Properties of current sheet thinning at x ≈-10 to-12RE

被引:44
作者
Artemyev, A. V. [1 ,2 ,3 ]
Angelopoulos, V. [1 ,2 ]
Runov, A. [1 ,2 ]
Petrokovich, A. A. [3 ]
机构
[1] Univ Calif Los Angeles, Dept Earth Planetary & Space Sci, Los Angeles, CA 90095 USA
[2] Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90024 USA
[3] RAS, Space Res Inst, Moscow, Russia
关键词
current sheet; substorm; magnetotail; MAGNETOTAIL CURRENT SHEET; NEAR-EARTH MAGNETOTAIL; PLASMA SHEET; GROWTH-PHASE; EQUILIBRIUM STRUCTURE; GEOMAGNETIC TAIL; PARTICLE MOTION; CLUSTER; CONVECTION; MODEL;
D O I
10.1002/2016JA022779
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 jy=0-1(Bx/z-Bz/x) (GSM coordinates). For 17 events when the spacecraft observed a gradual B-z decrease and j(y) increase, we find the following average scaling relations: for the current density jy approximate to Bz-7/4, for the lobe magnetic field BL approximate to Bz-1/4, and for the plasma density ni approximate to Bz-3/4. We show that the temperature of ions and electrons decreases and the plasma pressure gradient p/x rapidly increases during current sheet thinning. The scale Lx=(lnp/x)-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.
引用
收藏
页码:6718 / 6731
页数:14
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