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Earth, Planets and Space
Fig. 7. | Earth, Planets and Space

Fig. 7.

From: Magnetosonic resonances in the magnetospheric plasma

Fig. 7.

Distribution over the radius of the characteristic time τ needed for the asymptotic regime of the magnetospheric convection to set in for different solar wind velocities in the magnetosheath. Curves 1,2, 3 correspond to v0 = 200, 400, 800 km/s for an average amplitude of stochastic FMS oscillations in the magnetosheath .

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