Observation of the stellar field near the sun during a total eclipse

Details Observation of the stellar field near the sun during a total eclipse Observation of the stellar field near the sun during a total eclipse

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977c%26t....93..189d&link_type=abstract

Ciel et Terre, vol. 93, July-Aug. 1977, p. 189-203. In French.

Physics

Nonrelativistic Mechanics, Relativistic Effects, Solar Eclipses, Star Distribution, Stellar Radiation, Deviation, Einstein Equations, Inertia, Newton Theory, Riemann Manifold, Stellar Luminosity

Scientific paper

Deviation of stellar light emission in the neighborhood of the sun's mass is studied through evidence obtained during total eclipses in the period 1919 to 1973. The Einstein and Newtonian treatments of the deviation are reviewed; experimental techniques are discussed. In particular, placement of the sun in the experimental photographic plates and the data reduction method of fictive stars are mentioned.

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