Electron-Only Tail Current Sheets and Their Temporal Evolution

被引:17
|
作者
Hubbert, M. [1 ]
Qi, Y. [1 ]
Russell, C. T. [1 ]
Burch, J. L. [2 ]
Giles, B. L. [3 ]
Moore, T. E. [3 ]
机构
[1] Univ Calif Los Angeles, Earth Planetary & Space Sci, Los Angeles, CA 90095 USA
[2] Southwest Res Inst, San Antonio, TX USA
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
关键词
current sheet; magnetic reconnection; magnetotail; MAGNETIC RECONNECTION; DIFFUSION REGION; MAGNETOTAIL; FIELD;
D O I
10.1029/2020GL091364
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The Earth's magnetotail contains a current sheet separating the anti-Sunward field of the southern lobe from the sunward-pointing northern lobe. Herein, we report tail current sheets that are supported only by electron currents. We examine one electron-only current sheet in detail and briefly discuss 10 others. Three current sheets are interpreted in terms of the time-evolution of reconnection onset. These current sheets show evidence of parallel electron heating, perpendicular ion heating, and current sheet expansion. These features are consistent with electron and ion behavior during traditional "electron-ion" reconnection. Ground-based and in-situ data show that electron-ion reconnection occurs shortly after each "pre-ion reconnection" electron-only reconnection event. This suggests that electron-only reconnection can act as a precursor to electron-ion reconnection. We note that five events occur shortly after a period of electron-ion reconnection, which suggests that electron-only reconnection is more than merely a precursor to ion reconnection.
引用
收藏
页数:10
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