Self-excitation of auroral arcs in a three-dimensionally coupled magnetosphere-ionosphere system

Self-excitation of auroral arcs in a three-dimensionally coupled magnetosphere-ionosphere system
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三维耦合磁层-电离层系统中极光弧的自激

DOI:
10.1029/gl015i007p00717
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发表时间:
1988
影响因子:
5.2
通讯作者:
Tetsuya Sato
Tetsuya Sato
中科院分区:
地球科学1区
文献类型:
--
作者:
Kunihiko Watanabe;Tetsuya Sato

文献摘要

被引文献

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This paper presents the first full three-dimensional dynamic simulation of auroral arc formation. The magnetospheric and ionospheric dynamics are represented by one-fluid magnetohydrodynamic equations and two-fluid weakly ionized plasma equations, respectively. The feedback coupling between magnetospheric Alfven waves and ionospheric density waves results in a spontaneous generation of longitudinally elongated striations of field-aligned currents and ionospheric electron densities, which compare very well with many features of quiet auroral arcs.