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Radio noise source

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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,[1] 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.

References

  1. Joardar, Shubhendu; Claycomb, J. R. (2015-05-15) (in en). Radio Astronomy: An Introduction. Mercury Learning and Information. pp. 1-21–1-22. ISBN 978-1-937585-62-4. https://books.google.com/books?id=cjW_DgAAQBAJ&q=%22radio+noise+source+like+that+from+electrical%22&pg=SA1-PA21. 





Licensed under CC BY-SA 3.0 | Source: https://handwiki.org/wiki/Physics:Radio_noise_source
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