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AGU: Journal of Geophysical Research

 
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Abstract

Radio Interferometry at Three Kilometers Altitude above the Pacific Ocean. Part II: Celestial Sources

Grote Reber

Research Corporation 405 Lexington Avenue, New York City

Observations were secured at 20, 30, 50, and 100 Mc/s. Fluctuations are greatly reduced by averaging data. Cassiopeia is found to be an elliptical ring 2.3′ by 1.5′ inside a halo, a few minutes of arc in diameter. The halo increases in size and intensity relative to the pairing at lower frequencies. Cygnus contains a nucleus < 1′ wide by 2′ long in a halo about 4′ diameter. Hydra contains a source about 5′ wide. Observations of the sun confirm that the maximum obscuration is toward the east. Surges from Jupiter at 30 Mc/s are discussed.

Received 15 August 1958; .

Citation: Reber, G. (1959), Radio Interferometry at Three Kilometers Altitude above the Pacific Ocean. Part II: Celestial Sources, J. Geophys. Res., 64(3), 293–303.

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