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A 3072 Channel Surface Acoustic Wave Spectrum Analyser

Published online by Cambridge University Press:  25 April 2016

G. R. A. Ellis  and
P. J. Hall
G. R. A. Ellis
Affiliation:
Department of Physics, University of Tasmania
P. J. Hall*
Affiliation:
Department of Physcis, University of Tasmania
*
Present Address: School of Electrical Engineering, University of Sydney
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Abstract

A spectrum analyser based on SAW (surface acoustic wave) devices has been developed for Jupiter, solar and pulsar observations. It has an overall frequency range of 100 MHz and a frequency resolution of 30 kHz. A complete spectrum is produced every 80 μs. It is initially being used with a 4000 dipole broadband array in the frequency range 30-130 MHz and for Jupiter observations from 8-38 MHz.

Type
Instrumental
Information
Publications of the Astronomical Society of Australia , Volume 7 , Issue 1 , 1987 , pp. 34 - 35
Copyright
Copyright © Astronomical Society of Australia 1987

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References

Hall, P. J., Hamilton, P. A. and McCulloch, P. M., 1983, Proc. Astron. Soc. Aust., 5, 262.CrossRefGoogle Scholar
Hall, P. J., 1985, Ph.D thesis, University of Tasmania.Google Scholar