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Impact of angular irradiance distributions on coupling gains and energy yield of cell interconnection designs in silicon solar modules in tracking and fixed systems

dc.contributor.authorHaedrich, Ingrid
dc.contributor.authorErnst, Marco
dc.date.accessioned2023-12-07T00:48:32Z
dc.date.issued2021
dc.date.updated2022-09-04T08:16:41Z
dc.description.abstractCell interconnector designs such as light redirecting films (LRFs) and various geometric ribbon layouts are all aimed at improving the performance of crystalline silicon solar modules. However, due to the usually specular reflecting surface, the angular-dependent module performance, which is typically quantified with an incidence angle modifier, depends on the rotation of the module. We find that typical power measurements under standard test conditions at 1000 W m-2 and 25 °C cell temperature are not suited to identify the best performing design in real-world conditions. In this work, we therefore determine the optimum ribbon geometry based on its simulated energy yield in common installation configurations for solar modules based on industry-standard full and half-cut solar cells. We compare the effects of planar, triangular, LRFs, pentagonal and wire ribbon geometries, as well as fixed optimal inclination, building-integrated (facade), and single-axis tracking installation scenarios of modules in portrait and landscape orientation. Energy yield gains of 1.8% can be achieved for full cell modules with LRFs or pentagonal ribbons in single-axis tracking installation compared to a reference module with five planar ribbons. Critically, we find that changing the module orientation to landscape reduces this energy yield gain by nearly 50% for the modules with LRFs. This directional dependence is significantly reduced with the pentagonal ribbon structure. The installation scenario can have a similarly dramatic impact. The expectation of power gains for certain designs inferred from standard test conditions may not only show significantly lower gains in annual energy yield, but may even lead to yield losses, especially for building-integrated photovoltaic systems. For a typical full-cell module, for example, we have found that LRFs perform 2.5% better than standard planar ribbons under standard test conditions but can result in a 0.2% lower annual yield in a facade installation. Therefore, to fully evaluate the effectiveness of a specific ribbon design, the annual energy yield must consider the angular irradiance distribution and weather conditions at a specific location, the installation scenario, and the module orientation.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0022-3727en_AU
dc.identifier.urihttp://hdl.handle.net/1885/307715
dc.language.isoen_AUen_AU
dc.publisherInstitute of Physics Publishingen_AU
dc.rights© 2021 IOP Publishing Ltden_AU
dc.sourceJournal of Physics D: Applied Physicsen_AU
dc.subjectsolar modulesen_AU
dc.subjectinterconnectoren_AU
dc.subjectmetallisationen_AU
dc.subjectyield predictionen_AU
dc.subjectcell to moduleen_AU
dc.titleImpact of angular irradiance distributions on coupling gains and energy yield of cell interconnection designs in silicon solar modules in tracking and fixed systemsen_AU
dc.typeJournal articleen_AU
local.bibliographicCitation.issue22en_AU
local.bibliographicCitation.lastpage15en_AU
local.bibliographicCitation.startpage1en_AU
local.contributor.affiliationHaedrich, Ingrid, College of Engineering and Computer Science, ANUen_AU
local.contributor.affiliationErnst, Marco, College of Engineering and Computer Science, ANUen_AU
local.contributor.authoruidHaedrich, Ingrid, u5712688en_AU
local.contributor.authoruidErnst, Marco, u5457130en_AU
local.description.embargo2099-12-31
local.description.notesImported from ARIESen_AU
local.identifier.absfor400800 - Electrical engineeringen_AU
local.identifier.ariespublicationa383154xPUB18447en_AU
local.identifier.citationvolume54en_AU
local.identifier.doi10.1088/1361-6463/abe967en_AU
local.identifier.scopusID2-s2.0-85103107082
local.identifier.thomsonIDWOS:000627736400001
local.publisher.urlhttps://iopscience.iop.org/en_AU
local.type.statusPublished Versionen_AU

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