Comparative analysis of constant initial density vs. constant planetary mass-loss rate (same as Fig. 6). The left panel depicts the scenario in which a uniform initial density (ρ_p) around the planet was maintained across varying degrees of day-night anisotropy, as previously discussed in our analysis. In contrast, the right panel shows the outcome of maintaining a consistent planetary mass-loss rate (ṁ_p) by aligning it with the values of the isotropic case A_100%.