Potential and inductive electric fields in the magnetosphere during auroras |
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| Authors: | Walter J Heikkila RJ Pellinen C-G Fälthammar LP Block |
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| Institution: | 1. Center for Space Sciences, The University of Texas at Dallas, Box 688, Richardson, TX 75080, U.S.A.;2. Division of Geomagnetism, Finnish Meteorological Institute, Postbox 503 SF-00101, Helsinki 10, Finland;3. Royal Institute of Technology, Dept. of Plasma Physics S-10044, Stockholm 70, Sweden |
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| Abstract: | During quiescent auroras the large-scale electric field is essentially irrotational. The volume formed by the plasma sheet and its extension into the auroral oval is connected to an external source by electric currents, which enter and leave the volume at different electric potentials and which supply sufficient energy to support the auroral activity. The location of the actual acceleration of particles depends on the internal distribution of electric fields and currents. One important feature is the energization of the carriers of the cross-tail current and another is the acceleration of electrons precipitated through relatively low-altitude magnetic-field-aligned potential drops.Substorm auroras depend on rapid and (especially initially) localized release of energy that can only be supplied by tapping stored magnetic energy. The energy is transmitted to the charged particle via electric inductive fields.The primary electric field due to changing electric currents is redistributed in a complicated way—but never extinguished—by polarization of charges. As a consequence, any tendency of the plasma to suppress magnetic-field-aligned components of the electric fields leads to a corresponding enhancement of the transverse component. |
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