On the inversion phenomenon in radio star scintillation

Details On the inversion phenomenon in radio star scintillation On the inversion phenomenon in radio star scintillation

Oct 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968jatp...30.1823h&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, vol. 30, no. 10, pp. 1823-1826

Physics

Scientific paper

Some observations of the phenomenon known as [`]inversion' in records of scintillation of signals from the sources Cassiopeia A and Cygnus A are reviewed briefly. It is shown that the phenomenon is more likely to be explained by the finite angular diameters of these sources than, as suggested by previous authors, by the aperture size of the antenna used in making the observations. An experiment is suggested which should distinguish between these and other criteria which can bring about the observation of inversion.

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