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Properties of current sheet thinning at x~?10 to ?12 R_E

机译:电流片变薄的属性在x ~ ?12 R_E吗?

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We report on Time History of Events and Macroscale Interactions during Substorms (THEMIS) observations of current sheet thinning in Earth's magnetotail at around x=?10 to ?12 Earth radii. The THEMIS spacecraft configuration in October–December 2015 allows us to construct both gradients that contribute to the cross-tail current density j_y =μ_0~(?1) (σB_x∕σz ? σB_z∕σx) (GSM coordinates). For 17 events when the spacecraft observed a gradual B_z decrease and jy increase, we find the following average scaling relations: for the current density j_y ~ B_1~(?7∕4) , for the lobe magnetic field B_L~ B_z~(?1∕4) , and for the plasma density ni ~ B_z~(?3∕4) . We show that the temperature of ions and electrons decreases and the plasma pressure gradient σp∕σx rapidly increases during current sheet thinning. The scale L_x =(σ ln p∕σx)~(?1) decreases a few thousand kilometers. We also consider current carriers in thinning current sheets: both ion and electron current-dominated current sheets, preferentially located near dusk and midnight, respectively, are found.
机译:我们报告的历史事件和宏观尺度互动,在亚暴(裁判)观察地球的电流片变薄磁尾在x = ?THEMIS计划配置10 - 2015使我们能够构建梯度导致cross-tail电流密度j_y =μ_0 ~(? 1)(σ提出∕σz ?(GSM坐标)。飞船观察逐渐说是减少和司法院的增加,我们发现下面的平均比例电流密度的关系:j_y ~B_1 ~(? 7∕4),叶磁场B_L ~说是~(? 1∕4)和等离子体密度倪~说是~(? 3∕4)。和电子减少和等离子体的压力梯度σp∕σx在电流迅速增加表变薄。减少几千公里。考虑目前运营商在变薄表:离子和电子current-dominated当前表、优先附近的黄昏分别和午夜。

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