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The Colouring of White Noise
Published online by Cambridge University Press: 25 April 2016
Extract
The Mount Stromio optical pulsar detection equipment is built around a commercial two-track tape recorder: one track records timing pulses, and the other the pulses from a photomultiplier (Peterson 1974). Because of the modest frequency range of the recorder, it has been necessary to introduce a scaler between the recorder and photomultiplier in order to cope with bright sources.
- Type
- Equipment
- Information
- Publications of the Astronomical Society of Australia , Volume 2 , Issue 5 , September 1974 , pp. 280 - 282
- Copyright
- Copyright © Astronomical Society of Australia 1974
References
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