Comparison of two observations of anomalous redshifts observed in the neighborhood of the solar disk

Details Comparison of two observations of anomalous redshifts observed in the neighborhood of the solar disk Comparison of two observations of anomalous redshifts observed in the neighborhood of the solar disk

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974crasb.279..559d&link_type=abstract

Academie des Sciences (Paris), Comptes Rendus, Serie B - Sciences Physiques, vol. 279, no. 23, Dec. 2, 1974, p. 559-563. In Fre

Astronomy and Astrophysics

Astronomy

2

Occultation, Radio Sources (Astronomy), Red Shift, Solar Corpuscular Radiation, Energy Dissipation, Gamma Rays, Microwave Transmission, Optical Properties, Particle Emission, Particle Interactions, Pioneer 6 Space Probe, Plasma Waves, Solar Corona

Scientific paper

Comparison of the series of observations of anomalous redshifts made by Sadeh et al. (1968) on the radio source Taurus A with the anomalous redshift observed by Goldstein (1969) at the frequency emitted by the Pioneer 6 satellite. Observing at a frequency of 2292 MHz, Goldstein noted an anomalous redshift at the onset of occultation of the satellite by the sun. This shift consists of a superposition of an asymmetrical shift and a symmetrical shift. In a similar experiment, based on observations of the 21-cm hydrogen absorption line, Sadeh et al. also noted an anomalous redshift at the moment of solar occultation. An interpretation and comparison of these redshifts are made by assuming that the lost energy of the observed redshifts is carried away by lightweight particles which are emitted at the surface of the sun and strongly interact with gamma rays emitted by the source.

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