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Aperture synthesis

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Aperture synthesis is a type of interferometry that mixes signals from a collection instruments to produce measurements having the same angular resolution as an instrument the size of the entire collection.

This process is used in radio astronomy, most notably in Very Long Baseline Interferometry. It is also used by some RADAR systems, and even optical telescopes.

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This page was last modified 01:06, 10 Aug 2004.
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