Calibrating spectrometers for measurements of the spectral irradiance caused by solar radiation

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dc.identifier.uri http://dx.doi.org/10.15488/12681
dc.identifier.uri https://www.repo.uni-hannover.de/handle/123456789/12781
dc.contributor.author Schinke, Carsten
dc.contributor.author Pollex, Hendrik
dc.contributor.author Hinken, David
dc.contributor.author Wolf, Martin
dc.contributor.author Bothe, Karsten
dc.contributor.author Kröger, Ingo
dc.contributor.author Nevas, Saulius
dc.contributor.author Winter, Stefan
dc.date.accessioned 2022-08-24T11:37:57Z
dc.date.available 2022-08-24T11:37:57Z
dc.date.issued 2020
dc.identifier.citation Schinke, C.; Pollex, H.; Hinken, D.; Wolf, M.; Bothe, K. et al.: Calibrating spectrometers for measurements of the spectral irradiance caused by solar radiation. In: Metrologia 57 (2020), Nr. 6, 065027. DOI: https://doi.org/10.1088/1681-7575/abafc5
dc.description.abstract Measuring the spectral irradiance of solar radiation is required in many fields of science and technology. In this work, we present an in-depth discussion of the measuring procedure and required corrections for such measurements. We also describe our measurement uncertainty analysis, which is based on a Monte-Carlo procedure in accordance with the Guide to the expression of uncertainty in measurement (JCGM, Paris, 2008). For this purpose, fifteen uncertainty sources are identified, analyzed and described analytically. As a specific application example, we describe the instrumentation and procedure for determining the spectral irradiance of a solar simulator at the ISO/IEC 17 025 accredited solar cell calibration laboratory ISFH CalTeC and the corresponding measurement uncertainty analysis. Moreover, we provide a Python implementation for this calculation along with the paper. We show that for state-of-the-art instrumentation, significant uncertainty contributions arise from the reference lamp (primary calibration standard), stray light and signal-to-noise ratio. If sharp spectral features are present (which is common, e.g. for Xenon lamps), spectral bandwidth and wavelength uncertainty also contribute significantly to the overall uncertainty. © 2020 BIPM & IOP Publishing Ltd eng
dc.language.iso eng
dc.publisher Sèvres : Bureau International des Poids et Mesures
dc.relation.ispartofseries Metrologia 57 (2020), Nr. 6
dc.rights CC BY 4.0 Unported
dc.rights.uri https://creativecommons.org/licenses/by/4.0/
dc.subject Calibration eng
dc.subject Measurement uncertainty analysis eng
dc.subject Solar radiation eng
dc.subject Solar simulator eng
dc.subject Spectral irradiance eng
dc.subject Spectrometer eng
dc.subject Spectroradiometer eng
dc.subject Calibration eng
dc.subject Electric lamps eng
dc.subject Signal to noise ratio eng
dc.subject Solar cells eng
dc.subject Solar radiation eng
dc.subject Stray light eng
dc.subject Application examples eng
dc.subject Calibration laboratories eng
dc.subject Calibration standard eng
dc.subject Guide to the expression of uncertainty in measurements eng
dc.subject Measurement uncertainty analysis eng
dc.subject Monte Carlo procedures eng
dc.subject Science and Technology eng
dc.subject Uncertainty contributions eng
dc.subject Uncertainty analysis eng
dc.subject.ddc 600 | Technik ger
dc.title Calibrating spectrometers for measurements of the spectral irradiance caused by solar radiation
dc.type Article
dc.type Text
dc.relation.essn 1681-7575
dc.relation.doi https://doi.org/10.1088/1681-7575/abafc5
dc.bibliographicCitation.issue 6
dc.bibliographicCitation.volume 57
dc.bibliographicCitation.firstPage 065027
dc.description.version publishedVersion
tib.accessRights frei zug�nglich


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