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A Method for accurate measurement of heliostat mirror orientation

Thesis (MEng)--Stellenbosch University, 2017.

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Main Author: Swart, Benjamin Dawid
Other Authors: Treurnicht, J.
Format: Thesis
Language:en_ZA
Published: Stellenbosch : Stellenbosch University 2017
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access_status_str Open Access
author Swart, Benjamin Dawid
author2 Treurnicht, J.
author_browse Swart, Benjamin Dawid
Treurnicht, J.
author_facet Treurnicht, J.
Swart, Benjamin Dawid
author_sort Swart, Benjamin Dawid
collection Thesis
dc_rights_str_mv Stellenbosch University
description Thesis (MEng)--Stellenbosch University, 2017.
format Thesis
id oai:scholar.sun.ac.za:10019.1/101038
institution Stellenbosch University (South Africa)
language en_ZA
last_indexed 2026-06-10T12:45:26.037Z
license_str Other — see source repository
provenance_str_mv Harvested via OAI-PMH from SUNScholar — Stellenbosch University Repository
publishDate 2017
publishDateRange 2017
publishDateSort 2017
publisher Stellenbosch : Stellenbosch University
publisherStr Stellenbosch : Stellenbosch University
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source_str SUNScholar — Stellenbosch University Repository
spelling oai:scholar.sun.ac.za:10019.1/101038 A Method for accurate measurement of heliostat mirror orientation Swart, Benjamin Dawid Treurnicht, J. Engelbrecht, H. A. Stellenbosch University. Faculty of Engineering. Dept. of Electrical and Electronic Engineering. Heliostat UCTD Solar-powered aircraft Heliostat -- Mirrors -- Measurement Thesis (MEng)--Stellenbosch University, 2017. ENGLISH ABSTRACT: Heliostat tracking is a critical component of the solar field of concentrating solar power central receiver systems and can be the source of significant losses in power and profit when it lacks the necessary accuracy. The current industry norm seems to be open-loop tracking using an error model for a tracking error of one milliradian, with error model parameters requiring periodic recalibration. In this thesis a method is developed which is able to determine the orientation of all heliostats in the field simultaneously, providing near real-time feedback to the control system, removing the need for recalibration while maintaining an accurate tracking accuracy. The method works by determining the positions of three or more distinct points on the heliostat mirror surface. These points form a plane which is then used to calculate the heliostat normal vector. The performance of the method is analysed and quantified using simulations, and experiments are used to validate the theoretical models. Quantification of the system performance is used to determine the initial feasibility of the method. Results indicate that for the error sources included in the model it is theoretically possible to achieve a tracking error in the order of one milliradian or less. Furthermore, experimental results are found to differ by only 5% from theoretical results. This is promising and merits further investigation into the method as a possible solution to the current heliostat tracking problem. AFRIKAANSE OPSOMMING: Heliostaat volging (die vermo e om die son te volg) is 'n kritiese komponent van die sonveld in gekonsentreerde son-energie sentrale ontvangerstelsels. Indien die nodige akkuraatheid ontbreek, kan dit aansienlike energie{ en winsverliese tot gevolg h^e. Die huidige industry standaard is o enskynlik opelus-volging met 'n foutmodel wat 'n volgfout van een milliradiaal tot gevolg het, met foutmodel parameters wat periodiese herkalibrasie noodsaak. In hierdie tesis word 'n metode ontwikkel wat die ori entasie van al die heliostate in 'n veld tegelykertyd kan bepaal. Dit voorsien byna-intydse terugvoer aan die beheerstelsel wat herkalibrasie onnodig maak terwyl volging steeds akkuraat kan plaasvind. Die metode werk deur die posisies van drie of meer unieke punte op die heliostaatspie el se oppervlak te bepaal. Hierdie punte vorm 'n vlak wat gebruik kan word om die heliostaat se ori entasie te bereken. Die doeltreffendheid van die metode word geanaliseer en gekwantifiseer deur middel van simulasies en eksperimente word uitgevoer om die teoretiese modelle te bevestig. Die resultate wys dat vir die foutbronne wat in die model ingesluit is dit teoreties moontlik is om 'n volgfout in die orde van een milliradiaal of minder te behaal. Daar is ook bevind dat eksperimentele resultate met minder as 5% van teoretiese resultate verskil. Dit is belowend en verdien verdere ondersoek na hierdie metode as moontlike oplossing vir die huidige probleem met heliostaat volging. 2017-02-21T08:40:29Z 2017-03-29T12:00:50Z 2017-02-21T08:40:29Z 2017-03-29T12:00:50Z 2017-03 Thesis http://hdl.handle.net/10019.1/101038 en_ZA Stellenbosch University 128 pages : illustrations, maps application/pdf Stellenbosch : Stellenbosch University
spellingShingle Heliostat
UCTD
Solar-powered aircraft
Heliostat -- Mirrors -- Measurement
Swart, Benjamin Dawid
A Method for accurate measurement of heliostat mirror orientation
title A Method for accurate measurement of heliostat mirror orientation
title_full A Method for accurate measurement of heliostat mirror orientation
title_fullStr A Method for accurate measurement of heliostat mirror orientation
title_full_unstemmed A Method for accurate measurement of heliostat mirror orientation
title_short A Method for accurate measurement of heliostat mirror orientation
title_sort method for accurate measurement of heliostat mirror orientation
topic Heliostat
UCTD
Solar-powered aircraft
Heliostat -- Mirrors -- Measurement
url http://hdl.handle.net/10019.1/101038
work_keys_str_mv AT swartbenjamindawid amethodforaccuratemeasurementofheliostatmirrororientation
AT swartbenjamindawid methodforaccuratemeasurementofheliostatmirrororientation