Photovoltaics is the science of converting photons directly into electric current using semiconductor junctions. Every solar cell obeys the Shockley diode equation, and its performance is bounded by the Shockley-Queisser limit of roughly 33.7% for a single junction. Understanding the interplay between the solar spectrum, cell physics, module geometry, and environmental factors is essential for designing efficient solar installations.
These simulations let you decompose sunlight into its spectral components, trace the I-V characteristic curve of a solar cell, optimize module layout for maximum packing density, quantify shading losses from partial obstruction, and measure how rising temperatures erode cell efficiency. Each artifact reveals a different constraint that real-world solar engineers must navigate daily.