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Stewart, R. T., Sheridan, K. V. (1971) Multiple Magnetic-Loop Structure of a Type IV Solar Radio Outburst. Publications of the Astronomical Society of Australia, 2. 60-62 doi:10.1017/s1323358000012868

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Reference TypeJournal (article/letter/editorial)
TitleMultiple Magnetic-Loop Structure of a Type IV Solar Radio Outburst
JournalPublications of the Astronomical Society of Australia
AuthorsStewart, R. T.Author
Sheridan, K. V.Author
Year1971 (July)Volume2
PublisherCambridge University Press (CUP)
DOIdoi:10.1017/s1323358000012868Search in ResearchGate
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Mindat Ref. ID3603453Long-form Identifiermindat:1:5:3603453:2
GUID0
Full ReferenceStewart, R. T., Sheridan, K. V. (1971) Multiple Magnetic-Loop Structure of a Type IV Solar Radio Outburst. Publications of the Astronomical Society of Australia, 2. 60-62 doi:10.1017/s1323358000012868
Plain TextStewart, R. T., Sheridan, K. V. (1971) Multiple Magnetic-Loop Structure of a Type IV Solar Radio Outburst. Publications of the Astronomical Society of Australia, 2. 60-62 doi:10.1017/s1323358000012868
In(1971) Publications of the Astronomical Society of Australia Vol. 2. Cambridge University Press (CUP)

See Also

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Riddle, A. C., Sheridan, K. V. (1971) Evolution of a Jet-like Structure in the Late Phase of a Complex Solar Outburst. Publications of the Astronomical Society of Australia, 2. 62-65 doi:10.1017/s132335800001287x
Stewart, R. T., Sheridan, K. V., Kai, K. (1970) Evidence of Type II and Moving Type IV Solar Bursts Excited by a Common Shock Wave. Publications of the Astronomical Society of Australia, 1. 313-315 doi:10.1017/s1323358000012066
Robinson, R.D., Sheridan, K.V. (1982) A Study of Multiple Type II Solar Radio Events. Publications of the Astronomical Society of Australia, 4. 392-396 doi:10.1017/s132335800002124x
Sheridan, K. V. (1970) Radio Observations of the Structure of the Solar Corona. Publications of the Astronomical Society of Australia, 1. 304-305 doi:10.1017/s1323358000012029
Robinson, R. D., Tuxford, Jennifer M., Sheridan, K. V., 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, 5. 84-113 doi:10.1017/s1323358000021676
Stewart, R. T. (1977) Coronal Magnetic Structure near the Source Region of a Type II Radio Burst. Publications of the Astronomical Society of Australia, 3. 157-159 doi:10.1017/s1323358000015204
Stewart, R. T., Duncan, R. A., Suzuki, S., Nelson, G. J. (1978) Observations of High Brightness Temperatures in Moving Type IV Solar Radio Bursts. Publications of the Astronomical Society of Australia, 3. 247-249 doi:10.1017/s1323358000015411
Sheridan, K. V. (1978) Some Recent Explorations of the Solar Corona from the Culgoora Solar Radio Observatory. Publications of the Astronomical Society of Australia, 3. 185-194 doi:10.1017/s132335800002453x
Robinson, R. D. (1974) On the Polarization Characteristics of Moving Type IV Solar Radio Bursts. Publications of the Astronomical Society of Australia, 2. 258-261 doi:10.1017/s1323358000013795
Sheridan, K. V. (1970) 80 MHz Observations of the Movement of a Type IV Source out to 6 R®. Publications of the Astronomical Society of Australia, 1. 376-378 doi:10.1017/s1323358000012406
Hansen, R. T., Garcia, C. J., Grognard, R. J.-M., Sheridan, K. V. (1971) A Coronal Disturbance Observed Simultaneously with a White-Light Coronameter and the 80 MHz Culgoora Radioheliograph. Publications of the Astronomical Society of Australia, 2. 57-60 doi:10.1017/s1323358000012856
 
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