“…It becomes a “relative”
residual when normalized by the background
profile (red in Figure 1a). The unsigned magnitude of the (inherently bipolar) “relative”
residuals, the result of which is shown in Figure 1b, is considered to represent “ionospheric disturbance strength” at Mars, as has been commonly accepted in terrestrial ionospheric studies (e.g., Huang et al.,
2014; Song et al.,
2023) and in Gurnett et al. (
2010, Section 5) for Mars.…”