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60. Relation between optical solar features and solar radio emission

Published online by Cambridge University Press:  14 August 2015

H. W. Dodson
H. W. Dodson*
Affiliation:
McMath-Hulbert Observatory, University of Michigan, U.S.A.

Extract

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During the last five years, we at the McMath-Hulbert Observatory have been attempting to determine the characteristics of radio-frequency radiation associated with certain of the transient solar features that we normally observe on monochromatic spectroheliograms or in integrated light. We have had the privilege of using the original 200 Mc./s. records at Cornell University and the 2800 Mc./s. records at the National Research Council in Ottawa.

Type
Part V: The Active Sun
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 327 - 333
Copyright
Copyright © Cambridge University Press 1957 

References

References

1. Covington, A. E. and Broten, N. W. ‘Solar Disk at 10·3 cm.’, A.J. 119, 569, May 1954.Google Scholar
2. Dodson, H. W. ‘Intensity Measures of Calcium Plages for Comparison with 10·3 cm. Solar Radiation, 16 October 1951’, A.J. 119, 564, May 1954.CrossRefGoogle Scholar
3. Dodson, H. W. and Hedeman, E. R. ‘Detailed Study of the Development of an Active Solar Region, 1954 August 20–27’, M.N.R.A.S. (in the Press).Google Scholar
4. Dodson, H. W., Hedeman, E. R. and Chamberlain, J. ‘Ejection of Hydrogen and Ionized Calcium Atoms with High Velocity at the Time of Solar Flares’, A.J. 117, 66, January 1953.CrossRefGoogle Scholar
5. Dodson, H. W., Hedeman, E. R. and Owren, L. ‘Solar Flares and Associated 200 Mc./s. Radiation’, A.J. 118, 169, September 1953.CrossRefGoogle Scholar
6. Dodson, H. W., Hedeman, E. R. and Covington, A. E. ‘Solar Flares and Associated 2800 Mc./s. (10·7 cm.) Radiation’, A.J. 119, 541, May 1954.CrossRefGoogle Scholar

Reference

1. Hey, J. S. and Hughes, V. A. Nature , 173, 771, 1954.Google Scholar