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Hybrid simulations of mini-magnetospheres in the laboratory

L Gargaté1, R Bingham2, R A Fonseca1,3, R Bamford2, A Thornton4, K Gibson4, J Bradford2 and L O Silva1

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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.


PACS

52.72.+v Laboratory studies of space- and astrophysical-plasma processes

94.30.cq MHD waves, plasma waves, and instabilities

94.05.-a Space plasma physics

Subjects

Plasma physics

Environmental and Earth science

Dates

Issue 7 (July 2008)

Received 26 October 2007, in final form 21 January 2008

Published 4 June 2008



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