The Pierre Auger Observatory, PAO, has been created to detect highly energetic cosmic rays, with a macrogrid of stand-alone photovoltaic systems (PS) as a power source system. The Observatory's grid offers the largest source of statistics for stand-alone PS, 3.10 8 of each principal magnitude per year, creating the possibility of performing unprecedented research in this field. In this article we will describe the experimental setup and analyze the main capabilities of the PS as a source of research.