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1 August 1990 Recent progress on the infrared Michelson array
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Construction of a two-telescope Michelson spatial inteferometer to be operated at a nominal wavelength of 2.2 microns in the near-IR began in May 1987. Nearly all of the mechanical, electronic, and optical hardware of the Infrared Michelson Array (IRNMA) is currently in place and has been tested. Proof-of-concept has been demonstrated, and efforts are currently underway to improve the system operation to produce reliable, calibrated fringe visibilities.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
H. Melvin Dyck, James A. Benson, William L. Mason, Stephen T. Ridgway, and Robert R. Howell "Recent progress on the infrared Michelson array", Proc. SPIE 1237, Amplitude and Intensity Spatial Interferometry, (1 August 1990);


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