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    This article has been cited by the following publications. This list is generated based on data provided by CrossRef.
    Stanislavsky, A.A. Koval, A.A. and Konovalenko, A.A. 2013. Low-frequency heliographic observations of the quiet Sun corona. Astronomische Nachrichten, Vol. 334, Issue. 10, p. 1086.
    Robinson, R. D. Tuxford, Jennifer M. Sheridan, K. V. and Stewart, R. T. 1983. 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, Vol. 5, Issue. 01, p. 84.
    Suzuki, S. and Sheridan, K.V. 1982. On the Fundamental and Harmonic Components of Low-Frequency Type III Solar Radio Bursts. Publications of the Astronomical Society of Australia, Vol. 4, Issue. 04, p. 382.
    Sheridan, K. V. and Dulk, G. A. 1980. Radio Observations of Coronal Holes. Symposium - International Astronomical Union, Vol. 91, Issue. , p. 37.
    Dulk, G. A. 1980. Radio and White-Light Observations of Coronal Transients. Symposium - International Astronomical Union, Vol. 86, Issue. , p. 419.
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Some Recent Explorations of the Solar Corona from the Culgoora Solar Radio Observatory

  • K. V. Sheridan (a1)
Extract

The complex flare related events taking place in the solar corona are becoming better understood as more observations are made with high spatial and temporal resolution nearly simultaneously at widely separated radio frequencies. Similarly the magneto-plasma structures related to the so-called quiet Sun, which have been extensively studied during the recent cycle (No. 20), are now better understood because of such high resolution observations.

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Copyright
COPYRIGHT: © Astronomical Society of Australia 1978
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Publications of the Astronomical Society of Australia
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  • EISSN: 1448-6083
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