  We characterize the performance of a fixed grid of solar panels on the basis
of data taken under clear sky conditions over 12 months. We confirm that the
power output is linearly proportional to cos(theta), where theta is the angular
difference of direction toward the Sun and the vector perpendicular to the
panels. In order to confirm this we applied methods from astronomical
photometry reduction. From late March through August we find that the median
effective atmospheric extinction term is 0.145 mag/airmass. From October to
mid-March the median extinction term is 0.081 mag/airmass. The proportionality
"constant" scaling cos(theta) appears to be seasonally dependent, with the
smallest scaling factors occurring when the extinction term is largest.
Finally, we find that extinction-corrected power often underperforms the linear
relationship late in the morning or early in the afternoon. This is most likely
because the efficiency of solar panels depends on their operating temperature,
and the panel temperature increases over the course of time on a sunny day.
