Hostname: page-component-68945f75b7-l9cl4 Total loading time: 0 Render date: 2024-08-06T07:35:31.280Z Has data issue: false hasContentIssue false
  • English
  • Français

The design of high frequency antennas

Published online by Cambridge University Press:  12 April 2016

J. Delannoy
J. Delannoy*
Affiliation:
IRAM, 300 Rue de la Piscine, D.U. de GRENOBLE 38406, Saint Martin d’Heres - Cedex, FRANCE

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The conceptual guidelines in designing mm radio-telescope antennas are enlightened by some recent progress in their mechanical construction, and opto-radio-geometrical adjustment. This paper reviews concepts, illustrated in many existing solutions, including the new “phaseretrieval” holography for single dish adjustment (D.Morris, IRAM, 1982): 2 amplitude only maps at focus and out of focus, with enough dynamic range and signal to noise ratio, give surface errors within hours.

Type
Hardware for Interferometry
Information
International Astronomical Union Colloquium , Volume 131: Radio Interferometry: Theory, Techniques, and Applications , 1991 , pp. 15 - 25
Copyright
Copyright © Astronomical Society of the Pacific 1991

References

Delannoy, J. 1985, Proc. of ESO-IRAM-ONSALA Workshop, Aspenas, p.25–50, ed. ESO, Mimchen Google Scholar
Hills, R., Lasenby, A. 1988, Cambridge Annual Report, JCMT Google Scholar
IRAM, Internal Working Reports: WR, availalable on request by nr. (or title list) to the librarian, IRAM, GrenobleGoogle Scholar
Leighton, R.B. 1978, NSF Grant AST 73-04908 Final Technical Report, ed. Cal. Tech.Google Scholar
Lieske, J.H. et al. 1977, Astr. Ap., 58, p. 1–16.Google Scholar
Lieske, J.H. 1979, Astr. Ap., 73, p. 282–284; see also The Astronomical Almanac 1984, for nutation and othersGoogle Scholar
Ludwig, A.C. 1973, IEEE A.P., 21, p. 116–119 Google Scholar
Martin, R.N., Baars, J.W.M. 1990, Proc. of SPIE Conf. 1236 on Advanced Technology Optical Telescopes, The SMT project, TucsonGoogle Scholar
Mason, C. July 1990, SMA Documents List (Technical Memos) and private communicationGoogle Scholar
Morris, D. October 1982, IRAM internal report, Phase retrieval in the holography of Radio-Reflectors, GrenobleGoogle Scholar
Napier, P. 1983, private communication, NRAO Google Scholar
Norris, R.P. 1987, IAU Symp. 129, The Australia Telescope Long Baseline Array, Cambridge, Mass.Google Scholar
NRAO July 1990, Proposal from Associated Universities to NSF, The Millimeter ArrayGoogle Scholar
NRAO 1987, IAU Symp. 129, The Very Long Baseline Array, Cambridge, Mass.Google Scholar
Polyak, V.S., Bervalds, E.Ya. 1990, Precision Construction of Reflector Radiotelescopes, Riga (not yet translated from Russian).Google Scholar
Rudge, A.W., Adatia, N.A. 1978, Proc. IEEE 66, p. 1592–1619: Offset Parabolic Reflector Antennas, a ReviewCrossRefGoogle Scholar
Ruze, J. 1966, Proc. IEEE 54, p. 633–640, Antenna Tolerance Theory - A ReviewGoogle Scholar
Scott, P.F., Ryle, M. 1977, M.N.R.A.S., 178, p. 539–545 Google Scholar
Sovers, O.J., Fanselow, J.L. 1986, JPL Publication 83–39 Rev. 2, Observation Model for the VLBI Parameter Estimation Software “MASTERFIT”Google Scholar
Thompson, A.R. 1990, NRAO doc. 85–13, and private communicationGoogle Scholar
U.C., , Cal.Tech. 1985, Keck Observatory report 90, The design of the KECK Observatory and Telescope; also, 1988: ESO Conference on very large telescopes, ed. Ulrich, M.H., ESO, MunchenGoogle Scholar
Von Hoerner, S. 1967, Astr. J. 72, p. 35–47 Google Scholar
Welch, J. 1990, private communicationGoogle Scholar
Woody, D. Oct. 1988, Symp. on MM and Sub-MM Astronomy, Gravitational Deflection of the Leighton Telescopes, Kona, Hawaii Google Scholar