A Novel Approach to Thermal Design of Solar Modules: Selective-Spectral and Radiative Cooling

For commercial solar modules, up to 80% of the incoming sunlight may be dissipated as heat, potentially raising the temperature 20-30°C higher than the ambient. In the long run, extreme self-heating may Erode efficiency and shorten lifetime, thereby, dramatically reducing the total energy output by almost ∼10% Therefore, it is critically important to develop effective and practical cooling methods to combat PV self-heating. In this paper, we explore two fundamental sources of PV self-heating, namely, sub-bandgap absorption and imperfect thermal radiation. The analysis suggests that we redesign the optical and thermal properties of the solar module to eliminate the parasitic absorption (selective-spectral cooling) and enhance the thermal emission to the cold cosmos (radiative cooling). The proposed technique should cool the module by ∼10°C, to be reflected in significant long-term energy gain (∼ 3% to 8% over 25 years) for PV systems under different climatic conditions.