Maximizing photovoltaic (PV) generation requires evaluating how solar geometry and atmospheric extinction translate onto tilted module surfaces. This simulation computes dynamic extraterrestrial normal irradiance (\(G_{0n}\)), solar declination (\(\delta\)), zenith angle (\(\theta_z\)), relative air mass (\(AM\)), horizontal beam and global horizontal irradiance (\(G_b\), \(G_{GHI}\)), and extends the model to quantify direct beam capture on an equator-facing tilted PV surface (\(G_{b,tilted}\)).
The calculation sequence links top-of-atmosphere extraterrestrial formulations to clear-sky ground-level attenuation and surface orientation geometry:
Adjust the site latitude, day of the year, and panel tilt angle to analyze how surface orientation optimizes direct beam capture at solar noon.
The annual profile below tracks top-of-atmosphere horizontal irradiance versus ground-level global horizontal irradiance across all 365 days.
This sensitivity curve demonstrates how varying the module tilt angle affects direct beam collection on the selected day of the year, identifying optimal tilt positioning.