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A tuning routine to correct systematic influences in reference PV systems' power outputs

dc.contributor.authorKillinger, Sven
dc.contributor.authorBright, James
dc.contributor.authorLingfors, D.
dc.contributor.authorEngerer, Nicholas
dc.date.accessioned2020-12-20T20:51:34Z
dc.date.available2020-12-20T20:51:34Z
dc.date.issued2017
dc.date.updated2020-11-23T10:08:56Z
dc.description.abstractPower output measurements from PV systems are subject to a wide variety of systematic external and internal influences, such as shading, soiling, degradation, module and inverter quality issues and other system-level losses. All of these influences upon PV power measurements make the use of PV power output datasets for higher-level analysis problematic, particularly in their use as reference PV systems for estimating the power of a regional portfolio. To address these issues, we present a three-step method. Firstly, a parameterisation and quality control of power measurements is performed, which also corrects for consistent inefficiencies by a loss factor LF. Secondly, the detection of systematic de-ratings affecting PV system power output differently for each time step of the day (predominantly due to shading) together with the implementation of a subsequent “re-rating” of the power output measurements in a process referred to as tuning. The pivotal element of this approach is a 30-day running 90th percentile of the clear-sky index for photovoltaics kpv and the computation of a daily de-rating profile. Lastly, high kpv related variance in the early morning and evening is detected and filtered. Whilst these three methods are independent of each other, we suggest applying them in combination following the same order as in our paper. Cross-validations of these methods demonstrate significant improvements to the PV power measurement profiles, particularly in their use as reference PV systems for upscaling approaches. The RMSE falls from 0.174 to 0.09 W/Wp, rRMSE from 46.5% to 21.9%, MAPE from 47.9% to 20.8% and the correlation r increases from 0.767 to 0.919. Hence, we report overall improvements to RMSE, rRMSE, MAPE and r by 48%, 53%, 57% and 20%, respectively.
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0038-092X
dc.identifier.urihttp://hdl.handle.net/1885/217818
dc.language.isoen_AUen_AU
dc.publisherPergamon-Elsevier Ltd
dc.sourceSolar Energy
dc.titleA tuning routine to correct systematic influences in reference PV systems' power outputs
dc.typeJournal article
local.bibliographicCitation.lastpage1094
local.bibliographicCitation.startpage1082
local.contributor.affiliationKillinger, Sven, College of Science, ANU
local.contributor.affiliationBright, James, College of Science, ANU
local.contributor.affiliationLingfors, D., Uppsala University
local.contributor.affiliationEngerer, Nicholas, College of Science, ANU
local.contributor.authoruidKillinger, Sven, u1019708
local.contributor.authoruidBright, James, u1043569
local.contributor.authoruidEngerer, Nicholas, u4985661
local.description.notesImported from ARIES
local.identifier.absfor040103 - Atmospheric Radiation
local.identifier.absseo850504 - Solar-Photovoltaic Energy
local.identifier.ariespublicationu4351680xPUB162
local.identifier.citationvolume157
local.identifier.doi10.1016/j.solener.2017.09.001
local.identifier.scopusID2-s2.0-85029617356
local.type.statusPublished Version

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