Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67...10k&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Jan.-Feb. 1990, p. 10-20. In Russian.
Astronomy and Astrophysics
Astronomy
6
Astronomical Observatories, Radio Astronomy, Relativistic Theory, Doppler Effect, Gravitational Fields, Quasars, Radar Measurement, Radio Interferometers, Solar System
Scientific paper
The relativistic theory of astronomical coordinate systems is applied to derive data processing formulas for radio-interferometric observations of quasars and for Doppler and radar measurements inside the solar system. The calculations use the barycentric, geocentric, topocentric and/or satellite coordinate systems, generalizing Poincare's transformation formulas of special relativity theory in the case of curved space-time. Measurable relativistic effects are caused by the gravitational fields of the sun and planets and aberration corrections, which are obtained from the coordinate transformation formulas. Post-Newtonian and post-post-Newtonian relationships are obtained.
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