Investigation of a substorm following an extended interval of northward interplanetary magnetic field

被引：0

作者：

Lui, ATY ^{[1
]}

Williams, DJ ^{[1
]}

McEntire, RW ^{[1
]}

Ohtani, S ^{[1
]}

Zanetti, LJ ^{[1
]}

Bristow, WA ^{[1
]}

Greenwald, RA ^{[1
]}

Newell, PT ^{[1
]}

Christon, SP ^{[1
]}

Mukai, T ^{[1
]}

Tsuruda, K ^{[1
]}

Yamamoto, T ^{[1
]}

Kokubun, S ^{[1
]}

Matsumoto, H ^{[1
]}

Kojima, H ^{[1
]}

Murata, T ^{[1
]}

Fairfield, DH ^{[1
]}

Lepping, RP ^{[1
]}

Samson, JC ^{[1
]}

Rostoker, G ^{[1
]}

Reeves, GD ^{[1
]}

机构：

[1] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA

来源：

MAGNETOSPHERIC RESEARCH WITH ADVANCED TECHNIQUES | 1998年 / 9卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Strong northward interplanetary magnetic field was observed for an extended period by the Wind spacecraft at an upstream distance of similar to 200 R-E from February 8-10, 1995. Within this period was a brief break of southward IMF on February 9 which led to a substorm of moderate intensity (500 nT) with its expansion onset at similar to 0431 UT. In this paper, this substorm is examined with data from eleven spacecraft in space and two networks of ground stations covering both the northern and southern hemispheres. Detailed analysis of this event shows (1) an unusually long duration of the magnetospheric reconfiguration prior to expansion onset for this isolated substorm (2) new evidence for multiple particle acceleration sites during substorm expansion, and (3) indications for sunward plasma flow in the plasma sheet during the late expansion phase of a substorm not related to a single acceleration site (e.g., an X-line) moving from the near-Earth tail to the more distant tail.

引用

页码：9 / 16

页数：8