For an optimized cell performance of solar modules the width and distance between scribe lines is crucial. Whereas a too thin scribe line might lead to short or bridge circuits a distance deviation can, in the worst case, lead to crossing of the lines
Based on a high resolution matrix camera the Dr. Schenk Microscope Station for inspecting solar scribes has been developed as measurement solution with focus on this challenge. It is therefore the perfect enhancement to a surface inspection system.
The Microscope Station for solar scribe analysis enables timely reaction on deviations of the solar scribing process and by this helps to increase yield and optimize the production of solar panels.