Linear dispersion curves for KAWs propagating in the Venusian plasma for different values of solar wind electron temperature T_se and propagation angle. We show the effect of the solar wind electron temperature T_se, where T_se = 10 eV (orange), T_se = 15 eV (dashed mint green), T_se= 30 eV (dot-dashed pink). Other plasma parameters: n_O0 = 40 cm⁻³, n_H0 = 16 cm⁻³, n_sp0 = n_se0 = 17 cm⁻³, T_e = 10 eV, θ = 85°, and B₀ = 80 × 10⁻⁵ G. We also show the effect of angle, where θ = 85° (multicolored curves), θ = 80° (magenta curves), θ = 70° (blue curves), and θ = 60° (purple curves). We note that all solid curves are for T_se = 10 eV, dashed curves are for T_se = l5 eV, and dot-dashed curves are for T_se= 30 eV. Moreover, multicolored curves are used for θ = 85° to easily distinguish between the curves, which show only slight changes.