Sea interferometry, also known as sea-cliff interferometry, is a form of radio astronomy that uses radio waves reflected off the sea to produce an interference pattern.[1] It is the radio wave analogue to Lloyd's mirror.[2] The technique was invented and exploited in Australia between 1945 and 1948.[3]
- ^ "Radio Astronomy at Dover Heights: Sea interferometry". CSIRO. 2008-02-05. Retrieved 2024-03-24.
- ^ Bolton, J. G.; Slee, O. B. (December 1953). "Galactic Radiation at Radio Frequencies V. The Sea Interferometer". Australian Journal of Physics. 6 (4): 420–433. Bibcode:1953AuJPh...6..420B. doi:10.1071/PH530420.
- ^ Sullivan, W. T. III (1991). "Some highlights of Interferometry in early Radio Astronomy". In Cornwell, T. J.; Perley, R. A. (eds.). Radio interferometry: Theory, techniques, and applications; Proceedings of the 131st IAU Colloquium, ASP Conference Series. Vol. 19. San Francisco: Astronomical Society of the Pacific. p. 132. Bibcode:1991ASPC...19..132S. ISBN 0-937707-38-4.
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