Physics:Radio noise source
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Revision as of 18:12, 4 August 2021 by imported>PolicyEnforcerIA (attribution)
Short description: Device used to calibrate radio telescopes
A radio noise source is a device that emits radio waves at a certain frequency, used to calibrate radio telescopes such that received data may be compared to a known value, as well as to find the focal point of a telescope soon after construction, so that the wave guide and front end may be properly located.
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