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High Energy Transient Ionospheric Monitoring Network

Published online by Cambridge University Press:  25 April 2016

Paul J. Edwards
Paul J. Edwards*
Affiliation:
Department of Electronics, Engineering & Applied Physics, School of Information Sciences & Engineering, Canberra College of Advanced Education, GPO Box 1, Belconnen, ACT 2616
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Abstract

Continuous, wide sky coverage is essential for the detection and monitoring of infrequent, short-lived events of astrophysical interest such as supernova and nova explosions, variable X-ray sources, gamma ray bursts, gravity waves and stellar and solar flares. We propose to (1) examine past radio propagation records and (2) develop new computer based radio receivers to monitor and log ionospheric perturbations associated with these events.

Type
High Energy Astrophysics
Information
Publications of the Astronomical Society of Australia , Volume 8 , Issue 3 , 1990 , pp. 263 - 265
Copyright
Copyright © Astronomical Society of Australia 1990

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