Solar Lattice

Component

Module front glass

ID
comp:module-glass
IRI
https://solarlattice.org/kb/comp/module-glass
Status
active
Also known as
Superstrate, Front glazing, Glass front layer, Module glass

The front glass protects the solar cells from the outside environment while letting as much light as possible through to them. In single-glass modules the front superstrate is 3.2 mm thick. Dual-glass modules use front glass 2.0 or 2.5 mm thick with a back glass behind the cells. Thermally tempered glass has much higher surface compressive stress than the annealed or lightly hardened front glass used on thin-film CdTe modules, so non-tempered glass breaks at lower impact stress. Tempered glass shatters into small fragments, while on non-tempered glass the impact point is easy to find. Glass breakage can come from hail, stones and other impacts, bad clamping, transport, installation stress, mounting structure defects, or thermal stress from hot spots and burn marks. Broken glass often leads to broken hot cells. Glass corrosion or abrasion shows as a hazy, milky or rougher surface with changed colour and transparency. It can make the glass soil more easily, and sandstorms can abrade and weaken it. Dust on the glass lowers its transmittance and array current. Fungal biofilms can stay stuck to the glass after rain until it is cleaned on purpose. Snow left on the module surface blocks irradiance. Patchy snow causes current mismatch between strings and substrings.

Claims

typical_power_loss

c1 verified · fact 5–11 PERCENT

Conditions: Persistent production loss from fungal bio-soiling on module glass at solar farms in humid subtropical U.S. climates (North Carolina field work, 2024), recovered only by manual cleaning

At first this loss was put down to pollen. Later work pointed to sub-aerial biofilms on the glass.

verified by: joshuahamsaverified on: 2026-10-20

Referenced by

Data