Skip to content

Topic

Solar Energy

How sunlight becomes electricity, why a panel's output moves with heat, shade and cloud, and how to tell a healthy solar array from one that is failing.

The articles here start from the physics of the photovoltaic cell — light knocking electrons loose in silicon — and follow it outward to the module, the string and the inverter. That chain explains most of what owners actually see: why output falls on a hot, bright afternoon instead of rising, why a shadow over a few cells can drag down a whole string, and why an overcast day still produces power from diffuse light.

There are answers to the practical questions too: which way a panel should face and at what tilt, how monocrystalline, polycrystalline and thin-film cells differ, where maximum power point tracking happens in string, microinverter and optimizer systems, and what separates on-grid, off-grid and hybrid designs. The maintenance and troubleshooting guides cover cleaning without harming glass or coatings, how hail damages a module, and the usual reasons a system produces less than expected.

Everything is explained in engineering terms, with metric and imperial units side by side. There are no product reviews, brand picks or prices — only the mechanisms that stay true whichever panel is on the roof.

Solar Energy

Can Hail Damage Solar Panels?

Module glass survives most hail — but the expensive damage is the kind you cannot see. What the test standard proves, and what to check after a storm.

Updated 8 October 20267 min read