Bandgap imaging in Cu(In, Ga)Se2 photovoltaic modules by electroluminescence. (2nd December 2016)

• Record Type: Journal Article
• Authors: Bokalič, Matevž; Pieters, Bart E.; Gerber, Andreas; Rau, Uwe; Topič, Marko
• Is Part Of: Progress in photovoltaics. Volume 25:Number 2(2017)
• Page Start: 184
• Page End: 191
• Publication Date: 2016-12-02
• Subjects: characterization tools -- bandgaps -- electroluminescence -- photovoltaic devices -- solar cells; Solar cells -- Periodicals; Photovoltaic cells -- Periodicals; Solar power plants -- Periodicals; 621.31245
• DOI: 10.1002/pip.2846
• Languages: English
• ISSNs: 1062-7995

Abstract

Abstract: A unique non‐destructive characterization method for apparent bandgap imaging in photovoltaic (PV) devices based on acquisition of two electroluminescence (EL) images in different spectral ranges is presented. The method consists of a calibration procedure and a bandgap imaging procedure. Calibration has to be performed once per module type and EL imaging setup, and must provide a relation between the bandgap and the ratio between two spectrally independent EL images. After calibration, bandgap imaging only requires acquisition of two spectrally independent EL images followed by image processing, making the method very fast and suitable for in‐line PV module characterization with regard to spatial (in)homogeneity and production process stability. The method is demonstrated on a commercial state‐of‐the‐art Cu(In, Ga)Se2 PV module where apparent bandgap fluctuations between 1.07 and 1.15 eV are detected. Copyright © 2016 John Wiley & Sons, Ltd. Abstract : A non‐destructive bandgap imaging method based on electroluminescence imaging is presented and consists of a calibration and an imaging procedure. The apparent bandgap of the solar cell absorber is calculated from the ratio of two electroluminescence images acquired in different spectral ranges. Bandgap imaging is demonstrated on commercial Cu(In, Ga)Se2 photovoltaic module and reveals bandgap fluctuations between 1.07 and 1.15 eV.