Investigation of degradation in solar cells from different mc-Si materials

dc.contributor.authorJunge, Johannes
dc.contributor.authorHerguth, Axel
dc.contributor.authorHahn, Giso
dc.contributor.authorKreßner-Kiel, Denisedeu
dc.contributor.authorZierer, Robertdeu
dc.date.accessioned2011-09-29T07:27:59Zdeu
dc.date.available2011-09-29T07:27:59Zdeu
dc.date.issued2011
dc.description.abstractThe impact of light induced degradation on small lab-type 2x2 cm² solar cells made from standard p-type mc-Si material is compared to the degradation of lowly compensated UMG material on the one hand and intentionally Fe and Fe/Cu contaminated material (several ppma of Fe or Fe and Cu are introduced into the melt of electronic grade feedstock before ingot casting) on the other hand. The material is taken from three different ingot heights (bottom, middle and top), respectively. All cells are annealed at 200 °C in the dark for several minutes before they are exposed to one sun illumination and the development of the electrical parameters over time is determined. The reference and UMG material behave as expected and show a degradation which is correlated to the boron and interstitial oxygen concentration over the ingot height and therefore can be attributed to B-O related defects. The intentionally Fe and Cu contaminated samples in contrast show a degradation behavior that is more probably correlated to the distribution of the Fe and Cu contamination, as the absolute degradation towards the top of the ingot is higher for highly contaminated material (20 ppma Fe) than in the reference material and the observed time constants for degradation are different. Fe/Cu contaminated material exhibits too low cell performance in the top and bottom part of the ingot to show any significant degradation effects. The lowly contaminated material (2 ppma Fe) behaves like the reference material as long as the wafer material does not contain additional contaminants originating from the crucible walls. Material from near the crucible wall by contrast shows a stronger light induced degradation.eng
dc.description.versionpublished
dc.identifier.citationPubl. in: Energy Procedia ; 8 (2011). - pp. 52-57deu
dc.identifier.doi10.1016/j.egypro.2011.06.101deu
dc.identifier.ppn451450019
dc.identifier.urihttp://kops.uni-konstanz.de/handle/123456789/15921
dc.language.isoengdeu
dc.legacy.dateIssued2011-09-29deu
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Unported
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/
dc.subjectmc-Sideu
dc.subjectdegradationdeu
dc.subject.ddc530deu
dc.titleInvestigation of degradation in solar cells from different mc-Si materialseng
dc.typeJOURNAL_ARTICLE
dspace.entity.typePublication
kops.citation.bibtex
@article{Junge2011Inves-15921,
  year={2011},
  doi={10.1016/j.egypro.2011.06.101},
  title={Investigation of degradation in solar cells from different mc-Si materials},
  volume={8},
  issn={1876-6102},
  journal={Energy Procedia},
  pages={52--57},
  author={Junge, Johannes and Herguth, Axel and Hahn, Giso and Kreßner-Kiel, Denise and Zierer, Robert}
}
kops.citation.iso690JUNGE, Johannes, Axel HERGUTH, Giso HAHN, Denise KRESSNER-KIEL, Robert ZIERER, 2011. Investigation of degradation in solar cells from different mc-Si materials. In: Energy Procedia. 2011, 8, pp. 52-57. ISSN 1876-6102. Available under: doi: 10.1016/j.egypro.2011.06.101deu
kops.citation.iso690JUNGE, Johannes, Axel HERGUTH, Giso HAHN, Denise KRESSNER-KIEL, Robert ZIERER, 2011. Investigation of degradation in solar cells from different mc-Si materials. In: Energy Procedia. 2011, 8, pp. 52-57. ISSN 1876-6102. Available under: doi: 10.1016/j.egypro.2011.06.101eng
kops.citation.rdf
<rdf:RDF
    xmlns:dcterms="http://purl.org/dc/terms/"
    xmlns:dc="http://purl.org/dc/elements/1.1/"
    xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#"
    xmlns:bibo="http://purl.org/ontology/bibo/"
    xmlns:dspace="http://digital-repositories.org/ontologies/dspace/0.1.0#"
    xmlns:foaf="http://xmlns.com/foaf/0.1/"
    xmlns:void="http://rdfs.org/ns/void#"
    xmlns:xsd="http://www.w3.org/2001/XMLSchema#" > 
  <rdf:Description rdf:about="https://kops.uni-konstanz.de/server/rdf/resource/123456789/15921">
    <dc:contributor>Zierer, Robert</dc:contributor>
    <dc:contributor>Herguth, Axel</dc:contributor>
    <dc:contributor>Kreßner-Kiel, Denise</dc:contributor>
    <dspace:isPartOfCollection rdf:resource="https://kops.uni-konstanz.de/server/rdf/resource/123456789/41"/>
    <dcterms:hasPart rdf:resource="https://kops.uni-konstanz.de/bitstream/123456789/15921/2/Junge_159215.pdf"/>
    <dcterms:abstract xml:lang="eng">The impact of light induced degradation on small lab-type 2x2 cm² solar cells made from standard p-type mc-Si material is compared to the degradation of lowly compensated UMG material on the one hand and intentionally Fe and Fe/Cu contaminated material (several ppma of Fe or Fe and Cu are introduced into the melt of electronic grade feedstock before ingot casting) on the other hand. The material is taken from three different ingot heights (bottom, middle and top), respectively. All cells are annealed at 200 °C in the dark for several minutes before they are exposed to one sun illumination and the development of the electrical parameters over time is determined. The reference and UMG material behave as expected and show a degradation which is correlated to the boron and interstitial oxygen concentration over the ingot height and therefore can be attributed to B-O related defects. The intentionally Fe and Cu contaminated samples in contrast show a degradation behavior that is more probably correlated to the distribution of the Fe and Cu contamination, as the absolute degradation towards the top of the ingot is higher for highly contaminated material (20 ppma Fe) than in the reference material and the observed time constants for degradation are different. Fe/Cu contaminated material exhibits too low cell performance in the top and bottom part of the ingot to show any significant degradation effects. The lowly contaminated material (2 ppma Fe) behaves like the reference material as long as the wafer material does not contain additional contaminants originating from the crucible walls. Material from near the crucible wall by contrast shows a stronger light induced degradation.</dcterms:abstract>
    <dc:creator>Zierer, Robert</dc:creator>
    <foaf:homepage rdf:resource="http://localhost:8080/"/>
    <dcterms:isPartOf rdf:resource="https://kops.uni-konstanz.de/server/rdf/resource/123456789/41"/>
    <dc:creator>Herguth, Axel</dc:creator>
    <bibo:uri rdf:resource="http://kops.uni-konstanz.de/handle/123456789/15921"/>
    <dc:language>eng</dc:language>
    <dcterms:available rdf:datatype="http://www.w3.org/2001/XMLSchema#dateTime">2011-09-29T07:27:59Z</dcterms:available>
    <dc:rights>Attribution-NonCommercial-NoDerivs 3.0 Unported</dc:rights>
    <dc:creator>Junge, Johannes</dc:creator>
    <dc:contributor>Junge, Johannes</dc:contributor>
    <dc:contributor>Hahn, Giso</dc:contributor>
    <dcterms:issued>2011</dcterms:issued>
    <dspace:hasBitstream rdf:resource="https://kops.uni-konstanz.de/bitstream/123456789/15921/2/Junge_159215.pdf"/>
    <dcterms:rights rdf:resource="http://creativecommons.org/licenses/by-nc-nd/3.0/"/>
    <void:sparqlEndpoint rdf:resource="http://localhost/fuseki/dspace/sparql"/>
    <dc:creator>Kreßner-Kiel, Denise</dc:creator>
    <dc:date rdf:datatype="http://www.w3.org/2001/XMLSchema#dateTime">2011-09-29T07:27:59Z</dc:date>
    <dcterms:bibliographicCitation>Publ. in: Energy Procedia ; 8 (2011). - pp. 52-57</dcterms:bibliographicCitation>
    <dc:creator>Hahn, Giso</dc:creator>
    <dcterms:title>Investigation of degradation in solar cells from different mc-Si materials</dcterms:title>
  </rdf:Description>
</rdf:RDF>
kops.description.openAccessopenaccessgold
kops.flag.knbibliographytrue
kops.identifier.nbnurn:nbn:de:bsz:352-159215deu
kops.sourcefieldEnergy Procedia. 2011, <b>8</b>, pp. 52-57. ISSN 1876-6102. Available under: doi: 10.1016/j.egypro.2011.06.101deu
kops.sourcefield.plainEnergy Procedia. 2011, 8, pp. 52-57. ISSN 1876-6102. Available under: doi: 10.1016/j.egypro.2011.06.101deu
kops.sourcefield.plainEnergy Procedia. 2011, 8, pp. 52-57. ISSN 1876-6102. Available under: doi: 10.1016/j.egypro.2011.06.101eng
kops.submitter.emaillarysa.herasymova@uni-konstanz.dedeu
relation.isAuthorOfPublication860a28d6-d6c0-4ece-a83e-16a0e2f45794
relation.isAuthorOfPublication1ab265ef-6078-4a9d-a66b-bcaaf18e5b4e
relation.isAuthorOfPublicatione82405a2-e86b-44d7-8126-8cfdd7e627c9
relation.isAuthorOfPublication.latestForDiscovery860a28d6-d6c0-4ece-a83e-16a0e2f45794
source.bibliographicInfo.fromPage52
source.bibliographicInfo.toPage57
source.bibliographicInfo.volume8
source.identifier.issn1876-6102
source.periodicalTitleEnergy Procedia

Dateien

Originalbündel

Gerade angezeigt 1 - 1 von 1
Vorschaubild nicht verfügbar
Name:
Junge_159215.pdf
Größe:
769.61 KB
Format:
Adobe Portable Document Format
Beschreibung:
Junge_159215.pdf
Junge_159215.pdfGröße: 769.61 KBDownloads: 300

Lizenzbündel

Gerade angezeigt 1 - 1 von 1
Vorschaubild nicht verfügbar
Name:
license.txt
Größe:
1.92 KB
Format:
Plain Text
Beschreibung:
license.txt
license.txtGröße: 1.92 KBDownloads: 0