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Sun
Sun
Shielding
charges
Plasmapause
1 1 2
2
1 1 2
2
1
1
Dawn-dusk
electric field
Magnetopause
Steady state
strong convection
with shielded plasmasphere
Transient state
when magnetospheric
electric field decreases
Figure 3.24a A schematic diagram drawn in the equatorial plane showing how a rapid
decrease in magnetospheric convection could create electric field changes inside the
plasmasphere.
So lar win d
J
J
J
E
Plasmasheet
Plasmasheet
E
E
II
I
I
II
Dusk auroral oval
Dawn auroral oval
Polar cap
J
J
E
E
Daytime ionosphere
Region I
.
Region II
J
E
Daytime ionosphere
Region II
.
Region I
J
E
Figure 3.24b Circuit diagram looking from the sun. Polarities of closure currents are
shown for two different cases of field-aligned current imbalance.
display similar oscillations, as illustrated in Fig. 3.25a. These time variations are
too quick for the charges in the Alfvén layer to change and thus seem to be
consistent with the concept of very effective direct electric field penetration into
the plasmasphere. Power spectra of the electric field (from Alaska and Peru)
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