Phase stability, angular structure and position measurements with a radio-link interferometer

Details Phase stability, angular structure and position measurements with a radio-link interferometer Phase stability, angular structure and position measurements with a radio-link interferometer

Nov 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.177..335w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 177, Nov. 1976, p. 335-347. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

9

Phase Deviation, Radio Interferometers, Radio Sources (Astronomy), Fourier Transformation, Ionospheric Propagation, Microwave Transmission, Phase Error, Phase Locked Systems, Position (Location), Troposphere, Ultrahigh Frequencies

Scientific paper

Recent modifications to the Jodrell Bank-Mark III radio-link interferometer are described. It is shown that at frequencies up to 1666 MHz, the ionosphere is the most important source of phase instability in the improved instrument. The effect of the residual phase fluctuations on the determination of the angular structure of compact radio sources is investigated, and preliminary measurements of the positions of six sources are reported.

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