An astigmatic corrected target-aligned heliostat for high concentration
Conventional heliostats suffer from astigmatism for non-normal incidence. For tangential rays the focal length is shortened while for sagittal rays it is longer than the nominal focal length. Due to this astigmatism it is impossible to produce a sharp image of the sun, and the rays will be spread ov...
Gespeichert in:
Veröffentlicht in: | Solar energy materials and solar cells 1995, Vol.37 (2), p.191-202 |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 202 |
---|---|
container_issue | 2 |
container_start_page | 191 |
container_title | Solar energy materials and solar cells |
container_volume | 37 |
creator | Zaibel, R. Dagan, E. Karni, J. Ries, Harald |
description | Conventional heliostats suffer from astigmatism for non-normal incidence. For tangential rays the focal length is shortened while for sagittal rays it is longer than the nominal focal length. Due to this astigmatism it is impossible to produce a sharp image of the sun, and the rays will be spread over a larger area. In order to correct this the heliostat should have different curvature radii along the sagittal and tangential direction in the heliostat plane just like a non axial part of a paraboloid. In conventional heliostats, where the first axis, fixed with respect to the ground, is vertical while the second, fixed with respect to the reflector surface, is horizontal such an astigmatism correction is not practical because the sagittal and tangential directions rotate with respect to the reflector. We suggest an alternative mount where the first axis is oriented towards the target. The second axis, perpendicular to the first and tangent to the reflector, coincides with the tangential direction. With this mounting sagittal and tangential direction are fixed with respect to the reflector during operation. Therefore a partial astigmatism compensation is possible. We calculate the optimum correction and show the performance of the heliostat. We also show predicted yearly average concentrations. |
doi_str_mv | 10.1016/0927-0248(94)00206-1 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_16942628</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>0927024894002061</els_id><sourcerecordid>184663</sourcerecordid><originalsourceid>FETCH-LOGICAL-c364t-c22a01741eb479b3d73b928f17b22939a6488e6b26dfc3424835ab1dacec7a923</originalsourceid><addsrcrecordid>eNp9kMtKAzEUhoMoWKtv4GIWIroYza2ZZCOUolUouNF1yGTOTCPTSU1Swbc3Y4tLV4cD338uH0KXBN8RTMQ9VrQqMeXyRvFbjCkWJTlCEyIrVTKm5DGa_CGn6CzGD5wpwfgELedDYWJy3cYkZwvrQwCboCmSCR2k0vSuG3K7ht75mEwqWh-KtevWmR0sDCnkoB_O0Ulr-ggXhzpF70-Pb4vncvW6fFnMV6VlgqfSUmowqTiBmleqZk3FakVlS6qaUsWUEVxKEDUVTWsZz_eymalJYyzYyijKpuh6P3cb_OcOYtIbFy30vRnA76ImQnEqqMwg34M2-BgDtHob3MaEb02wHq3pUYkelWjF9a81TXLs6jDfRGv6NpjBuviXZTNJ8k0Ze9hjkH_9chB0tA6yj8aN_nTj3f97fgAvYIBX</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>16942628</pqid></control><display><type>article</type><title>An astigmatic corrected target-aligned heliostat for high concentration</title><source>ScienceDirect Journals (5 years ago - present)</source><creator>Zaibel, R. ; Dagan, E. ; Karni, J. ; Ries, Harald</creator><creatorcontrib>Zaibel, R. ; Dagan, E. ; Karni, J. ; Ries, Harald</creatorcontrib><description>Conventional heliostats suffer from astigmatism for non-normal incidence. For tangential rays the focal length is shortened while for sagittal rays it is longer than the nominal focal length. Due to this astigmatism it is impossible to produce a sharp image of the sun, and the rays will be spread over a larger area. In order to correct this the heliostat should have different curvature radii along the sagittal and tangential direction in the heliostat plane just like a non axial part of a paraboloid. In conventional heliostats, where the first axis, fixed with respect to the ground, is vertical while the second, fixed with respect to the reflector surface, is horizontal such an astigmatism correction is not practical because the sagittal and tangential directions rotate with respect to the reflector. We suggest an alternative mount where the first axis is oriented towards the target. The second axis, perpendicular to the first and tangent to the reflector, coincides with the tangential direction. With this mounting sagittal and tangential direction are fixed with respect to the reflector during operation. Therefore a partial astigmatism compensation is possible. We calculate the optimum correction and show the performance of the heliostat. We also show predicted yearly average concentrations.</description><identifier>ISSN: 0927-0248</identifier><identifier>EISSN: 1879-3398</identifier><identifier>DOI: 10.1016/0927-0248(94)00206-1</identifier><language>eng</language><publisher>Amsterdam: Elsevier B.V</publisher><subject>Applied sciences ; Energy ; Exact sciences and technology ; Natural energy ; Q1 ; Solar collectors ; Solar energy ; Solar radiation ; Solar thermal conversion</subject><ispartof>Solar energy materials and solar cells, 1995, Vol.37 (2), p.191-202</ispartof><rights>1995</rights><rights>1995 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c364t-c22a01741eb479b3d73b928f17b22939a6488e6b26dfc3424835ab1dacec7a923</citedby><cites>FETCH-LOGICAL-c364t-c22a01741eb479b3d73b928f17b22939a6488e6b26dfc3424835ab1dacec7a923</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/0927-0248(94)00206-1$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,780,784,3548,4022,27922,27923,27924,45994</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=3581483$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Zaibel, R.</creatorcontrib><creatorcontrib>Dagan, E.</creatorcontrib><creatorcontrib>Karni, J.</creatorcontrib><creatorcontrib>Ries, Harald</creatorcontrib><title>An astigmatic corrected target-aligned heliostat for high concentration</title><title>Solar energy materials and solar cells</title><description>Conventional heliostats suffer from astigmatism for non-normal incidence. For tangential rays the focal length is shortened while for sagittal rays it is longer than the nominal focal length. Due to this astigmatism it is impossible to produce a sharp image of the sun, and the rays will be spread over a larger area. In order to correct this the heliostat should have different curvature radii along the sagittal and tangential direction in the heliostat plane just like a non axial part of a paraboloid. In conventional heliostats, where the first axis, fixed with respect to the ground, is vertical while the second, fixed with respect to the reflector surface, is horizontal such an astigmatism correction is not practical because the sagittal and tangential directions rotate with respect to the reflector. We suggest an alternative mount where the first axis is oriented towards the target. The second axis, perpendicular to the first and tangent to the reflector, coincides with the tangential direction. With this mounting sagittal and tangential direction are fixed with respect to the reflector during operation. Therefore a partial astigmatism compensation is possible. We calculate the optimum correction and show the performance of the heliostat. We also show predicted yearly average concentrations.</description><subject>Applied sciences</subject><subject>Energy</subject><subject>Exact sciences and technology</subject><subject>Natural energy</subject><subject>Q1</subject><subject>Solar collectors</subject><subject>Solar energy</subject><subject>Solar radiation</subject><subject>Solar thermal conversion</subject><issn>0927-0248</issn><issn>1879-3398</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1995</creationdate><recordtype>article</recordtype><recordid>eNp9kMtKAzEUhoMoWKtv4GIWIroYza2ZZCOUolUouNF1yGTOTCPTSU1Swbc3Y4tLV4cD338uH0KXBN8RTMQ9VrQqMeXyRvFbjCkWJTlCEyIrVTKm5DGa_CGn6CzGD5wpwfgELedDYWJy3cYkZwvrQwCboCmSCR2k0vSuG3K7ht75mEwqWh-KtevWmR0sDCnkoB_O0Ulr-ggXhzpF70-Pb4vncvW6fFnMV6VlgqfSUmowqTiBmleqZk3FakVlS6qaUsWUEVxKEDUVTWsZz_eymalJYyzYyijKpuh6P3cb_OcOYtIbFy30vRnA76ImQnEqqMwg34M2-BgDtHob3MaEb02wHq3pUYkelWjF9a81TXLs6jDfRGv6NpjBuviXZTNJ8k0Ze9hjkH_9chB0tA6yj8aN_nTj3f97fgAvYIBX</recordid><startdate>1995</startdate><enddate>1995</enddate><creator>Zaibel, R.</creator><creator>Dagan, E.</creator><creator>Karni, J.</creator><creator>Ries, Harald</creator><general>Elsevier B.V</general><general>Elsevier</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>1995</creationdate><title>An astigmatic corrected target-aligned heliostat for high concentration</title><author>Zaibel, R. ; Dagan, E. ; Karni, J. ; Ries, Harald</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c364t-c22a01741eb479b3d73b928f17b22939a6488e6b26dfc3424835ab1dacec7a923</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1995</creationdate><topic>Applied sciences</topic><topic>Energy</topic><topic>Exact sciences and technology</topic><topic>Natural energy</topic><topic>Q1</topic><topic>Solar collectors</topic><topic>Solar energy</topic><topic>Solar radiation</topic><topic>Solar thermal conversion</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zaibel, R.</creatorcontrib><creatorcontrib>Dagan, E.</creatorcontrib><creatorcontrib>Karni, J.</creatorcontrib><creatorcontrib>Ries, Harald</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><jtitle>Solar energy materials and solar cells</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zaibel, R.</au><au>Dagan, E.</au><au>Karni, J.</au><au>Ries, Harald</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>An astigmatic corrected target-aligned heliostat for high concentration</atitle><jtitle>Solar energy materials and solar cells</jtitle><date>1995</date><risdate>1995</risdate><volume>37</volume><issue>2</issue><spage>191</spage><epage>202</epage><pages>191-202</pages><issn>0927-0248</issn><eissn>1879-3398</eissn><abstract>Conventional heliostats suffer from astigmatism for non-normal incidence. For tangential rays the focal length is shortened while for sagittal rays it is longer than the nominal focal length. Due to this astigmatism it is impossible to produce a sharp image of the sun, and the rays will be spread over a larger area. In order to correct this the heliostat should have different curvature radii along the sagittal and tangential direction in the heliostat plane just like a non axial part of a paraboloid. In conventional heliostats, where the first axis, fixed with respect to the ground, is vertical while the second, fixed with respect to the reflector surface, is horizontal such an astigmatism correction is not practical because the sagittal and tangential directions rotate with respect to the reflector. We suggest an alternative mount where the first axis is oriented towards the target. The second axis, perpendicular to the first and tangent to the reflector, coincides with the tangential direction. With this mounting sagittal and tangential direction are fixed with respect to the reflector during operation. Therefore a partial astigmatism compensation is possible. We calculate the optimum correction and show the performance of the heliostat. We also show predicted yearly average concentrations.</abstract><cop>Amsterdam</cop><pub>Elsevier B.V</pub><doi>10.1016/0927-0248(94)00206-1</doi><tpages>12</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0927-0248 |
ispartof | Solar energy materials and solar cells, 1995, Vol.37 (2), p.191-202 |
issn | 0927-0248 1879-3398 |
language | eng |
recordid | cdi_proquest_miscellaneous_16942628 |
source | ScienceDirect Journals (5 years ago - present) |
subjects | Applied sciences Energy Exact sciences and technology Natural energy Q1 Solar collectors Solar energy Solar radiation Solar thermal conversion |
title | An astigmatic corrected target-aligned heliostat for high concentration |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-12T10%3A04%3A48IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=An%20astigmatic%20corrected%20target-aligned%20heliostat%20for%20high%20concentration&rft.jtitle=Solar%20energy%20materials%20and%20solar%20cells&rft.au=Zaibel,%20R.&rft.date=1995&rft.volume=37&rft.issue=2&rft.spage=191&rft.epage=202&rft.pages=191-202&rft.issn=0927-0248&rft.eissn=1879-3398&rft_id=info:doi/10.1016/0927-0248(94)00206-1&rft_dat=%3Cproquest_cross%3E184663%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=16942628&rft_id=info:pmid/&rft_els_id=0927024894002061&rfr_iscdi=true |