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Coherence limits for very-long-baseline interferometryThe quality of the frequency standards used in very-long-baseline interferometry (VBLI) limits the coherent integration time and the accuracy of geodetic experiments except in special cases when clock instabilities can be made to cancel out by using differential interferometry. Formulas are derived for estimating the coherence of these interferometers from the Allan variances of the frequency standards. Experiments using extremely high-quality frequency standards, such as hydrogen masers, may be limited by the phase noise that results from atmospheric and ionospheric fluctuations.
Document ID
19820032390
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Rogers, A. E. E.
(Haystack Observatory Westford, MA, United States)
Moran, J. M., Jr.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 10, 2013
Publication Date
December 1, 1981
Publication Information
Publication: IEEE Transactions on Instrumentation and Measurement
Volume: IM-30
Subject Category
Astronomy
Accession Number
82A15925
Funding Number(s)
CONTRACT_GRANT: NAS5-25053
CONTRACT_GRANT: NSF AST-79-20168
Distribution Limits
Public
Copyright
Other

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