Image Details
Caption: Figure 7.
Temperatures (eV) for different electron components in each column with a similar format to that of Figure 1 but for other selection criteria. The first row is the same as that in Figure 1, but the next four are, in the following order, low Mach number, high Mach number, quasi-perpendicular, and quasi-parallel shocks. Similar to Figure 1, the total numbers of finite points for each panel are the same for each color-coded line (label in panel (f)). To the far right are the total number of VDFs analyzed for each criterion for reference.
© 2019. The American Astronomical Society.