Fig. 8
TIE-GCM simulation results for magnetically quiet equinox conditions (\(\mathit{Kp}=0\)), at 1200 UT, for (left) low solar activity (\(F _{10.7}=72~\mbox{sfu}\)) and (right) high solar activity (\(F_{10.7}=172~\mbox{sfu}\)). (a)–(b) Neutral winds at 110 km. (c)–(d) Hight-integrated Pedersen conductivity. (e)–(f) Electrostatic potential at 300 km. (g)–(h) Equivalent current function at 110 km