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Radioastronomy through an Artificial Ionospheric Window—Spacelab 2 Observations

Published online by Cambridge University Press:  25 April 2016

G. R. A. Ellis ,
A. Klekociuk ,
G. T. Goldstone  and
Michael Medillo
G. R. A. Ellis
Affiliation:
Physics Department, University of Tasmania
A. Klekociuk
Affiliation:
Physics Department, University of Tasmania
G. T. Goldstone
Affiliation:
Department of Science, Hobart
Michael Medillo
Affiliation:
Department of Astronomy, Boston University
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Abstract

Observations of the galactic background radio emission at a number of frequencies between 2.7 MHz and 1.07 MHz were made in association with the plasma depletion experiments of Spacelab-2 to test the concept of making low frequency radio observations through an artificial ionospheric window. Following the Shuttle OMS burn at a time when foF2 was 1.99 MHz, a decrease in the maximum ionospheric electron density of approximately 30% occurred. The first observations of the radio emission at high galactic latitudes with good angular resolution (25 degrees) were obtained during this event.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 6 , Issue 3 , 1986 , pp. 331 - 333
Copyright
Copyright © Astronomical Society of Australia 1986

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References

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