English

Evaluation of the ALMA Prototype Antennas

Astrophysics 2009-11-11 v1

Abstract

The ALMA North American and European prototype antennas have been evaluated by a variety of measurement systems to quantify the major performance specifications. Nearfield holography was used to set the reflector surfaces to 17 microns RMS. Pointing and fast switching performance was determined with an optical telescope and by millimeter wavelength radiometry, yielding 2 arcsec absolute and 0.6 arcsec offset pointing accuracies. Path length stability was measured to be less than or approximately equal to 20 microns over 10 minute time periods using optical measurement devices. Dynamical performance was studied with a set of accelerometers, providing data on wind induced tracking errors and structural deformation. Considering all measurements made during this evaluation, both prototype antennas meet the major ALMA antenna performance specifications.

Keywords

Cite

@article{arxiv.astro-ph/0609329,
  title  = {Evaluation of the ALMA Prototype Antennas},
  author = {Jeffrey G. Mangum and Jacob W. M. Baars and Albert Greve and Robert Lucas and Ralph C. Snel and Patrick Wallace and Mark Holdaway},
  journal= {arXiv preprint arXiv:astro-ph/0609329},
  year   = {2009}
}

Comments

83 pages, 36 figures, AASTex format, to appear in PASP September 2006 issue