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Les indices de limite aurorale calcules par Gussenhoven et al. (1983) a partir des donnees sur les precipitations d'electrons ont ete utilises pour etudier la reponse de l'ovale auroral du secteur de minuit aux variations de Bz. Les resultats peuvent etre interpretes en termes de reconnexion preferentielle du cote aube de la magnetosphere

Influence of the transverse component of the interplanetary magnetic field on the size of the auroral oval.