Radio noise source

This is an old revision of this page, as edited by Metamorforme42 (talk | contribs) at 17:46, 8 September 2022 (Undid revision 1108919278 by Nojo walton (talk): WP:CIRCULAR reference). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

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.