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Investigations of Solar Prominence Dynamics Using Laboratory Simulations
[摘要] Laboratory experiments simulating many of the dynamical features of solar coronal loops have been carried out. These experiments manifest collimation, kinking, jet flows, and S-shapes. Diagnostics include high-speed photography and x-ray detectors. Two loops having opposite or the same magnetic helicity polarities have been merged and it is found that counter-helicity merging provides much greater x-ray emission. A non-MHD particle orbit instability has been discovered whereby ions going in the opposite direction of the current flow direction can be ejected from a magnetic flux tube.
[发布日期] 2008-05-28 [发布机构] 
[效力级别]  [学科分类] 原子、分子光学和等离子物理
[关键词] HELICITY;INSTABILITY;MAGNETIC FLUX;PHOTOGRAPHY;SOLAR PROMINENCES plasma;solar;magnetohydrodynamics [时效性] 
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