Nutating a Cassegrain telescope’s secondary mirror is a convenient method of steering the telescope beam through a small angle. Using this principle we have constructed a high performance beam switch for a millimeter wave telescope. A low mass, graphite-epoxy laminate secondary mirror is driven by linear electric motors operated in a frequency compensated control loop. By design, the nutator exerts little net oscillating torque on the telescope structure, resulting in virtually vibration free operation. The inherent versatility of beam switching by subreflector nutation allowed us to test a variety of switching waveforms without making any hardware changes. To reduce the peak stresses on the mechanical linkage between the mirror and the motors and to attain a minimum transition time between mirror positions, we use a digitally generated driving waveform tailored to the system’s transfer function. The nutator can shift the telescope beam by 10 arcminutes, a 1.25° rotation of the 75-cm-diam secondary mirror, in an interval of 8 ms and it can sustain a switching frequency of 10 Hz.
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