THE MAGNETOPAUSE AND BOUNDARY-LAYER FOR SMALL MAGNETIC SHEAR - CONVECTION ELECTRIC-FIELDS AND RECONNECTION

被引:58
作者
PASCHMANN, G
SONNERUP, B
PAPAMASTORAKIS, I
BAUMJOHANN, W
SCKOPKE, N
LUHR, H
机构
[1] DARTMOUTH COLL,THAYER SCH ENGN,HANOVER,NH 03755
[2] TECH UNIV BRAUNSCHWEIG,INST GEOPHYS & METEOROL,W-3300 BRAUNSCHWEIG,GERMANY
[3] RES CTR CRETE,HERAKLION,GREECE
[4] UNIV CRETE,DEPT PHYS,HERAKLION,GREECE
关键词
D O I
10.1029/GL017i011p01829
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Convection electric fields, Ec = −Vp×B, measured during a magnetopause/boundary layer encounter at low latitude by the AMPTE/IRM spacecraft, are shown to yield an accurate determination of the magnetopause normal vector, N, even though the magnetic shear across the magnetopause was small. The average plasma velocity along N is used to deduce a boundary layer thickness of about 1.3 RE. Analysis of Ec in the magnetopause itself reveals the existence of a deHoffmann‐Teller frame in which the flow is nearly field aligned and approximately Alfvénic, indicating that the magnetopause was a rotational discontinuity; this is interpreted as a signature that magnetic‐field reconnection was occurring somewhere on the magnetopause. Copyright 1990 by the American Geophysical Union.
引用
收藏
页码:1829 / 1832
页数:4
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