Influence of solar tracking error on the performance of a small-scale linear Fresnel reflector
Solar tracking systems are an indispensable requirement for optimal efficiency in small-scale linear Fresnel reflector systems. A thorough study of the influence of solar tracking errors on energy production is, therefore, required. The power produced by each mirror at any moment is also explicitly...
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| Autor*in: |
Barbón, A. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2020transfer abstract |
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| Schlagwörter: |
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12 |
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Enthalten in: Technologies and practice of CO - HU, Yongle ELSEVIER, 2019, an international journal : the official journal of WREN, The World Renewable Energy Network, Amsterdam [u.a.] |
|---|---|
| Übergeordnetes Werk: |
volume:162 ; year:2020 ; pages:43-54 ; extent:12 |
| Links: |
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| DOI / URN: |
10.1016/j.renene.2020.07.132 |
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| 245 | 1 | 0 | |a Influence of solar tracking error on the performance of a small-scale linear Fresnel reflector |
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| 520 | |a Solar tracking systems are an indispensable requirement for optimal efficiency in small-scale linear Fresnel reflector systems. A thorough study of the influence of solar tracking errors on energy production is, therefore, required. The power produced by each mirror at any moment is also explicitly computed, as well as its variation under error. We study the large effect that the distance between the mirror and the absorber tube, solar time, and the day of the year have on the variation of power. Our results provide the foundations for the analysis of small-scale solar tracking systems. Solar tracking errors of less than 0.09 ∘ are acceptable (they cause power losses less than 1 % ), whereas errors larger than 0.36 ∘ start being noticeable (power losses greater than 3 % ). | ||
| 520 | |a Solar tracking systems are an indispensable requirement for optimal efficiency in small-scale linear Fresnel reflector systems. A thorough study of the influence of solar tracking errors on energy production is, therefore, required. The power produced by each mirror at any moment is also explicitly computed, as well as its variation under error. We study the large effect that the distance between the mirror and the absorber tube, solar time, and the day of the year have on the variation of power. Our results provide the foundations for the analysis of small-scale solar tracking systems. Solar tracking errors of less than 0.09 ∘ are acceptable (they cause power losses less than 1 % ), whereas errors larger than 0.36 ∘ start being noticeable (power losses greater than 3 % ). | ||
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| 700 | 1 | |a Bayón, L. |4 oth | |
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10.1016/j.renene.2020.07.132 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001202.pica (DE-627)ELV05202542X (ELSEVIER)S0960-1481(20)31208-8 DE-627 ger DE-627 rakwb eng Barbón, A. verfasserin aut Influence of solar tracking error on the performance of a small-scale linear Fresnel reflector 2020transfer abstract 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Solar tracking systems are an indispensable requirement for optimal efficiency in small-scale linear Fresnel reflector systems. A thorough study of the influence of solar tracking errors on energy production is, therefore, required. The power produced by each mirror at any moment is also explicitly computed, as well as its variation under error. We study the large effect that the distance between the mirror and the absorber tube, solar time, and the day of the year have on the variation of power. Our results provide the foundations for the analysis of small-scale solar tracking systems. Solar tracking errors of less than 0.09 ∘ are acceptable (they cause power losses less than 1 % ), whereas errors larger than 0.36 ∘ start being noticeable (power losses greater than 3 % ). Solar tracking systems are an indispensable requirement for optimal efficiency in small-scale linear Fresnel reflector systems. A thorough study of the influence of solar tracking errors on energy production is, therefore, required. The power produced by each mirror at any moment is also explicitly computed, as well as its variation under error. We study the large effect that the distance between the mirror and the absorber tube, solar time, and the day of the year have on the variation of power. Our results provide the foundations for the analysis of small-scale solar tracking systems. Solar tracking errors of less than 0.09 ∘ are acceptable (they cause power losses less than 1 % ), whereas errors larger than 0.36 ∘ start being noticeable (power losses greater than 3 % ). Solar tracking system Elsevier Small-scale linear fresnel reflector Elsevier Solar tracking error Elsevier Bayón-Cueli, C. oth Bayón, L. oth Ayuso, P. Fortuny oth Enthalten in Elsevier Science HU, Yongle ELSEVIER Technologies and practice of CO 2019 an international journal : the official journal of WREN, The World Renewable Energy Network Amsterdam [u.a.] (DE-627)ELV002723662 volume:162 year:2020 pages:43-54 extent:12 https://doi.org/10.1016/j.renene.2020.07.132 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U AR 162 2020 43-54 12 |
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10.1016/j.renene.2020.07.132 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001202.pica (DE-627)ELV05202542X (ELSEVIER)S0960-1481(20)31208-8 DE-627 ger DE-627 rakwb eng Barbón, A. verfasserin aut Influence of solar tracking error on the performance of a small-scale linear Fresnel reflector 2020transfer abstract 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Solar tracking systems are an indispensable requirement for optimal efficiency in small-scale linear Fresnel reflector systems. A thorough study of the influence of solar tracking errors on energy production is, therefore, required. The power produced by each mirror at any moment is also explicitly computed, as well as its variation under error. We study the large effect that the distance between the mirror and the absorber tube, solar time, and the day of the year have on the variation of power. Our results provide the foundations for the analysis of small-scale solar tracking systems. Solar tracking errors of less than 0.09 ∘ are acceptable (they cause power losses less than 1 % ), whereas errors larger than 0.36 ∘ start being noticeable (power losses greater than 3 % ). Solar tracking systems are an indispensable requirement for optimal efficiency in small-scale linear Fresnel reflector systems. A thorough study of the influence of solar tracking errors on energy production is, therefore, required. The power produced by each mirror at any moment is also explicitly computed, as well as its variation under error. We study the large effect that the distance between the mirror and the absorber tube, solar time, and the day of the year have on the variation of power. Our results provide the foundations for the analysis of small-scale solar tracking systems. Solar tracking errors of less than 0.09 ∘ are acceptable (they cause power losses less than 1 % ), whereas errors larger than 0.36 ∘ start being noticeable (power losses greater than 3 % ). Solar tracking system Elsevier Small-scale linear fresnel reflector Elsevier Solar tracking error Elsevier Bayón-Cueli, C. oth Bayón, L. oth Ayuso, P. Fortuny oth Enthalten in Elsevier Science HU, Yongle ELSEVIER Technologies and practice of CO 2019 an international journal : the official journal of WREN, The World Renewable Energy Network Amsterdam [u.a.] (DE-627)ELV002723662 volume:162 year:2020 pages:43-54 extent:12 https://doi.org/10.1016/j.renene.2020.07.132 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U AR 162 2020 43-54 12 |
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Influence of solar tracking error on the performance of a small-scale linear Fresnel reflector |
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Solar tracking systems are an indispensable requirement for optimal efficiency in small-scale linear Fresnel reflector systems. A thorough study of the influence of solar tracking errors on energy production is, therefore, required. The power produced by each mirror at any moment is also explicitly computed, as well as its variation under error. We study the large effect that the distance between the mirror and the absorber tube, solar time, and the day of the year have on the variation of power. Our results provide the foundations for the analysis of small-scale solar tracking systems. Solar tracking errors of less than 0.09 ∘ are acceptable (they cause power losses less than 1 % ), whereas errors larger than 0.36 ∘ start being noticeable (power losses greater than 3 % ). |
| abstractGer |
Solar tracking systems are an indispensable requirement for optimal efficiency in small-scale linear Fresnel reflector systems. A thorough study of the influence of solar tracking errors on energy production is, therefore, required. The power produced by each mirror at any moment is also explicitly computed, as well as its variation under error. We study the large effect that the distance between the mirror and the absorber tube, solar time, and the day of the year have on the variation of power. Our results provide the foundations for the analysis of small-scale solar tracking systems. Solar tracking errors of less than 0.09 ∘ are acceptable (they cause power losses less than 1 % ), whereas errors larger than 0.36 ∘ start being noticeable (power losses greater than 3 % ). |
| abstract_unstemmed |
Solar tracking systems are an indispensable requirement for optimal efficiency in small-scale linear Fresnel reflector systems. A thorough study of the influence of solar tracking errors on energy production is, therefore, required. The power produced by each mirror at any moment is also explicitly computed, as well as its variation under error. We study the large effect that the distance between the mirror and the absorber tube, solar time, and the day of the year have on the variation of power. Our results provide the foundations for the analysis of small-scale solar tracking systems. Solar tracking errors of less than 0.09 ∘ are acceptable (they cause power losses less than 1 % ), whereas errors larger than 0.36 ∘ start being noticeable (power losses greater than 3 % ). |
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| title_short |
Influence of solar tracking error on the performance of a small-scale linear Fresnel reflector |
| url |
https://doi.org/10.1016/j.renene.2020.07.132 |
| remote_bool |
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| author2 |
Bayón-Cueli, C. Bayón, L. Ayuso, P. Fortuny |
| author2Str |
Bayón-Cueli, C. Bayón, L. Ayuso, P. Fortuny |
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| doi_str |
10.1016/j.renene.2020.07.132 |
| up_date |
2024-07-06T21:53:58.915Z |
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