Hybrid simulations of mini-magnetospheres in the laboratory

被引:23
作者
Gargate, L. [1 ]
Bingham, R. [2 ]
Fonseca, R. A. [1 ,3 ]
Bamford, R. [2 ]
Thornton, A. [4 ]
Gibson, K. [4 ]
Bradford, J. [2 ]
Silva, L. O. [1 ]
机构
[1] Inst Super Tecn, Inst Plasmas & Fusao Nucl, GoLP, P-1049001 Lisbon, Portugal
[2] Rutherford Appleton Lab, Space Sci & Technol Dept, Sci & Technol Facil Council, Didcot OX11 0QX, Oxon, England
[3] Inst Super Ciencias Trabalho & Empresa, DCTI, P-1649026 Lisbon, Portugal
[4] Univ York, Dept Phys, York YO10 5DD, N Yorkshire, England
关键词
D O I
10.1088/0741-3335/50/7/074017
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
Solar energetic ions are a known hazard to both spacecraft electronics and to manned space flights in interplanetary space missions that extend over a long period of time. A dipole-like magnetic field and a plasma source, forming a mini-magnetosphere, are being tested in the laboratory as means of protection against such hazards. We investigate, via particle-in-cell hybrid simulations, using kinetic ions and fluid electrons, the characteristics of the mini-magnetospheres. Our results, for parameters identical to the experimental conditions, reveal the formation of a mini-magnetosphere, whose features are scanned with respect to the plasma density, the plasma flow velocity and the intensity of the dipole field. Comparisons with a simplified theoretical model reveal a good qualitative agreement and excellent quantitative agreement for higher plasma dynamic pressures and lower B-fields.
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页数:9
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