On the relationship between bursty flows, current disruption and substorms

被引:42
作者
Angelopoulos, V [1 ]
Mozer, FS
Mukai, T
Tsuruda, K
Kokubun, S
Hughes, TJ
机构
[1] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[2] Inst Space & Astronaut Sci, Kanagawa 229, Japan
[3] Nagoya Univ, Solar Terr Environm Lab, Toyokawa 442, Japan
[4] Natl Res Council Canada, Herzberg Inst Astrophys, Ottawa, ON K1A 0R6, Canada
关键词
D O I
10.1029/1999GL900601
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
A current disruption (CD) event was observed by the Geotail spacecraft at (X, Y)(GSM)=(-10.0, 1.9) R-E within 1 min from the onset of a substorm. The event was selected as one of four near-Earth current disruption events identified in a search of three years of Geotail data. Fast ion flows accompanied the magnetic field dipolarization, rendering this event a near-Earth bursty bulk flow (BBF) event. The gradient anisotropy of the 30-44 keV ions at the onset of the flow is consistent with an Earthward motion of the heated plasma and agrees with the direction of Aux and energy transport. The aurora and the associated electrojet moved from low to high latitudes during substorm expansion. Our observations show that CDs and BBFs are qualitatively similar phenomena in the near-Earth tail, both associated with poleward-moving (classical) auroral substorms.
引用
收藏
页码:2841 / 2844
页数:4
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