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Flare-associated bursts at 18 Mc/s

Published online by Cambridge University Press:  14 August 2015

Constance Warwick  and
J. W. Warwick
Constance Warwick
Affiliation:
National Bureau of Standards, Boulder, Colorado, U.S.A.
J. W. Warwick
Affiliation:
High Altitude Observatory, Boulder, Colorado, U.S.A.

Extract

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The occurrence of increased radio noise at the onset of short-wave fadeouts (SWF's) was noted by Appleton [1], who attributed the enhancements to solar emission. Payne-Scott [2], observing at about 19 Mc/s, measured burst intensities and times of occurrence to compare these high-frequency phenomena with radio events in the VHF range from 50 to 100 Mc/s.

Type
Part II: The Sun
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 203 - 207
Copyright
Copyright © Stanford University Press 1959 

References

1. Appleton, E. Nature , 156, 534, 1945; Phil. Mag. 37, 73, 1946.Google Scholar
2. Payne-Scott, R. Aust. J. Sci. Res. A 2, 214, 1949.Google Scholar
3. Lee, R. H. Electronics , 30, 162, 1957.Google Scholar
4. Shain, C. A., and Mitra, A. P. J. Atmos. Terr. Phys. 5, 316, 1954.Google Scholar
5. Maxwell, A., Swarup, G., and Thompson, A. R. Proc. I.R.E. 46, 142, 1958.Google Scholar
6. Dodson, H., Hedeman, R., and Covington, A. E. Ap. J. 119, 541, 1954.Google Scholar
7. Wild, J. P., Murray, J. D., and Rowe, W. C. Aust. J. Phys. 7, 439, 1954.Google Scholar
8. Goldberg, L., Dodson, H., and Müller, E. Ap. J. 120, 83, 1954.Google Scholar
9. Dodson, H., and Hedeman, R. J. Geophys. Res. 63, 77, 1958.Google Scholar