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The Association of Type III Bursts and Coronal Transient Activity

Published online by Cambridge University Press:  14 August 2015

B. V. Jackson ,
G. A. Dulk  and
K. V. Sheridan
B. V. Jackson
Affiliation:
University of Colorado at Boulder, U.S.A.
G. A. Dulk
Affiliation:
University of Colorado at Boulder, U.S.A.
K. V. Sheridan
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia

Extract

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Metric Type III radio bursts are nearly always associated with solar active regions. In particular, the occurrence of Type III bursts within a few minutes of the onset of the solar flares (Wild et al. 1954) is well known. During the Skylab period, a broad peak in the number of isolated Type III bursts occurred about 5 h prior to large Hα solar flares (Jackson and Sheridan 1979).

Type
Part V. Coronal and Interplanetary Responses to Short Time Scale Phenomena: - Observations
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 379 - 380
Copyright
Copyright © Reidel 1980 

References

Jackson, B. V., Sheridan, K. V., Dulk, G. A., and McLean, D. J.: 1978, Proc. Astron. Soc. Australia, 31, 241.Google Scholar
Jackson, B. V., and Hildner, E.: 1978, Solar Phys. 60, 155.Google Scholar
Jackson, B. V., and Sheridan, K. V.: 1979, Proc. Astron. Soc. Australia, in press.Google Scholar
Wild, J. P., Roberts, J. A., and Murray, J. D.: 1959, Nature, 173, 532.Google Scholar