Scatter plot of the representative heights of the EOVSA microwave source (estimated by intersecting the EOVSA lines of sight with the plane defined by the Sun’s rotation axis and the geometric center of the SXR source; see Fig. 3) versus the corresponding mean magnetic field strengths. Vertical and horizontal bars indicate uncertainties in height and magnetic field strength, respectively. The green and orange lines show empirical magnetic field height profiles from Fedenev et al. (2023) overplotted for reference. The correspondence indicates that our reconstructed magnetic field values are physically plausible and lie within the expected range for active region loops.