• DocumentCode
    1374004
  • Title

    Antenna reflector metrology: the Australia Telescope experience

  • Author

    Kesteven, M.J. ; Parsons, B.F. ; Yabsley, D.E.

  • Author_Institution
    Div. of Radiophys., CSIRO, Epping, NSW, Australia
  • Volume
    36
  • Issue
    10
  • fYear
    1988
  • fDate
    10/1/1988 12:00:00 AM
  • Firstpage
    1481
  • Lastpage
    1484
  • Abstract
    A description is given of some refinements to the traditional theodolite and tape technique for surveying the reflector surface of large antennas. The theodolite is positioned in the structural axis about 40 cm above the antenna vertex. There are six rings of panels, ranging in size from 1.4 m×0.7 m to 2 m×2 m, with 160 panels in all in each antenna. Targets are placed near the corners of each panel. In brief, each target´s position is defined by two measurements: its distance from the theodolite, and the angle between the antenna axis and the line of sight to target, the zenith angle. The equipment and the procedures used are reported. The authors examine the accuracy achieved in each measurement and discuss the consequent panel positional accuracy. In applications (to radio telescope antennas 18-m and 22-m in diameter), surface accuracies of 0.25 mm root mean square (RMS) have been achieved
  • Keywords
    antenna reflectors; distance measurement; radiotelescopes; reflector antennas; Australia Telescope; antenna reflector; antenna vertex; distance measurement; panel positional accuracy; radio telescope antennas; reflector surface; tape; theodolite; Antenna measurements; Australia; Computer errors; Computer vision; Metrology; Position measurement; Radio astronomy; Reflector antennas; Root mean square; Telescopes; Theodolites;
  • fLanguage
    English
  • Journal_Title
    Antennas and Propagation, IEEE Transactions on
  • Publisher
    ieee
  • ISSN
    0018-926X
  • Type

    jour

  • DOI
    10.1109/8.8636
  • Filename
    8636