NASA NTRS · 19910055829
A picosecond accuracy relativistic VLBI model via Fermi normal coordinates
Abstract
Fermi normal coordinates are used to construct transformations relating solar system barycentric coordinates to local inertial geocentric coordinates. Relativistic corrections to terrestrial VLBI measurements are calculated, and this formalism is developed to include corrections needed for picosecond accuracy. A calculation of photon time delay which includes effects arising from the motion of gravitational sources is given.
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Shahid-Saless, Bahman, Hellings, Ronald W., Ashby, Neil. 1991-06-01. A picosecond accuracy relativistic VLBI model via Fermi normal coordinates. https://ntrs.nasa.gov/citations/19910055829
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