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Ionospheric control of the magnetosphere: conductance

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Academic year: 2021

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Figure

Fig. 1. (a) The maximum field-aligned current into the ionosphere and (b) the cross polar cap potential versus the Pedersen conductance
Fig. 2. A plot of the Pedersen conductance as a function of solar zenith angle. This shows the solar driven conductance, a scattering term which causes the conductance to be smoother across the  ter-minator, and a nightside constant conductance

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