Author:
Magun A.,Stewart R.T.,Robinson R.D.
Abstract
To date the Culgoora radioheliograph has recorded seven continuum bursts simultaneously at its three operating frequencies of 160, 80 and 43 MHz. In every case the radio emission is found to originate from stationary sources whose heights increase with decreasing frequency. The implications of these new observations are discussed below.
Publisher
Cambridge University Press (CUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
17 articles.
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1. Radio Observations of Coronal Phenomena and Solar Flares;Physics of Solar Planetary Environments: Proceedings of the International Symposium on Solar-Terrestrial Physics, June 7-18,1976 Boulder, Colorado, Volume I;2013-03-19
2. ORIGIN OF CORONAL SHOCK WAVES ASSOCIATED WITH SLOW CORONAL MASS EJECTIONS;The Astrophysical Journal;2010-06-29
3. Secondary peaks in solar microwave outbursts;Solar Physics;1983-04
4. A Catalogue of Major Metre-Wavelength Solar Events Recorded by the Dapto and Culgoora Solar Radio Observatories (1961-1981);Publications of the Astronomical Society of Australia;1983
5. Galaxies and their Environment;Extragalactic Astronomy;1982