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Phase Calibration of the Proposed Millimeter Array

Published online by Cambridge University Press:  19 July 2016

M. A. Holdaway
M. A. Holdaway*
Affiliation:
National Radio Astronomy Observatory, * Socorro, New Mexico, 87801

Extract

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The Millimeter Array (MMA) is proposed to operate on baselines of up to 3 km at frequencies up to 350 GHz. Since no operating interferometer can indicate the expected phase stability on such baselines on high, dry sites, NRAO has undertaken a site survey, measuring the opacity and estimating the phase stability on baselines ranging from about 100 m to 5 km with a tipping radiometer. Radiometers have sampled the atmospheres at South Baldy, NM, and Springerville, AZ, and NRAO has recently started taking data at the 12,200 foot VLBA site on Mauna Kea.

Type
Imaging Techniques
Information
Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 101 - 104
Copyright
Copyright © Kluwer 1994 

References

Holdaway, M.A., 1991, A Millimeter Wavelength Phase Stability Analysis of the South Baldy and Springerville Sites, MMA Memorandum 68, NRAO: Socorro, NM Google Scholar
Holdaway, M.A., 1992a, Possible Phase Calibration Schemes for the MMA, MMA Memorandum 84, NRAO: Socorro, NM Google Scholar
Holdaway, M.A., 1992b, Paired Antenna Phase Calibration: Residual Phase Errors and Configuration Study, MMA Memorandum 88, NRAO: Socorro, NM Google Scholar
Kühr, H., et al, 1979, MPIFR Preprint No. 55.Google Scholar
Schwab, F.R., 1992, Lower Tropospheric Wind Speed Statistics at Albuquerque, NM, Winslow, AZ, and Hilo, HA, MMA Memorandum 75, NRAO: Socorro, NM Google Scholar