Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984tdar.nasar...1m&link_type=abstract
In its The Telecommunications and Data Acquisition Rept. p 1-16 (SEE N85-13980 05-32)
Astronomy and Astrophysics
Astronomy
Deep Space Network, Error Analysis, Radio Sources (Astronomy), Very Long Base Interferometry, Atomic Clocks, Digital Systems, Earth Ionosphere, Quasars, Signal To Noise Ratios, Solar Wind, Troposphere
Scientific paper
The potential accuracy attainable for (delta) VLBI positional measurements (submilliarc second level) is reached by simultaneously observing pairs of compact radio sources whose angular separation are smaller than the beamwidth of each antenna. Simultaneous (delta) VLBI (SVLBI) enables significant cancellation of measurement errors. Solar plasma is the dominant fluctuating error source in SVLBI positional measurements since there is enhanced cancellation of the troposphere and ionosphere, and complete cancellation of oscillator instabilities. Of the nonfluctuating error sources, errors due to universal time predominate. By performing SVLBI experiments over several years with many different close pairs of radio sources, limits can be placed on reference frame stability. Intrinsic properties of the sources, such as source structure and proper motion, will limit measurements. The SVLBI differential phase and corruptive noise sources will be discussed here along with estimated results.
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