NEAR-EARTH SUBSTORM ONSET - A COORDINATED STUDY

被引:17
|
作者
PERSSON, MAL
OPGENOORTH, HJ
PULKKINEN, TI
ERIKSSON, AI
DOVNER, PO
REEVES, GD
BELIAN, RD
ANDRE, M
BLOMBERG, LG
ERLANDSON, RE
BOEHM, MH
AIKIO, AT
HAGGSTROM, I
机构
[1] FINNISH METEOROL INST,SF-00101 HELSINKI,FINLAND
[2] SWEDISH INST SPACE PHYS,UMEA DIV,S-90187 UMEA,SWEDEN
[3] JOHNS HOPKINS UNIV,APPL PHYS LAB,LAUREL,MD 20723
[4] MAX PLANCK INST EXTRATERR PHYS,W-8046 GARCHING,GERMANY
[5] UNIV OULU,DEPT PHYS,SF-90570 OULU,FINLAND
[6] SWEDISH INST SPACE PHYS,S-98128 KIRUNA,SWEDEN
[7] LOS ALAMOS NATL LAB,DIV SPACE SCI & TECHNOL,LOS ALAMOS,NM 87545
[8] ROYAL INST TECHNOL,ALFVEN LAB,S-10044 STOCKHOLM 70,SWEDEN
关键词
D O I
10.1029/94GL01426
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We present simultaneous satellite and ground-based measurements of a substorm. Throughout the initial substorm expansion, southward drifting arcs are observed poleward of the expanding substorm aurora, indicating two independent systems of particle precipitation. Freja passes the brightening onset arc in the topside ionosphere near the moment of the substorm onset, observing an Alfven wave, field aligned current and oxygen ion outflow. The substorm onset occurs at low magnetospheric L-shells, near the poleward edge of the region of trapped particles. The location and time for the substorm injection are confirmed by geostationary spacecraft together with magnetometers, all-sky cameras and radar on the ground. We believe that the substorm onset may be triggered by modification of the oxygen content of the inner magnetosphere during the growth-phase caused by ionospheric ion outflow.
引用
收藏
页码:1875 / 1878
页数:4
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