Key points are not available for this paper at this time.
The ALMA (Atacama Large Millimeter Array) North American and European prototype antennas have been evaluated by a variety of measurement systems to quantify the major performance specifications. Near‐field holography was used to set the reflector surfaces to 17 μm rms. Pointing and fast‐switching performance was determined with an optical telescope and by millimeter‐wavelength radiometry, yielding 2 '' absolute and 0 6 offset pointing accuracies. Path‐length stability was measured to be ≲20 μm 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.
Mangum et al. (2006) studied this question.