Equatorward shift of the cleft during magnetospheric substorms as observed by Isis 1

作者: F. Yasuhara , S.-I Akasofu , J. D. Winningham , W. J. Heikkila

DOI: 10.1029/JA078I031P07286

关键词: Electron precipitationSubstormSolar windPhysicsEclipticDipole model of the Earth's magnetic fieldGeophysicsLatitudeMagnetic dipGeomagnetic storm

摘要: Isis 1 satellite observations of the cleft position during magnetospheric substorms show that shifts equatorward as interplanetary B sub z component turns southward and substorm activity increases it back toward higher latitudes subsides returns northward. Also, unusually low for (less than 70 deg invariant latitude) were found geomagnetic storms with significant Dst values large negative values. Significant occur in location no accompanying effect seen AE index; however, is observed to be these periods.

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