RELAXATION OF TWISTED MAGNETIC FIELD IN SOLAR FLARE PROMINENCE

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作者
王家龙
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[1] Beijing Observatory
[2] Academia
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<正> The relaxation of a twisted magnetic rope-like prominence ejected by a flare is described in this paper The values of the force-free factor for various periods of during the untwisting process of the event are given. The associated axial current (~1011 A) in the prominence and the rate of the energy release with time are obtained. The estimated induced E. M. F. which might be responsible for the acceleratiion of particles is about 2.8×10~9 V in average.
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页码:1308 / 1316
页数:9
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