Interaction of counter-streaming plasma flows in a dipole magnetic field

被引:3
作者
Shaikhislamov, I. F. [1 ]
Posukh, V. G. [1 ]
Melekhov, A. V. [1 ]
Prokopov, P. A. [1 ]
Boyarintsev, E. L. [1 ]
Zakharov, Yu P. [1 ]
Ponomarenko, A. G. [1 ]
机构
[1] RAS, SB, Dept Laser Plasma, Inst Laser Phys, Pr Lavrentyeva 13-3, Novosibirsk 630090, Russia
关键词
counter-streaming plasmas; laser-produced plasma; magnetised background; magnetosphere; SOLAR-WIND INTERACTION; HYBRID SIMULATIONS; MAGNETOSPHERE; INFLATION; EXPANSION; ASTEROIDS; MODEL; SAIL;
D O I
10.1088/0741-3335/58/11/115002
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
The transient interaction of counter-streaming super-sonic plasma flows in a dipole magnetic dipole is studied in a laboratory experiment. First quasi-stationary flow is produced by theta-pinch and forms a magnetosphere around the magnetic dipole, while laser beams focused at the surface of the dipole cover launch a second explosive plasma expanding outward from the inner dipole region. The laser plasma is energetic enough to disrupt the magnetic field and to sweep through the background plasma for large distances. Probe measurements showed that far from the initially formed magnetosphere laser plasma carries within itself a magnetic field of the same direction but an order of magnitude larger than the vacuum dipole field at considered distances. Because no compression of the magnetic field at the front of the laser plasma was observed, the realised interaction is different from previous experiments and theoretical models of laser plasma expansion into a uniform magnetized background. It was deduced based on the obtained data that, while expanding through the inner magnetosphere, laser plasma picks up a magnetised shell formed by background plasma and carries it for large distances beyond the previously existing magnetosphere.
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页数:10
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