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The Colouring of White Noise

Published online by Cambridge University Press:  25 April 2016

A. J. Kalnajs  and
B. A. Peterson
A. J. Kalnajs
Affiliation:
Mt Stromlo and Siding Spring Observatory, Research School of Physical Sciences, Australian National University
B. A. Peterson
Affiliation:
Mt Stromlo and Siding Spring Observatory, Research School of Physical Sciences, Australian National University
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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

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References

Feller, W., An Introduction to Probability Theory and Its Applications, Vol. 2, Wiley and Sons, New York (1966).Google Scholar
Peterson, B.A., Proc. Astron. Soc. Aust., 2, 278.CrossRefGoogle Scholar