Before revision: DP1-Current Interaction between solar wind plasma and the polar geomagnetic field produces a global-scale magnetospheric electric convection field directed from dawn to dusk with a potential difference of about 15 kV during quiet magnetospheric conditions, increading substantially during disturbed conditions.
After revision: DP1-Current Interaction between solar wind plasma and the polar geomagnetic field produces a global-scale magnetospheric electric convection field directed from dawn to dusk with a potential difference of about 15 kV during quiet magnetospheric conditions, increasing substantially during disturbed conditions.