Earthquake fault zones have geometrical and material heterogeneities that reflect their past history and can strongly affect future earthquakes and seismic motion generated by the faults (e.g., Ben-Zion, 2008;Stierman, 1984). The Southern San Andreas Fault (SSAF) has not experienced a large earthquake over the past 300 years and is considered to pose a significant seismic hazard (Field et al., 2014). Various studies attempted to derive seismic velocity models for the SSAF (e.g., Ajala et al., 2019;Shaw et al., 2015), but they lack resolution on internal fault zone components such as sharp bimaterial interfaces and damage zones. Imaging these features, as well as properties of the top structure which may be compared with geological information, require dense seismic arrays that cross the fault zone of interest (e.g.,