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The correlation of solar radio bursts by magnetic activity and cosmic rays

Published online by Cambridge University Press:  14 August 2015

A. R. Thompson
A. R. Thompson*
Affiliation:
Harvard Radio Astronomy Station, Fort Davis, Texas, U.S.A.

Extract

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The sweep-frequency equipment at the Harvard Radio Astronomy Station, Fort Davis, Texas, has now been running continuously since 1956 September, recording solar radio activity in the frequency range from 100 to 580 Mc/s. The following contribution describes preliminary investigations of the correlation of the radio data with solar corpuscular emissions. This work was initiated to examine the well-known suggestions that the origins of the type II and type III radio bursts are associated with the ejection of auroral particles and cosmic rays respectively.

Type
Part II: The Sun
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 210 - 213
Copyright
Copyright © Stanford University Press 1959 

References

1. Dodson, H. W., and Hedeman, E. R. J. Geophys. Res. 63, 77, 1958.Google Scholar
2. Wild, J. P., Roberts, J. A., and Murray, J. D. Nature , 173, 532, 1954.Google Scholar
3. Tandberg-Hanssen, E. Unpublished report, 1956.Google Scholar