Fig. 3From: Effects of the interplanetary magnetic field y component on the dayside auroraAveraged electron energy flux (in erg/cm2-s) deposited into the dark (solar zenith angle: SZA > 108°) a Northern Hemisphere (NH) and the dark b Southern Hemisphere (SH) for positive IMF By (> 2 nT). c, d Are in the same format as (a) and (b) but for negative IMF By (< − 2 nT)Back to article page