In addition to providing detailed observations of solar nonthermal phenomena (eg. flares) at unprecedented angular resolution, scattering measurements towards background sources offer an excellent opportunity to study the structure of turbulence in the solar corona. Previous occultation studies below 100 MHz have been limited to using the Crab as a background source; the SKA instrument would open up many more sources as possible targets and achieve the angular resolution required to properly compliment higher frequency (eg. 330 MHz VLA) studies.