A mechanism of the auroral substorm expansion onset: electric discharge in the double layer

Yan Song, R. Lysak
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Abstract

Magnetospheric substorms often occur when a significant amount of energy from the solar wind is deposited and stored in the magnetotail during the growth phase and release explosively in the expansion phase, which accelerates charged particles causing the rapid auroral intensification. A physical mechanism is needed to release the energy explosively. The formation of double layers is a likely mechanism for the energy release and the acceleration of particles and triggers the onset of the expansion phase. We suggest that the localized parallel electric field that forms the double layer results from the displacement current complying with Ampere’s law for the dynamic case. The double layers are embedded in low density cavities surrounded by enhanced magnetic stresses. Positive feedback in the electric field generation may cause rapid release of the accumulated energy. The Poynting flux carried by Alfven waves continuously supplies the energy to maintain strong electric fields during the rapid development of auroral substorms.
极光亚暴开始膨胀的机制:双层放电
当太阳风的大量能量在生长阶段沉积并储存在磁尾中,并在膨胀阶段爆炸性地释放出来,从而加速带电粒子导致极光迅速增强时,往往会发生磁层亚暴。爆炸性释放能量需要一种物理机制。双电层的形成很可能是能量释放和粒子加速的机制,并触发膨胀阶段的开始。我们认为,形成双层的局部平行电场是由符合动态情况下安培定律的位移电流产生的。双层嵌入低密度空腔,周围是增强的磁应力。电场产生的正反馈可能导致累积能量的快速释放。在极光亚暴迅速发展的过程中,阿尔芬波所携带的 Poynting 通量不断为维持强电场提供能量。
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