum and the bound-bound transition radiation from H- and He-like At ions. A possible scenario for the axial magnetic field evolution during an X-ray pulse is outlined. (C) 2002 MAIK "Naukal/Interperiodica".
引用
收藏
页码:296 / 302
页数:7
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