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Simulation study of near-Earth space disturbances: 2. Auroral substorms

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Figure

Fig. 1 The H-component of the magnetic disturbance at 70 MLAT and 48 MLTs. The upper and lower envelops are regarded as AU and ALindices, respectively
Fig. 2 Field-aligned current in the ionosphere (negative upward). The contour line indicates the ionospheric electric potential at an interval of 5kV
Fig. 3 (Top) AU and AL indices and (bottom) field-aligned currents (negative upward) as a function of MLAT and time
Fig. 4 Plasma pressure in thef Y-Z plane at X = − 7.0 Re (left), and in the X-Z plane at Y = − 1.5 Re (right) at a 3.7, b 14.6, c 29.5, d 43.7, e 55.7, and 69.5 min
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