Obtained disk scale heights at different Galactocentric radii R. Each point corresponds to a cell in the middle and right panels of Figure 5. The black solid line shows the best-fit exponential model of the Galactic flare, and the transparent orange lines are obtained by drawing random samples from the uncertainties associated with h_z0 and h_fl, as explained in the text. Given that the y-axis is on a logarithmic scale, the exponential form adopted in Equation (10) appears as a linear function.