Fig. 18.

Angular distribution comparisons between MagEIS-A and -B at three different $L$ values (columns) for uncorrected and background-corrected data (rows) during conjunctions. These data are plotted versus local pitch angle for three selected energy channels, one each from LOW, M75, and HIGH. We indicate particles observed moving opposite to the local magnetic field direction with the supplement of their local pitch angles, ${\alpha }_{loc}>{90}^{\circ }$