Physics
Scientific paper
Jun 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979cuni.reptr....h&link_type=abstract
Final Technical Report, 1 Sep. 1976 - 31 Aug. 1978 Cornell Univ., Ithaca, NY. Center for Radiophysics and Space Research.
Physics
Gravitational Fields, Polarized Electromagnetic Radiation, Radio Waves, Sun, Time Lag, Deflection, Helios Satellites, Orthogonality, Radiation Measurement, Solar Gravitation, Universities
Scientific paper
Two parallel investigations into the degree, if any, to which orthogonally polarized rays are deflected differently on passing through the gravitational field of the sun were previously conducted. The first involved very long and intermediate length baseline radio interferometry. The second was initially based on observations of radiation transmitted by the Pioneer 6 spacecraft, on passing behind the sun in 1968. This work was extended by using Helios-A and Helios-B spacecraft. It was calculated that the differential deflection between orthogonally polarized components is less than one part in 10 to the 7th power of the total gravitational deflection, or less than about 10 to the -7th power arc sec, in total.
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