Figure 5.

The angular scattering functions for the South/Pole/Aitken Basin magnetic anomaly for different cuts in solar zenith angle. (a, d, and g) The number of observations per bin. (b, e, and h) The two-dimensional scattering function; (c, f, and i) the reduced, one-dimensional angular scattering function as a function of the azimuthal angle. The red dashed line in Figures 5f and 5i show the empirical fit, as discussed in the text.