Near-Earth Reconnection Contributing to Recovery Phase of Geomagnetic Storm

被引:0
|
作者
Liu, Terry Z. [1 ]
Angelopoulos, Vassilis [1 ]
Nishimura, Yukitoshi [2 ,3 ]
Shen, Yangyang [1 ]
Shi, Xueling [4 ,5 ]
Hartinger, Michael D. [1 ,6 ]
机构
[1] Univ Calif Los Angeles, Dept Earth Planetary & Space Sci, Los Angeles, CA 90095 USA
[2] Boston Univ, Dept Elect & Comp Engn, Boston, MA USA
[3] Boston Univ, Ctr Space Phys, Boston, MA USA
[4] Virginia Tech, Dept Elect & Comp Engn, Blacksburg, VA USA
[5] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO USA
[6] Space Sci Inst, Boulder, CO USA
基金
美国国家航空航天局; 加拿大创新基金会;
关键词
geomagnetic storm; magnetotail reconnection; dipolarizing flux bundles; plasma injections; ring current; current wedges; INNER MAGNETOSPHERE;
D O I
10.1029/2024GL112730
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Recent observations show very near-Earth reconnection (similar to 8-13RE) could efficiently power the ring current during the main phase of geomagnetic storms, but whether the recovery phase might be contributed remains unclear. During the recovery phase of the May 2024 major geomagnetic storm, intense auroral brightening and geomagnetic disturbances were observed at midnight, indicative of particle injections. Current wedges observed by mid-latitude ground magnetometers around midnight suggest dipolarizing flux bundles (DFBs). The latitude of the auroral brightening was clearly lower than usual, suggesting near-Earth reconnection (NERX) was closer to Earth than during substorms (similar to 20-30RE). GOES-18 at midnight detected magnetic field and plasma signatures consistent with DFBs, following an extremely thin current sheet likely compressed by strong upstream dynamic pressure. These results indicate NERX could have been close enough for resultant DFBs to penetrate geosynchronous orbit and contribute to the ring current during the recovery phase. This scenario deserves further examination in future.
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页数:7
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