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    Progress in track-mounted heliostat

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    Author
    Davila-Peralta, C.
    Rademacher, M.
    Emerson, N.
    Chavez-Lopez, G.
    Sosa, P.
    Cabanillas, R.
    Peon-Anaya, R.
    Flores-Montijo, N.
    Didato, N.
    Angel, R.
    Affiliation
    Steward Observatory Solar Lab, University of Arizona
    Issue Date
    2020
    
    Metadata
    Show full item record
    Publisher
    American Institute of Physics Inc.
    Citation
    Davila-Peralta, C., Rademacher, M., Emerson, N., Chavez-Lopez, G., Sosa, P., Cabanillas, R., ... & Angel, R. (2020, December). Progress in track-mounted heliostat. In AIP Conference Proceedings (Vol. 2303, No. 1, p. 030011). AIP Publishing LLC.
    Journal
    AIP Conference Proceedings
    Rights
    Copyright © 2020 Author(s).
    Collection Information
    This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
    Abstract
    A novel concept is presented for a track-mounted heliostat for central receiver plants, intended to be manufacturable at low cost and to reach an installed cost of ~ $60 /m2 when implemented in high volume. Cost reduction is achieved by using steel in the structurally most efficient form of spaceframe structures. These spread the load broadly, halving the quantity of steel per square meter of reflecting area compared to a conventional post /fishbone heliostat design . The structure is turned in azimuth on wheels on a large diameter ground track, eliminating the need for an expensive, heavy slewing bearing. A preliminary finite-element design of a 22 m2 heliostat with spaceframe azimuth and elevation structures has a total steel mass of mass of 15 kg/m2 supporting 10 kg/m2 of glass reflectors and survives 145 km/h wind. Here we report of field tests of engineering performance of a first prototype of the lower, azimuth spaceframe mounted on a 7 m diameter concrete track. The moving structure with wheels and drive weighs 11 kg/m2 and has a measured lowest resonant frequency of 7.5 Hz, when loaded with a simulated elevation structure. The prototype incorporates inclinometers which measure alignment of the azimuth and elevation axes to better than 0.2 mrad. Absolute azimuth rotation angle measured via an incremental encoder on the drive motor encoder and metal reference bars in the concrete track was found to be accurate to 0.35 mrad. Combining the tip/tilt, azimuth rotation and servo errors in quadrature gives a total of 0.49 mrad in tracker orientation, providing encouragement that our full heliostat system target of 1 mrad RMS pointing accuracy (double the orientation accuracy) should be achievable. © 2020 American Institute of Physics Inc.. All rights reserved.
    Note
    12 month embargo; published online: 11 December 2020
    ISSN
    0094-243X
    ISBN
    9780740000000
    DOI
    10.1063/5.0028486
    Version
    Final published version
    ae974a485f413a2113503eed53cd6c53
    10.1063/5.0028486
    Scopus Count
    Collections
    UA Faculty Publications

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