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A Harmonic Analysis Solution to the Parkes Spectrometer Baseline Ripple
Published online by Cambridge University Press: 25 April 2016
Extract
The arrangement whereby the front end of a radio astronomical receiver is located at the focal plane of a paraboloidal telescope causes the incoming waves to be reflected between focal plane and vertex. The result is a sometimes simple, sometimes complex wave pattern on the output of an associated spectrometer and is known as baseline ripple.
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- Copyright © Astronomical Society of Australia 1981