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Item type:Publication, The advantages of ga-graded obtained by growth profile modification and Na incorporation on Cu(In,Ga)Se2 solar cells(2014-01-01) ;Sakdanuphab, Rachsak ;Chatraphorn, SojiphongYoodee, KajornyodCu(In,Ga)Se<inf>2</inf> (CIGS) compound is a p-type semiconductor that has been used as light absorber layer in high efficiency thin film solar cell. The CIGS compound can be adjusted the band gap energy by varying the ratio of [Ga]/([In] +[Ga]) ratio (x). From theoretical and simulation, it was found that band gap grading in CIGS thin films showed the advantages to increase the efficiency of solar cells. Generally, the band gap grading can be done by the growth of non homogeneous x-ratio in depth of CIGS thin films. In this work, we develop two approaches to create band gap grading in CIGS thin films; (1) modifying the growth profile and (2) using Na incorporation in the growth process. The effects of Ga-graded would be revealed and compared with homogeneous CIGS thin films. CIGS thin films were grown on soda-lime glass and Al<inf>2</inf>O<inf>3</inf> coated soda-lime glass substrates by molecular beam deposition method. The growth process was based on 2-stage and 3-stage growth profiles. The as grown films were characterized for their structural property, chemical composition and optical transmission as well as solar cell performance. The Auger electron spectroscopy in depth profiles revealed the variation of x- ratio increasing from the surface toward the back contact in CIGS films with our modified growth profile and Na incorporation. This result indicated Ga-graded in CIGS thin films. The structural property of Gagraded CIGS films showed the (112) preferred orientation of the chalcopyrite structure with a broad asymmetric spectrum related to the inhomogeneous structure. The optical transmission measurements of the Ga-graded CIGS film showed the broad transition near the absorption edge indicating the effect of the band gap grading as a result of the variation in depth of the Ga-content. From I-V measurements, the solar cell efficiencies significantly increase due to the advantages of Ga-graded constitute. © (2014) Trans Tech Publications, Switzerland. - Some of the metrics are blocked by yourconsent settings
Item type:Publication, Development of thin film a-SiO:H/a-Si:H double-junction solar cells and their temperature dependence(2013-11-01) ;Sriprapha, Kobsak ;Hongsingthong, Aswin ;Krajangsang, Taweewat ;Inthisang, SorapongJaroensathainchok, SuttinanHydrogenated amorphous silicon oxide (a-SiO:H)/hydrogenated amorphous silicon (a-Si:H) double-junction solar cells with a high open-circuit voltage (V<inf>oc</inf>) and a low temperature coefficient (TC) were developed using a wide bandgap a-SiO:H film as the intrinsic (i) layer of the top cell. It was found that with an increasing carbon dioxide (CO<inf>2</inf>)/silane (SiH <inf>4</inf>) ratio, the optical bandgap (E<inf>opt</inf>) of the a-SiO:H films increased remarkably while the photogain tended to decrease. By employing an optimized a-SiO:H film as the i top layer of the a-SiO:H/a-Si:H solar cell, an initial conversion efficiency (η) of 10.2% was obtained. This solar cell showed a higher η than the conventional a-Si:H/a-Si:H structure, a result of incremental improvements in the V<inf>oc</inf> and short-circuit current density (J<inf>sc</inf>), which were attributed to the wider bandgap of the intrinsic top layer. It was found that the TC for η of the a-SiO:H/a-Si:H solar cell was -0.10%/°C, slightly lower than that of the a-Si:H/a-Si:H solar cell, whose TC value is about -0.15%/°C. The light-induced degradation (LID) ratio for η of the a-SiO:H/a-Si:H solar cell was approximately 19%, which was 2% lower than that of the a-Si:H/a-Si:H solar cell. These results have demonstrated the great potential of the i-a-SiO:H films as absorber layers of top cells in multi-junction silicon-based thin-film solar cells. The a-SiO:H/a-Si:H solar cells with low TCs and low LID ratios are attractive for their potential use in high-temperature environments or tropical regions. © 2013 Elsevier B.V.
