Radio noise source: Difference between revisions

Revision as of 02:12, 19 August 2005

Revision as of 15:04, 5 March 2006

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A '''radio noise source''' is a device that emits [[radio wave]]s at a certain [[frequency]], used to [[calibrate]] [[radio telescope]]s 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.

[[Category:Noise]]

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