Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-29T07:31:16.837Z Has data issue: false hasContentIssue false

The Solar U-Burst at Metre Wavelengths

Published online by Cambridge University Press:  25 April 2016

N. R. Labrum
Affiliation:
Division of Radiophysics, CSIRO, Sydney
R. T. Stewart
Affiliation:
Division of Radiophysics, CSIRO, Sydney

Extract

The U-burst, first identified by Maxwell and Swarup and Haddock, is a type of solar radio event lasting ~ 10 s in which the frequency of the emission at first drifts rapidly downwards, then increases again. On the dynamic spectrum record the burst has the appearance of an inverted letter U.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1970

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Maxwell, A. and Swamp, G., Nature, 181, 36 (1958).Google Scholar
2 Haddock, F. T., Proc. I.R.E., 46, 1 (1958).Google Scholar
3 Haddock, F. T., ‘Paris Symposium on Radio Astronomy’, ed., Bracewell, R. N., Stanford University Press, Stanford 1959, p. 188.Google Scholar
4 Takakura, T., Space Science Rev., 5, 80 (1966).Google Scholar
5 Newkirk, G., Ap. J., 133, 983 (1961).CrossRefGoogle Scholar
6 Stewart, R. T., Aust. J. Phys., 18, 67 (1965).Google Scholar
7 Weiss, A. A. and Stewart, R. T., Aust. J. Phys., 18, 143 (1965).Google Scholar
8 Zheleznyakov, V. V. and Zaitsev, V. V., Astr. Zh., 45, 19 (1968). Trans. Soviet Astron. A.J., 12, 14 (1968).Google Scholar
9 Smerd, S. F., Wild, J. P. and Sheridan, K. V., Aust. J. Phys., 15, 180 (1962).Google Scholar