IMF By and seasonal dependence of the electric field in the inner magnetosphere

Details IMF By and seasonal dependence of the electric field in the inner magnetosphere IMF By and seasonal dependence of the electric field in the inner magnetosphere

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsm43a1148m&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #SM43A-1148

Physics

2712 Electric Fields (2411), 2730 Magnetosphere: Inner, 2736 Magnetosphere/Ionosphere Interactions, 2784 Solar Wind/Magnetosphere Interactions

Scientific paper

It is known that the electric field pattern at high-latitudes depends on the polarity of the Y component of the interplanetary magnetic field (IMF By) and season. In this study we investigate the above relationships in the inner magnetosphere by using the perigee data from Cluster passing through the magnetic equator. The data consist of both components of the electric field perpendicular to the magnetic field obtained by the electron drift instrument (EDI). These data are sorted by polarities of IMF By and Bz and by seasons or hemispheres. The possible causes of the dependence of the electric fields on IMF By and seasons are discussed.

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